Figure F.11. Figure similar to g. 5.2, here we added a smaller ontributionof
a ℓ0 = 100µ
Ktothemultipoles,suhthat weanobservetheonsetoftheseparation proessofthevetors. Mollweideprojetion oftheskywithquadrupole(upperrow)andotopole(lowerrow)multipolevetors[equation(5.5) ℄. Themeshonsistsofsteps
in
30 ◦
. Displayedaretenpairsofquadrupolevetors(smalldots)andtheirtenareavetors[equation(5.6)(bigdots)℄aswellastentriplesofotopolevetors(smalldots)
and theirarea vetors(bigdots);togethernessisindiatedbyolour. Thearbitrary
signofthevetorshasbeenusedtogaugethemall tothenorthernhemisphere. The
statistially isotropi and Gaussianase (leftolumn) isbrokenbythe imprintof a
moderateaxialeet
a ℓ0 = 100µ
K(rightolumn)whereuponmultipolevetorsstartto movetothepoleandareavetorsstart tomovetotheequatorialplane. Thefull
separation an be observed when adding strong ontributions
a ℓ0 ∼ 1000µ
K, .f.g. 5.2.
0
20 40
60
80
100 0 20
40 60
80 100 1.4
1.6 1.8 2 2.2 2.4 2.6 2.8 3 3.2
N(S nn )/10 3 3 2.5 2 1.5
a 30 axial [ µ K]
a 20 axial [ µ K]
0
50
100
150
200 0 50
100 150
200 1
1.5 2 2.5 3 3.5 4
N(S nn )/10 3 3.5 3 2.5 2 1.5
a 30 axial [µK]
a 20 axial [ µ K]
Figure F.12. Testing theeetofasymmetriadditiveontributions
a axial ℓ0
ontheintrinsiross alignmentofquadrupoleandotopole. Here,theross alignmenttest
is denedas
S nn ≡ P |ˆ n (2;,1,2) · n ˆ (3;,i,j) |
;notethe dierent pre-fatorasomparedto (5.8) . Like in g. F.10, we have plotted the arbitrarily saled (
×10 −3
) numberofMonteCarlosthat are,for givenvaluesof
a axial ℓ0
,onsistentwithanexperimental value ofS nn ≃ 2.62
,thathas beenobtainedfrom WMAP(1yr)leaned maps. ThetotalnumberofMonteCarlosisagain
10 5
. Theupperandlowergureshowthesametest, onlywith adierentrange ofsimulations. Fromtheuppergure,weseethat
indeed,intrinsialignmentsareapparentlyuredbyaddingaxialontributionsupto
∼ 100µ
K.Inthelowergurewe seethat,wheninreasinga axial ℓ0
further,this isonlyaloalmaximum.Thisisperfetlyonsistentwithourndingsg.5.3.
[AA06℄ Havard Alnes and Morad Amarzguioui, CMB Anisotropies Seen by an o-Center Observer
in a Spherially Symmetri Inhomogeneous Universe, Phys. Rev. D74 (2006), 103520,
astro-ph/0607334.
[AA07℄ , The Supernova Hubble Diagram foro-Center Observers in a Spherially Symmetri
InhomogeneousUniverse,Phys.Rev.D75(2007),023506,astro-ph/0610331.
[ACW07℄ LottyAkerman,SeanM.Carroll,andMarkB.Wise,ImprintsofaPrimordialPreferredDiretion
ontheMirowaveBakground,Phys.Rev.D75(2007),083502,astro-ph/0701357.
[AFMS93℄ J.V.Arnau,M.J.Fullana,L.Monreal,andD.Saez,OntheMirowaveBakgroundAnisotropies
Produed byNonlinearVoids,Astrophys.J.402(1993),359368.
[AFZ06℄ GarryW.Angus,BenoitFamaey,andHongSheng Zhao,CanMONDTake aBullet? Analytial
Comparisons ofThree Versionsof MONDBeyond SpherialSymmetry,Mon.Not.Roy.Astron.
So.371(2006),138,astro-ph/0606216.
[AJW06℄ L.RaulAbramo,LaerteSodreJr.,andCarlosAlexandreWuenshe,Anomaliesinthelow CMB
MultipolesandExtendedForegrounds,Phys.Rev.D74(2006),083515,astro-ph/0605269.
[Akh02℄ EvgenyK.Akhmedov,VauumEnergyandRelativistiInvariane,2002,hep-th/0204048.
[Ale06℄ StephonH.S.Alexander,IsCosmiParityViolationResponsiblefortheAnomaliesintheWMAP
Data?,2006,hep-th/0601034.
[ALST07℄ RalfAurih,S.Lustig,F.Steiner,andH.Then,CMBAlignmentinMulti-Conneted Universes,
Class.Quant.Grav.24(2007),18791894,astro-ph/0612308.
[APO℄ TeamAPOD,TheoialNASAsite`AstronomyPitureoftheDay'athttp://apod.nasa.gov/
apod/lib/aptree.html.
