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Key West, Florida, located on the border of two great bodies of water, the Gulf of Mexico and the Atlantic Ocean, offers vacationers the opportunity to witness some of the planets most remarkable aquatic creatures. The thriving marine environment of the Florida Keys including brilliantly colored tropical fish, endangered sea turtles, huge manta rays, and, of course, the fish that swim at the top of the oceans food chain, the sharks. Our expert naturalist guides will transport you into the back country flats to see these sleek toothy predators in their natural environment. You will learn everything there is to know about these amazing voracious fish.
Key West Shark Adventures Information
On our Key West shark adventures we bring you into the saltwater flats, you will be transported aboard a sleek catamaran that has a minimal draft in order to maneuver through the shallows of this area. Our Key West shark adventures experts then draw the sharks to the boat by releasing an alluring scent into the water. As the odor drifts out into the currents and flats, the sharks will detect it with their remarkably sensitive sense of smell. You will be astounded by the amount of swarming sharks that will surround the hull.
The shark species that may be viewed on these adventures include bull sharks, lemon sharks, nurse sharks, and black tip sharks. Occasionally, passengers on our shark watching expeditions may even spot a tiger shark or a hammerhead. Since the waters in flats are usually crystal-clear, viewers will have no difficulty seeing every small detail of these alpha hunters.
Wild Dolphin Encounter and Snorkel
Watching dolphins frolic in the gorgeous waters off the coast of Key West will be the highlight of your vacation. You may even have an opportunity to snorkel beside these friendly and intelligent creatures. Youll have the chance to snorkel above the only living coral reef in the continental United States.
09:00 AM12:30 PM02:30 PM
Shark Adventure
Join our nature guides for a trip into saltwater flats and channels to witness a variety of the oceans toothy apex predators: the sharks. In addition to possibly seeing bull sharks, hammerheads, lemon sharks, nurse sharks, black tip reef sharks and occasionally tiger sharks, you can see plenty of other local wildlife species.
Sail Snorkel Kayak
Sail the turquoise waters off Key West, Florida, aboard our skipjack sailing vessel, the Danger. Go snorkeling above some of the most beautiful coral reefs on the planet. Explore the nature preserve of the Mangrove Islands on a guided sea kayaking excursion.
09:00 AM02:00 PM


1st or second choice candidates who seek for Federal University of Agriculture, Makurdi (FUAM), Admission 2019/2020 should see requirements, Application Process and be Ready for the Unified Tertiary Matriculation Examination.
VERY IMPORTANT: The Federal University of Agriculture, Makurdi (FUAM) Post UTME Admission Form for the 2019/2020 is not available at the moment…we will advice that you to stick around or better bookmark this very page once the FUAM Post UTME Admission Form 2019 is out this page will be updated immediately.
While waiting for the Federal University of Agriculture, Makurdi (FUAM) Post UTME Admission Form/DE Screening Exercise for the 2019/2020 see how it was conducted previously.
All applicants seeking admission into FUAM are hereby invited to register on-line for the 2018/2019 academic session admission. Any candidate who fails to participate in the screening exercise will not be considered for admission into the Federal University of Agriculture, Makurdi.
Candidates who selected University of Agriculture, Makurdi as first choice in the 2018/2019 Unified Tertiary Matriculation Examination (UTME) and scored 170 marks and above are invited for the Post-UTME Screening exercise slated to commence on 2nd October, 2018.
How to Apply for FUAM Post UTME.
The Date, Time and Venue of your Screening will be communicated to you.
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Vehicle Networking & Connectivity
Volkswagen's CARIAD and STMicroelectronics to Co-Develop Chip for Software-Defined Vehicles
CARIAD, the software unit of Volkswagen Group, and STMicroelectronics will shortly launch the joint development of an automotive system-on-chip (SoC), a new cooperation model for software-defined cars.
Together, CARIAD and ST are developing tailored hardware for connectivity, energy management, and over-the-air updates designed to make vehicles fully software-defined, secure, and future-proof.
The planned cooperation targets the new generation of Volkswagen Group vehicles that will be based on the unified and scalable software platform. At the same time, the parties are moving to agree that TSMC, one of the world's leading dedicated semiconductor foundry companies, will manufacture the SoC wafers for ST. With this move, CARIAD aims to secure the chip supply for the Volkswagen Group's cars years in advance.
As part of its semiconductor strategy, CARIAD will enter into direct relationships with semiconductor suppliers at the Tier 2 and Tier 3-level for the Volkswagen Group for the first time. In the future, CARIAD plans to direct Tier 1 suppliers of the Group to use only the SoC co-developed with ST and ST's standard Stellar microcontroller for CARIAD's zone architecture.
This co-development is a first for CARIAD and ST. "With the co-development of the system-on-chip with ST ahead of us, we are consistently pursuing our semiconductor strategy. The SoC we are designing will be optimally matched to our software – without compromise. In this way, we can offer our Group's customers the best performance for their cars," says CARIAD CEO Dirk Hilgenberg. "The use of a single, optimized architecture in all Volkswagen electronic control units will give us an enormous boost for the efficient development of our software platform." This efficiency will allow all electronic control unit (ECU) devices – from microcontrollers to SoCs – to run on a common basic software in the future.
The new SoC aims to complement ST's high-performance Stellar microcontroller family by extending its power-efficient real-time capabilities to service-oriented environments. CARIAD is contributing its specific target requirements and functionalities for the Volkswagen Group vehicles and will help extend the architecture of ST's 32-bit Stellar Automotive microcontroller.
CARIAD will include both the jointly developed SoCs based on Stellar and the standard Stellar microcontroller in its new AU1 processor family. Its range offers CARIAD flexible scaling for various applications in the car to meet the needs of all Volkswagen Group brands. The chips are being designed for all applications in the areas of networking, drivetrain, energy management, and comfort electronics – in zone controllers or in servers in VW's operating system, VW.OS. Building on Stellar's unique attributes, the entire AU1 processor family will be able to map future function extensions via over-the-air updates. Using a common device architecture will enable CARIAD experts to develop only one basic software for all electronic control units (ECU), substantially reducing complexity and accelerating development. Moreover, the Stellar architecture encourages the integration of numerous functions into individual ECUs. This is designed to reduce the number of ECUs in the car, increasing the cost effectiveness and reliability for the software company.
The collaboration with ST enables CARIAD to further expand its expertise in semiconductors and gain additional experience in their co-development.
For more information, visit https://cariad.technology.
Automotive - Vehicle Networking & Connectivity
Processing - Chips & SoCs
IoT Medical Device Security Risks and Mitigation
Avalue Announces Leading-Edge Digital Paper Products
Digital Medical Surgery Tools Are Becoming Commonplace. Finding the Right Solutions Partner Is Key
Product of the Week: APLEX's PhanTAM Stainless Steel Panel PC and Display Solution Series
Powering the Next Generation of Connected-Health Wearables and Hearables with Solid-State Lithium Microbatteries

redpajama_set_name: RedPajamaCommonCrawl


text:
package org.bremersee.comparator.spring.converter;

import java.util.Objects;
import org.bremersee.comparator.model.SortOrders;
import org.bremersee.comparator.model.SortOrdersTextProperties;
import org.springframework.core.convert.converter.Converter;
import org.springframework.lang.NonNull;

/**
 * The sort orders converter.
 *
 * @author Christian Bremer
 */
public class SortOrdersConverter implements Converter<String, SortOrders> {

  private final SortOrdersTextProperties properties;

  /**
   * Instantiates a new sort orders converter.
   */
  public SortOrdersConverter() {
    this(SortOrdersTextProperties.defaults());
  }

  /**
   * Instantiates a new sort orders converter.
   *
   * @param properties the properties
   */
  public SortOrdersConverter(SortOrdersTextProperties properties) {
    this.properties = Objects
        .requireNonNullElse(properties, SortOrdersTextProperties.defaults());
  }

  @Override
  public SortOrders convert(@NonNull String source) {
    return SortOrders.fromSortOrdersText(source, properties);
  }
}

redpajama_set_name: RedPajamaGithub


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Debate to begin in US Senate on Biden's $1.9 trillion Covid-19 relief bill
The Senate voted on Thursday to take up the bill in a party-line 51-50 vote, with Democratic Vice President Kamala Harris breaking the tie. But Republicans delayed the start of the debate by forcing the hours-long reading of the full text of the 628-page measure.
Joe Biden nominates transgender woman as assistant health secretary of US: Report
The announcement makes Rachel Levine, a 64-year-old pediatrician, to be the first openly transgender federal official to be confirmed by the US Senate, The Washington Post reported on Tuesday.
Replacing Obamacare by new law in US risk to biz: Dr Reddy's
New Delhi, Jun 25 () Homegrown pharma major Dr Reddy's believes that replacing 'Obamacare' by another law in the US will pose risk to its business that can have adverse material effect on financial performance.
Seema Verma confirmed by Senate for top health post in Trump administration
Verma, who has been described by the White House as the "unquestionably qualified" first generation Indian-American, was confirmed by the Senate by a vote of 55-43.
9h	Govt extends HLL Lifecare bid submission deadline till February 28


The Descendant Charts are read from left to right with the oldest ancestor on the left. By clicking on any ancestor in a Descendant Chart, you will be taken to a Person Page that will provide the known detail on that person.
Page created by John Cardinal's Second Site v3.0.7.


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Live Drugs (Gatefold)
2LP | NEW | 2020
SUPER HIGH QUALITY RECORDS
Rock Indie
LIVE DRUGS is a collection culled from over 40 hard drives of recorded live shows spread out across years of touring behind multiple albums. It's the first volume to capture the band's live interpretations and a document showcasing the evolution of the band's live show over the years. It's also a portrait of the enduring relationship between Granduciel and LIVE DRUGS's co-producer Dominic East, a longtime friend, guitar tech and stage manager. Today, they present it's lead single, "Pain (Live)," "a hypnotic and excellent blast of heartland rock" (Entertainment Weekly). LIVE DRUGS is sequenced to reflect how a typical 70-minute show would flow. It thrives on live set staples immortalized on record for the first time and illustrates how years of live performance nurtures an evolution of the songs. This includes "Buenos Aires Beach" from the band's 2008 full-length debut, Wagonwheel Blues, and a cover of Warren Zevon's "Accidentally like a Martyr."


For the past two years, Lopez High School has not participated in track-related sporting events. This year the Lobos a triumphant return to the track for Lopez School with 11 students on the roster. Of the 11 participating on the track team this year, six are exchange students and five are local kids. The Lobos will be represented on the track by three women, and eight men.
All the students on the team are new to track, according to coach Larry Berg, they are still trying out different events, attempting to discover their niche. Berg has coached the Lopez football team for 30 years, and basketball for 24, he is new to coaching track so this is a learning experience for him as well.
The first meet the team will attend will be in La Conner on Thursday, March 17 at 3:30 p.m. The season for track will continue until the end of May. According to Berg, no track meets will be held at the Lopez School because the track is not structurally suitable for hosting events.


