text:
Q: ObjectiveC framework not export some classes I have developed a tool called EzoRed (ezored.com). It generate a framework for ios or aar for android with native code (c++).
When i get the generated xcode project and drag/drop into my sample project, i use the framework without problems. When i drag the generated framework only (With Debug version of framework everything is working fine, but with Release is not working.), my app compile, install on device or simulator but when i run i get error:

I use the nm tool to check exported symbols and see that only *Impl classes was exported. See:

nm -gU build/ios/Release-universal/EzoRed.framework/EzoRed

0000000000010a88 S _OBJC_CLASS_$_EZRAudioStreamerPlatformServiceImpl
0000000000010b28 S _OBJC_CLASS_$_EZRGreetingMessagePlatformServiceImpl
00000000000109e8 S _OBJC_CLASS_$_EZRHttpClientPlatformServiceImpl
0000000000010ab0 S _OBJC_METACLASS_$_EZRAudioStreamerPlatformServiceImpl
0000000000010b50 S _OBJC_METACLASS_$_EZRGreetingMessagePlatformServiceImpl
0000000000010a10 S _OBJC_METACLASS_$_EZRHttpClientPlatformServiceImpl
0000000000010d30 D __ZTIPU39objcproto28EZRHttpClientPlatformService11objc_object
0000000000010fa0 D __ZTIPU42objcproto31EZRAudioStreamerPlatformService11objc_object
0000000000011200 D __ZTIPU44objcproto33EZRGreetingMessagePlatformService11objc_object
0000000000010d18 D __ZTIU39objcproto28EZRHttpClientPlatformService11objc_object
0000000000010f88 D __ZTIU42objcproto31EZRAudioStreamerPlatformService11objc_object
00000000000111e8 D __ZTIU44objcproto33EZRGreetingMessagePlatformService11objc_object
000000000000c700 S __ZTSPU39objcproto28EZRHttpClientPlatformService11objc_object
000000000000c9c0 S __ZTSPU42objcproto31EZRAudioStreamerPlatformService11objc_object
000000000000cca0 S __ZTSPU44objcproto33EZRGreetingMessagePlatformService11objc_object
000000000000c740 S __ZTSU39objcproto28EZRHttpClientPlatformService11objc_object
000000000000ca00 S __ZTSU42objcproto31EZRAudioStreamerPlatformService11objc_object
000000000000cce0 S __ZTSU44objcproto33EZRGreetingMessagePlatformService11objc_object

It is very strange because everything compile without problem.
With Debug version of framework everything is working fine. But with Release is not working.
Some checks:
It was included in bridge file:
https://github.com/ezored/sample-app/blob/master/source/ios/SampleApp/SampleApp/SampleApp-Bridging-Header.h
It was on CMakeLists.txt:
https://github.com/ezored/sample-app/blob/master/vendor/target-ios-master/CMakeLists.txt#L132
It compiles and install without problems, but not run. It show the up message.
All project files are here, anyone can download and run:
https://github.com/ezored/sample-app
The commands used are:
cmake --build . --config Debug  (is exported all files correct)
cmake --build . --config Release  (is exported only *Impl files)

The xcode direct command has the same effect:
xcodebuild build -configuration "Debug"  (is exported all files correct)
xcodebuild build -configuration "Release"  (is exported only *Impl files)

What im doing wrong? Thanks for any help.

A: The solution that i found is put on my CMakeLists.txt the line:

CXX_VISIBILITY_PRESET default

Because on file ios.cmake i have the lines:

set(CMAKE_CXX_FLAGS "${XCODE_IOS_PLATFORM_VERSION_FLAGS} ${BITCODE} -fvisibility=hidden -fvisibility-inlines-hidden -fobjc-abi-version=2 -fobjc-arc ${CXX_FLAGS}")

https://github.com/ezored/target-ios/blob/master/build/files/ios.cmake#L284
I dont know if it is a best practice and i will try aprove the app on App Store with it.


Come out and support your Grade 12 graduates tomorrow night prior to the Rick Hansen regular season game.
Winner of tonight's game will determine the regular season champions in the AAA Fraser Valley East League. Wear your blue and white and come cheer on the Grizzlies!!
Previous Gr 8 Boys Win Fraser Valley East Championship!!
Next All Fraser Valley Basketball Championship tournaments are postponed due to weather.


Using Bluetooth technology with access control readers.
Have you seen the new ECKey – EK6 and EK7 that turns your smartphone into a key by using new Bluetooth technology.
Add Reply: Using Bluetooth technology with access control readers.


text:
<?php

namespace PHPCD\Element\ConstantInfo;

use PHPCD\Collection\Collection;

/**
 * @method ConstantInfo[] getIterator()
 */
class ConstantCollection extends Collection
{
    /**
     * @var ConstantInfo[]
     */
    protected $collection = [];

    /**
     * @param ConstantInfo $constantInfo
     *
     * @return $this
     */
    public function add(ConstantInfo $constantInfo)
    {
        $this->collection[$constantInfo->getName()] = $constantInfo;

        return $this;
    }
}

redpajama_set_name: RedPajamaGithub


Jennifer Chiu, L.E. is a Licensed Esthetician in the State of Georgia. She holds an Esthetics License, Masters in Makeup artistry from Glo Minerals and Reflexology Certification from Georgia Career Institute. Jennifer stays up to date on continuing education and takes advantage of learning new products and procedures.
Jennifer brings to Truffles McDonough location over 7 years of expertise in skin and spa services. Her specialties include acne treatments, chemical peels, LED Light therapy, and microdermabrasion. Jennifer is also highly trained in makeup artistry and has done advanced makeup classes for the past 4 years.


text:
using System;
using System.Linq;
using System.Threading.Tasks;
using MongoDB.Bson.Serialization;
using NServiceBus.Extensibility;
using NServiceBus.Sagas;

namespace NServiceBus.Persistence.MongoDB.Sagas
{
    public class SagaPersister : ISagaPersister
    {
        private readonly MongoDbSagaRepository _repo;

        public SagaPersister(MongoDbSagaRepository repo)
        {
            _repo = repo;
        }

        public async Task Save(IContainSagaData sagaData, SagaCorrelationProperty correlationProperty, SynchronizedStorageSession session, ContextBag context)
        {
            DocumentVersionAttribute.SetPropertyValue(sagaData, 0);
            await EnsureUniqueIndex(sagaData.GetType(), correlationProperty?.Name).ConfigureAwait(false);

            await _repo.Insert(sagaData).ConfigureAwait(false);
        }

        private Task EnsureUniqueIndex(Type sagaDataType, string propertyName)
        {
            if (propertyName == null)
            {
                return Task.FromResult(0);
            }

            var classmap = BsonClassMap.LookupClassMap(sagaDataType);
            var uniqueFieldName = GetFieldName(classmap, propertyName);

            return _repo.EnsureUniqueIndex(sagaDataType, uniqueFieldName);
        }

        public Task Update(IContainSagaData sagaData, SynchronizedStorageSession session, ContextBag context)
        {
            var versionProperty = DocumentVersionAttribute.GetProperty(sagaData);

            var classmap = BsonClassMap.LookupClassMap(sagaData.GetType());
            var versionFieldName = GetFieldName(classmap, versionProperty.Key);

            return _repo.Update(sagaData, versionFieldName, versionProperty.Value);
        }

        public Task<TSagaData> Get<TSagaData>(Guid sagaId, SynchronizedStorageSession session, ContextBag context) where TSagaData : IContainSagaData
        {
            return _repo.FindById<TSagaData>(sagaId);
        }

        public Task<TSagaData> Get<TSagaData>(string propertyName, object propertyValue, SynchronizedStorageSession session, ContextBag context) where TSagaData : IContainSagaData
        {
            var classmap = BsonClassMap.LookupClassMap(typeof(TSagaData));
            var propertyFieldName = GetFieldName(classmap, propertyName);

            return _repo.FindByFieldName<TSagaData>(propertyFieldName, propertyValue);
        }

        public Task Complete(IContainSagaData sagaData, SynchronizedStorageSession session, ContextBag context)
        {
            return _repo.Remove(sagaData);
        }

        private string GetFieldName(BsonClassMap classMap, string property)
        {
            var element = classMap.AllMemberMaps.First(m => m.MemberName == property);
            return element.ElementName;
        }
    }
}