[Arn62℄ Arnowitt,D.,Deser,S.andMisnerC.W.,inGravitation: AnIntrodutiontoCurrentResearh,
NewYork: Wiley,editedbyWitten,Louis,1962.
[AS72℄ MiltonAbramowitzandIreneA.Stegun,HandbookofMathematialFuntions,DoverPubliations
In.,NewYork,1972.
[AS03℄ LuisRaulAbramoandJr.Sodre,Laerte,CantheLoalSuperlusterExplainthelowCMB
Mul-tipoles?,2003,astro-ph/0312124.
[Ast℄ Think Astronomy, Homepage of the Think Astronomy ommunity at http://www.think
astronomy.om.
[B
+
03a℄ C. Bennett et al., First Year Wilkinson Mirowave Anisotropy Probe (WMAP) Observations:
ForegroundEmission,Astrophys.J.Suppl.148(2003),97,astro-ph/0302208.
[B
+
03b℄ C.L.Bennettet al.,FirstYearWilkinsonMirowaveAnisotropy Probe(WMAP)Observations:
PreliminaryMapsandBasiResults,Astrophys.J.Suppl.148(2003),1,astro-ph/0302207.
[B
+
06a℄ James Bok et al., Task Fore on Cosmi Mirowave Bakground Researh, 2006,
astro-ph/0604101.
[B
+
06b℄ Maru²aBrada£et al.,Strongand WeakLensingUnited III:MeasuringtheMass Distributionof
theMergingGalaxyCluster1E0657-56,Astrophys.J.652(2006),937947,astro-ph/0608408.
[BBS91℄ K.G.Begeman,A.H.Broeils,andR.H.Sanders,ExtendedRotationCurvesofSpiralGalaxies
-DarkhaloesandModied Dynamis,Mon.Not.Roy.Astron.So.249(1991),523.
[BBS07℄ DanielBabih,CullenH.Blake,andCharlesSteinhardt,WhatCantheCosmiMirowave
Bak-groundTellUsAbouttheOuterSolarSystem?,2007,arXiv:0705.0986[astro-ph℄.
[BdVS06℄ D.Boyanovsky,HetorJ.deVega,and N.G.Sanhez,CMBQuadrupoleSuppression.I:Initial
Conditionsof InationaryPerturbations,Phys.Rev.D74(2006),123006,astro-ph/0607508.
[Beh03℄ JulianeBehrend,OntheAveragingProblem inGeneralRelativity. Diplom thesis,Universityof
Heidelberg,2003,Availablee.g.athttp://www.thphys.uni-h eid elbe rg.d e/ behrend/.
[Bek04℄ JaobD.Bekenstein, RelativistiGravitationTheoryfortheMONDParadigm,Phys.Rev.D70
(2004),083509,astro-ph/0403694.
[BG83℄ M.BirkinshawandS.F.Gull,ATestforTransverseMotionsofClustersofGalaxies,Nature302
(1983),315317.
[BG06℄ H.BalasinandDanielGrumiller,SigniantRedutionof GalatiDarkMatterbyGeneral
Rel-ativity,2006,astro-ph/0602519.
[BKH05℄ KrzysztofBolejko,AndrzejKrasi«ski,andCharlesHellaby,Formationof Voids intheUniverse
withintheLemaître-TolmanModel,Mon.Not.Roy.Astron.So.362(2005),213.
[BL93℄ J.BiakandT.Ledvinka,Relativisti Disksassoures oftheKerrmetri,Phys.Rev.Lett.71
(1993),16691672.
[BM06℄ RihardA.Battyeand AdamMoss,AnisotropiPerturbationsDuetoDarkEnergy,Phys.Rev.
D74(2006),041301,astro-ph/0602377.
[BM07℄ J. R. Brownstein and J.W. Moat, TheBullet Cluster 1E0657-558 Evidene Shows Modied
GravityintheAbseneofDarkMatter,2007,astro-ph/0702146.
[BMN06℄ TirthabirBiswas,RezaMansouri,andAlessioNotari,NonlinearStrutureFormationand
Appar-entAeleration: anInvestigation,2006,astro-ph/0606703.
[BN07℄ TirthabirBiswasandAlessioNotari,Swiss-CheeseInhomogeneousCosmology&theDarkEnergy
Problem,2007,astro-ph/0702555.
[Bol05℄ Krzysztof Bolejko, Supernovae Ia Observations in the Lemaitre-Tolman Model, 2005,
astro-ph/0512103.
[Bol07℄ ,EvolutionofCosmiStruturesinDierentEnvironmentsintheQuasispherialSzekeres
Model,Phys.Rev.D75(2007),043508,astro-ph/0610292.
[Bon47℄ H.Bondi,SpheriallySymmetriModelsinGeneralRelativity,Mon.Not.Roy.Astron.So.107
(1947),410,reprintedwithhistorialommentsinGen.Rel.Grav.31(1999),1777.