The first pizzeria in the USA, Lombardi's, set a series of events in motion that would make pizza the classic it is today. 13% of Americans eat pizza on any given day.
As everyone knows, we can top a pizza with whatever we want, and some toppings have even started debates and arguments between pizza lovers. Banana (Curry Pizza) or pineapple (Hawaiian) pizza usually gets half of the party frowning, while the other half finds it delicious.
But now there's a pizza that everyone can agree on – with sausages topping and filled crust, writes the site Delish.
The best thing about pizza is that you can choose any topping your heart desires. Tuna, pineapple, banana, chicken, beef or sausage – it's all up to you. With sausages, you'd usually think of salami. But now people can get their pizza with normal hot dog sausages.
Domino's Pizza has released a new pizza called – just that – Hot Dog Pizza.
It comes in two variants: a baked Calzone filled with mozzarella, sliced hot dog, and yellow mustard; and a delicious pizza with sausage-style meat on top and hot dog sausage stuffing in the crust.
Besides sliced hot dog sausages, we find mozzarella and mustard on the pizza as well, according to Delish.
However, Dominos didn't stop there, and also unleashed a mix between a burger and a pizza. This fast food Frankenstein is composed of tomato sauce, mozzarella, beef meatballs, onions, pickles, tomatoes, and a bit of burger sauce.
It bears the completely-and-utterly unexpected name: The Burger Pizza.
However, these American-inspired products are only available in France at the moment. So maybe if you are planning a trip to Paris you can visit any Domino's store and taste the American Dream, from Europe, so you don't get homesick. Or just wait until it comes to the States.
What a dream for all hot dog, pizza and burger lovers! Now press SHARE so your friends can book their trip to Paris as well!