text:
Siegfried Bieber
Captain of the 13th Division
Siegfried Bieber is a quiet man who enjoys chess, is learning the rules to shogi, and can often be seen reading outdoors when not on a mission. He is growing very skilled at Shunpo, and has achieved near-mastery of Hakudo.
His demeanor in combat is usually very serious, and either frightened, determined, or annoyed, depending on how the fight is going. He is not averse to dirty fighting when the opportunity presents itself, believing that fair fights are for those who have nothing worth protecting.
He was close to Kayzumai Yen, and seriously affected by his death.
Since calling out former Captain Girikio and assuming his former position, Siegfried has gained a great deal of confidence in his abilities, along with substantially greater mastery of them. He commands his Division as best he can, and has come to understand what he's been fighting for. He values the lives of innocent mortals and his subordinates over almost anything else, and will put himself through anything to protect any one of them.
He's coming to terms with the idea that Arrancar are people, just like anyone else, an idea that was almost unthinkable to him in the past, through a combination of Mia, Kayi, and Isara.
Wears a normal kimono, save for a buckled belt with his name and former rank (Vice Captain) embroidered on it. His footwear is also a bit odd, using Roman-style sandals instead of the traditional geta whenever possible. His black hair typically is a mess of the "bed-head" variety. Now that he is Captain, he also wears the burnt, battered haori of 13th Division, and has vowed not to cease wearing it until he's made up for its bad karma.
His eyes have gotten a bit more open in his time as Captain, to becoming simply hooded, letting those who have worked with him find out for the first time that his eyes are green.
He has a somewhat heavier build than the average Japanese man, and is in top physical condition.
General Abilities
Siegfried is a master of Hakudo, and proficient with whips. His flash steps capacity is nearly limitless, and his speed within them is on the higher end of Captain capacity. He is able to read the general intentions of those who are sufficiently akin to normal humans or Hollows from their body language, and possesses the ability to throw his voice. His Kido is not outstanding, though he can perform up to Hado 63 (Raikoho), inefficiently and with incantation. His repertoire without incantation is limited to most bakudo below thirty, and Hado up to Shakkaho. He has recently been trained in the art of Shunko, and though he has not mastered it yet, he's getting reasonably close.
Zanpaktou, Ingakumo (Fate Spider)
Sealed form: a sword breaker
Shikai, "Oridase, Ingakumo!" (Weave, Fate Spider!)
The sword breaker rapidly covers itself and Bieber's right forearm with what appears to be spider silk. A single strand of the stuff extends from the tip of the blade, long enough to serve as a whip.
This spider silk is extremely concentrated spirit energy, drawn from the wielder. As such, it is considerably stronger than most substances, allowing parrying with the spiderweb gauntlet. More importantly, the single strand extending from the tip serves much like a monomolecular blade, able to slice through pretty much anything.
First Shikai special ability (unnamed, as it is not strictly an attack): Siegfried can spend more of his spiritual energy to extend the blade. He can extend the range to roughly twice the length of a bullwhip, but is not skilled enough to do it in the middle of a slice. It can be used to extend the gauntlet as well, but it takes a while when not concentrating too heavily on it.
Kumo no Soshaku (Spider's Bite): Siegfried can consume all of the spiritsilk on his arm and blade (severing his connection to the whip in the process) to deliver a single, extremely enhanced punch. Striking force is roughly equivalent to direct contact with an exploding grenade.
Bankai, "Yokuyokuna Ingakumo" (Careful Fate Spider)
A quick burst of reiatsu first billows from Siegfried, then collapses back in, quite possibly pulling things with low momentum to him. His body is now covered in spiritsilk armor, and his face is covered by a spiritsilk ski mask. His zanpaktou's sealed form remains in his right hand, now with only a binding around its handle to prevent disarming.
This form presents him with dramatically improved resilience, as well as the ability to create nearly infinite whips from any point on his body, though the range can only be improved at the cost of much greater windup time. Furthermore, his spiritsilk now has the special ability of numbing (within the space of one post) and then completely paralyzing (within the space of two) any body part in which he can strike a bleeding wound. This does not work with his whips, as they move too quickly to transfer an adequate dose of poison.
Lastly, he can now perform Kumo no Soshaku with any part of his body, or multiple parts at once. This is more useful in bankai, as he can use his reiatsu to seal cuts in his armor, and even regrow parts of it from scratch, up to a total of two extra sets of armor.
Revealed Bankai Techniques
Spider Jet: A technique which uses the explosive capacity of Kumo no Soshaku for propulsion, allowing him to reach speeds matched only by the true speed demons of the Seireitei.
Radiant Spider Armor: Using extremely small-scale Kumo no Soshaku to send tiny whips into the air, Siegfried can create a field of blades which has easily cut through immense blocks of stone without any further effort on his part.
Ingakumo appears as a large spider, which communicates telepathically. It is somewhat reserved, like its master, but can be sociable enough. If Siegfried goes too long without training to understand it, Ingakumo will start to nag him.
Siegfried has yet to need to confront his Inner Hollow, instead simply confronting his own moral failings. Thus, he has never seen his Inner World. However, it is an immense web, with everything he's ever done, thought, or experienced connected to and supported by one another.
Siegfried & Tatskete vs. Augustus's minions
Flawed Victory- defeated three Identicals and the first form of the super-gillian, but were unable to prevent it or Augustus from escaping
Siegfried vs. Foreign Vizard John
Loss- Utterly defeated in a match in which both opponents promised to use only their sealed blades. However, managed to temporarily convince John to help the Shinigami
Siegfried vs. Toshiko Yogushi
Victory- Won through close-quarters combat and his bankai's paralysis poison
Siegfried & Akako vs. Abishai
Draw/Loss- Abishai beat upon both of them quite brutally, but was gravely injured by simultaneous detonations of one and a half suits of Siegfried's armor, and Akako's Hado 88. Abishai had a bit more strength left than both of them, but failed to finish them off, and shortly collapsed from the strain of combat.
Siegfried vs. Darius Kiljaeran
Inconclusive- Siegfried managed to acquire a small tempo advantage before the fight was called off due to Espada presence.
Siegfried vs. Toho Tohon
Loss- Utter, utter loss
Siegfried vs. Owynn ap Morrigana
Victory- In a battle of fairy tale trivia, Siegfried was losing out, as the enemy had the remarkable power to become precisely strong enough to defeat his present enemy, along with impressive resistance to zanpaktou. However, this was ultimately undone by the allies that Siegfried was able to summon. After Siegfried injured the Fae with Thunder Roar Cannon while Maru of 3rd Division held him in place, Captain Kiljaeran, Siegfried, and the swordless Commander General Hayashi were able to beat Owynn into committing a rather vicious suicide by activating his Final Coronation. This battle was ultimately won by those three, Captain Satoshi, Gunnery Sergeant Luther Wilson of ARC, and a mysterious entity claiming to be an agent of Fate.
Siegfried vs. Männlicheinlädt Gottheit
Victory- Siegfried ultimately overpowered the bonded Bount via a Spider Jet into Kumo no Soshaku. However, as neither particularly wanted to fight or kill the other, just how things would have gone if he'd been using his whips, and his enemy using his wind control more viciously, has yet to be determined.
Siegfried is about 180 years old. For about 150 of them, he's been a Shinigami. He was born to a fairly well-off commoner family, but grew a bit apart from them during his time at the Academy, as he didn't have chances to see them very often. In the same time, he met and became friends with Akako, Yen, and Tatskete. He got high marks in most classes, though he was strictly average in kido. He was sent to the 13th division, where he worked as an unseated officer with few issues.
He proved adept at his work, learning the name of his sword breaker about eighty years ago, and working his way up to 3rd seat of 13th Division. Shortly after Tsukino Nukari came in, Siegfried was promoted to Vice Captain, as the former 13th Division Vice Captain died holding off an adjuchas-class menos grande until backup arrived. He worked well with his new duties, serving with distinction in both the QuinShin War and the first Toho insurrection. He had few problems until Captain Girikio left on his mission.
In that time, Siegfried was never appointed Acting Captain, so he found enforcing discipline a bit difficult, and more than a bit at odds with his personality. He wound up leading by example, and taking considerably more patrols than the Division average. Then came the second Toho insurrection…
Siegfried has been steadily developing a martial art based around the unique abilities of his zanpaktou.
Named Techniques
Spider Art 1: Spider's Bite
Spider Art 2: Spider Jet
Spider Art 3: Radiant Spider Armor
Spider Art 4: Screw Attack- A mass-destruction technique, presently just a thought experiment, in which Siegfried creates monomolecular whips up to a few miles in length, then spins rapidly, slashing the entire radius around him repeatedly. For obvious reasons, this would not be used in most regions of Soul Society or the Mortal World
Spider Art 5: Rankyaku- A long range kick, in which whips extend from Siegfried's foot as he kicks, slashing over a wide area, without leaving much space to dodge between them
Spider Art 6: Spider Molting- A technique that creates a vertical rip on the interior of his armor. This allows him to escape his armor with Shunpo when it is attacked, setting up a counterattack by making it appear as though his opponent managed to hit.
Spider Art 7: Spider Cocoon- A technique that can only be performed directly after taking advantage of Spider Molting, this technique involves wrapping a nearby enemy up in Siegfried's armor, which rapidly seals itself around them, making movement nearly impossible.
Spider Art 8: Prey Liquifaction- The finale of Spider Molting, this technique splits apart the armor strands on one side of the cocooned enemy, allowing them to serve as monomolecular whips. They are then dragged through the enemy, likely resulting in the prey's body being torn apart.
Spider Art 9: Spider's Flechette Bite- This technique is a variant on Kumo no Soshaku, which, rather than drawing upon all of the silk in a region, draws upon only the inner layer of it, resulting in a smaller blast, but one that sends all the thousands of whip strands created by the tearing of the silk above the explosion into the body of the opponent.
Spider Art 10: Spider Flail- This technique uses Ingakumo's silk to create a thicker whip with a broad head, allowing for smashing attacks, among other things.
Whip Sword (his shikai)
Razor Floss (both shikai and bankai)
Contemplate Our Navels (his inability to come to a decision during the beginning of the Ryoka Invasion arc)
Calling the Old Man Out(his fight with Girikio)
Armor is Useless (averted, by and large; he would've ended up much worse off if it weren't for his spidersilk armor when dealing with Abishai and the Super Gillian; also, it fuels all his super moves, from his whips to the many applications of Kumo no Soshaku)
The Chains of Commanding (since his ascension to Captain, his primary source of stress has been the danger that his Division has to be put through to do their jobs. Thus far, he's accepted it, but woe betide any who harm those underneath him.)
Offense: 100/100
Physical Strength: 90/100
Agility: 90/100
Intelligence: 70/100
Defense: 70/100
Kido: 50/100
Total: 470/600
http://revlid.deviantart.com/art/Siegfried-Bieber-Colour-131934676
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Cell Biology of Disease and Exercise
ymqk

redpajama_set_name: RedPajamaCommonCrawl


text:
package org.opencloudb.mpp;

import java.sql.SQLSyntaxErrorException;
import java.util.HashMap;
import java.util.LinkedHashMap;
import java.util.Map;
import java.util.Set;

import org.opencloudb.route.RouteResultset;

