SCALARTENSOR THEORIES OF GRAVITY AND ITS APPLICATION NTU


















- Slides: 18
SCALAR-TENSOR THEORIES OF GRAVITY AND ITS APPLICATION NTU Physics/CTS Theory Seminar May. 13 th. 2009 Seokcheon (sky) Lee (李碩天) Institute of Physics, Academia Sinica & Le. Cos. PA, National Taiwan University
OUTLINE 2 Observational Evidences of the Accelerating Universe Dark Energy vs. Modified Gravity Scalar-Tensor Theories Background Evolutions and Perturbations (Observables) Summary MAY. 13 TH. 2009 SKY LEE // NTU & CTS
ACCELERATING UNIVERSE 3 Accelerating Universe CMB LSS Clusters Wtotal= 1. 0 Locations of Peaks WM= 0. 3 Power spectra t 0 = 13. 7 Gyr SNe 1 a q 0 < 0 Brightness MAY. 13 TH. 2009 H-value SKY LEE // NTU & CTS
4 B ACKGROUND E VOLUTION Luminosity Distance MAY. 13 TH. 2009 SKY LEE // NTU & CTS
5 DARK ENERGY VS. MODIFIED GRAVITY Bad Management (original background) or Someone was here (source of disturbance)? MAY. 13 TH. 2009 SKY LEE // NTU & CTS
DARK ENERGY VS. MODIFIED GRAVITY 6 Still require Dark Matter in both theories except Te. Ve. S MAY. 13 TH. 2009 SKY LEE // NTU & CTS
DARK ENERGY MODELS I 7 Cosmological constant Quintessence MAY. 13 TH. 2009 SKY LEE // NTU & CTS
DE II : QUARTESSENCE 8 (UNIFICATION OF DM & DE) MAY. 13 TH. 2009 SKY LEE // NTU & CTS
MODIFIED GRAVITY I 10 A broad class of alternative gravity theories Y : matter fields f : a scalar field MAY. 13 TH. 2009 SKY LEE // NTU & CTS
11 MODIFIED GRAVITY II MAY. 13 TH. 2009 SKY LEE // NTU & CTS
SCALAR-TENSOR GRAVITY I 13 MAY. 13 TH. 2009 SKY LEE // NTU & CTS
STG II 14 MAY. 13 TH. 2009 SKY LEE // NTU & CTS
STG III 15 MAY. 13 TH. 2009 SKY LEE // NTU & CTS
STG IV 16 MAY. 13 TH. 2009 SKY LEE // NTU & CTS
PERTURBATION QUANTITIES 21 MAY. 13 TH. 2009 SKY LEE // NTU & CTS
PERTURBATION QUANTITIES (CONTINUED) 22 MAY. 13 TH. 2009 SKY LEE // NTU & CTS
OBSERVABLES 23 MAY. 13 TH. 2009 SKY LEE // NTU & CTS
SUMMARY 24 STG is one of well motivated and known alternative theories of gravity. Accurate measurements for the background evolutions to constraint the parameters of theories. Compare with perturbation observables. Probably we can distinguish the origin of acceleration from both background and perturbation evolutions. MAY. 13 TH. 2009 SKY LEE // NTU & CTS