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2023 Congress at a Glance
2023 Herzberg and Plenary Speakers
Comité organisateur du congrès 2023
Comité organisateur local 2023
Hébergement 2023
Liste des conférenciers invités 2023
Meilleure présentation d'étudiant(e) 2023
Directives pour la publication des résumés gagnants dans PaC
Soumission des résumés 2023
Journée des symposiums 2023 – 20 juin
Organiser les congrès
Congrès de l'ACP 2022
Atelier pour les étudiants, dimanche 5 juin
La série estivale sur la communication scientifique – Le Conseil consultatif des étudiants (CCÉ) de l'ACP
Informations importantes si vous vous rendez à Hamilton
Où manger au campus de McMaster et des alentours
Transportation à l'Université McMaster
Quoi faire à Hamilton
Visa et voyages internationaux
COVID-19: Mesures et exigences de l'Université McMaster
Le Congrès en un coup d'œil
Programme du Congrès – lien
Atelier sur la politique scientifique
Journée des symposiums – 7 juin
Symposium des physiciens du secteur privé
Atelier pour enseignants du secondaire
merc. 8 juin, Banquet – Info et Menus
Petit-déjeuner / Stationnement sur le campus
Instructions pour les présentateurs oraux
Frais d'inscription 2022
Termes et conditions et politique de remboursement
Instructions pour les présentateurs d'affiches
Meilleure présentation d'étudiant 2022
Soumission des résumés
Opportunités de commandites / kiosques 2022
Les commandites 2022
Les exposants 2022
Comité organisateur local originale de 2020
Herzberg et les conférenciers pléniers 2022
Comité organisateur du congrès
Congrès virtuel de l'ACP 2021 – 6-11 juin
Assemblée générale annuelle virtuelle de l'ACP 2021 (AGA)
Congress at a Glance
Informations pour tous les conférenciers
Journée du symposium – 8 juin 2021
Symposium du secteur privé
Meilleur présentation d'étudiant(e)
Les lauréats de 2021 pour les meilleures présentations étudiantes
Processus et frais d'inscription pour 2021
Conditions générales et politique de remboursement – Congrès virtuel de l'ACP 2021
2021 Atelier pour les enseignants du secondaire/Cegep (anglais seulement)
Congrès virtuel de l'ACP 2020, 8-12 juin plus activités additionnelles du 15 juin au 16 juillet
Considering a career outside of academia?
Prix de la meilleure présentation orale pour étudiants
Soumission de résumés
Announces COVID-19 (11 mars, 2020)
Congrès l'ACP 2019 – Simon Fraser University (Burnaby, C-B)
2019 Graduate Students at Congress (en anglais seulement)
Gagnants du prix du congrès
Aperçu du congrès 2019
Instructions pour les présentations orales
Instructions pour présentation d'affiche
Liste des conférenciers pléniers et Herzberg 2019
Journée de colloques – Sujets / Coordinateurs
Visites – TRIUMF/ Observatoire Trottier / Laboratoires de SFU
S'inscrire maintenant – les frais augmentent le 28 mai
Conseils pour l'inscription au Congrès de l'ACP 2019
Inscription à l'arrivée
Compétition pour la meilleure communication étudiante 2019
Gagnants – Prix des affiches des étudiants de l'ACP
Commanditaires 2018
Opportunités de commandites / kioskes 2019
Comité de programmation du congrès 2019
Comité organisateur local du congrès 2019
2019 Changements au programme
Matériaux pour l'assemblée générale annuelle 2019
Élection du 5 juin : conseil d'administration de l'ACP 2019-2020
Conférence publique commémorative Herzberg 2018
Liste des conférenciers pléniers 2018
Politique d'annulation et de remboursement
Matière molle Canada 2018
Comité Organisateur Local
Opportunités de commandites 2018
Visites de laboratoires
Étudiants diplômés au congrès
Le Banquet des récipiendaires de médailles de l'ACP
Les délégués observant le Ramadan
L'expérience de Halifax
Affiche-Directives
Oral-Directives
Prix de Divisions
Instructions – Affiche
Aperçu du Congrès
Exposants au Congrès de l'ACP 2017
Conférenciers invites 2017
Partenaires et commanditaires du congrès de l'ACP 2016
Journée des enseignants
Commanditaires et partenaires du Congrès de l'ACP 2015
Journée des enseignants 2015
La Conférence d'étudiants diplômés de physique CAM
Historique du lieu de CAM et de la participation
CAM 2017
Formulaire en ligne de Déclaration d'intérêt à la CCUWiP 2023
Renseignements sur la demande pour accueillir la CCUWiP 2023
Autres conférences parrainées
Formulaire de soumission d'événements
En 2000, le conseil de l'ACP a décidé de remplacer par une conférence publique la conférence plénière du dimanche, à son congrès annuel. On l'a appelée « Conférence publique commémorative Herzberg » en l'honneur du Dr Gerhard Herzberg, lauréat du prix Nobel et membre de longue date de l'ACP, en reconnaissance de son désir avoué de sensibiliser aux sciences le public, en particulier les jeunes, et de les leur faire apprécier. L'aide au conférencier Herzberg est assurée, en partie, par un legs du Dr Herzberg.
La conférence inaugurale s'est tenue au Unicentre Auditorium de l'Université de Victoria, le dimanche 17 juin 2001, à compter de 19 h, sous le titre « Gravitational Waves: A New Window onto the Universe ». Le Dr Kip Thorne, de l'Université Caltech, l'a prononcée.
Veuillez trouver ci-après la liste détaillée des conférenciers (du plus récent au plus ancien), leurs notices biographiques ainsi qu'un résumé de leurs propos.
2022 Conférence publique commémorative Herzberg
2022 McMaster University, Lundi 6 juin 2022, 19 h 30 HAE
DONNA STRICKLAND, University of Waterloo
Generating High-Intensity, Ultra-short Optical Pulses
Aucun enregistrement disponible
Résumé (disponible en anglais seulement)
With the invention of lasers, the intensity of a light wave was increased by orders of magnitude over what had been achieved with a light bulb or sunlight. This much higher intensity led to new phenomena being observed, such as violet light coming out when red light went into the material. After Gérard Mourou and I developed chirped pulse amplification, also known as CPA, the intensity again increased by more than a factor of 1,000 and it once again made new types of interactions possible between light and matter. We developed a laser that could deliver short pulses of light that knocked the electrons off their atoms. This new understanding of laser-matter interactions, led to the development of new machining techniques that are used in laser eye surgery or micromachining of glass used in cell phones.
Conférencier (disponible en anglais seulement)
Donna Strickland is a professor in the Department of Physics and Astronomy at the
University of Waterloo and is one of the recipients of the Nobel Prize in Physics 2018
for developing chirped pulse amplification with Gérard Mourou, her Ph.D. supervisor at the time.
Strickland earned a B.Eng. from McMaster University and a Ph.D. in optics from the
The University of Rochester. Strickland was a research associate at the National Research
Council Canada, a physicist at Lawrence Livermore National Laboratory and a member
of technical staff at Princeton University. In 1997, she joined the University of
Waterloo, where her ultrafast laser group develops high-intensity laser systems for
nonlinear optics investigations.
Strickland served as the president of Optica in 2013 and is a fellow of Optica, SPIE,
the Royal Society of Canada and the Royal Society. She is an honorary fellow of the
Canadian Academy of Engineering and the Institute of Physics, an international member
of the US National Academy of Science and member of the Pontifical Scientific
Academy. Strickland was named a Companion of the Order of Canada.
2021Conférence publique commémorative Herzberg
Congrès virtuel, dimanche 6 juin 2021, 18 h 00 HAE, Plate-forme virtuelle du congrès Underline
FRANK WILCZEK, Massachusetts Institute of Technology (MIT)
Quanta of the Third Kind: Anyons
For many years physicists divided the world of quantum particles into two kingdoms – bosons and fermions. Anyons are particles with a sort of memory, that fall outside those kingdoms. In recent decades theorists have produced an enormous literature about the possible occurrence and properties of anyons. It is only in the last few months, however, that clear experimental confirmation has appeared. I will review the theoretical background and describe the breakthrough experiments. Anyons will be central in a new and promising method of information processing: topological quantum computing.
Frank Wilczek is a theoretical physicist, author, and intellectual adventurer. He has received many prizes for his work, including a Nobel Prize in Physics.
Frank has made seminal contributions to fundamental particle physics, cosmology and the physics of materials. His current theoretical research includes work on Axions, Anyons, and Time Crystals. These are concepts in physics which he named and pioneered. Each has become a major focus of research world-wide. In recent years Frank has become fascinated with prospects for expanding perception (especially color perception) through technology. He is developing hardware and software tools for this. Frank has authored several well-known books and writes a monthly "Wilczek's Universe" feature for the Wall Street Journal. His latest book, "Fundamentals: Ten Keys to Reality", distils the most profound and mind-expanding insights of modern science, and explores their implications for questions that are usually considered philosophical or even theological. Early reviews have been enthusiastic, including this from the New York Times: "Whether or not you're accustomed reading physics for pleasure, the Nobel Laureate Frank Wilczek's *Fundamentals* might be the perfect book for the winter of this plague year … Wilczek writes with breathtaking economy and clarity, and his pleasure in his subject is palpable . . ."
Wilczek received a B.S. at the University of Chicago in 1970, and a PhD in physics at Princeton University in 1974. Currently he is the Herman Feshbach professor of physics at the MIT; Founding Director of the T. D. Lee Institute and Chief Scientist at Wilczek Quantum Center, Shanghai Jiao Tong University; Distinguished Professor at Arizona State University; and Professor at Stockholm University.
He has been married to Betsy Devine since 1973. They have two daughters.
Le congrès en personne de 2020 a été annulé en mars 2020 en raison de la pandémie de COVID-19. La conférence publique Herzberg 2020 de Donna Strickland a été reportée jusqu'à ce que le Congrès reprenne son format en personne. Nous avons été en mesure d'offrir certains autres éléments du programme du Congrès 2020 de manière virtuelle via Zoom.
2019 Simon Fraser University, lundi 3 juin 2018, à 19 h 30
MANU PRAKASH, Stanford University
« La science frugale à l'ère de la curiosité »
La science est confrontée au défi de l'accessibilité. Bien que l'information et la connaissance deviennent rapidement disponibles à tout dans le monde, l'expérience de la science est considérablement limitée. Une approche visant à résoudre ce défi est la démocratisation de l'accès à des outils scientifiques. Manu Prakash croit que cela peut être atteint par le biais de la « science frugale »; une philosophie qui sous-tend à la conception, au développement et au déploiement d'outils scientifiques à la fois extrêmement abordables et puissants pour les masses. En utilisant des exemples provenant de son propre travail (le Foldscope : un microscope en origami à un dollar et le Paperfuge : une centrifugeuse à haute vitesse à vingt-cinq cents), le Dr Prakash décrira le processus d'identification des défis, la conception de solutions et le déploiement de ces outils à l'échelle mondiale afin de faire naître la curiosité et des recherches scientifiques ouvertes dans les communautés du monde entier. En faisant le lien entre l'éducation scientifique, la santé mondiale et la surveillance environnementale, il explorera le rôle des outils « simples » pour faciliter l'accès à une meilleure santé humaine et planétaire dans un monde aux ressources limitées.
Manu Prakash est professeur associé de bio-ingénierie à l'Université Stanford, œuvrant dans le domaine de la biologie physique et la science frugale. Il associe sa passion pour la science fondamentale au développement de technologies abordables et accessibles pouvant être utilisées pour l'éducation scientifique, la recherche et la santé publique dans des environnements pauvres en ressources, dans le but de démocratiser l'accès aux outils scientifiques. Il est surtout connu pour le développement du microscope en papier extrêmement abordable, le Foldscope, ainsi que du Paperfuge, une centrifugeuse manuelle à vingt cents faite de papier et de ficelle. En 2016, il s'est vu attribuer la bourse MacArthur, une bourse du corps professoral HHMI-Gates, la distinction d'Explorateur émergent du National Geographic en 2015 ainsi que le Prix du nouvel innovateur du directeur du NIH, parmi d'autres nombreuses reconnaissances.
Manu Prakash est titulaire d'un baccalauréat en technologie de l'institut indien de technologie de Kanpur (2002) ainsi que d'un doctorat de l'Institut de technologie du Massachusetts (MIT) (2008). Il a été un jeune boursier de la Société des boursiers de Harvard (de 2008 à 2011) avant de rejoindre le corps enseignant de l'Université Stanford, où il est actuellement professeur adjoint dans le département de bio-ingénierie, est actuellement membre du programme de biophysique de l'École de médecine et du Centre pour l'innovation en santé mondiale, de même que boursier du corps professoral de Stanford ChEM-H, et il est membre affilié de l'Institut pour l'environnement Woods. Il occupe de plus le poste de boursier du corps professoral HHMI-Gates et celui d'enquêteur BioHub. Titulaire de nombreux brevets, sa recherche a par ailleurs été largement publiée.
2018 – Conférence publique commémorative Herzberg
2018 Dalhousie University, lundi 11 juin 2018, à 19 h 30
NERGIS MAVALVALA, Laser Interferometer Gravitational-wave Observatory (LIGO)/Massachusetts Institute of Technology
L'Univers gauchi : la quête centenaire d'Einstein à la découverte des ondes gravitationnelles
(Photo by Darren McCollester/for MacArthur Foundation)
Les annonces récentes de la toute première détection d'ondes gravitationnelles émanant de la collision d'étoiles à neutrons et de trous noirs ont amorcé une nouvelle ère de l'astrophysique de ces ondes. Einstein avait prédit les ondes gravitationnelles il y a 100 ans. Je décrirai l'histoire scientifique, technologique et humaine derrière ces découvertes qui ouvrent de toutes nouvelles perspectives sur certains événements les plus violents et tordus de l'Univers.
Conférencière
Nergis Mavalvala est une physicienne dont les recherches sont axées sur la détection d'ondes gravitationnelles à partir des événements violents qui, dans le cosmos, créent des vagues et des ondulations dans le tissu espace-temps. Elle était membre de l'équipe scientifique qui a annoncé la première détection directe d'ondes gravitationnelles, nées de la collision de trous noirs, à l'aide des détecteurs du Laser Interferometer Gravitational-wave Observatory (LIGO) en février 2016. Mme Mavalvala a reçu un B.A. du Wellesley College en 1990 et un doctorat de l'Institut de technologie du Massachusetts (MIT) en 1997. Elle sera chercheuse postdoctorale, puis chercheuse à l'Institut de technologie de Californie entre 1997 et 2002. Depuis, elle est professeure de physique à l'Institut de technologie du Massachusetts où elle est maintenant professeure « Marble » de physique, directrice adjointe du Département de physique et lauréate d'un prix « génie » MacArthur 2010. Dans ses temps libres, elle adore faire du vélo sur de longues distances, divers sports et fréquenter les membres de sa famille.
2017 Université Queen's, lundi 29 mai 2017, à 19 h 30, Centre Isabel Bader
ARTHUR B. McDONALD, Université Queen's, et le SNOLAB
« Questions profondes, noires : les neutrinos et la matière noire à l'ONS et à SNOLAB »