[Bon77℄ W.B.Bonnor,ARotatingDustCloudinGeneralRelativity,J.Phys.A:Math.Gen.10(1977),
16731677.
[Bon80℄ ,TheRigidlyRotatingRelativistiDustCylinder,J.Phys.A:Math.Gen.13(1980),2121
2132.
[BT94℄ JamesBinneyandSottTremaine,GalatiDynamis,PrinetonUniversityPress,PrinetonNew
Jersey,1994.
[BTT07a℄ NikolaosBrouzakis,NikolaosTetradis,andEleftheriaTzavara,LightPropagationandLarge-Sale
Inhomogeneities,2007,astro-ph/0703586.
[BTT07b℄ , The Eet of Large-Sale Inhomogeneities on the Luminosity Distane, JCAP 0702
(2007),013,astro-ph/0612179.
[BTV07℄ ArmandoBernui,ConstantinoTsallis,andThyrsoVillela,DeviationfromGaussianityinthe
Cos-mi MirowaveBakground Temperature Flutuations,Europhys. Lett.78(2007),19001,
astro-ph/0703708.
[Bu01℄ ThomasBuhert,OnAveragePropertiesofInhomogeneousFluidsinGeneralRelativity: Perfet
FluidCosmologies,Gen.Rel.Grav.33(2001),13811405,gr-q/0102049.
[Bu07℄ ,DarkEnergyfromStruture-AStatusReport,2007,arXiv:0707.2153[gr-q℄.
[C
00℄ M. N. Célérier, Do we Really See a Cosmologial Constant in the Supernovae Data?, Astron.
Astrophys.353(2000),6371,astro-ph/9907206.
[C
+
06a℄ Douglas Cloweet al., ADiret Empirial Proof of theExistene of Dark Matter, 2006,
astro-ph/0608407.
[C
+
06b℄ AndresCurtoetal.,TestingGaussianityonArheopsData,2006,astro-ph/0612148.
[Car69℄ BrandonCarter, Killing HorizonsandOrthogonallyTransitiveGroupsinSpae-Time,J.Math.
Phys.10(1969),70.
[CCT06℄ LuigiCampanelli,P.Cea,andL.Tedeso,EllipsoidalUniverseCanSolveTheCMBQuadrupole
Problem,Phys.Rev.Lett.97(2006),131302,astro-ph/0606266.
[Chr84℄ D.Christodoulou,ViolationofCosmiCensorshipintheGravitationalCollapseofaDustCloud,
CommuniationsinMathematialPhysis93(1984),171195.
[CHR02℄ J.E. Carlstrom,G.P.Holder,and E.D.Reese,Cosmology with theSunyaev-Zel'dovihEet,
Ann.Rev.Astron.Astrophys.40(2002),643680,astro-ph/0208192.
[CHS04℄ CraigJ.Copi,DraganHuterer,andGlennD.Starkman,MultipoleVetors-ANewRepresentation
oftheCMBSky andEvideneforStatistialAnisotropyorNon-Gaussianityat
2 ≤ ℓ ≤ 8
,Phys.Rev.D70(2004),043515,astro-ph/0310511.
[CHSS06℄ CraigJ.Copi,D.Huterer,D.J.Shwarz,andG.D.Starkman,OntheLarge-AngleAnomaliesof
theMirowaveSky,Mon.Not.Roy.Astron.So.367(2006),79102,astro-ph/0508047.
[CHSS07℄ CraigCopi,DraganHuterer,DominikShwarz,andGlennStarkman,TheUnorrelatedUniverse:
StatistialAnisotropyandtheVanishingAngularCorrelationFuntioninWMAPYears1-3,Phys.
Rev.D75(2007),023507,astro-ph/0605135.
[Cle85℄ D.P.Clemens,Massahusetts-StonyBrookGalatiPlaneCOSurvey-TheGalatiDisk
Rota-tionCurve,Astrophys.J.295(1985),422428.
[CMB℄ CMBFAST, Uro²Seljak and Matias Zaldarriaga, homepage of CMBFAST athttp://fa-www.
harvard.edu/~mzaldarr/CMB FAST /mb fas t.ht ml orhttp://www.mbfast.org/.
[CPKL03℄ CarloR.Contaldi,MaroPeloso,LevKofman,andAndreiLinde,SuppressingthelowerMultipoles
intheCMBAnisotropies,JCAP0307(2003),002,astro-ph/0303636.
[Cro06℄ DanielJ.Cross,CommentsontheCooperstok-TieuGalaxy Model,2006,astro-ph/0601191.
[CS98℄ M.N.CélérierandJ.Shneider,ASolutiontotheHorizonProblem: aDelayedBigBang
Singu-larity,Phys.Lett.A249(1998),37.
[CS02℄ M.N.CélérierandP.Szekeres,TimelikeandNullFoussingSingularitiesinSpherialSymmetry:
A Solution to the Cosmologial Horizon Problem and a Challenge to the Cosmi Censorship
Hypothesis,Phys.Rev.D65(2002),123516.