import com.akiban.sql.StandardException;
import com.akiban.sql.parser.AggregateNode;
import com.akiban.sql.parser.BinaryOperatorNode;
import com.akiban.sql.parser.BinaryRelationalOperatorNode;
import com.akiban.sql.parser.ColumnReference;
import com.akiban.sql.parser.ConstantNode;
import com.akiban.sql.parser.CursorNode;
import com.akiban.sql.parser.FromBaseTable;
import com.akiban.sql.parser.FromList;
import com.akiban.sql.parser.FromSubquery;
import com.akiban.sql.parser.FromTable;
import com.akiban.sql.parser.GroupByList;
import com.akiban.sql.parser.InListOperatorNode;
import com.akiban.sql.parser.JoinNode;
import com.akiban.sql.parser.NodeTypes;
import com.akiban.sql.parser.NumericConstantNode;
import com.akiban.sql.parser.OrderByColumn;
import com.akiban.sql.parser.OrderByList;
import com.akiban.sql.parser.QueryTreeNode;
import com.akiban.sql.parser.ResultColumn;
import com.akiban.sql.parser.ResultColumnList;
import com.akiban.sql.parser.ResultSetNode;
import com.akiban.sql.parser.RowConstructorNode;
import com.akiban.sql.parser.SelectNode;
import com.akiban.sql.parser.SubqueryNode;
import com.akiban.sql.parser.UnaryLogicalOperatorNode;
import com.akiban.sql.parser.UnionNode;
import com.akiban.sql.parser.ValueNode;
import com.akiban.sql.parser.ValueNodeList;
import com.akiban.sql.unparser.NodeToString;

public class SelectSQLAnalyser {

	private static String andTableName(SelectParseInf parsInf,
			FromBaseTable fromTable) throws StandardException {
		String tableName = fromTable.getOrigTableName().getTableName();
		String aliasName = fromTable.getTableName().getTableName();
		if ((aliasName != null) && !aliasName.equals(tableName)) {// store alias
			// ->real
			// name
			// relation
			parsInf.ctx.tableAliasMap.put(aliasName, tableName.toUpperCase());
		}
		tableName = tableName.toUpperCase();
		Map<String, Set<ColumnRoutePair>> columVarMap = parsInf.ctx.tablesAndCondtions
				.get(tableName);
		if (columVarMap == null) {
			columVarMap = new LinkedHashMap<String, Set<ColumnRoutePair>>();
			parsInf.ctx.tablesAndCondtions.put(tableName, columVarMap);
		}
		return tableName;
	}

	/**
	 * anlayse group ,order ,limit condtions
	 *
	 * @param rrs
	 * @param ast
	 * @throws SQLSyntaxErrorException
	 */
	public static String analyseMergeInf(RouteResultset rrs, QueryTreeNode ast,
			boolean modifySQLLimit) throws SQLSyntaxErrorException {
		CursorNode rsNode = (CursorNode) ast;
		NumericConstantNode offsetNode = null;
		NumericConstantNode offCountNode = null;
		ResultSetNode resultNode = rsNode.getResultSetNode();
		if (resultNode instanceof SelectNode) {
			Map<String, Integer> aggrColumns = new HashMap<String, Integer>();
			boolean hasAggrColumn = false;
			SelectNode selNode = (SelectNode) resultNode;
			ResultColumnList colums = selNode.getResultColumns();
			for (int i = 0; i < colums.size(); i++) {
				ResultColumn col = colums.get(i);
				ValueNode exp = col.getExpression();
				if (exp instanceof AggregateNode) {
					hasAggrColumn = true;
					String colName = col.getName();
					String aggName = ((AggregateNode) exp).getAggregateName();
					if (colName != null) {
						aggrColumns
								.put(colName, MergeCol.getMergeType(aggName));
					}
				}
			}
			if (!aggrColumns.isEmpty()) {
				rrs.setMergeCols(aggrColumns);
			}
			rrs.setHasAggrColumn(hasAggrColumn);
			GroupByList groupL = selNode.getGroupByList();
			if (groupL != null && !groupL.isEmpty()) {
				String[] groupCols = new String[groupL.size()];
				for (int i = 0; i < groupCols.length; i++) {
					groupCols[i] = groupL.get(i).getColumnName();
				}
				rrs.setGroupByCols(groupCols);
			}
		}
		OrderByList orderBy = rsNode.getOrderByList();
		if (orderBy != null && !orderBy.isEmpty()) {
			LinkedHashMap<String, Integer> orderCols = new LinkedHashMap<String, Integer>();

			for (int i = 0; i < orderBy.size(); i++) {
				OrderByColumn orderCol = orderBy.get(i);
				ValueNode orderExp = orderCol.getExpression();
				if (!(orderExp instanceof ColumnReference)) {
					throw new SQLSyntaxErrorException(
							" aggregated column should has a alias in order to be used in order by clause");
				}
				orderCols.put(orderExp.getColumnName(),
						orderCol.isAscending() ? OrderCol.COL_ORDER_TYPE_ASC
								: OrderCol.COL_ORDER_TYPE_DESC);
			}
			rrs.setOrderByCols(orderCols);
		}
		if (rsNode.getOffsetClause() != null) {
			offsetNode = (NumericConstantNode) rsNode.getOffsetClause();
			rrs.setLimitStart(Integer
					.parseInt(offsetNode.getValue().toString()));

		}
		if (rsNode.getFetchFirstClause() != null) {
			offCountNode = (NumericConstantNode) rsNode.getFetchFirstClause();
			rrs.setLimitSize(Integer.parseInt(offCountNode.getValue()
					.toString()));
		}
		if (modifySQLLimit && offsetNode != null) {
			offsetNode.setValue(0);
			offCountNode.setValue(rrs.getLimitStart() + rrs.getLimitSize());
			try {
				return new NodeToString().toString(ast);
			} catch (StandardException e) {
				throw new SQLSyntaxErrorException(e);
			}
		} else {
			return null;
		}

	}

	public static void analyse(SelectParseInf parsInf, QueryTreeNode ast)
			throws SQLSyntaxErrorException {
		try {
			analyseSQL(parsInf, ast, false);
		} catch (StandardException e) {
			throw new SQLSyntaxErrorException(e);
		}
	}

	private static void addTableName(FromSubquery theSub, SelectParseInf parsInf)
			throws StandardException {
		FromList fromList = ((SelectNode) theSub.getSubquery()).getFromList();
		if (fromList.size() == 1) {
			FromTable fromT = fromList.get(0);
			if (fromT instanceof FromBaseTable) {
				FromBaseTable baseT = ((FromBaseTable) fromT);
				String tableName = baseT.getOrigTableName().getTableName();
				String corrName = theSub.getCorrelationName();
				if (corrName != null) {
					andTableName(parsInf, baseT);
					parsInf.ctx.tableAliasMap.put(corrName,
							tableName.toUpperCase());

				}
			}

		}

	}

	private static void analyseSQL(SelectParseInf parsInf, QueryTreeNode ast,
			boolean notOpt) throws StandardException {
		SelectNode selNode = null;
		switch (ast.getNodeType()) {
		case NodeTypes.CURSOR_NODE: {
			ResultSetNode rsNode = ((CursorNode) ast).getResultSetNode();
			if (rsNode instanceof UnionNode) {
				UnionNode unionNode = (UnionNode) rsNode;
				analyseSQL(parsInf, unionNode.getLeftResultSet(), notOpt);
				analyseSQL(parsInf, unionNode.getRightResultSet(), notOpt);
				return;
			} else if (!(rsNode instanceof SelectNode)) {
				System.out.println("not select node "
						+ rsNode.getClass().getCanonicalName());
				return;
			}
			selNode = (SelectNode) rsNode;
			break;
		}
		case NodeTypes.SELECT_NODE: {
			selNode = (SelectNode) ast;
			break;
		}
		case NodeTypes.SUBQUERY_NODE: {
			SubqueryNode subq = (SubqueryNode) ast;
			selNode = (SelectNode) subq.getResultSet();
			break;
		}
		case NodeTypes.FROM_SUBQUERY: {
			FromSubquery subq = (FromSubquery) ast;
			selNode = (SelectNode) subq.getSubquery();
			break;
		}
		default: {
			System.out.println("todo :not select node "
					+ ast.getClass().getCanonicalName());
			return;
		}
		}

		FromList fromList = selNode.getFromList();
		int formSize = fromList.size();
		String defaultTableName = null;
		if (formSize == 1) {
			FromTable fromT = fromList.get(0);
			if (fromT instanceof FromBaseTable) {
				FromBaseTable baseT = ((FromBaseTable) fromT);
				defaultTableName = baseT.getOrigTableName().getTableName();
			}

		}
		for (int i = 0; i < formSize; i++) {
			FromTable fromT = fromList.get(i);
			if (fromT instanceof FromBaseTable) {
				andTableName(parsInf, (FromBaseTable) fromT);

			} else if (fromT instanceof JoinNode) {
				JoinNode joinNd = (JoinNode) fromT;
				// FromSubquery
				ResultSetNode leftNode = joinNd.getLeftResultSet();
				if (leftNode instanceof FromSubquery) {
					FromSubquery theSub = (FromSubquery) leftNode;
					addTableName(theSub, parsInf);
					analyseSQL(parsInf, theSub, notOpt);

				} else {
					andTableName(parsInf, (FromBaseTable) leftNode);
				}
				ResultSetNode rightNode = joinNd.getRightResultSet();
				if (rightNode instanceof FromSubquery) {
					FromSubquery theSub = (FromSubquery) rightNode;
					addTableName(theSub, parsInf);
					analyseSQL(parsInf, theSub, notOpt);

				} else {
					andTableName(parsInf, (FromBaseTable) rightNode);
				}

				BinaryRelationalOperatorNode joinOpt = (BinaryRelationalOperatorNode) joinNd
						.getJoinClause();
				addTableJoinInf(parsInf.ctx,
						(ColumnReference) joinOpt.getLeftOperand(),
						(ColumnReference) joinOpt.getRightOperand());

			} else if (fromT instanceof FromSubquery) {
				analyseSQL(parsInf, ((FromSubquery) fromT).getSubquery(),
						notOpt);
			} else {
				System.out.println("warn,todo " + fromT.getClass().toString());
			}
		}

		ValueNode valueNode = selNode.getWhereClause();
		if (valueNode == null) {
			return;
		}
		analyseWhereCondition(parsInf, notOpt, defaultTableName, valueNode);
	}

	public static void analyseWhereCondition(SelectParseInf parsInf,
			boolean notOpt, String defaultTableName, ValueNode valueNode)
			throws StandardException {
		// valueNode.treePrint();
		if (valueNode instanceof BinaryOperatorNode) {
			BinaryOperatorNode binRelNode = (BinaryOperatorNode) valueNode;
			ValueNode leftOp = binRelNode.getLeftOperand();
			ValueNode wrightOp = binRelNode.getRightOperand();
			tryColumnCondition(parsInf, defaultTableName,
					binRelNode.getMethodName(), leftOp, wrightOp, notOpt);