En descendant à deux kilomètres sous terre et en créant un laboratoire ultra-propre, il est possible de s'attaquer à certaines questions très fondamentales concernant notre Univers : Comment le Soleil se consume t-il?; Quelles sont les particules de matière noire qui composent 27 % de notre Univers?; Quelles sont les propriétés des neutrinos, ces particules insaisissables qui sont l'une des composantes fondamentales de la nature?
L'Observatoire de neutrinos de Sudbury (ONS) a permis d'observer, chez les neutrinos, de nouvelles propriétés qui débordent le modèle standard des particules élémentaires et confirment l'exactitude poussée des modèles sur la manière dont le Soleil se consume. Le laboratoire agrandi SNOLAB permet d'accueillir le monde dans des expériences en collaboration où l'on cherche les propriétés des particules de matière noire, en quête d'autres propriétés des neutrinos et pour capter les signaux neutrino émis par les supernovae de notre galaxie, la Terre et le Soleil. On décrira les avantages découlant de l'aménagement de l'un des laboratoires ayant la radioactivité la plus faible du monde et la science fondamentale qui en émane.
Arthur McDonald naît à Sydney, Nouvelle-Écosse, au Canada. Il est diplômé en physique de l'Université Dalhousie (B.Sc., M.Sc.) et de Caltech (doctorat), et titulaire de neuf grades honorifiques. Il est chargé d'études aux Laboratoires de l'EACL à Chalk River de 1969 à 1982; professeur à l'Université Princeton de 1982 à 1989; professeur à l'Université Queen's de Kingston, au Canada de 1989 à 2013, et professeur émérite en 2013. À partir de 1989, il est directeur de l'Initiative de collaboration scientifique de l'Observatoire de neutrinos de Sudbury (ONS). Entre autres, il est Compagnon de l'Ordre du Canada; colauréat du Prix Nobel de physique 2015 et de la médaille Benjamin Franklin en physique 2007; colauréat du prix d'innovation 2016 de physique fondamentale (Breakthrough Prize in Fundamental Physics) et du Prix Polanyi 2006 pour la collaboration scientifique de l'ONS. Il poursuit ses travaux de recherche fondamentale sur les neutrinos et la matière noire au laboratoire souterrain SNOLAB. Il est membre du conseil d'administration de l'Institut Périmètre.
2016 University of Ottawa, Monday, June 13, 2016, 7:30 P.M., The Shaw Centre
VICTORIA KASPI, Department of Physics, McGill Univeristy
The Cosmic Gift of Neutron Stars
Although they are thousands of light years away, neutron stars can act as very precise cosmic beacons — a celestial gift that sheds light on some of the most interesting problems in modern science. We will explore these strange objects, explain how astronomers are using them to study issues ranging from the origins of the Universe to the very nature of matter, and even listen to the cosmic symphony they create.
Victoria Kaspi is a Professor of Physics at McGill University, where she holds the Lorne Trottier Chair in Astrophysics and Cosmology, and a Canada Research Chair in Observational Astrophysics. She is also Director of the newly created McGill Space Institute.
She received a B.Sc. (Honours) in Physics from McGill University in 1989, and an M.A. and Ph.D. in Physics from Princeton University in 1991 and 1993 respectively. From 1994-96, she held a Hubble Postdoctoral Fellowship at the Jet Propulsion Laboratory and California Institute of Technology. She was an Assistant Professor of Physics at the Massachusetts Institute of Technology from 1997-2000, and joined the McGill Department of Physics in 2000.
Prof. Kaspi uses techniques of radio and X-ray astronomy to study rapidly rotating, highly magnetized neutron stars. She has done significant work involving radio pulsars and magnetars. More specifically, she has contributed among other things to the study of binary pulsar dynamics, the neutron star population, as well as the study of magnetars, the most highly magnetized objects known in the Universe.
Prof. Kaspi has been the recipient of numerous awards and honours, including the Killam Prize in 2015, NSERC's John C. Polanyi Award in 2011, the Prix du Québec in 2009, the Harvard University Sackler Lectureship in 2009. She is the R. Howard Webster Foundation Fellow of the Canadian Institute for Advanced Research, and a Fellow of the Royal Society of Canada. In 2010 she was inducted as a Fellow of the Royal Society of London, and elected to the U.S. National Academy of Sciences, and was inducted into the American Academy of Arts and Sciences in 2015
2015 University of Alberta, Monday, June 15, 2015, 7:30 P.M., Myer Horowitz Theatre
MIGUEL ALCUBIERRE, Nuclear Sciences Institute, National Autonomous University of Mexico
Faster than the Speed of Light
In this talk I will give a short introduction to some of the basic concepts of Einstein's special theory of relativity, which is at the basis of all of modern physics. In particular, I will concentrate on the concept of causality, and why causality implies that nothing can travel faster than the speed of light in vacuum. I will later discuss some of the basic ideas behind Einstein's other great theory, General Relativity, which is the modern theory of gravity and postulates that the geometry space-time is dynamic and the presence of large concentrations of mass and energy produce a "curvature" in space-time. I will then talk about how the curvature of space-time can be used in several ways to travel "faster than the speed of light" by distorting the geometry away from that of flat space. In particular, I will discuss the ideas behind the geometric model for a "warp drive".
Prof. Miguel Alcubierre was born in Mexico City in 1964. He obtained his Physicist degree from the National University in Mexico (UNAM) in 1988, and a PhD in Physics from the University of Wales in 1994. He later worked for several years as an Adjunct Professor at the Max Planck Institute for Gravitational Physics in Potsdam, Germany. Since 2002 he joined the Nuclear Sciences Institute at UNAM where he is now a Full Professor, and since June 2012 the Director. His research is in the area of numerical relativity, which is concerned with the computational simulation of astrophysical systems using Einstein's theory of general relativity. In this area he has concentrated on the study of sources of gravitational waves, and particularly black hole collisions. He is author of more than 50 publications, as well as a textbook published by Oxford University Press.
2014 Laurentian University, Monday, June 16, 2014, 7:30 P.M., Rooms FA-054+5+6, A-226
JOHN ELLIS, King's College, London, UK
The Higgs Boson and Beyond
Where do we come from? What are we? Where are we going? The discovery of the Higgs Boson at the LHC provides new insights into these basic questions about the Universe, marking the start of a new era in fundamental physics, and opening new vistas in astrophysics and cosmology as well as particle physics.
John Ellis currently holds the Clerk Maxwell Professorship of Theoretical Physics at King's College in London. After his 1971 PhD from Cambridge University, he worked at SLAC, Caltech, and CERN (Geneva), where he was Theory Division Leader for six years. His research interests focus on the phenomenological aspects of elementary particle physics and its connections with astrophysics, cosmology and quantum gravity. Much of his work relates directly to interpreting results of searches for new particles. He was one of the first to study how the Higgs boson could be produced and discovered. He is currently very active in efforts to understand the Higgs particle discovered recently at CERN, as well as its implications for possible new physics such as dark matter and supersymmetry. He also studies possible future particle accelerators, such as the Compact Linear Collider (CLIC) and future circular colliders, is known for his relentless efforts to promote global collaboration in particle physics. John Ellis was awarded the Maxwell Medal (1982) and the Paul Dirac Prize (2005) by the Institute of Physics. He was elected Fellow of the Royal Society of London in 1985 and of the Institute of Physics in 1991, and is an Honorary Fellow of King's College Cambridge and of King's College London.
2013 Université de Montréal, Monday, May 27, 2013, 7:30 P.M., K500, Salle Ernest-Cormier, Pavillon Roger-Gaudry
SERGE HAROCHE, Collège de France & École Normale Supérieure, Paris
Juggling with Photons in a Box to Explore the Quantum World
We know since Einstein seminal paper of 1905 on the photoelectric effect that light, known since Maxwell to be an electromagnetic wave, is also made of discrete quanta, the photons. This strange wave-particle dualism has opened the way to the quantum theory and revolutionized physics. When they discussed among themselves the counter- intuitive quantum concepts, the fathers of the theory – Einstein, Bohr and Schrödinger among them – used to describe « thought experiments » in which they imagined that they freely manipulated photons, electrons or atoms and observed their weird behaviour. At the same time, they believed that these ideal experiments would be forever impossible to turn into actual ones in the laboratory. A major difficulty to realize these experiments with photons is that they are very fragile and elusive particles, usually destroyed upon detection. Technological advances have recently changed this state of affairs and made it possible to manipulate photons in ways which were previously thought impossible. I will describe this adventure and show how we have built a "photon box" in which we can count light quanta without destroying them, as we can do with marbles in a bag. We have also "tailored" the light trapped in the box and generated laboratory versions of the famous Schrödinger cat which the Austrian physicist imagined to be suspended between life and death. In our case, the "cat" is made of photons instead of atoms and it is maintained "half-way" between two states which classical physicists would consider to be incompatible. By studying this strange behaviour, we get a deeper knowledge about the quantum laws and we learn tricks that we hope to use one day for developing new technologies which could improve the precision of measurements, the secrecy of communications or the power of computer simulations.
Dr. Serge Haroche is professor of quantum physics at the Collège de France and the Ecole Normale Supérieure de Paris. He is the recipient, with David Wineland, of the 2012 Nobel Prize in physics.
2012 University of Calgary, Monday, June 11, 2012, 7:30 P.M., Red & White Club, McMahon Stadium
ANTON ZEILINGER, University of Vienna
Quantum Information: From the Foundations to a New Technology
In this presentation for the general public, Dr. Zeilinger will explain some of the fundamental issues in quantum mechanics and show how their application opens up new avenues to a completely novel future information technology. Among the fundamental concepts the randomness of individual events was rejected by Albert Einstein in his famous statement "God does not play dice". The concept of quantum superposition implies that a system can be in states which classically exclude each other like the states "alive" and "dead" of Schrödinger's famous cat. And the concept of entanglement implies that two or more systems can be separated over large distances and still form one unity. This was rejected by Einstein as "spooky action" at a distance. All these concepts lead to exciting and novel applications like quantum computation, quantum communication, quantum cryptography and quantum teleportation. In the talk, Zeilinger will sketch some of the most recent results in this extremely active world-wide research program and present his personal reasons why he believes that someday in the future, we will have absolutely secure communication and ultrafast computation based on these quantum phenomena. This development confirms once more that the most interesting possibilities for novel applications arise from deep fundamental investigations.
Anton Zeilinger is professor of physics at the University of Vienna and director at the Institute of Quantum Optics and Quantum Information of the Austrian Academy of Sciences. His pioneering conceptual and experimental contributions to the foundations of quantum physics have become the cornerstone of the rapidly evolving field of quantum information. His future research goals include quantum communication and quantum teleportation using satellites and ultrafast optical quantum computers. The stages of his career include M.I.T., Collège de France, Technical University of Munich, and Oxford University. Among his prizes are the Inaugural Newton Medal of the U.K.
2011 Memorial University of Newfoundland, Monday, June 13, 2011, 7:30 P.M., Arts & Culture Centre, St. John's, NL
ROLF HEUER, DIRECTOR-GENERAL, CERN
The search of a deeper understanding of our universe at the Large Hadron Collider: the World's Largest Particle Accelerator
With the start of the Large Hadron Collider (LHC) at CERN, particle physics enters a new era. The LHC will provide a deeper understanding of the universe and the insights gained could change our view of the world. Dr. Heuer will explain some of the reasons for the excitement surrounding the LHC. The LHC is expected to yield insights into the origin of mass, the nature of dark matter and the existence of hidden extra dimensions. The talk will address the exciting physics prospects offered by the LHC, and present first results taken by the LHC since the start of data taking in March last year.
CERN, located in Geneva Switzerland, is one of the world's largest and most respected centres for scientific research. Prof. Heuer is widely recognized for his leadership in the development of experimental techniques, and the construction and running of large subatomic particle detector systems.
2010 University of Toronto, Monday, June 7, 2010, 7:30 P.M., MedSci Auditorium
CHARLES TOWNES, UNIVERSITY OF CALIFORNIA AT BERKELEY
50th Anniversary of the Laser
In the early 1950s I thought and worked hard at trying to find a way to obtain an oscillator for frequencies higher than those available from known electronics, in order to do very high resolution spectroscopy. Finally, I suddenly had the idea to put enough excess atoms or molecules in an upper state, and provide stimulated emission. My student Jim Gordon and I made this work first in the microwave range, primarily as a test. The resulting maser (for microwave amplification by simulated emission of radiation) generated an exciting field and many people jumped into it to make microwave oscillators and amplifiers. But after a few years I pushed myself to move on to much shorter wavelengths. Arthur Schawlow and I then wrote a paper on how such stimulated emission oscillators could be produced at wavelengths as short as those of light – we called it an optical maser, but it soon was renamed the laser (light amplification by stimulated emission of radiation). After publication of our theoretical discussion, many scientists were excited and the first working system was made by Theodore Maiman at the Hughes Labs, a pulsed ruby laser. The first continuously oscillation system was made by one of my former students, Ali Javan, with Wm. Bennett and Don Herriot at the Bell Telephone Labs. Industry by then recognized the importance of this field, and all the first lasers were built in industrial labs. Lasers are now a wonderful field for science and for a wide variety of technical applications — all an outgrowth of spectroscopy, a field Herzberg helped develop importantly. I presently use lasers to do infrared interferometry on stars with three separate telescopes. Lasers have helped astronomy in many ways, in particular producing a rapid growth of interferometry for measurement of stellar sizes and shapes. Our interferometer is the only one, however, which uses heterodyne detection, provided by laser local oscillators, which hence allows interferometry in very narrow bandwidths which can avoid spectral lines due to surrounding gas. This allows measurement of old and active stars quite directly, without interference from their emitted gases. I will report some of the measurements, showing the changes in size of some stars, the dust shells they have blown off and expansion of these shells, along with other details not seen until such techniques became possible.
