Tsujikawa, Phys. Rev. D 77, 023507 (2008)
Tsujikawa, Phys. Rev. D 77, 023507 (2008) Tsujikawa, Phys. Rev. D 77, 023507 (2008)
Recent work >No. B-3[Martinelli, Melchiorri and Amendola, Phys. Rev. D 79, 123516 (2009)]Cf. [Nozari and Azizi, Phys. Lett. B 680, 205 (2009)]・It has been shown that in the Hu-Sawicki model, the transitionfrom the phantom phase to the non-phamtom one can also occur.From [Martinelli,Melchiorri andAmendola, Phys. Rev.D 79, 123516 (2009)]n =1F 0 (R 0 )=à 0.01F 0 (R 0 )=à 0.03F 0 (R 0 )=à 0.1Ω m =0.24
We reconstruct an explicit model of F(R) gravitywith realizing the crossing of the phantom divide.No. B-4< Preceding work >From [Amendola and Tsujikawa,Phys. Lett. B 660, 125 (2008)]F(R)=(R 1/c à Λ) c・ Example:c, Λ : Constantsc =1.8Phantom phaseNon-phantom phase
- Page 66 and 67: Conclusions of Sec. IV >No. 64・
- Page 68 and 69: ・We assume the flat FLRW space-ti
- Page 70 and 71: No. 45p =0.001p =0.01p = à 0.1p =0
- Page 72 and 73: (b). Logarithmic f(T) theory >No. 4
- Page 74 and 75: The best-fit values >No. 42The mini
- Page 76 and 77: (4) Solar system constraintsf(R) gr
- Page 78 and 79: (4) Stability of the late-time de S
- Page 80 and 81: Data fitting of w(z) (3) >No. B-7Fr
- Page 82 and 83: Bekenstein-Hawking entropy on the a
- Page 84 and 85: Hu-Sawicki modelStarobinsky’s mod
- Page 86 and 87: (a). Exponential f(T) theory >No. 1
- Page 88 and 89: (c). Combined f(T) theory >No. 16
- Page 90 and 91: p : Constantú Mand P M : Energy de
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- Page 94 and 95: ・It is known that the finite-time
- Page 96 and 97: Other models >No. A-10・Appleby-Ba
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- Page 100 and 101: Cosmological evolutions of , and in
- Page 102 and 103: Initial conditions >Models of (i),
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- Page 108 and 109: Second law of thermodynamics >[KB a
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- Page 112 and 113: 5-year WMAP data on >・ For the fl
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- Page 118: (5) Existence of a matter-dominated
Recent work >No. B-3[Martinelli, Melchiorri and Amendola, <strong>Phys</strong>. <strong>Rev</strong>. D 79, 123516 (2009)]Cf. [Nozari and Azizi, <strong>Phys</strong>. Lett. B 680, 205 (2009)]・It has been shown that in the Hu-Sawicki model, the transitionfrom the phantom phase to the non-phamtom one can also occur.From [Martinelli,Melchiorri andAmendola, <strong>Phys</strong>. <strong>Rev</strong>.D 79, 123516 (2009)]n =1F 0 (R 0 )=à 0.01F 0 (R 0 )=à 0.03F 0 (R 0 )=à 0.1Ω m =0.24
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