		} else if (valueNode instanceof SubqueryNode) {
			analyseSQL(parsInf, valueNode, notOpt);
		} else if (valueNode instanceof UnaryLogicalOperatorNode) {
			UnaryLogicalOperatorNode logicNode = (UnaryLogicalOperatorNode) valueNode;
			boolean theNotOpt = logicNode.getOperator().equals("not") | notOpt;
			analyseWhereCondition(parsInf, theNotOpt, defaultTableName,
					logicNode.getOperand());
		} else if (valueNode instanceof InListOperatorNode) {
			if (notOpt) {
				return;
			}
			InListOperatorNode theOpNode = (InListOperatorNode) valueNode;
			parseIncondition(defaultTableName, theOpNode, parsInf.ctx);
			// addConstCondition(theOpNode.getLeftOperand().getNodeList().get(0),
			// theOpNode.getRightOperandList(), "IN", ctx,
			// defaultTableName, notOpt);
		} else {

			System.out.println("todo parse where cond\r\n "
					+ valueNode.getClass().getCanonicalName());
			// valueNode.treePrint();
		}
	}

	private static void tryColumnCondition(SelectParseInf parsInf,
			String defaultTableName, String methodName, ValueNode leftOp,
			ValueNode wrightOp, boolean notOpt) throws StandardException {
		// 简单的 column=aaa的情况
		if (leftOp instanceof ColumnReference) {
			addConstCondition(leftOp, wrightOp, methodName, parsInf,
					defaultTableName, notOpt);
			return;
		} else if (wrightOp instanceof ColumnReference) {
			addConstCondition(wrightOp, leftOp, methodName, parsInf,
					defaultTableName, notOpt);
			return;
		}
		// 左边 为(a=b) ,(a>b)
		if (leftOp instanceof BinaryOperatorNode) {
			BinaryOperatorNode theOptNode = (BinaryOperatorNode) leftOp;
			tryColumnCondition(parsInf, defaultTableName,
					theOptNode.getMethodName(), theOptNode.getLeftOperand(),
					theOptNode.getRightOperand(), notOpt);

		} else if (leftOp instanceof InListOperatorNode) {
			InListOperatorNode theOpNode = (InListOperatorNode) leftOp;
			addConstCondition(theOpNode.getLeftOperand().getNodeList().get(0),
					theOpNode.getRightOperandList(), "IN", parsInf,
					defaultTableName, notOpt);
		}
		// 右边 为(a=b) ,(a>b)
		if (wrightOp instanceof BinaryOperatorNode) {
			BinaryOperatorNode theOptNode = (BinaryOperatorNode) wrightOp;
			tryColumnCondition(parsInf, defaultTableName,
					theOptNode.getMethodName(), theOptNode.getLeftOperand(),
					theOptNode.getRightOperand(), notOpt);
		} else if (wrightOp instanceof InListOperatorNode) {
			InListOperatorNode theOpNode = (InListOperatorNode) wrightOp;
			addConstCondition(theOpNode.getLeftOperand().getNodeList().get(0),
					theOpNode.getRightOperandList(), "IN", parsInf,
					defaultTableName, notOpt);
		}

	}

	private static String getTableNameForColumn(String defaultTable,
			ColumnReference column, Map<String, String> tableAliasMap) {
		String tableName = column.getTableName();
		if (tableName == null) {
			tableName = defaultTable;
		} else {
			// judge if is alias table name
			String realTableName = tableAliasMap.get(tableName);
			if (realTableName != null) {
				return realTableName;
			}
		}
		return tableName.toUpperCase();
	}

	private static void parseIncondition(String tableName,
			InListOperatorNode theOpNode, ShardingParseInfo ctx) {
		ValueNodeList columnLst = theOpNode.getLeftOperand().getNodeList();
		ValueNodeList columnValLst = theOpNode.getRightOperandList()
				.getNodeList();
		int columnSize = columnLst.size();
		for (int i = 0; i < columnSize; i++) {
			ValueNode columNode = columnLst.get(i);
			if (!(columNode instanceof ColumnReference)) {
				continue;
			}
			ColumnReference columRef = (ColumnReference) columNode;
			tableName = getTableNameForColumn(tableName, columRef,
					ctx.tableAliasMap);
			String colName = columRef.getColumnName();
			final Object[] values = new Object[columnValLst.size()];
			for (int j = 0; j < values.length; j++) {
				ValueNode valNode = columnValLst.get(j);
				if (valNode instanceof ConstantNode) {
					values[j] = ((ConstantNode) valNode).getValue();
				} else {
					// rows
					RowConstructorNode rowConsNode = (RowConstructorNode) valNode;
					values[j] = ((ConstantNode) rowConsNode.getNodeList()
							.get(i)).getValue();

				}

			}
			ctx.addShardingExpr(tableName, colName, values);
		}
	}

	private static void addTableJoinInf(ShardingParseInfo ctx,
			ColumnReference leftColum, ColumnReference rightColm)
			throws StandardException {
		// A.a=B.b
		String leftTable = ctx.getTableName(leftColum.getTableName());
		String rightTale = ctx.getTableName(rightColm.getTableName());
		ctx.addJoin(new JoinRel(leftTable, leftColum.getColumnName(),
				rightTale, rightColm.getColumnName()));

	}

	private static void addConstCondition(ValueNode leftOp, ValueNode wrightOp,
			String method, SelectParseInf parsInf, String defaultTableName,
			boolean notOpt) throws StandardException {

		if (wrightOp instanceof ConstantNode) {
			if (notOpt) {
				return;
			}
			ColumnReference leftColumRef = (ColumnReference) leftOp;
			String tableName = getTableNameForColumn(defaultTableName,
					leftColumRef, parsInf.ctx.tableAliasMap);
			parsInf.ctx.addShardingExpr(tableName, leftOp.getColumnName(),
					((ConstantNode) wrightOp).getValue());

		} else if (wrightOp instanceof RowConstructorNode) {
			if (notOpt) {
				return;
			}
			if (!(leftOp instanceof ColumnReference)) {
				return;
			}
			String tableName = getTableNameForColumn(defaultTableName,
					(ColumnReference) leftOp, parsInf.ctx.tableAliasMap);
			ValueNodeList valList = ((RowConstructorNode) wrightOp)
					.getNodeList();
			final Object[] values = new Object[valList.size()];
			for (int i = 0; i < values.length; i++) {
				ValueNode valNode = valList.get(i);
				values[i] = ((ConstantNode) valNode).getValue();

			}
			parsInf.ctx.addShardingExpr(tableName, leftOp.getColumnName(),
					values);
		} else if (wrightOp instanceof ColumnReference) {
			ColumnReference wrightRef = (ColumnReference) wrightOp;
			if (leftOp instanceof ConstantNode) {
				if (notOpt) {
					return;
				}
				String tableName = getTableNameForColumn(defaultTableName,
						wrightRef, parsInf.ctx.tableAliasMap);
				parsInf.ctx.addShardingExpr(tableName, leftOp.getColumnName(),
						((ConstantNode) leftOp).getValue());

			} else if (leftOp instanceof ColumnReference) {

				ColumnReference leftCol = (ColumnReference) leftOp;
				addTableJoinInf(parsInf.ctx, leftCol, wrightRef);

			} else {
				System.out.println("todo ,parse condition: "
						+ leftOp.getClass().getCanonicalName());
			}
		} else if (wrightOp instanceof SubqueryNode) {
			analyseSQL(parsInf, ((SubqueryNode) wrightOp).getResultSet(),
					notOpt);
		} else {
			System.out.println("todo ,parse condition: "
					+ wrightOp.getClass().getCanonicalName());
		}

	}
}


text:
CDC has new warning on measles
US may soon lose its elimination status
Fred Bodimer
ST. LOUIS (KMOX) — The Centers for Disease Control and Prevention says the United States is on the verge of losing its measles elimination status.
Due to such a low number of cases, the World Health Organization back in 2000 officially declared measles eliminated in the United States. But now, with more than 1,000 cases reported this year, that elimination status may be at risk.
"If that continues to the one-year cutoff point, bang! They take back the elimination card," said Dr. William Schaffner in an interview with CNN. Dr. Schaffner is an infectious disease specialist at Vanderbilt University Medical Center and a longtime adviser to the CDC on vaccine issues.
Related: Worst measles outbreak in 27 years continues to grow
"Losing the elimination status of measles is an embarrassment," Dr. Schaffner told CNN. "Public health will be embarrassed. It's like having a black eye."
A decision could come as soon as Oct. 1.
"I'm concerned it will reduce the motivation of other ministers of health around the world in trying to eliminate measles in their countries because they'll say "Gee if the U.S. couldn't maintain it, why should we work so hard on this?" Schaffner said.
The biggest outbreak in America is occurring in New York state — where a nearly year-long measles outbreak has hit a community of Orthodox Jews, many of whom oppose vaccination.
Related: Does your child need the measles vaccine?
"My concern is that enough people aren't immunizing their kids," said SLU Care's Dr. Ken Haller, a pediatrician at SSM Health Cardinal Glennon Children's Hospital. "We might start getting to a pint where we have a critical mass of un-immunized children so that if measles gets introduced into a community, that may be the spark to spread from one kid to another to another and that may be allow for the measles to get re-established in the United States. And then we may have a really hard time getting rid of it."
Dr. Haller said misinformation about the danger of the measles vaccine remains out there — and that is part of the reason for the insurgence of the disease.
"To be a parent and be scared for your child's safety is normal, rational and healthy," Dr. Haller told KMOX. "And if someone brings these concerns up to me, I'm very glad to hear it. What I talk to parents about at that point is not that there's anything wrong with being scared for your child's safety, but if you are going to be scared, be scared of the appropriate thing — which are diseases like the measles."
For more on measles, go to the CDC website.
Video of Get Vaccinated and Prevent Measles
© 2019 KMOX (Entercom). All rights reserved.