[CS05℄ AsanthaCoorayandNaokiSeto,DidWMAP seeMovingLoalStrutures?,JCAP0512(2005),
004,astro-ph/0510137.
[CT05a℄ FredI.Cooperstokand S.Tieu,GeneralRelativityResolvesGalati Rotation WithoutExoti
DarkMatter,2005,astro-ph/0507619.
[CT05b℄ ,PerspetivesonGalatiDynamisviaGeneralRelativity,2005,astro-ph/0512048.
[CT06℄ , Galati Dynamis via General Relativity and the Exoti DarkMatter Enigma, Mod.
Phys.Lett.A21(2006),21332142.
[D
+
03℄ A.G.Doroshkevihetal.,Gauss-LegendreSkyPixelization(GLESP)forCMBMaps,2003,
astro-ph/0305537.
[D
+
07℄ Tamara M.Davis et al., Srutinizing Exoti Cosmologial Models Using ESSENCE Supernova
DataCombined withOtherCosmologialProbes,2007,astro-ph/0701510.
[DL03℄ TamaraM.DavisandCharlesH.Lineweaver,ExpandingConfusion: CommonMisoneptionsof
CosmologialHorizonsandtheSuperluminalExpansionoftheUniverse,2003,astro-ph/0310808.
[dOCT06℄ AngeliadeOliveira-CostaandMaxTegmark,CMBMultipoleMeasurementsinthePreseneof
Foregrounds,Phys.Rev.D74(2006),023005,astro-ph/0603369.
[dOCTZH04℄ AngeliadeOliveira-Costa,MaxTegmark,MatiasZaldarriaga,andAndrew Hamilton,The
Sig-niane of the Largest Sale CMB Flutuations in WMAP, Phys. Rev. D69 (2004), 063516,
astro-ph/0307282.
[DPS
+
07℄ V.Dikarev, O.Preuÿ, S.Solanki,H. Krüger,and A.Krivov, TheMirowave Anisotropy Probe
Mission,EarthMoonandPlanets(2007),47.
[Dre88℄ A. Dressler, The Supergalati Plane Redshift Survey - A Candidate for the Great Attrator,
Astrophys.J.329(1988),519526.
[DS02℄ SottDodelsonandEwanStewart,Saledependentspetralindexinslowrollination,Phys.Rev.
D65(2002),101301.
[DZS78℄ A.G.Doroshkevih,I.B.Zeldovih,andR.A.Siuniaev,FlutuationsoftheMirowaveBakground
RadiationintheAdiabatiandEntropiTheoriesofGalaxyFormation,AstronomiheskiiZhurnal
55(1978),913921.
[EBGL04℄ HansKristianEriksen,A.J.Banday,K.M.Gorski, andP.B.Lilje,Foreground Removalby an
Internal Linear CombinationMethod: Limitations and Impliations, Astrophys. J.612 (2004),
633646,astro-ph/0403098.
[EHB
+
04℄ H.K.Eriksen,F.K.Hansen,A.J.Banday,K.M.Górski,andP.B.Lilje,Asymmetriesin the
CosmiMirowaveBakgroundAnisotropyField,Astrophys.J.605(2004),1420.
[Ein17℄ AlbertEinstein,Kosmologishe Betrahtungen zur AllgemeinenRelativitätstheorie,Sitzungsber.
Preuss.Akad.Wiss.Berlin(Math.Phys.)1917(1917),142152.
[EM07℄ Kari Enqvist and Teppo Mattsson,The Eet of Inhomogeneous Expansionon the Supernova
Observations,JCAP0702(2007),019,astro-ph/0609120.
[Enq07℄ KariEnqvist,Lemaître-Tolman-Bondi Modeland AeleratingExpansion,2007,arXiv:0709.2044
[astro-ph℄.
[ER02℄ Roberto Emparan and Harvey S. Reall, Generalized Weyl Solutions, Phys. Rev. D65 (2002),
084025,hep-th/0110258.
[ES79℄ D. M.Eardleyand L.Smarr, Timefuntions inNumerialRelativity: MarginallyBound Dust
Collapse,Phys.Rev.D19(1979),22392259.
[ETJ
+
97℄ M.Einasto,E.Tago, J.Jaaniste,J.Einasto,andH.Andernah,TheSuperluster-VoidNetwork
I.TheSuperlusterCatalogueand Large-SaleDistribution,Astron.Astrophys.Suppl.Ser.123
(1997),119133,astro-ph/9610088.
[EvE98℄ GeorgeF.R. Ellisand HenkvanElst, Cosmologialmodels Cargese Letures 1998,1998,
gr-q/9812046.
[EvEM01℄ GeorgeF.R.Ellis,Henkvan Elst,andRoyMaartens, GeneralRelativisti AnalysisofPeuliar
Veloities,Class.Quant.Grav.18(2001),51155124,gr-q/0105083.
