Eos of Dark Energy ae=-1-+ 3 3d a 3 Epoch: Inflation Radiation Matter Today 1 wde CHDE is a single parameter (d)model like ACDM ode d a 29d (1-92)3(1+wm)+8
EoS of Dark Energy Epoch: Inflation Radiation Matter Today < CHDE is a single parameter (d) model like
More General Analysis Friedman Equation 3M2H2=pm+p+pm+9,+2t=1 Pm=Pmoa 8=Qm03M2H Pr= Proa 4=93MH2a 092||92m=(1-9d atre Ha h 0v2m0 +r0/a de Equation of motion for CHDE a+r dode @de d 1-g2(1+ma-2y2 I+ro/a d a d- 0 a de 9+ 4 1+r 0
More General Analysis Equation of motion for CHDE Friedman Equation
Interaction With Background Pm+3HPn(1+wm)=Q pde + 3Hpde(l + wde)=-Q General Equation of motion for CHDE 1-92)|3(wm+1)+8 2 video 3M2H EoS for Dark energy 8 2 vide 0 wde 33d 3H pde
Interaction With Background General Equation of motion for CHDE EoS for Dark energy
Holographic Dark Energy Characterized by Total Comoving Horizon(nHDE) Z P Huang ylw, arXiv: 1202.2590
Holographic Dark Energy Characterized by Total Comoving Horizon (ηHDE) Z.P. Huang, YLW, arXiv:1202.2590
Holographic Dark Energy Characterized by Total Comoving Horizon(nHDE) Total comoving horizon of the universe da 1 a(t' 0 i'h'a' Characteristic Length Scale L of Universe from Causality L Ch>I h Energy density of holographic dark energy Pde 3d2M2L-2=3(Cnd)MEn Rescaled independent parameter Fractional DE Density cd\3MF=Bn回>1 when ch pde
Holographic Dark Energy Characterized by Total Comoving Horizon (ηHDE) Total comoving horizon of the universe Characteristic Length Scale L of Universe from Causality Energy density of holographic dark energy Rescaled independent parameter & Fractional DE Density