Charles Hard Townes was born in Greenville, South Carolina and attended Furman University in Greenville, from which he received a B.Sc. in Physics and a B.A. in Modern Languages. He completed the Master of Arts degree in Physics at Duke University and then took his Ph.D. at the California Institute of Technology. He was a member of the technical staff of Bell Telephone Laboratories from 1933 to 1947. Appointed to Columbia University in 1948, he continued microwave research to study the structure of atoms, molecules and nuclei. In 1951, Dr. Townes conceived the idea of the maser and in early 1954, the first amplification and generation of electromagnetic waves by stimulated emission were obtained in ammonia. In 1958, Dr. Townes and his brother-in- law, Dr. A.L. Schawlow, showed theoretically that masers could be made to operate in the optical and infrared region. The first working laser was demonstrated (by Ted Maiman) in 1960. From 1959 to 1961, Dr. Townes served as Vice President and Director of Research of the Institute for Defense Analyses in Washington, D.C., advising the U.S. government. In 1961, Dr. Townes was appointed Provost and Professor of Physics at the Massachusetts Institute of Technology. He was appointed University Professor at the University of California in 1967, principally located at the Berkeley campus. He was co-recipient (with Drs. Basov and Prokhoroff) of the 1964 Nobel Prize in physics for the maser/laser principle. Dr. Townes has served on a number of scientific committees advising governmental agencies and has been active in professional societies. This includes being a member, and vice chairman, of the Science Advisory Committee to the President of the U.S. and Chairman of the Advisory Committee for the first human landing on the moon. He also served on the boards of General Motors and of the Perkins Elmer Corporations.
2009 Université de Moncton, Monday, June 8, 2009, 7:30 P.M., Theatre Capitol, Moncton, NB
LAURENT DRISSEN, UNIVERSITE LAVAL
The Splendours and Miseries of Massive Stars
The most massive stars in the universe are also the most fascinating. Exceedingly rare, they nevertheless play an important role in galactic ecology and in the chemical evolution of the cosmos. They are born in gigantic molecular clouds and they light up with an enormous outpouring of ultraviolet radiation. Pressure exerted by these forms of light on heavy elements present in the stellar atmosphere results in a very powerful wind which enriches the regions between the stars and injects large amounts of energy in their surroundings. The life of massive stars is brief – a hundredth of that of ordinary, sun-like stars – and ends in a gigantic explosion detectable to distances of billions of light-years. With the help of beautiful images obtained by the largest ground-based and space telescopes, I will describe the life and death of these stars which illuminate our universe.
Laurent Drissen grew up between Montreal and the countryside of the Eastern Townships where he spent most of his week-ends and his summer vacations. Obviously, the country sky was lit up with stars, and it is there that his passion for the Galaxy and the cosmos was born. He obtained his Ph.D. (1990) from the Université de Montréal under the supervision of Prof. Anthony Moffat, one of the world experts on Wolf-Rayet stars. His first experiences as a professional astronomer were at the Mont Mégantic Observatory, then at the Canada-France- Hawaii telescope. He also observed at the AAT (Australia), the Wise Observatory (Israel), CTIO and ESO (Chile) and Mount Lemmon (Arizona). He then moved to Baltimore, Maryland, where he worked at the Space Telescope Science Institute in the early times of the Hubble Telescope (from 1990 to 1994). He came back to Québec in 1995 to work with the astrophysics group at Laval University. Since 2001, he has held the Canada research chair in astrophysics (massive stars and hyperspectral imagery) at the same university. He works on massive stars and their influence on their surroundings, and he also builds, in collaboration with his fantastic students, innovative astronomical instruments such as a wide-field imaging spectrometer. He teaches classical physics, quantum mechanics, stellar structure and evolution, and he supervises four graduate students.
2008 Université Laval, Sunday, June 8, 2008, 7:30 P.M., Theatre de la cite universitaire, U.Laval
RAYMOND LAFLAMME, INSTITUTE FOR QUANTUM COMPUTING/UNIVERSITY OF WATERLOO
Harnessing the Quantum World
Information processing devices are pervasive in our society; from the 5 dollar watches to a multi-billion dollar satellite network. These devices have allowed the information revolution which is developing around us. It has transformed not only the way we communicate or entertain ourselves but also the way we do science and even the way we think. All this information is manipulated using the classical approximation to the laws of physics, but we know that there is a better approximation: the quantum mechanical laws. Would using quantum mechanics for information processing be an impediment or could it be an advantage? This is the fundamental question at the heart of quantum information processing (QIP). QIP is a young field with an incredible potential impact reaching from the way we understand fundamental physics to technological applications. I will give an introduction to quantum information by stressing recent interesting developments. I will also comment on the effort in this field at Waterloo and in Canada.
Raymond Laflamme was born in Quebec city and did his undergraduate studies in Physics at Universite Laval. He then moved to Cambridge, England, where he survived Part IIIof Mathematical Tripos before doing a PhD in the Department of Applied Mathematics and Theoretical Physics (DAMTP) under the direction of Stephen Hawking. He and DonPage are responsible for having changed Hawking's mind on the reversal of the direction of time in a contracting Universe (see his book "Abrief history of time"). After his PhD,Ray became a Killam post- doctoral fellow at UBC where he met his future wife Janice Gregson. Ray moved back to Cambridge in 1990 as a Research Fellow at Peterhouse.He finally settled down for 9 years at Los Alamos National Laboratory. He arrived as a Director funded post-doctoral fellow, became an Oppenheimer Fellow in 1994, just afterthe birth of his son Patrick. His daughter Jocelyne was born in 1995 and he became Technical Staff in 1997. In 2001 he joined the newly founded Perimeter Institute for TheoreticalPhysics and the University of Waterloo where he and Michele Mosca have started the Institute for Quantum Computing. Raymond Laflamme holds a Canada Research Chair (CRC) in Quantum Information.
2007 University of Saskatchewan, Sunday, June 17, 2007, 7:00 P.M., TCU Place
CARL WIEMAN, UNIVERSITY OF BRITISH COLUMBIA
A Science Education in the 21st Century: Using the Tools of Science to Teach Science
Guided by experimental tests of theory and practice, science has advanced rapidly in the past 500 years. Guided primarily by tradition and dogma, science education meanwhile has remained largely medieval. Research on how people learn is now revealing how many teachers badly misinterpret what students are thinking and learning from traditional science classes and exams. However, research is also providing insights on how to do much better. The combination of this research with modern information technology is setting the stage for a new approach that can provide the relevant and effective science education for all students that is needed for the 21st century. I will discuss the failures of traditional educational practices, even as used by "very good" teachers, and the successes of some new practices and technology that characterize this more effective approach. Some applications to technical presentations will also be mentioned.
Carl Wieman grew up in the forests of Oregon and was educated at MIT and Stanford. Dr. Wieman, a long- term Distinguished Professor of Physics at the University of Colorado, joined UBC in January 2007. He has carried out research in a variety of areas of atomic physics and laser spectroscopy, and was awarded the Nobel Prize in Physics in 2001 for the creation and study of Bose-Einstein condensation in a dilute vapor. His work on innovations in teaching physics to a broad range of students, on student beliefs about physics, and on problem-solving skills has been recognized by several prestigious awards.
2006 Brock University, Sunday, June 11, 2006, 7:00 P.M., Sean O'Sullivan Theatre
ERNEST L. MCFARLAND, UNIVERSITY OF GUELPH
Energy: Where on Earth are We Going?
Physics is important in your everyday life. There is growing concern about humankind's ever-increasing use of energy and the associated environmental impacts such as global warming. Oil is no longer cheap, and attention is now being paid to other sources of energy. This talk will consider the consumption of fossil fuels, as well as use of wind, solar and nuclear energy, and their environmental consequences. Many aspects of basic physics, important in the utilization of energy sources, will be discussed.
Ernest L. McFarland is a Professor Physics, a recipient of the CAP Medal for Excellence in Undergraduate Teaching and a 3M Teaching Fellowship. Prof. McFarland has co-authored a textbook: Energy, Physics and the Environment which provides a foundational quantiative account of energy and related environmental issues.
2005 University of British Columbia, Sunday, June 5, 2005, 7:00 P.M., Chan Centre
CLIFFORD WILL, WASHINGTON UNIVERSITY, ST. LOUIS
Was Einstein Right?
How has the most celebrated scientific theory of the 20th century held up under the exacting scrutiny of planetary probes, radio telescopes, and atomic clocks? After 100 years, was Einstein right? In this lecture, celebrating the 100th anniversary of Einstein's "miracle year" and the World Year of Physics, we relate the story of testing relativity, from the 1919 measurements of the bending of light to the 1980s measurements of a decaying double-neutron-star system that reveal the action of gravity waves, to a 2004 space experiment to test whether spacetime "does the twist". We will show how a revolution in astronomy and technology led to a renaissance of general relativity in the 1960s, and to a systematic program to try to verify its predictions. We will also demonstrate how relativity plays an important role in daily life.
Clifford Will is Professor of Physics, and member of the McDonnell Center for the Space Sciences at Washington University in St.Louis. Born in Hamilton, Canada in 1946, he received a B.Sc. in Applied Mathematics and Theoretical Physics from McMaster University in 1968, and a Ph.D. in Physics from the California Institute of Technology in 1971. He was an Enrico Fermi Fellow at the University of Chicago (1972-74), and an Assistant Professor of Physics at Stanford University (1974-81), From 1975 to 1979, he was an Alfred P. Sloan Foundation Fellow. In 1981 he joined Washington University as Associate Professor, in 1985 became Full Professor of Physics, and from 1991 – 2002 served as Chairman of the Department. In 1986 he was selected by the American Association of Physics Teachers to be the 46th annual Richtmyer Memorial Lecturer. He was elected a Fellow of the American Physical Society in 1989 and of the American Academy of Arts and Sciences in 2001. In recognition of his theoretical work related to the Hulse-Taylor Binary Pulsar, he was an invited guest of the Nobel Foundation at the 1993 Nobel Prize Ceremonies honoring discoverers Joseph Taylor and Russell Hulse. During 1996-97, he was both a J. William Fulbright Fellow and a Guggenheim Foundation Fellow, and in 1996, he was named Distinguished Alumnus in the Sciences by McMaster University. In 2004 he received the Fellows Award of the St. Louis Academy of Sciences, and was elected President of the International Society on General Relativity and Gravitation. He has published over 160 scientific articles or abstracts, including 13 major review articles, 23 popular or semi-popular articles, and two books: Theory and Experiment in Gravitational Physics (Cambridge University Press, 1981; 2nd Edition, 1993), and Was Einstein Right? (Basic Books, 1986; 2nd Edition, 1993). Was Einstein Right? was selected one of the 200 best books of 1986 by the New York Times Book Review, and won the 1987 American Institute of Physics Science-Writing Award in Physics and Astronomy. It has been translated into French, German, Japanese, Italian, Spanish, Portuguese, Korean, Greek, Chinese and Persian. His research interests include tests of general relativity, gravitational radiation, black holes, cosmology, and the physics of curved spacetime.
2004 Winnipeg, Manitoba, Sunday, June 13, 2004, 7:00 P.M., Delta Hotel, Ballrooms A/B/C
P. JAMES E. PEEBLES, PRINCETON UNIVERSITY
A Cosmic Picture Show : Images from Astronomy
Some of the astronomical images I will present are meant to illustrate what we know about the large-scale nature of the world around us and how we have gone about discovering it; others are chosen just because they're pretty. Some of the images are close to what you can see with a pair of binoculars; others are numerical representations of what you would `see' if you had Superman's X-ray eyes, or eyes sensitive to radio waves or neutrinos. I'll show historical examples of the learning process in astronomy, both good — Hubble's classification of the galaxies B and not so good — Lowell's idea that he was seeing canals on Mars — and illustrations drawn from current debates about what is happening on scales ranging from black holes in the centers of galaxies to the expansion of the universe.
Born April 25, 1935 in Winnipeg, Manitoba, Canada, naturalized U.S. citizen 1991. Married to Alison Peebles with three children, Lesley, Ellen and Marion, six grandchildren. 1958 BS University of Manitoba; 1962 Ph.D. Princeton University; 1961-1962 Instructor, Princeton; 1962-64 Research Associate, Princeton; 1964-65 Research Staff Member, Princeton; 1965-68 Assistant Professor, Princeton; 1968-72 Associate Professor, Princeton; 1972-84 Professor Princeton; 1984-2000 Albert Einstein Professor of Science , Princeton; 2000 Albert Einstein Professor of Science Emeritus, Princeton. Professional Societies: Fellow, American Academy of Arts and Sciences; Fellow, American Physical Society; Fellow, Royal Society; Fellow, Royal Society of Canada; Fellow, U.S. National Academy of Sciences; Member, American Astronomical Society; Member, American Association for the Advancement of Science. Awards: 1977, A.C. Morrison Award in National Science, NY Academy of Sciences; 1981, Eddington Medal, Royal Astronomical Society; 1982, Heineman Prize, American Astronomical Society; 1986, Doctor of Science, University of Toronto; 1986, Doctor of Science, University of Chicago; 1989, Doctor of Science, McMaster University; 1989, Doctor of Science, University of Manitoba; 1992, Robinson Prize, University of Newcastle upon Tyne; 1992, Henry Norris Russell Lectureship of the AAS; 1994, Silliman Lectureship, Yale; 1994, Feshbach Lecturer, MIT; 1995, Bruce Medal, Astronomical Society of the Pacific; 1995, Lemaitre Award, Universite catholique de Louvain; 1995, de Vaucouleurs Lectureship, University of Texas; 1996, McPherson Lecturer, McGill University, October; 1996, Doctor of Science, Universite catholique de Louvain, October; 1997, Danz Professor, University of Washington May; 1997, Klein Lecturer, University of Stockholm, June; 1997, Jansky Lectureship, NRAO; 1997, Doctor Honoris Causa, Universidad Nacional de Cordoba, December; 1998, Gold Medal, Royal Astronomical Society, UK; 2000, Peter S. Gruber Foundation Award, September; 2001, Oort Professor, Leidon University, May; 2001, Harvey Prize Technion University, Israel; 2003, Tomalla Foundation Prize, University of Geneva, June