[FBNP
+
06℄ YasushiFukazawa,J.G.Betoya-Nonesa,J.Pu,A.Ohto,andN.Kawano, SalingMass Proles
AroundElliptialGalaxiesObservedwithChandraandXMM-Newton,Astrophys.J.636(2006),
698,astro-ph/0509521.
[FGM
+
06℄ PeterE.Freeman,C.R.Genovese,C.J.Miller,R.C.Nihol,andL.Wasserman,Examiningthe
EetoftheMap-MakingAlgorithmonObservedPowerAsymmetryinWMAPData,Astrophys.
J.638(2006),1,astro-ph/0510406.
[FI86℄ J.E.FeltenandR.Isaaman,SaleFatorsR(t)andCritialValuesoftheCosmologialConstant
Λ
inFriedmannUniverses,ReviewsofModernPhysis58(1986),689698.[Fis07℄ AndréFisher,UntersuhungderkosmishenMikrowellenstrahlungmitHilfeMaxwellsher
Mul-tipolvektoren. Diplom thesis, Bielefeld University, 2007, Available e.g. at http://www.physik.
uni-bielefeld.de/osmolog y/th eses .ht ml.
[Fri05℄ PrisillaC.Frish,TentativeIdentiationofInterstellarDustinHeliosphereNose,Astrophys.J.
632(2005),L143L146,astro-ph/0506293.
[FRV04℄ FranesFerrer,Syksy Rasanen,andJussiValiviita,Correlated IsourvaturePerturbationsfrom
MixedInaton-CurvatonDeay,JCAP0410(2004),010,astro-ph/0407300.
[FS07℄ J.R.FergussonandEdwardP.S.Shellard,Primordialnon-GaussianityandtheCMBBispetrum,
Phys.Rev.D76(2007),083523,astro-ph/0612713.
[FSA94℄ M.J.Fullana,D.Saez,andJ.V.Arnau,OntheMirowave Bakground AnisotropyProduedby
GreatAttrator-likeStrutures,Astrophys.J.Suppl.94(1994),116.
[FSSB01℄ P.Fouqué,J.M.Solanes,T.Sanhis,andC.Balkowski,Struture,MassandDistaneoftheVirgo
ClusterfromaTolman-Bondi Model,Astron.Astrophys.375(2001),770780,astro-ph/0106261.
[G
+
05℄ J.RihardIIIGottetal.,AMapoftheUniverse,Astrophys.J.624(2005),463,astro-ph/0310571.
[Gar06a℄ David Garnkle, Inhomogeneous Spaetimes as a Dark Energy Model, Class. Quant. Grav. 23
(2006),48114818,gr-q/0605088.
[Gar06b℄ , The Need for Dark Matter in Galaxies, Class. Quant. Grav. 23 (2006), 1391,
gr-q/0511082.
[GCP06℄ A. E. Gumrukuoglu, Carlo R. Contaldi, and Maro Peloso, CMB Anomalies from Reli
Anisotropy,2006,astro-ph/0608405.
[Gfr℄ Gfroerer,TimothyH.,personalhomepageofathttp://webphysis.davidso n.ed u/f aul ty/ thg/ ,
CopyrightduetoBrooks/Cole-Thomson.
[GH04℄ Christopher Gordon and Wayne Hu, ALow CMBQuadrupole from DarkEnergy Isourvature
Perturbations,Phys.Rev.D70(2004),083003,astro-ph/0406496.
[GHHC05℄ ChristopherGordon,WayneHu,DraganHuterer,andThomasM.Crawford,SpontaneousIsotropy
Breaking: AMehanismforCMBMultipoleAlignments,Phys.Rev.D72(2005),103002,
astro-ph/0509301.
[GHS07℄ TuhinGhosh,AmirHajian,andTarunSouradeep,UnveilingHiddenPatternsinCMBAnisotropy
Maps,Phys.Rev.D75(2007),083007,astro-ph/0604279.
[GHW90℄ H.P.Gush,M.Halpern,and E.H.Wishnow,RoketMeasurement ofthe
Cosmi-Bakground-Radiationmm-WaveSpetrum,Phys.Rev.Lett.65(1990),537540.
[H
+
03℄ G.Hinshawet al., First Year Wilkinson Mirowave Anisotropy Probe (WMAP) Observations:
AngularPowerSpetrum,Astrophys.J.Suppl.148(2003),135,astro-ph/0302217.
[H
+
07℄ ,Three-YearWilkinsonMirowaveAnisotropyProbe(WMAP)Observations:Temperature
Analysis,Astrophys.J.Suppl.170(2007),288,astro-ph/0603451.
[Haj07℄ Amir Hajian, Analysis of the Apparent Lak of Power in the Cosmi Mirowave Bakground
AnisotropyatLargeAngularSales,2007,astro-ph/0702723.
[HBB
+
96℄ G.Hinshaw, A. J.Branday, C.L.Bennett, K.M. Gorski,A. Kogut, C.H. Lineweaver, G.F.