text:
Gubernatorial Hopefuls Mostly Agree on Universal Health Care
Courthouse News Service | Monday, Oct 23, 2017
By Don Debendictus, Courthouse News
ANAHEIM (CN) – The four Democrats running to be California's next governor vowed to resist the Trump administration, protect the state's newly enacted sanctuary status, increase affordable housing and boost jobs and education during their first joint forum Sunday.
But the top two candidates – Lt. Gov. Gavin Newsom and former LA Mayor Antonio Villaraigosa – split on support for a single-payer health care system in California.
Newsom strongly endorsed pending, if vague, legislation to establish universal health coverage for everyone in the Golden State. Villaraigosa called the plan in stalled Senate Bill 562 unworkable because it lacks any funding source for its estimated $400 billion annual cost.
"When you're governor, you got to make the tough choices," Villaraigosa said. "You can't just say, I want pie in the sky, because that doesn't put food on people's tables. So what I would do as governor is to create a public option that allows people to buy into Medicare."
Speaking to an audience of several hundred health care union members, Villaraigosa said he would never "sell you snake oil. We all agree that we need to get there, but we need a plan to get there."
Newsom said the real issue is leadership and California should lead the nation. "I'm not going to wait around for the debate to unfold in Washington, D.C. Sure, I support Medicare for all, but you got to shape the debate in California," he said.
He minimized concerns about cost as "mythology," noting that total health care costs in California currently run about $368 billion annually, with taxpayers footing over 70 percent of the bill. But a single-payer system would drive down those costs through efficiencies and economy of scale, he said.
"A single-payer system provides the ability to provide more efficiency and more cost controls," he said.
Now in his second term as lieutenant governor, Newsome has consistently led the other Democratic gubernatorial candidates in fundraising and polling, although Villaraigosa is expected to draw significant support from the Los Angeles area. The top two vote-getters in California's June primary, regardless of party, will go on to run in the general election in November 2018.
The other Democrats at Sunday's forum before the National Union of Healthcare Workers were state Treasurer John Chiang and Delaine Eastin, the state's superintendent of public instruction from 1995 to 2003. The top two Republicans in the race, John Cox and Travis Allen, were invited to the forum but did not attend, according to the union.
Chiang, who previously served two terms as state controller, supports universal health care but urged a slow but steady approach.
"We don't have to go all-in to provide all the services all at once. Let's make sure that what we're implementing, we can scale up appropriately and show its effectiveness in the program."
Eastin gave the strongest support of the four to the stalled SB 562. A single-payer system would cost more now, she said, but save money later. "The fact of the matter is people are dying in California because we do not have affordable health care coverage for everybody," she said.
Cost increases could be paid for through a gross-receipts tax and a small hike to the state income tax. "We're now paying for a big, for-profit industry that is hosing the state and the people and is not doing a good job by the sickest people," she said.
On other issues, the four candidates all support a month-old law declaring California a "sanctuary state."
Eastin and Villaraigosa in particular said the Constitution's 10th Amendment could be used to defend California from the Trump administration on that and other issues – much as Republican-led states used the amendment, which guarantees state authority, against Obama administration programs.
"The 10th Amendment has been waved in our face for decades" by Republicans, Eastin said. "It's time for us to wave it back."
Support for improved health care coverage in California clearly mattered to members of the National Union of Healthcare Workers. Following the candidate forum, some 350 union stewards voted to endorse Newsom for the governorship, with Eastin coming in second after a runoff vote. Newsom drew 53 percent of the final vote, the union said.
The candidate forum was not conducted as a debate. Rather it was "conversation with a competitive edge," according to moderator John Donvan, a former ABC News reporter and anchor. Four local journalists and three union members each submitted a set of questions to the candidates.
Coincidentally, the NUHW convention took place at an Anaheim hotel about a block from the state Republican Party convention, where erstwhile Trump operative and Breitbart News chief Steve Bannon unleashed an attack on former President George W. Bush and other mainstream Republicans on Friday.
The following day, Gold Star father Khizr Khan, who famously brandished a pocket Constitution at Trump last year, called for unity. "When so much of this nation is worried about the direction of this nation, we will set it right, we will fix it, we will change the course," he said, according to news accounts.
Mike Duryea says:
Monday, Oct 23, 2017 at
That it will bankrupt this state? Oh yeah, they are lunatics just like those currently in office.
Ronda Montgomery says:
Wow………..threat or a warning? Wake up CA………..Brown has stripped the state of it's money, it's dignity and it's law abiding CITIZENS. You're left with debt, illegals and sanctuary status….to protect criminals. If you know these four will follow in his footsteps……………run in the other direction.
Susan McCoun-DeCenzo says:
But I do like that house…
Christine Curtis Marshall says:
we will know this state is OVER if Pelosi and Waters, don't get the the boot next election. Please let Calif secede and become one with themselves. Hollywood can handle everything…they've done pretty well so far.
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We're two college students living in the food capitals of the US — the Bay Area and New York City. We enjoy sampling food from a wide variety of cuisines and exploring unique gastronomical creations. On Welcome to The Gourmet Life, we hope to share some of our favorite restaurant picks and general food commentary.
Hope you enjoy and bon appétit!


MIAMI (AP) _ Five years after a violent confrontation with his first wife, Jose Canseco was arrested Thursday and charged with beating his second wife.
Police charged the 33-year-old Oakland Athletics outfielder with battery for hitting his wife, Jessica, during an argument in a friend's car in Miami at 2:30 a.m.
Canseco was released from the Dade County Jail after posting a $2,000 bond. Under Florida law, those arrested on domestic violence charges are automatically jailed until appearing before a judge.
If convicted, Canseco could be sentenced to up to one year in jail.
His lawyer, Louis Hillman, confirmed the couple are in the process of getting a divorce.
In the 1992 altercation with his first wife, Esther, Canseco was accused of aggravated assault for ramming his car into her new car. The prosecution dropped the charges after Canseco agreed to community service and counseling.
On Thursday, Dade County Judge Mark King Leban ordered the baseball star to keep away from his current wife, who told prosecutors she was terrified of Canseco.
Assistant State Attorney Karen Anderson said Jessica Canseco wants her husband to stay away from her and the couple's infant daughter, who turned 1 year old on Wednesday. His wife asked that any visits by Canseco be supervised.
In granting the order, Liban warned Canseco that any attempt at contact could result in a second charge punishable by up to a year in jail.
As is usual practice in Dade County, Canseco did not appear in court but followed the proceedings via closed-circuit television while still inside the jail next door.
According to Miami police, Canseco and his wife got into an argument as they were returning from their daughter's birthday party. They were both passengers in a car driven by a friend.
``It turned violent ... Mr. Canseco grabbed Mrs. Canseco by the hair, then hit her a few times,″ said police Lt. Bill Schwartz.
Canseco, sitting in the back seat, reached forward to his wife, who was sitting in the front passenger seat, and grabbed her by the hair, then slapped her in the face and the back of the head, police said.
Once back home, Mrs. Canseco, who had a bruise under her left eye, called police. The friend, who was driving, backed up her account of the incident.
Canseco, who filed for free agency last week, hit 23 home runs and had 74 runs batted in.


text:
require "spec_helper"

describe Mongoid::Relations::Bindings::Embedded::Many do

  let(:person) do
    Person.new
  end

  let(:address) do
    Address.new
  end

  let(:target) do
    [ address ]
  end

  let(:metadata) do
    Person.relations["addresses"]
  end

  describe "#bind_all" do

    let(:binding) do
      described_class.new(person, target, metadata)
    end

    context "when the documents are bindable" do

      before do
        binding.bind(:continue => true)
      end

      it "parentizes the documents" do
        address._parent.should == person
      end

      it "sets the inverse relation" do
        address.addressable.should == person
      end
    end

    context "when the documents are not bindable" do

      before do
        address.addressable = person
      end

      it "does nothing" do
        person.addresses.expects(:<<).never
        binding.bind
      end
    end
  end

  describe "#bind_one" do

    let(:binding) do
      described_class.new(person, target, metadata)
    end

    context "when the document is bindable" do

      let(:address_two) do
        Address.new
      end

      before do
        binding.bind_one(address_two, :continue => true)
      end

      it "parentizes the document" do
        address_two._parent.should == person
      end

      it "sets the inverse relation" do
        address_two.addressable.should == person
      end
    end

    context "when the document is not bindable" do

      it "does nothing" do
        person.addresses.expects(:<<).never
        binding.bind_one(address)
      end
    end
  end

  describe "#unbind" do

    let(:binding) do
      described_class.new(person, target, metadata)
    end

    context "when the documents are unbindable" do

      before do
        binding.bind(:continue => true)
        binding.unbind(:continue => true)
      end

      it "removes the inverse relation" do
        address.addressable.should be_nil
      end
    end

    context "when the documents are not unbindable" do

      it "does nothing" do
        person.expects(:addresses=).never
        binding.unbind
      end
    end
  end
end


text:
\section{Introduction}

A recent power-counting renormalizable model for Gravity was proposed by Horava~\cite{Horava:2008ih}. This scenario is based on an anisotropy between space and time coordinates, which is expressed via the
scalings $t\rightarrow b^z t$ and  $x\rightarrow b x$, where $z$ is a dynamical critical exponent. Same recent papers on this topic can be found in Ref. \cite{Koutsoumbas:2010pt}.

Although Horava Lifshitz (HL) Gravity violates local Lorentz invariance in the UV, General Relativity (GR) is expected to be recovered in the infrared IR limit. This implies a very special renormalization group flow for the couplings of the model, in particular  it is expected that the coupling $\lambda$ in the extrinsic curvature term of the action has the behavior $\lambda \rightarrow 1$, i.e. that it flows towards its GR value. But there is no theoretical study supporting this specific
behavior. In addition, there are several other potential inconsistencies in
HL Gravity which have been discussed (see for example
\cite{Charmousis:2009tc} and references therein). More specifically, the breaking of 4D diffeomorphism invariance
introduces an additional scalar mode which may lead to strong coupling problems or instabilities, and in this way prevents HL Gravity from fully reproducing GR in the IR limit.