2003 University of Prince Edward Island, Sunday, June 8, 2003, 7:00 P.M., Chi-Wan Young Sports Centre
DAVID SOUTHWOOD, DIRECTOR OF SCIENCE, EUROPEAN SPACE AGENCY
Space Near and Far – Exploring our Universe and Our Place in It
The exploration of space is more than a scientific endeavour, although science and physics, in particular, are at the root of it. Any modern technically developed society needs for its own health to look outwards and also backward to its origins. Space science does these tasks in the grandest ways, looking outwards to its limits of the ability to see and to measure, and backwards to whence our galaxy, our planet, indeed ourselves came. Such themes will be explored, using Europe's space programme for illustration.
Professor Southwood took up post as Director of Science at the European Space Agency (ESA) on May 1, 2001. From 1997 to 2000, he was head of Earth Observation strategy at the European Space Agency where he introduced a new programme in Earth science, "The Living Planet". After his going back to academia in April 2000, his return to ESA to lead the space science programme was announced in late 2000. David Southwood is a space physicist who spent the bulk of his career at the Blackett Laboratory, the Physics Department of Imperial College London. He went to Imperial first as a PhD student in 1966. After postdoctoral work in the USA, in the Institute of Geophysics and Planetary Physics at the University of California Los Angeles, he returned to the Imperial College faculty in 1971 eventually becoming head of the Blackett Laboratory, the Physics Department of Imperial College from 1994-1997. He has retained for many years links with UCLA and returned there as a Regents Professor in 2000. He completed a thesis on ULF waves in the Earth's magnetosphere, using both ground-based and early satellite data. Subsequent research interests ranged from the deployment of magnetometer arrays on the ground to exploring the magnetic environments of Jupiter and Saturn with spacecraft. He has worked on a variety of space missions over the past thirty-five years, working with the American and Russian programmes as well as with European partners. His most recent instrumental work was building the magnetometer on the NASA Cassini Saturn orbiter, with has now passed Jupiter and will reach Saturn in 2004. David Southwood has sat on many senior science committees in Britain and at the international level in Europe and in COSPAR. He has been chairman of the Science Programme Committee (SPC) and the Space Science Advisory Committee (SSAC). He has published more than 200 publications and scientific articles.
2002 Québec City Convention Centre (2nd Level), Sunday, June 2, 2002, 7:00 P.M., Room 2000 A
ERIC CORNELL, UNIVERSITY OF COLORADO
Bose-Einstein Condensation Experiments in an Ultracold Atomic Gas
At temperatures under one millionth of a degree from absolute zero, a dilute vapour of ultra-cold atoms may undergo Bose-Einstein condensation. The resulting substance is an ideal environment for a host of experiments in quantum mechanics at the interface between condensed-matter and atomic physics. I will present a representative sample of past and current work.
Eric Cornell received his B.S. from Stanford University in 1985, and his PhD from MIT in 1990. His doctoral research, with Dave Pritchard, was on precision mass spectroscopy of single trapped molecular ions. Cornell went to JILA in Boulder, Colorado in 1990. Since 1992 he has been a senior scientist with the National Institute of Standards and Technology. He is a Fellow of JILA and Professor Adjoint in the Physics Department of the University of Colorado. Research interests center around various aspects of ultracold atoms, including BoseEinstein condensation and experiments on atoms guided by optical forces inside hollow glass fibers and by magnetic forces along lithographically patterned wires. Cornell received the Stratton Award from NIST in 1995, the Carl Zeiss Award in 1996, the Fritz London Prize in 1996, the Presidential Early Career Award for Scientists and Engineers in 1996, the 1997 I.I. Rabi Award, the 1997 King Faisal International Prize for Science, the 1995-96 AAAS Newcomb- Cleveland Prize, the 1997 Alan T. Waterman Award, the Lorentz Medal in 1998, in 1999 the R. W. Wood Prize and the Benjamin Franklin Medal in Physics, and in 2000 was elected as a Fellow of the Optical Society of America and a Member of the National Academy of Sciences. He shares the 2001 Nobel Prize in Physics with Carl Wieman and Wolfgang Ketterle.
2001 University of Victoria, Sunday, June 17, 2001, 7:00 P.M., Unicentre Auditorium
KIP THORNE, CALTECH UNIVERSITY
Gravitational Waves : A New Window Onto the Universe
Gravitational waves are ripples of warpage in the fabric of spacetime, generated by the birth of the universe, by collisions of black holes, and by other cataclysmic events in the distant universe. Next year an international network of ground-based detectors (LIGO, VIRGO, GEO and TAMA) will begin a search for gravitational waves with wavelengths about the size of the Earth. In 2010, the joint US/European LISA mission (three spacecraft 5 million kilometers apart that track each other with laser beams) will begin a search for gravitational waves with wavelengths the size of the solar system. In this lecture Thorne will describe these gravitational-wave detectors, the remarkable technology that they rely on (such as controlling the quantum mechanical behavior of 40 kilogram objects), and the revolution that they may bring in our understanding of the universe.
Kip Thorne received his B.S. degree from Caltech in 1962 and his Ph.D. from Princeton University in 1965. He returned to Caltech as an Associate Professor in 1967 and become Professor of Theoretical Physics in 1970, The William R. Kenan, Jr. Professor in 1981, and The Feynman Professor of Theoretical Physics in 1991. He was cofounder (with R. Weiss and R.W.P. Drever) of the LIGO (laser Interferometer Gravitational Wave Observatory) Project and is a member of the LISA (Laser Interferometer Space Antenna) International Science Team. Along with other numerous awards and recognition, Dr. Thorne has been a Woodrow Wilson Fellow, a Danforth Foundation Fellow, a Fulbright Fellow, and a Guggenheim Fellow, and has served on the International Committee on General Relativity and Gravitation, the Committee on US-USSR Cooperation in Physics, and the National Academy of Science's Space Science Board.
NOTE: In 1999 and 2000, the CAP had public lectures at each of its conferences, but it was only in 2001 that it became known as the "Herzberg Public Lecture". The list of speakers, with abstracts, appears below:
2000 York University, Sunday, June 4, 2000, 7:00 P.M., Burton Auditorium, Fine Arts Building
ROBERT PARK, UNIVERSITY OF MARYLAND, AMERICAN PHYSICAL SOCIETY
Voodoo Science
A best-selling health guru insists that his brand of spiritual healing is firmly grounded in quantum theory: half the population believes Earth is being visited by space aliens who have mastered faster-than-light travel, and educated people are wearing magnets in their shoes to draw energy from the Earth. Did we set the public up for this? In our eagerness to hare speculative new ideas at the frontier of science, have we conveyed the message that the universe is so strange that anything is possible? What can we tell people that will help them judge which claims are science and which are voodoo?
1999 UNIVERSITY OF NEW BRUNSWICK, FREDERICTON, SUNDAY, JUNE 6, 1999, 7:00 P.M., MACLAGGAN AUDITORIUM, NURSE'S BUILDING
ROBERT (BOB) MCDONALD, HOST OF CBC'S 'QUIRKS AND QUARKS' PROGRAM
Science in the Third Millennium : A Journalist's Perspective
All science and technology we use today, with the exception of mathematics, was developed within the last thousand years. Our knowledge grew out of the Dark Ages and reached the moon and beyond. The second millennium will be looked upon by future generations as the age of the discoveries, where we explored planet Earth, saw it in its true context, and found more invisible worlds within the microscopic universes of the cell and the atom. Now, on the verge of the third millennium we are entering a new age where the most powerful tools ever developed are changing the face of the planet and the very foundation of life itself. As a journalist, it has been my extreme pleasure to witness some of these amazing discoveries and meet the astonishing people who have brought us to the greatest enlightenment humanity has every known. It is also a time of tremendous challenge to the survival of the human species, but as I am a believer in the power of scientific knowledge and the ingenuity of human tool making, we have the ability to meet those challenges, if only common sense prevails.
NOTE: From 1991 until 1998, the CAP had keynote speakers at each of its conferences. It was only in 1999 that we started to have public lectures.. The list of keynote speakers, with abstracts when available, appears below:
1998 UNIVERSITY OF WATERLOO, SUNDAY, JUNE 14, 1998, 7:30 P.M., THEATRE OF THE ARTS
STEVEN CHU, PHYSICS DEPARTMENT, STANFORD UNIVERSITY
Laser Cooling and Trapping of Atoms and Particles
A brief history of the laser cooling and trapping of atoms will be presented, covering some of the major techniques that have been developed over the past 15 years. The cooling and trapping technology is already being applied in numerous areas of science and engineering. Applications to be discussed include atomic clocks, atom interferometers used to measure fundamental constants and inertial sensors, and applications in polymer science and biology.
1997 UNIVERSITY OF CALGARY, SUNDAY, JUNE 8, 1997, 7:30 P.M., ALBERTA ROOM
CAROL CHRISTIAN, DIRECTOR, PUBLIC OUTREACH, SPACE TELESCOPE SCIENCE INSTITUTE
Recent Results from the Hubble Space Telescope
No abstract was available for this talk.
1996 UNIVERSITY OF OTTAWA, SUNDAY, JUNE 16, 1996, 7:30 P.M., MONTPETIT AUDITORIUM
SIR JOHN MADDOX, FORMER EDITOR OF "NATURE" MAGAZINE
Where is Science Heading?
1995 LAVAL UNIVERSITY, SUNDAY, JUNE 11, 1995, 7:30 P.M., THEATRE DE LA CITE UNIVERSITAIRE
PROF. ARTHUR L. SCHAWLOW, STANFORD UNIVERSITY
Fifty Years of Physics and Physicists
In 1945, quantum mechanics was twenty years old. Physicists were aware of it, but most engineers were not, and few of them actually used it. Nuclear physics appeared to be the most important frontier, partly because it seemed to offer the possibilities of limitless, cheap energy. Atomic physics, especially optical spectroscopy, was widely thought to be unglamorous. Most research equipment was constructed by the scientists themselves as they needed it. However, the wartime achievements of physicists attracted increasing support from governments and industry, and that stimulated the growth of an instrument industry producing increasingly sophisticated devices. Discoveries in condensed matter physics such as nuclear magnetic resonance, transistors, integrated circuits and lasers have opened up vast industries and provided powerful new tools for physics research. Huge teams have been assembled to build and attend giant machines for particle physics, nuclear fusion research and astronomy. Now faced with competitive pressures, industry has drastically reduced basic research and governments have cut back their support. Fascinating problems still confront us, even to understand the full meaning of quantum mechanics. Progress with continue, but it will be slowed in ways that we may not fully realize.
1994 UNIVERSITY OF REGINA, SUNDAY, JUNE 26, 1994, 7:30 P.M., EDUCATION BUILDING AUDITORIUM
PROF. ALLAN BROMLEY, STERLING PROFESSOR OF THE SCIENCES, YALE UNIVERSITY
Physics and the 21st Century
After more than half a century of remarkable discoveries, applications and new insights on the structure of the universe and our place in it, physics and physicists, world wide, are facing a crisis of confidence. At a time when celebration would seem appropriate, instead a siege mentality is settling in. But there are reasons for optimism. Physics, at least, is becoming truly international: beyond the discoveries within our field, it is spawning an accelerating flow of new technologies and new understanding in our sister sciences – all of which improve our quality of life and our understanding of, utilization of, and accommodation to nature. As we prepare to enter the 21st century, it is essential that physicists, both young and old, regain the breadth of vision and of interest that characterized the giants of our past. There is great adventure ahead.
1993 SIMON FRASER UNIVERSITY, SUNDAY, JUNE 13, 1993, 7:00 P.M., IMAGES THEATRE
[No information published in Congress program]
1992 UNIVERSITY OF WINDSOR, SUNDAY, JUNE 14, 1992, 7:30 P.M., ERIE HALL, ROOM 1120
PROF. KENNETH WILSON, OHIO STATE UNIVERSITY
Overall Issues for Educational Reform in the U.S.
Reform of mathematics and science education is a major concern in the U.S. Problems in Canada exist, too, but I cannot speak for them. However, reform of mathematics and science education only makes sense as part of an overall reform effort. This talk addresses key overall issues of U.S. reform. Namely :
• Should there be a single reform process that does not overwhelm teachers and schools?
• How does one ensure maximum feedback to individual students practising higher order skills in a large class?
• Should teachers have extensive time during their work week for collaborative study of teaching and educational change? (In the Far East, teachers spend no more than four hours in class per day, leaving time for study and professional activity.)
• Should students be given more responsibility for their own learning in and out of class?
• There is a lot of design work in teaching, from preparation of materials and software to scheduling of students and teachers to planning of classroom organization. Can a technical assistance framework be established which offloads this design burden from individual teachers and schools but, through constant redesign, supplies teachers and students with designs maximally beneficial to them?
• How does one engage broad political support for the overall reform that is needed?
• What changes in research universities are needed to support reform of schools?
• How does one achieve unbiased evaluation of educational programs and the overall progress of reform?
1991 UNIVERSITY OF MANITOBA, SUNDAY, JUNE 16, 1991, 7:00 P.M., UNIVERSITY OF MANITOBA AUDITORIUM
RICHARD TAYLOR, STANFORD LINEAR ACCELERATOR CENTRE
Inside the Proton
No abstract available for this talk.
NOTE: From 1946 to 1990, the CAP had an opening reception and plenary speakers (no keynote speaker) at each of its conferences. Any conference where there was an opening address given, the name of the speaker is listed below. Otherwise, we have listed only conference locations and dates. (1946-1982 will be added later)
1990 MEMORIAL UNIVERSITY OF NEWFOUNDLAND, JUNE 25-28, 1990
1989 UNIVERSITY OF GUELPH, JUNE 26-28, 1989
1988 UNIVERSITY OF MONTREAL (JOINT WITH APS), JUNE 19-22, 1988
1987 UNIVERSITY OF TORONTO, JUNE 14-17, 1987
1986 UNIVERSITY OF ALBERTA, JUNE 22-25, 1986
1985 UNIVERSITY OF NEW BRUNSWICK, JUNE 23-26, 1985
1984 UNIVERSITY OF SHERBROOKE, JUNE 17-20, 1984
1983 UNIVERSITY OF VICTORIA (JOINT WITH CASCA), JUNE 26-30, 1983
OPENING ADDRESS: THE HONORABLE DONALD J. JOHNSTON, MINISTER OF STATE, ECONOMIC DEVELOPMENT AND SCIENCE & TECHNOLOGY[/vc_column_text][/vc_column][/vc_row]