Smoot, and E. L. Wright, Two-Point Correlations in the COBE DMR Four-Year Anisotropy
Maps,Astrophys.J.Lett.464(1996),L25,astro-ph/9601061.
[HBM
+
05℄ FrodeK.Hansen,E.Branhini,P.Mazzotta,P.Cabella,andK.Dolag,AFull-SkyPreditionof
theSZEet fromDiuseHot GasintheLoalUniverseandtheupperLimitfromtheWMAP
Data,Mon.Not.Roy.Astron.So.361(2005),753762,astro-ph/0502227.
[HEB
+
05℄ DavidW.Hogg,DanielJ.Eisenstein,MihaelR.Blanton,NetaA.Bahall,J.Brinkmann,JamesE.
Gunn,andDonaldP.Shneider,CosmiHomogeneityDemonstratedwithLuminousRedGalaxies,
Astrophys.J.624(2005),5458.
[HES℄ TeamHESE,Oial siteof theHigh Energy Spae EnvironmentBranh http://heseweb.nrl.
navy.mil/gamma/.
[HMM97℄ NeilP.Humphreys,RoyMaartens,andDavidR.Matravers,AnisotropiObservationsinUniverses
withNonlinearInhomogeneity,Astrophys.J.477(1997),47,astro-ph/9602033.
[HN99℄ Jai-han HwangandHyerimNoh, TheSahs-Wolfe Eet: GaugeIndependeneand a General
Expression,Phys.Rev.D59(1999),067302,astro-ph/9812007.
[Hog00℄ DavidW.Hogg,DistaneMeasuresinCosmology,2000,astro-ph/9905116.
[HPLN02℄ J.Hwang,T.Padmanabhan,O.Lahav,andH.Noh,Onthe1/3FatorintheCMBSahs-Wolfe
Eet,Phys.Rev.D65(2002),043005,astro-ph/0107307.
[HS95℄ WayneHuandNaoshiSugiyama,Toward UnderstandingCMBAnisotropiesand Their
Implia-tions,Phys.Rev.D51(1995),25992630,astro-ph/9411008.
[HS04℄ PaulHuntandSubirSarkar,MultipleInationandtheWMAP`Glithes',Phys.Rev.D70(2004),
103518,astro-ph/0408138.
[HS07℄ ,MultipleInationandtheWMAP`Glithes'II.DataAnalysisandCosmologial
Param-eterExtration,2007,arXiv:0706.2443[astro-ph℄.
[HSLB04℄ MihaelJ.Hudson,RussellJ.Smith,JohnR.Luey,andEnzoBranhini,StreamingMotionsof
Galaxy Clusters Within12000 km/s -V. ThePeuliar VeloityField, Mon.Not. Roy.Astron.
So.352(2004),61,astro-ph/0404386.
[HST℄ TeamHST,OialsiteoftheHubbleSpaeTelesopeathttp://hubblesite.org/.
[HTET01℄ M.O.Hanski,G.Theureau,T.Ekholm,andP.Teerikorpi,KinematisoftheLoalUniverse.IX.
ThePerseus-Pises Superlusterand the Tolman-Bondi Model, Astron.Astrophys.378 (2001),
345360,astro-ph/0109080.
[Hub29℄ EdwinHubble,ARelationBetweenDistaneandRadialVeloityAmongExtraGalatiNebulae,
Pro.Nat.Aad.Si.15(1929),168173.
[HW04℄ Stefan Hofmann and Oliver Winkler, The Spetrum of Flutuations in Inationary Quantum
Cosmology,2004,astro-ph/0411124.
[IAB
+
03℄ E. Iodie, M.Arnaboldi, F.Bournaud, F.Combes, L.S.Sparke, W.van Driel, andM.
Capa-ioli,Polar RingGalaxiesandtheTullyFisher Relation: ImpliationsfortheDarkHaloShape,
Astrophys.J.585(2003),730.
[INN02℄ H.Iguhi,T.Nakamura,andK.Nakao,IsDarkEnergytheOnlySolutiontotheApparent
Ael-erationofthePresentUniverse?,Prog.Theor.Phys.108(2002),809818,astro-ph/0112419.
[IRWG07℄ Mustapha Ishak, James Rihardson, Delilah Whittington, and David Garred, DarkEnergy or
Apparent Aeleration Due to a Relativisti Cosmologial Model More Complex than FLRW?,
2007,arXiv:0708.2943[astro-ph℄.
[IS06℄ KaikiTaroInoue and JosephSilk, Loal Voids astheOrigin of Large-angle Cosmi Mirowave
BakgroundAnomalies,Astrophys.J.648(2006),2330,astro-ph/0602478.
[IS07℄ ,LoalVoidsastheOriginofLarge-angleCosmiMirowaveBakgroundAnomalies: The
EetofaCosmologialConstant,Astrophys.J.664(2007),650659,astro-ph/0612347.
[Isl85℄ JamalN. Islam,RotatingFields inGeneralRelativity, Cambridge UniversityPress,Cambridge,
1985.