In Ref.\cite{Horava:2010zj} a new Covariant HL Gravity is formulated by Horava and Melby-Thompson (HM), which includes an additional $U(1)$ symmetry and two additional auxiliary fields $A$ (Gauge field) and $\nu$ (prepotential), aiming at resolving the above mentioned inconsistences of standard HL Gravity. Indeed $U(1)$ symmetry eliminates the extra scalar mode curing the strong coupling problems in the IR limit, for $\lambda=1$. However, as it is shown by da Silva  in Ref. \cite{daSilva:2010bm}, $U(1)$ symmetry can not force the value of the parameter $\lambda$ to be equal to 1, since an action with the $U(1)$ symmetry and $\lambda\neq 1$, can be formulated. Note that the scalar mode is eliminated even for $\lambda\neq1$ as it shown in \cite{daSilva:2010bm, Huang:2010ay}. However, because the coupling $\lambda$ deviates from 1, stability and strong coupling problems (in the matter sector) arising, for details see \cite{Huang:2010ay,Borzou:2011mz}. Previous work on Covariant HL Gravity, can be obtain in Refs. \cite{Wang:2010wi,Kluson:2010zn,Alexandre:2010cb,Greenwald:2010fp}. Cosmology has been examined in \cite{Wang:2010wi}, while for spherically symmetric solutions, for $\lambda=1$,  the reader may consult Refs. \cite{Alexandre:2010cb,Greenwald:2010fp}. Also, star solutions has been obtained in Ref. \cite{Greenwald:2010fp}.

We would like to note that Covariant HL Gravity, as formulated by HM in \cite{Horava:2010zj}, incorporates an additional assumption for the field $A$, according to which $A$ is assumed as a part of the metric in the IR limit, via the replacement $N\rightarrow N-A/c^2$. Although, in the present paper we discuss the HM assumption for $A$, we mainly adopt the alternative point of view \cite{Alexandre:2010cb,Greenwald:2010fp}, unless otherwise stated, according to which space time metric is given by the standard ADM form of Eq. (\ref{ADM}) below.

In this paper we study spherically symmetric vacuum solutions in the framework of Covariant HL Gravity for $\lambda \neq1$, for an action which includes all possible terms allowed by renormalizability requirement \cite{Kiritsis:2009sh} . In particular,  we adopt that $\lambda$ is a running coupling constant  \cite{daSilva:2010bm} , and we study if in the IR limit $\lambda\rightarrow 1$ we can recover Newton's Law, which is necessary in order to agree with experimental data. The main result of this work, which is discussed also in conclusions, is that if $\lambda$ is a running coupling constant, Newton's law can not be recovered in the IR limit $\lambda\rightarrow 1$.  At this point it is worth to note that solutions for $\lambda=1$, as they presented in Ref. \cite{Alexandre:2010cb}, gives Schwarzschild geometry expressed in Painlev\'e-Gullstrand coordinates (for zero Gauge field $A$),
so that they are compatible with Newton 's Law (and more generally with solar system tests). However, these solutions cannot be recovered continuously in the IR limit when $\lambda\rightarrow 1$ (see Sec. \ref{case2} below).

The paper is organized as follows. In Sec.\ref{sec2} we summarize the most important features of the Covariant HL Gravity. We consider then in Sec.\ref{sps} the most general ansatz for spherically symmetric solutions, including
a nonzero radial shift function, and we derive the equations of motion and the corresponding constraints. In Secs. \ref{case1}, \ref{case2} and \ref{case3} we present the solutions considering three situations (note that in case \ref{case3} only the asymptotic behavior of the solutions is examined), in Sec. \ref{cp7} we discuss the HM point of view for $A$ ,and finally Sec. \ref{con} contains our conclusions.

\section{Covariant Horava-Lifshitz Gravity} \label{sec2}

The action of Covariant HL gravity is structured by a set of
five fields: $N(t)$, $N_{i}(x,t)$, $g_{ij}(x,t)$, $A(x,t)$ and
$\nu(x,t)$  $(i=1,2,3)$. Note that $N(t)$, $N_{i}(x,t)$, $g_{ij}(x,t)$ are the standard fields that appear
in the Arnowitt, Deser and Misner (ADM) form of the space-time metric
\begin{equation} \label{ADM}
ds^2=-  c^2 N^2 dt^2+g_{ij} \left(dx^i+N^i dt\right)\left(dx^j+N^j
dt\right)~,
\end{equation}
where $c$ is the velocity of light, with dimension $[c]=z-1$.
In addition, $N$ and $N_i$ are the "lapse" and "shift" functions which are used in general
relativity in order to split space-time dimensions, and
$g_{ij}$ is the spatial metric of signature (+,+,+). Note that
here we are interested for the projectable version of the model which
implies that the lapse function $N(t)$ depends only on the time coordinate. For the
dimensions of "lapse" and "shift" functions we obtain $[N]=0, ~~[N_i]=z-1~$.
The auxiliary fields $A(x,t)$ (potential) and $\nu(x,t)$ (prepotential)
are nondynamical fields with dimensions $[A]=2z-2,~~[\nu]=z-2~$.
The full action of the model is formulated as
\bea\label{action}
S&=&\frac{2}{\kappa^2}\int dt d^dx\sqrt{g}\Big\lbrace N\left[ K_{ij}K^{ij}-\lambda K^2-V+\nu\Theta^{ij}\left(2K_{ij}+\nabla_i\nabla_j\nu\right)\right]\nn
&&~~~~~~~~~~~~~~~~~~+2 (1-\lambda) K\nabla \nu+ (1-\lambda)\left(\nabla \nu\right)^2-A\left(R-2\Omega\right)\Big\rbrace ,
\eea
in which $d=3$ is the spatial dimension, $\kappa^2$ is an overall
coupling constant with dimension $[\kappa^2]=z-d$, and the extrinsic curvature is
\be
K_{ij}=\frac{1}{2 N} \left\{\dot{g}_{ij}-\nabla_i N_j-\nabla_j N_i\right\},~~ i,j=1,2,3,
\ee
where the symbol $\Theta^{ij}$ is defined as
\be
\Theta^{ij}=R^{ij}-\frac{1}{2}R g^{ij}+\Omega g^{ij}~.
\ee
Note that this choice for $z=3$ is an immediate consequence of
power counting renormalizability request.

For the construction of the potential term $V$ we have considered the most general form which includes all possible
renormalizable operators, relevant and marginal with dimension up to six. As the form of the potential is quite extended for this short report we will not present it here. For details, the interested reader may consult Refs. \cite{Wang:2010wi,Alexandre:2010cb} and references therein.

This new model, as the original HL gravity, is invariant under the foliation preserving diffeomorphism, $ Diff({\cal M},{\cal F})$, where ${\cal M}$ is the spacetime manifold, provided with a preferred foliation structure ${\cal F}$.
However, the action of Eq. (\ref{action}) has an additional symmetry, in particular
it remains invariant under a $U(1)$ Gauge symmetry, according to which the fields of the model transform as
\begin{eqnarray}\label{gauge}
&&\delta_\alpha N=0, ~~~  \delta_\alpha g_{ij}=0, ~~~\delta_\alpha N_{i}(x,t)=N \nabla_{i}\alpha \nonumber \\ &&\delta_\alpha A(x,t)=\dot{\alpha}-N^{i}\nabla_{i}\alpha, ~~~\delta_\alpha\nu=\alpha,
\end{eqnarray}
where $\alpha$ is an arbitrary spacetime function. Accordingly, the full symmetry of the action of Eq. (\ref{action})
is the extended Gauge symmetry:  $U(1)\times Diff({\cal M},{\cal F})$.

\section{Spherically Symmetric solutions with $\lambda\neq 1$   } \label{sps}

We consider the most general static spherically symmetric metric, of the form:
\be\label{metric}
ds^2=-c^2 N^2 dt^2+\frac{1}{f(r)}\left(dr+n(r)dt\right)^2+r^2\left(d\theta^2+\sin^2\theta d\phi^2\right),
\ee
where $n(r)=N^{r}(r)$ is the radial component of shift functions, and $N_r=n(r)/f(r)$ since $g_{rr}=1/f(r)$.

From Eq. \ref{action} we find the action
\be\label{S1}
S\propto\int dtd^3x\sqrt{g}\Big\lbrace N\left( T-V\right)-A R\Big\rbrace, ~~T=K_{ij}K^{ij}-\lambda K^2  ,
\ee
in which we consider the Gauge fixing $\nu=0$, we set $\Omega=0$ and $\Lambda=0$ , and where
\bea
&&T=\frac{1-\lambda}{N^2}[2 n'f+n f']^2-\frac{8\lambda}{ N^2 r^2}\left[\frac{2 \lambda-1}{\lambda}n^2f^2+2 r n  n' f^2 +r  f f' n^2\right] \nn
&&-\frac{r^2}{\sqrt{f(r)}}A R=\frac{2}{\sqrt{f(r)}} A(r) \left(r f'+f-1\right).
\eea
For the exact form of the potential term, see our previous work \cite{Alexandre:2010cb}.

From variation with respect to $A$ we find $R=0$, or equivalently we obtain
\be
f(r)=1-\frac{2 B}{r},
\ee
where $B$ is an integration constant. Variation with respect to $n$ and $f$ give respectively the following two equations of motion:
\bea \label{em.1}
(\lambda-1)\left[r^2 n f''+3 r^2 n'f'+2\left(r^2 n''+2 r n'+2 n\right)f\right]+2(2\lambda-1)r f' n=0,
\eea
and
\bea \label{em.2}
&&A'+\frac{A}{2r}\left( 1-\frac{1}{f}\right)+\frac{4nf}{\sqrt r}(n\sqrt r)'={\cal O}V+\\
&&+(1-\lambda)\left[ \frac{8n^2f}{r}+\frac{rn^2}{4f}(f')^2+r(n')^2f-2rn(n'f)'-rn^2f''-2n^2f'\right],\nonumber
\eea
where a prime denotes a derivative with respect to $r$ and the differential operator ${\cal O}$ is defined as
\be
{\cal O}=\frac{r N}{4f}-\frac{\sqrt f N}{2r}\sum_{n=0}^3(-1)^n
\frac{d^n}{dr^n}\left(\frac{r^2}{\sqrt f}\frac{\partial}{\partial f^{(n)}}\right).
\ee
The exact form of ${\cal O}V$ can be found in our previous work \cite{Alexandre:2010cb}.
Finally, the variation of the action with respect to $N(t)$ gives the so called Hamiltonian constraint
\be \label{hamiltonian}
\int_{0}^{\infty}dr \frac{r^2}{\sqrt{f(r)}}(T+V)=0,
\ee
where, using a time redefinition, the lapse function $N(t)$ is set to unity ($N(t)=1$).