text:
'Dear Evan Hansen', You're the Charlie-Browniest, You Blockhead
Ben Platt as EVAN, Kaitlyn Dever as ZOE in DEAR EVAN HANSEN
About a year after Hamilton took the theater world by storm, another stage musical came out called Dear Evan Hansen. While it came nowhere near to earning the hype of Lin-Manuel Miranda's cultural juggernaut, Dear Evan Hansen definitely received love from the theater crowd, winning numerous awards and accolades. Never seeing the theatrical production and just hearing others' takes, I always pictured Dear Evan Hansen as a Charlie Brown-esque story for contemporary times. Photos of Ben Platt sporting his polo shirt and khakis even visually supported my thesis. I knew the story dealt with suicide, social anxiety, and feeling like an outsider. And the literary device of a student hashing out his emotions through letters even seems on brand. Doesn't that sound familiar, Charlie Brown?
But while Hamilton's transition from stage to screen earned adulation, Dear Evan Hansen has been panned by critics and audiences alike. How did it all go so wrong?
Ben Platt as EVAN, Nik Dodani as JARED in DEAR EVAN HANSEN
Dear Evan Hansen stars Ben Platt as the titular main character. Ben suffers from severe anxiety and depression. His therapist suggests he write affirming letters to himself as a way of working out his feelings. Ben feels rather invisible. His one source of unconditional love is his hard working single mother, Heidi (Julianne Moore), whose work schedule keeps her away from home most of the time. One of Evan Hansen's letters falls into the hands of Connor Murphy (Colton Ryan; Uncle Frank), an unhappy boy who has problems of his own. After Connor takes his own life, Evan gets swept into a succession of lies when Connor's parents (played by Amy Adams and Danny Pino) think Connor wrote Evan's letter as a goodbye note to Evan. Evan, who feels starved for attention and wants more than anything to belong somewhere, allows himself to get swept into the masquerade of being the parents' only lifeline to their now-dead son. He wants to tell them the truth, but the parents seem to want -- to need-- to know that Connor had a friend. But as the lies pile up and Evan begins to benefit from his deception in ways he never imagined, telling the truth becomes the last thing Evan wants to do. The movie is directed by Steven Chbosky (The Perks of Being a Wallflower), adapted for the screen by Steven Levenson, with music and lyrics by Benj Pasek and Justin Paul.
So how does it play on screen? The best part, hands down, is the music itself. Ben Platt can sing, as can the rest of the cast, who presumably all do their own vocals. Especially after watching the drab repetitive musical numbers in Annette (the last musical I watched), listening to well-crafted musical numbers with melodic cadence and lyrics that tell a story felt like a breath of fresh air. Most of the numbers are heart wrenching and occasionally sappy. The one exception is the humorous "Sincerely, Me," during which Evan and his tech-savvy friend Jared Kalwani (Nik Dodani) compose fake emails that Connor wrote to his supposed pal, Evan. This gives Colton Ryan as Connor an opportunity to join in the fun of acting out an imaginary friendship with Evan postmortem, adding a much-needed dose of levity to the proceedings. Julianne Moore's delivery of "So Big/So Small" and Amandla Stenberg's in "The Anonymous Ones" were also favorites that evoked tears. Musicals are by and large an emotionally-driven medium so it's no surprise that tears fell as I sat through these numbers.
Ben Platt as EVAN, Julianne Moore as HEIDI in DEAR EVAN HANSEN
Unfortunately, just having good songs isn't enough to make this movie musical memorable. The biggest issue remains the casting of Ben Platt. His Broadway acting gained critical acclaim, but what plays well on stage does not translate into the intimacy of the screen. I found myself unable to connect with him emotionally, even during his most gut wrenching songs. His age and bad haircut notwithstanding, when he is so close to the camera his performance just doesn't feel authentic. He acts like a person who is pretending to be awkward and anxious instead of really feeling those things. I believed the performances of Stenberg, Kaitlyn Dever, Adams, Moore, and even Ryan. I did not believe Platt. While everyone agrees that he looks too old, those that defend him argue that Platt knows the character and that no one could replace him. By that logic, Shia LeBeouf should have played himself in Honey Boy instead of channeling his efforts into giving Noah Jupe and Lucas Hedges everything they needed to emulate him. Should Shia have played himself since no one else can do it better? Platt could have trained a surrogate, perhaps even one with actual diagnosed medical anxiety, to be the new Evan. The success of the show should matter more than one person's need to own their part.
Amandla Stenberg as ALANA in DEAR EVAN HANSEN
And then there's the story itself.Dear Evan Hansen became a critical darling for the theater crowd, but the cushion of wealth it takes to afford such luxuries guarantees that the largest percentage of theater attendees will be wealthy, white, middle-aged, and comfortable being in large crowds. It's not exactly the type of situation that attracts teens with depression, social anxiety, or any number of issues this play wants to bring to the forefront. Rather, it's someone's attempt to manufacture what they think it's like for teens. The point which clarified this most comes when Evan sings "You Will Be Found," in front of the school. The trope of the loser coming in front of the school and performing their socks off, gaining respect from the cool kids, usually makes me smile. Think of Napoleon Dynamite showing off his Michael Jackson moves in that movie. Sure, it's a little unrealistic, but it's a moment where the character gets to hold their head high and show they have something to offer. The dopamine the character (and us) feels is its own reward. But in Evan's case, as he sings about never being alone, students record the song, which sprouts a litany of social media posts from admiring viewers. Evan goes viral as everyone shares, tagging on lazy "You gotta see this!" retweets. This moment, which is supposed to feel like a good thing, made the contents of my stomach curdle, highlighting the artificial and temporary nature of social media fame.
This scene really serves as a microcosm to the emotional lack at the heart of Dear Evan Hansen. The issues at stake are worth handling on screen and many have succeeded in going there. Dear Evan Hansen was brought to film to be a showpiece for Ben Platt and try to repeat the success of Hamilton being adapted for the small screen. It should have stayed on the stage where it belongs. Translating it to the screen just highlighted that this is a show and far from a story that has the power to heal or inspire actual change. See it for the musical performances; don't expect something that comes close to exploring the pain of the human condition.
Release info: In theaters September 24, 2021
Final score: 2.5 out of 5
drama movie review musicals Universal Pictures