[J
+
07a℄ N. Jarosik et al., Three-Year Wilkinson Mirowave Anisotropy Probe (WMAP) Observations:
BeamProles,DataProessing,Radiometer Charaterizationand SystematiErrorLimits,
As-trophys.J.Suppl.170(2007),263,astro-ph/0603452.
[J
+
07b℄ MyungkookJamesJeeet al.,Disoveryof a RinglikeDarkMatterStrutureintheCoreof the
GalaxyClusterCl0024+17,2007,arXiv:0705.2171[astro-ph℄.
[JBE
+
06℄ T.R.Jae, A.J.Banday,H.K.Eriksen,K.M.Gorski,and F.K.Hansen, BianhiType VII
h
ModelsandtheWMAP 3-yearData,2006,astro-ph/0606046.
[JW85℄ B.J.T.JonesandR.F.G.Wyse,TheIonisationofthePrimevalPlasmaattheTimeof
Reom-bination,Astr.Astrophys.149(1985),144150.
[Kan69℄ R.Kantowski,TheComaCluster asa SpherialInhomogeneityinRelativistiDust,Astrophys.
J.155(1969),1023.
[KE06℄ Dale D. Koevski and HaraldEbeling, On The Origin of the Loal Group's Peuliar Veloity,
Astrophys.J.645(2006),10431053,astro-ph/0510106.
[Ker63℄ G.D.Kerr,GravitationalFieldofaSpinningMassasanExampleofAlgebraiallySpeialMetris,
Phys.Rev.Lett.11(1963),237.
[KH02℄ AndrzejKrasi«skiandCharlesHellaby,StrutureFormationintheLemaître-TolmanModel,Phys.
Rev.D65(2002),023501.
[KH04a℄ ,FormationofaGalaxy withaCentralBlakHoleintheLemaître-TolmanModel,Phys.
Rev.D69(2004),043502.
[KH04b℄ ,MoreExamplesofStrutureFormationintheLemaître-TolmanModel,Phys.Rev.D69
(2004),023502.
[KH05℄ ,StrutureFormationinthe Lemaître-Tolman CosmologialModel(ANon-Perturbative
Approah), in: Topisin MathematialPhysis,GeneralRelativity andCosmology.Proeedings
ofaSymposiumontheOassionofthe75thBirthdayofPleba«ski,Mexio,2005.
[KH06℄ ,AlternativeMethodsofDesribing StrutureFormationin theLemaître-TolmanModel,
Phys.Rev.D73(2006),023518.
[KKN
+
07℄ TomohiroKai,HiroshiKozaki,Ken-ihiNakao,YasusadaNambu,andChul-MoonYoo,Can
Inho-mogenetiesAeleratetheCosmi VolumeExpansion?,Prog.Theor.Phys.117(2007),229240,
gr-q/0605120.
[KKZ97℄ Hans-VolkerKlapdor-KleingrothausandKaiZuber,Teilhenastrophysik,B.G.Teubner,Stuttgart,
1997.
[KLS
+
93℄ A.Kogut,C.Lineweaver,G.F.Smoot,C.L.Bennett,A.Banday,N.W.Boggess,E.S.Cheng,
G.deAmii,D.J.Fixsen,G.Hinshaw,P.D.Jakson,P.Janssen,M.andKeegstra,K.Loewenstein,
P.Lubin,J.C.Mather,L.Tenorio,R.Weiss,D.T.Wilkinson,andE.L.Wright,DipoleAnisotropy
intheCOBEDierentialMirowaveRadiometersFirst-YearSkyMaps,Astrophys.J.419(1993),
1,astro-ph/9312056.
[KM06℄ Tomi Koivisto and David F.Mota, Dark Energy Anisotropi Stress and Large Sale Struture
[KME04℄ DaleD.Koevski,ChristopherR.Mullis,andHaraldEbeling,TheDipoleAnisotropyoftheFirst
All-SkyX-rayClusterSample,Astrophys.J.608(2004),721730,astro-ph/0403275.
[Kom58℄ ArthurKomar,CovariantConservationLawsinGeneralRelativity,Phys.Rev.113(1958),no.3,
934.
[Kor05℄ MikolajKorzynski, Singular Diskof Matterin theCooperstok and TieuGalaxy Model, 2005,
astro-ph/0508377.
[Kra97℄ AndrzejKrasi«ski,InhomogeneousCosmologialModels,CambridgeUniversityPress,Cambridge,
1997.
[KS07℄ MasahiroKawasakiandToyokazuSekiguhi,CosmologialConstraintsonIsourvatureandTensor
Perturbations,2007,arXiv:0705.2853[astro-ph℄.
[Lem33℄ A.G.Lemaître,L'Universen Expansion, Ann.So. Si.BruxellesA53(1933),51,reprinted in
EnglishwithhistorialommentsinGen.Rel.Grav.29(1997),637.
[Les04℄ Julien Lesgourgues, An Overview of Cosmology, 2004, Leture Notes for the SummerStudents
ProgramofCERN(2002-2004),astro-ph/0409426.