\subsection{Nonzero $B\neq 0$ and zero shift function $n=0$} \label{case1}

In this case, for $n=0$ , the equations of motion (\ref{em.1}) and (\ref{em.2}) and the Hamiltonian constraint (\ref{hamiltonian})
are independent of $\lambda$, hence they are identical with the equations in the case of $\lambda=1$ which has been examined in
detail in our previous work of Ref. \cite{Alexandre:2010cb}. We will not aim to present these results again, but we would like to
note that spherically symmetric solutions in this case ($n=0$) are physically relevant only in the framework HM approach when the
auxiliary field $A$ is considered as a part of the spacetime geometry. The conclusion here is that solutions, with zero shift
function and $B\neq 0$, can be compatible with experiment even for $\lambda \neq 1 $, if we adopt HM approach for $A$. On the other
hand, for the case we are interested in, where $A$ is independent of the metric, this class of solutions has no physical interpretation
as it can not reproduce Newton's Law.

\subsection{Zero $B=0$ and nonzero shift function $n(r)\neq 0$.} \label{case2}

A more interesting class of solutions is the one with nonzero shift function $n(r)\neq 0$, for which we make
the choice $B=0$. Note, that if $B\neq 0$ the potential term $V$ blows up for $r \rightarrow 0$, see our previous
work \cite{Alexandre:2010cb}, hence, in order to satisfy the Hamiltonian constraint we have to introduce an unphysical
lower bound in space. We would like to stress that if we set $f=1$ (or we chose  $B=0$) it is possible to satisfy the
Hamiltonian constraint avoiding this unphysical lower bound. In particular, as we will see here, the only way to satisfy
the Hamiltonian constrain and the equations of motion is to set $n=0$, such that the system describes just a Minkowsky metric.

In this case, the potential $V$ vanishes and the Hamiltonian constraint reads
\be\label{case2hc}
\int_0^\infty dr\left\{ (1-\lambda)\left[ 4n^2+4rnn'+(rn')^2\right] -2(rn^2)'\right\rbrace =0~.
\ee
The equation (\ref{em.1}) reads, for any $\lambda\ne1$,
\be\label{case2equan}
n''+\frac{2}{r}n'+\frac{2}{r^2}n=0~,
\ee
and the equation (\ref{em.2}) reads
\be\label{equaf=1}
A'+\frac{4n}{\sqrt r}(n\sqrt r)'=\frac{1-\lambda}{r}\left[ 8n^2-2r^2nn''+r^2(n')^2\right] ~.
\ee
A solution of eq.(\ref{case2equan}) of the form $n\propto r^\alpha$ gives $\alpha=-1/2\pm i\sqrt7/2$, such that
\be\label{case2soln}
n(r)=\frac{1}{\sqrt r}\left(a\cos(k\ln r)+b\sin(k\ln r)\right)~~,~~~~k=\frac{\sqrt7}{2}~,
\ee
where $a,b$ are constants of integration. The solution (\ref{case2soln}) has to satisfy the Hamiltonian constraint
(\ref{case2hc}), and one first notices that all the terms in the integrand are of the form
\be
\frac{1}{r}\cos^2(k\ln r)~~,~\mbox{or}~~~\frac{1}{r}\sin^2(k\ln r)~~,~\mbox{or}~~~\frac{1}{r}\cos(k\ln r)\sin(k\ln r)~,
\ee
such that one can first check if it is possible to cancel the integrand. For this, the identification of terms proportional
to $\cos^2(k\ln r)$ gives
\be
4abk=(1-\lambda)(3a/2+bk)^2~,
\ee
the identification of terms proportional to $\sin^2(k\ln r)$ gives
\be
-4abk=(1-\lambda)(3b/2-ak)^2~,
\ee
and the identification of terms proportional to $\sin(k\ln r)\cos(k\ln r)$ gives
\be
(1+3\lambda)k(b^2-a^2)=(1-\lambda)ab~.
\ee
One can easily see that the only solution for these
last three equations is $a=b=0$. \\
If one wishes to cancel the whole integral appearing in eq.(\ref{case2hc}),
one has to introduce a regularization, since the following integrals do not converge
\be
\int_0^\infty \frac{dr}{r} \cos^2(k\ln r)=\int_{-\infty}^\infty du\cos^2(ku)=\infty~.
\ee
We will therefore use instead the regularization
\bea
\int_{-L}^L du\cos^2(ku)=\int_{-L}^L du\sin^2(ku)&=&\frac{L}{k}\nonumber \\
\int_{-L}^L du\cos(ku)\sin(ku)&=&0~,
\eea
where $L$ can be factorized in the Hamiltonian constraint (\ref{case2hc}) and does not appear in the result. This
constraint gives then
\be
\frac{9}{4}a^2+\frac{9}{4}b^2+k^2(a^2+b^2)=0~,
\ee
such that $a=b=0$.\\
As a consequence, the only possibility to have $\lambda\ne 1$ and $f(r)=1$ is $n=0$, which corresponds to flat space-time.
On the other hand solutions, for $\lambda=1$ and $B=0$, exhibit Schwarzschild geometry, expressed in Painlev\'e-Gullstrand
coordinates, (for zero Gauge field $A$) as they are presented in Ref. \cite{Alexandre:2010cb}, hence they are compatible
with Newton's Law, and more generally with solar system tests. However, we see here that these solutions (Schwarzschild
geometry in Painlev\'e-Gullstrand coordinates) can not be recovered continuously in the IR limit when $\lambda\rightarrow 1$,
as for $\lambda\ne 1$ the model has the only trivial solutions with flat space-time geometry.

\subsection{Nonzero $B\neq 0$ and nonzero shift function $n\neq0$} \label{case3}

In the most general case when $f=1-2 B/r$ ($B\neq 0$), Eq. (\ref{em.1}) can be written as
\be
n''+\frac{2}{r}n'+\frac{2}{r^2}n=\frac{2B}{r}\left( n''+\frac{n'}{2r}+\frac{n}{r^2}\frac{\lambda-2}{\lambda-1}\right) ~,
\ee
As in this case we can not find an exact result, it is reasonable to look for an asymptotic solution of the form
\be\label{expansion}
n(r)=\sum_{p=0}^\infty \left( \frac{B}{r}\right)^p n_p(r)~,
\ee
where the small parameter is $B/r$, and $\lambda\ne1$ is {\it fixed}. We will discuss the regime of validity of this expansion at the end of this subsection. For the first two orders we obtain
\bea
n_0''+\frac{2}{r}n_0'+\frac{2}{r^2}n_0&=&0\\
\left( \frac{n_1}{r}\right) ''+\frac{2}{r}\left( \frac{n_1}{r}\right)'+\frac{2}{r^2}\left( \frac{n_1}{r}\right) &=&
\frac{2}{r}\left(n_0''+\frac{n_0'}{2r}+\frac{n_0}{r^2}\frac{\lambda-2}{\lambda-1} \right)~, \nonumber
\eea
such that $n_0$ is given by Eq. (\ref{case2soln}). It is then easy to see that the solution
\be
n_1=\frac{1}{\sqrt r}\left( \tilde a\cos(k\ln r)+\tilde b\sin(k\ln r)\right)~, ~~k=\frac{\sqrt7}{2}~,
\ee
satisfies the previous differential equation, if the constants $\tilde a,\tilde b$ are given by
\bea\label{abtilde}
\tilde a&=&\left( 1+\frac{(1+\sqrt7)(\lambda-2)}{4(\lambda-1)}\right) a-\frac{\sqrt7}{2}b\\
\tilde b&=&\frac{\sqrt7}{2}a+\left( 1+\frac{(1+\sqrt7)(\lambda-2)}{4(\lambda-1)}\right)b\nonumber~,
\eea
where $a$ and $b$ are the constants of integration appearing in $n_0$ (see Eq. (\ref{case2soln})).
To the first order in $B/r$ we therefore have
\be \label{nasympt}
n=\frac{1}{\sqrt r}\left( a+\frac{\tilde a B}{r}+\cdots\right) \cos(k\ln r)+
\frac{1}{\sqrt r}\left( b+\frac{\tilde b B}{r}+\cdots\right) \sin(k\ln r)~.
\ee

We would like to warn the reader that, for $B\neq 0$, we can obtain only the asymptotic behavior of the solutions,
as the equations of motion can not be solved analytically. Additionally, we have not checked if solutions with the
above asymptotic behavior of Eq. (\ref{nasympt}) indeed satisfy the Hamiltonian constraint. However, it is clear
that the oscillating behavior of Eq. (\ref{nasympt}) is not compatible with Newton's Law: in particular we have for
the potential $\phi(r)=- n^2/2 c^2$ (for details on the derivation, see \cite{Alexandre:2010cb}) the following expression
\be \label{potential1}
\phi(r)=\frac{a^2+b^2}{2 r}+\frac{a^2-b^2}{2 r}\cos(2 k\ln r)+\frac{a b}{ r}\sin(2 k\ln r)+O\left(\frac{1}{r^2}\right),
\ee
where we see that the oscillating terms are of the same order of magnitude as the Newton potential, and cannot be canceled
for nonzero values of the constants of integration $a$ and $b$.