Shock wrote: "Sorry, I'm late. I guess surprise volcanic eruptions really bring out the crazies." Chris skidded to a halt just shy of the group inspecting the energy wall. "Forcefield huh?" Then he spotted the new guy with Kirk and Tony. Figuring they weren't in that much of a hurry, Chris extended his hand. "You look new. I'm Shock."
"Hmm? What's that?", Thom asked, looking first at the outstretched hand, then the newcomer's face. "Ah, yes! 'Shock', you said?", he added shaking hands warmly. "Dr. Thomas Flynn, the Magus Errant. Tell me, have you ever seen a Class 2 force effect like this before?" Taking Shock by the shoulder, Thom reaches out to lightly touch the blue energy field. Tracing an idle pattern along its surface, he continues. "A refraction index that low?!? You could breach it with a paper airplane, but for the fact it has three times the power it needs pumping through it. That's what stopping us. The emitter'll burn itself out in and hour or two, if we had the time to wait."
Colin collects the blades and hands them to Prism.
"Can you read these symbols?"
While she examines them, he fires a few blasts at the dust on the ground that was their opponents.
"You really can't be to careful with undead."
Chris shrugged. "Do we ever have time to wait?"
Prism looked at piles of dust that were once people she had sworn to protect. Frustration and anger still boiled in her, even as she released her focus on the blade and channeled her energies to illuminating the cavern.
"Unlikely." she replied as she took one of the blades in hand, "I am not versed in your world's writing." she said, examining the weapon and it's markings all the same for a moment. "It is not of my world. she confirmed.
She levitated a mask that had fallen nearby, and regarded it intently for a moment, staring hard at the space where it's eyes would have been while Photon blasted away at the dust.
"What is an Anubis?" She asked out loud. When she had heard the word, it had not carried any understanding or meaning to her through her gifts, which meant it was likely a name of a person, a place or a thing her own experience had no point of reference to, such as the first time she had heard the word 'pizza'.
Making the assumption that the writing is not Illuminarian.
for any insights looking at the blade or mask.
Kirk had to admit that Binder had come up with an interesting twist on the principle of force field. He spent a several moments quietly examining the energy wall.
"Tell me, have you ever seen a Class 2 force effect like this before?" Taking Shock by the shoulder, Thom reaches out to lightly touch the blue energy field. Tracing an idle pattern along its surface, he continues. "A refraction index that low?!? You could breach it with a paper airplane, but for the fact it has three times the power it needs pumping through it. That's what stopping us. The emitter'll burn itself out in and hour or two, if we had the time to wait."
"Which is half our problem of course, and I'm sure something Binder took into consideration." Hornet answered as he continued to look over the force field.
Technology Check: _: 1D20+16 = +16 = 20, hhhmmmm nope! Gonna spend that shiny, new HP to re-roll that crap.
Re-rolled Technology Check: _: 1D20+16 = +16 = 25, that'll end up being a 35 total.
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"Ancient Egyptian devil," he says with a shrug. He pauses, thinking she may not get the reference entirely.
"God of the Underworld. Where the dead go."
He looks around for anything they might have missed. Maybe Elena might know someone who could give him some details on these daggers.
The dust of the former living and unloving creatures is dispersed across the cavern by Photons blast though whether I has a positive effect is unknown to any but the most adept of magi.
The green blades seem to have lost a bit of their sickly parlor and the whispers of death and draining the living are reduced to a soft sibilant hissing like a vague background breeze that ruffles leaves here and there.
The writings seem symbolic as much as anything to Prism while she understands the basics of hieroglyphics and similar written languages though she lacks the contextual and cultural understanding to decipher more then the most vague of wordings much less put them into a context of actual sentences.
the golden masks give off a similar vibe to the knives in that vague unsettling way but for the most part seem to be exactly what they appear. jackal faced masks made of some combination of gold and leather with arcane glyphs on them and the smell of something long dead coming from the masks interior face.
Colin as he looks around though gets the vaguest idea that there might be something more here. the way the chamber is set up is reminiscent of something hed read about in some journal about arcane cults, specifically the Villainous agency DEMON. Something about preparing the land for a ritual and the site being 'marked' in some way.
Further research by someone more adept in such matter would be appropriate but for now the runes and glyphs remains a mystery. However he can deduce a couple things, the markings have been here for sometime perhaps as far back as a century or more. The blood and such though is recent meaning the work of the mummies if such they were is recent within the last year.
As the two look around they hear the barely audible scrabbling of small feet as Gretchen his tiny boots barely making a sound as he runs into the cavern. He looks around a few seconds in that quirky curious manner before his yellowish eyes alight on the pair. He waves at them with a pointed toothed grin as he rushes over to Colin.
"Gretchen has message from Elena, Gretchen got it here as quick as could be, Gretchen did he did." the little goblin blurts out as he reaches into his back pouch and pulls out what looks like a handheld childs toy phone that has had various gidgets and gadgets attached to it. the little goblin whirls the dial with a pointed finger and rotates a small crank on the side, before handling the plastic red handset to Collin with a grin.
Its only at this time that Colin realizes that for some reason the earpiece he had been given from Elena has been utterly silent. Not even the vague background noise that hed become accustomed to over the last week. Perhaps too deep in the ground or something about the cavern.
Gretchens awkward looking device though works shockingly like a charm as when put to his ears he can clearly hear Elena calling his name.
"Photon you there?'" she asks the worried tone evident in her voice "Answer me please we lost contact and I haven't been able to break through whatever's interfering."
18s good enough for some basic info which well pass on here.
hopefully do this without the humidity induced migraine ive been running the last week.
Thomas and Kirk both easily see what they're looking for as they study Binders force field. The trap is typical of the supervillain, genius in its simplicity and elegant in design and economical in power and efficiency. Completely expected from a man who was once described by Defender of the Champions in a Superhype listing of top 10 geniuses, " Who knew you could do so much with Superglue?"
The force field is incredibly powerful capable of reflecting even the most powerful of attacks and creates a barrier that crosses into the walls and floors a good fifteen feet in every direction creating an impassable obstacle, and while its power supply with burn itself out eventually whatever Binder and the Ultimates are doing will be long since completed.
Again very much in the style of Binder, delay and hinder.
Thomas fortunately as the former Archmagus is not bound by simple things like walls and doors, when one knows the sidereal paths a wall is just another thing to walk through and doors can be found anywhere one chooses to look for them.
Thomas has two options one he can open a small dimensional portal and allow Hornet to bypass the field at small size and appear next to the device and use his tech skill to shut it down.
or he can use a dimensional step spell to walk them right past the force field using the mirror refracting qualities of the field to his advantage.
If hornet goes a DC 25 tech check will easily shut down the device.
And faceplants, as if he'd walked into a glass door.
"The hell???", he mutters, rubbing his nose. Peering around the portal's side, he sees the exit next to emitter. Except the exit appears to only be about six inches across. Feeling around the 'surface' of the entrance he finds a 'hole' corresponding to the exit. Stretching his whole arm through, he still can't quite reach the emitter. Realizing this, he pulls back out, stands and straightens his coat. Turning to Hornet, he asks, "How small can you shrink?"
OoC wrote: I'll spend a hp and if necessary I'll write up an appropriate teleport power.
"Thanks, Gretchen," Colin says as he takes the phone.
"Elena, it's Colin. We ran into some zombie and cult trouble while checking out some things down here. Looks like someone was trying to prep some big ritual, but we need someone more magically inclined for anything specific. Also, I ran into a very capable woman named Prism who is also friends with Grethchen."
"Right!", Thomas began, rubbing his hands together. "Cavern itself is ten, fifteen feet across, there's the emitter. Looks to be twenty feet back, right? Give or take?", he asked no one in particular.
Kirk was nodding his head silently in agreement, as he'd come to the same conclusion in his own calculations. Apparently their friend preferred to work things out loud.
"That would mean it extends into the walls another, say, fifteen feet. Blasting around it'd take almost as much time as blasting through it."
"Or digging around it from any direction either." Kirk added.
Kirk watched with interest in the magical display, as far as he cared magic was just a different kind of science. He knew there were rules as to what a mage could do, Kirk had learned that much from talks he'd had with Kris. To see a different magician in action was a chance to learn a little more about the subject.
"Enough to use your portal." The shrinking hero answers before demonstrating. "Give me a minute to deal with Binder's power supply." Never bothering to return to his normal size, the bug-sized hero went right to work on disabling the device. Though he did make it a point to memorize the design of it, as Binder did have several good ideas in use in it, so much so that it was almost a shame that the Insect Avenger had to break it.
Once Thomas gets the portal open, Hornet will go through and try to disable the emitter.
Hornet's Technology Check: _: 1D20+16 = +16 = 31, that'll do it.
"Former I think. And I am pretty sure there are the good kinds to. Norse have Valkyrie, not sure what Egyptians have," Colin responds.
He briefly wonders what the woman must think of him, being so nonchalant about the victims. People turned to zombies are usually killed first, at least all the ones he had dealt with in the past. He's never heard of any being saved before, so as soon as "zombie" was said - well he was already upset.
Thomas nodded approvingly as Hornet worked to deactivate the emitter. Ah, he's actually studying it. Excellent! I think I'm going to like these fellows.
Hornet slips easily through the somewhat snug opening in the fabric of space and time and ends up right next to a small pocket of space near the shield generator. Kirk once again has to admire the ingenuity Binder presents, the simplicity of form and function that is clearly a step ahead of the current generation.
Still Kirk is no slouch himself and after a few brief moments he figures out the right combination of buttons, switches, and wires to press, flip, or cut. The device wirrs and beeps, and then shuts down freeing the group to proceed as the wall blocking their progress disappears.
Somewhere down below the Ultimate's await along with any other sinister traps they may have set.
Yep easy peasy shut it down get a bit of insight on the devices functions as well for future reference and the four of you may proceed.
Quick Edit no need to spend a hp or anything Magus is good to go.
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