[Lew32℄ T. Lewis, Some Speial Solutions of the Equations of Axially Symmetri Gravitational Fields,
Pro.Roy.So.Lond.A136(1932),176.
[LFB
+
88℄ D.Lynden-Bell,S.M.Faber,D.Burstein,R.L.Davies,A.Dressler,R.J.Terlevih,andG.
Weg-ner, Spetrosopy and Photometryof ElliptialGalaxies. V-Galaxy Streaming toward thenew
SupergalatiCenter,Astrophys.J.326(1988),1949.
[Lid04℄ ChrisLidman,ObservingDistantTypeIaSupernovaewiththeESOVLT,TheEuropean
Organi-sationforAstronomialResearhintheSouthernHemisphereMessenger118(2004),24.
[LM05℄ Kate Land and Joao Magueijo, The Axis of Evil, Phys. Rev. Lett. 95 (2005), 071301,
astro-ph/0502237.
[LM07℄ , The Axis of Evil Revisited, Mon.Not. Roy. Astron. So. 378(2007), 153158,
astro-ph/0611518.
[Lon98℄ Malom S. Longair, Galaxy Formation, Astronomyand Astrophysis Library, Springer, Berlin
HeidelbergNewYork,1998.
[Lon07℄ MihaelJ.Longo,DoestheUniverseHaveaHandedness,2007,astro-ph/0703325.
[LP96℄ David Langloisand TsviPiran, DipoleAnisotropy from anEntropy Gradient, Phys. Rev. D53
(1996),29082919,astro-ph/9507094.
[LRSH04℄ John Luey, David Radburn-Smith, and Mike Hudson, Beta, Loal SNIa Data and the Great
Attrator,2004,Appearinginthe ProeedingsoftheMeetingonNearbyLargeSaleStrutures
andtheZoneofAvoidane,CapeTown,SouthAfria,28Mar-2Apr2004,astro-ph/0412329.
[LS07℄ NanLiand DominikJ.Shwarz, Onthe Onsetof CosmologialBakreation,Phys. Rev. D76
(2007),083011,gr-q/0702043.
[LSS℄ Team LSST, Site of the proposed Large Synopti Survey Telesope at http://www.lsst.org/
lsst_home.shtml.
[LWR
+
03℄ J.P.Luminet,J.Weeks,A.Riazuelo,R.Lehouq,andJ.P.Uzan,DodeahedralSpaeTopology
as an Explanation for Weak Wide-Angle Temperature Correlations in the Cosmi Mirowave
Bakground,Nature.425(2003),593,astro-ph/0310253.
[M
91℄ AttilaMészáros,OnShellCrossingintheTolmanMetri,Mon.Not.Roy.Astron.So.253(1991),
619624.
[M
+
04℄ MaximMarkevithet al.,DiretConstraints ontheDarkMatterSelf-Interation Cross-Setion
fromtheMergingCluster1E0657-56,Astrophys.J.606(2004),819824,astro-ph/0309303.
[Maa98℄ RoyMaartens, Covariant Veloityand DensityPerturbationsin Quasi-Newtonian Cosmologies,
Phys.Rev.D58(1998),124006,astro-ph/9808235.
[Man05℄ RezaMansouri,Strutured FRWUniverse leads toAeleration: ANon-PerturbativeApproah,
2005,astro-ph/0512605.
[Mas05℄ KarenL.Masters,Cosmology intheVeryLoalUniverse-WhyFlowModelsMatter,2005,
Ap-pearingintheProeedingsofthe22ndTexasSymposiumonRelativistiAstrophysisatStanford
University,Stanford,California,13-17De2004,astro-ph/0503271.
[Max79℄ JamesC.Maxwell,ATreatiseonElitriityandMagnetism-VolumeI,DoverPubliationsIn.,
NewYork,1979.
[MCC
+
94℄ J.C.Mather,E.S.Cheng,D.A.Cottingham,R.E.Eplee,Jr.,D.J.Fixsen,T.Hewagama,R.B.
Isaaman, K.A.Jensen,S.S.Meyer,P.D.Noerdlinger, S.M.Read,L.P.Rosen,R.A.Shafer,
E.L.Wright, C.L.Bennett,N.W.Boggess,M.G.Hauser,T.Kelsall,S.H.Moseley,Jr.,R.F.
Silverberg,G.F.Smoot,R.Weiss,andD.T.Wilkinson,MeasurementoftheCosmiMirowave
BakgroundSpetrumbytheCOBEFIRASInstrument,Astrophys.J.420(1994),439444.
[MDW
+
07℄ M.Maturi,K.Dolag,A.Waelkens,V.Springel,andT.Ensslin,TheAtualRees-SiamaEet
fromtheLoalUniverse,2007,arXiv:0708.1881[astro-ph℄.
[Mes63℄ LeonMestel,OntheGalatiLawofRotation,Mon.Not.Roy.Astron.So.126(1963),553.