holography for cosmology(ppt)(20101013110454060)

holography for cosmology(ppt)(20101013110454060)

ID:14363438

大小:3.47 MB

页数:66页

时间:2018-07-28

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1、IntroductionPartI:HolographicdictionaryPartII:NewholographicmodelsConclusionsHolographyforCosmologyKostasSkenderisInstituteforTheoreticalPhysicsGravitationandAstroParticlePhysicsAmsterdam(GRAPPA)KdVInstituteforMathematicsUniversityofAmsterdamKostasSkenderisHolographicNon-GaussianityIntroductionPartI

2、:HolographicdictionaryPartII:NewholographicmodelsConclusionsGRAPPAAnewinitiativeformedbythreephysicsinstitutes:InstituteforTheoreticalPhysics(ITFA)Affiliatemembers:J.deBoer,E.Verlinde,K.Skenderis,M.Taylor,P.vanderSchaarInstituteforHighEnergyPhysics(IHEF)Affiliatemembers:S.Bentvelsen,E.deWolf,E.Laenen,

3、P.Kooijman,P.deJongAntonPannekoekInstitute(API)forastronomyAffiliatemembers:R.Wijers,A.Watts,M.vanderKlis,S.Markoff,R.WijnandsWearecurrentlysearchingforatleastfournewfacultymembersinseniorandjuniorranks,tenuredortenure-track.KostasSkenderisHolographicNon-GaussianityIntroductionPartI:Holographicdictio

4、naryPartII:NewholographicmodelsConclusionsOutline1Introduction2PartI:HolographicdictionaryCosmologicalPerturbationsThedomain-wall/cosmologycorrespondenceHolography:aprimerCorrelatorsforholographicRGflowsHolographyforcosmology3PartII:Newholographicmodels4ConclusionsKostasSkenderisHolographicNon-Gaussi

5、anityIntroductionPartI:HolographicdictionaryPartII:NewholographicmodelsConclusionsIntroductionOverthelasttwodecades,strikingnewobservationshavetransformedcosmologyfromaqualitativetoaquantitativescience.KostasSkenderisHolographicNon-GaussianityIntroductionPartI:HolographicdictionaryPartII:Newholograp

6、hicmodelsConclusionsCOBE(1989)KostasSkenderisHolographicNon-GaussianityIntroductionPartI:HolographicdictionaryPartII:NewholographicmodelsConclusionsWMAP(2001)KostasSkenderisHolographicNon-GaussianityIntroductionPartI:HolographicdictionaryPartII:NewholographicmodelsConclusionsPlanck(2009)KostasSkende

7、risHolographicNon-GaussianityIntroductionPartI:HolographicdictionaryPartII:NewholographicmodelsConclusionsPrimordialperturbationsTheprimordialperturbationsoffersomeofourbestcluesastothefundamentalphys

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