Let us come back to the expansion (\ref{expansion}).
This expansion is valid as long as $(B/r)n_{p+1}<<n_p$, and we define the critical
distance $r_c$ below which the expansion is not valid anymore, and $(B/r_c)n_{p+1}(r_c)\simeq n_p(r_c)$.
If we consider then the first two terms of the expansion, as well as
the expressions (\ref{abtilde}) for $\tilde a$ and $\tilde b$, we obtain
\be
\frac{1}{\sqrt r_{c}}\simeq \frac{B}{r_{c}^{3/2}}\frac{1}{\lambda-1}~,
\ee
such that $r_{c}\simeq B/(\lambda-1)$. Finally, for $r<<r_c$ and from Eq. (\ref{em.1}), we see that $n(r)\to0$
when $\lambda \rightarrow 1$, while the asymptotic behavior of Eq. (\ref{expansion}) is valid only for $r>>r_c$,
with $r_c\to\infty$ when $\lambda\to1$.

\section{Comments on the HM interpretation for $A$ as a part of spacetime metric } \label{cp7}

The IR asymptotic behavior for $A$, which now is assumed as a part of  spacetime metric, can be obtain by using Eq. (\ref{em.2}):
\be
A_{IR}=c^2+A_0+\frac{K_1-A_0 B}{r}+K_2\frac{\cos(2 k\ln r)}{r}+K_3\frac{\sin(2 k\ln r)}{r}+O\left(\frac{1}{r^2}\right),
\ee
in which we have kept only the leading terms of the order of $1/r$, and $A_0$ is a constant of integration.
In the expression for $A_{IR}$, the constants $K_1,K_2,~K_3$ are
\bea
K_1&=& 6(1-\lambda) (a^2+b^2)\\
K_2&=&  \frac{1}{8} [(\lambda+6)(b^2-a^2)+2 \sqrt{7}(5\lambda-4)a b ]\nonu
K_3&=& \frac{1}{8} [\sqrt{7}(5\lambda-4)(b^2-a^2)-2(\lambda+6) a b ] \nonumber~.
\eea
In what follows we set $A_0=-c^2$.

In the case of HM theory the "Newtonian" potential, if we drop higher order terms ($1/r^n$ with $n\geq 2$), is given by the equation
\bea \label{potential2}
\phi(r)&=&-\frac{f (r) n^2+2 A_{IR}}{2 c^2}\\
&=&\frac{Z1}{r}+Z_2\frac{\cos(2 k\ln r)}{r}+Z_3\frac{\sin(2 k\ln r)}{r}+O\left(\frac{1}{r^2}\right)\nonumber
\eea
where
\bea
Z_1&=& \left(6\lambda-\frac{25}{4}\right) (\hat{a}^2+\hat{b}^2)- B\\
Z_2&=& -\frac{1}{8} [(\lambda+4)(\hat{b}^2-\hat{a}^2)+2 \sqrt{7}(5\lambda-4)\hat{a} \hat{b} ]\nonu
Z_3&=& -\frac{1}{8} [\sqrt{7}(5\lambda-4)(\hat{b}^2-\hat{a}^2)-2(\lambda+4) \hat{a} \hat{b }] \nonumber~.
\eea
where $\hat{a}=a/c$ and $\hat{b}=b/c$. It is possible to cancel simultaneously $Z_2$ and $Z_3$ only for $a=b=0$, since the following system
of linear equations
\bea
&&  (\lambda+4)x+2 \sqrt{7}(5\lambda-4)y=0 \\
 && \sqrt{7}(5\lambda-4)x-2(\lambda+4) y=0 \nonumber~,
\eea
where $x=\hat{b}^2-\hat{a}^2$ and $y=\hat{a} \hat{b}$
has negative determinant, $D=-2(\lambda+4)^2-14 (5\lambda-4)^2<0$. However, if we set $Z_1=2 M$ and keep suitably
small the parameters $\hat a,\hat b<<\sqrt{M}$ (so small that the oscillations are not observable) we can recover the Newtonian potential (and the Schwarzschild metric) even for $\lambda \neq 1$, so HM theory can
not fix $\lambda$ to unity. In addition for $\lambda=1$ the oscillating terms do not vanish.

\section{Conclusions} \label{con}

We have studied spherically symmetric solutions of Covariant
Horava Lifshitz Gravity for $\lambda\neq 1$, namely we have assumed that $\lambda$ is a
running coupling as it presented in Ref. \cite{daSilva:2010bm}. We found that, for zero radial shift
function $n(r)=0$ and $B\neq 0$, spherically symmetric solutions are independent on the running coupling $\lambda$,
hence they are identical with solutions when $\lambda=1$ which have been analyzed previously in \cite{Alexandre:2010cb}.
For nonzero radial shift function $n(r)\neq 0$ and $B=0$, we show that the only solution of the
model is the flat space-time metric if $\lambda\neq 1$. In the general case: $n(r)\neq 0 $ and $B\neq 0$,
numerical work is necessary for analyzing the spectrum of solutions and checking if they satisfy the Hamiltonian constraint,
which is beyond the scope of this note. However, in this case it is possible to obtain the asymptotic form of the
metric which is enough in order to compare with experimental data.

In this paper we mainly focus to the question whether spherically symmetric solutions can be compatible with
experiment in the IR limit $\lambda\rightarrow 1$. In particular we have shown that if we adopt the  position
that $A$ is independent of the space-time metric (hence the Newtonian potential is given by Eq. (\ref{potential1})),
it is impossible to recover Newtonian physics in the IR limit. If $B=0$ the only spherically symmetric solution has
flat space-time metric, so in the limit $\lambda\rightarrow 1$ we can not recover continuously solutions for $\lambda=1$,
which are in agrement with solar system tests (see Ref. \cite{Alexandre:2010cb}). Also, for $B\neq 0$, oscillating behavior
of solutions in the IR limit is non compatible with Newton's Law.

According to the altenative HM approach, $A$ is assumed as a part of the potential according to the equation (\ref{potential2}).
In this case, as we show in Sec. \ref{cp7}, it is possible to recover Newton Law (or more general Schwarzschild spacetime geometry)
by adjusting suitably the integration constants $\hat a,\hat b<<\sqrt{M}$, independently of the value of $\lambda$. As a result
the limit $\lambda\rightarrow 1$ is not necessary in order to achieve agrement with solar system tests (or equivalently even
for $\lambda\neq 1$ we could have agreement with experiment).

From the above discussion we conclude that, if we adopt that the auxiliary field $A$ is not a part of the metric, Newtonian
potential can not be recovered in the IR limit $\lambda\rightarrow 1$. Therefore we have to invoke a
mechanics for fixing $\lambda$ to unity (for example a new symmetry) and construct a model which is physically relevant, as
only solutions for $\lambda=1$ and $B=0$ are compatible with experimental data.

\vspace{0.5cm}

\nin{\bf Acknowledgments}  This work is supported by the Royal Society, UK.

\vspace{0.5cm}

redpajama_set_name: RedPajamaArXiv


First there were rumours that Brymo had left Chocolate City, then the record label released a statement denying the rumour, and now Brymo has gone on Twitter to set the record straight. Like Jesse Jagz, he has also left Chocolate City, though the record company is insisting he still has a valid contract with them.
'He still has three years and two albums to deliver, that's what his contract says', a rep for the label said.


transportation costs as well as the associated fuel requirements.
bottled water where for every bottle filled, three times its volume is wasted.
Once returned, bottles are washed, sterilized and reused again and again.
less C02 after the first use of each bottle.


Kid's Omega-3 DHA helps your child live out their potential.
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Changes to certain federal constitutional laws
Vladimir Putin signed Federal Constitutional Law On Amendments to Certain Federal Constitutional Laws.
This Federal Constitutional Law was drafted in order to implement the provisions of the Law of the Russian Federation on introducing an amendment to the Constitution of the Russian Federation, On Improving the Regulation of Certain Aspects of the Organisation and Functioning of Public Authority, concerning the Federation Council's authority to terminate, upon a submission from the President of the Russian Federation, the appointment of the Chairman of the Constitutional Court of the Russian Federation, its deputies and judges; the Chairman of the Supreme Court of the Russian Federation, its deputies and judges, chairmen, deputy chairmen and judges of the cassation and appeal courts, the Intellectual Property Rights Court, if they commit acts that compromise the judge's honour and dignity, as well as in other cases provided for by the federal constitutional law that prevent a judge from exercising his/her powers.
The law aims to establish the procedure for the implementation of the new powers the President of the Russian Federation is vested with under Article 83(f3) of the Constitution of the Russian Federation.
The law provides for making corresponding amendments to the Federal Constitutional Law On the Judicial System of the Russian Federation, as well as to other federal constitutional laws, including the Federal Constitutional Law On Arbitration Courts in the Russian Federation, the Federal Constitutional Law On Military Courts in the Russian Federation, and the Federal Constitutional Law On Courts of General Jurisdiction in the Russian Federation.
Published in section: Documents
http://en.kremlin.ru/acts/news/64573


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TV showrunners are the new rock stars. Right, Vince and Shonda? VIDEO INTERVIEW
Today's Guest: Neil Landau, screenwriter, UCLA School of Film professor, author, The TV Showrunner's Roadmap Watch this exclusive Mr. Media interview with Neil Landau, screenwriter, UCLA School of Film professor and author of The TV Showrunner's Roadmap, by clicking on the video player above! Mr. Media is recorded live before a studio audience full... Continue Reading →
Eureka's Niall Matter challenges Mr. Media to hunky nerd-off! VIDEO INTERVIEW
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Melrose Place returns; get the scoop from Thomas Calabro! PODCAST INTERVIEW
When last we spoke, Thomas Calabro was preparing to host ACME Comedy's "ACME Saturday Night" live show and being described as a former star of the late lamented TV series "Melrose Place." THOMAS CALABRO podcast excerpt: "The name, Melrose Place, remains the same but everything about it is different, so it's sort of like... Continue Reading →
NBA baller turned actor Rick Fox settles in at Melrose Place! PODCAST INTERVIEW
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Desperate Housewives hubby Doug Savant for kids, Listerine! PODCAST INTERVIEW
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Once and Again, but Billy Campbell will always be our Rocketeer! PODCAST INTERVIEW
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Ali Landry and David Charvet face The Superstars! PODCAST INTERVIEW
My best friend Bruce Kessler and I would be glued to ABC's "Wide World of Sports" during the 1970s when it aired its 'Superstars" competitions, pitting athletes and celebrities against one another in sports which no one had a natural advantage or, usually, much experience. Now ABC has once more brought back that old... Continue Reading →
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