Diego Saez-Gomez
Diego Saez-Gomez Diego Saez-Gomez
Index Friedmann-Lemaître-Robertson-Walker (FLRW) cosmologies in F(R) gravity The cosmological evolution in viable F(R) gravities, and their scalar-tensor counterpart. Future singularities and Little Rip. Testing F(R) gravity with SNe Ia data: a simple model F(R,T) gravity and cosmological perturbations
Brief Article The Author April 6, 2012 FLRW cosmologies 1 w>−1, quintessence fluid , w = −1, cosmological constant , Cosmological Principle: assumes that the Universe is the same in every point (at large scales), what from w
- Page 1: Cosmological constraints on modifie
- Page 5 and 6: FLRW cosmologies 12 3 No Big Bang (
- Page 7 and 8: FLRW cosmologies Future singulariti
- Page 9 and 10: Viable f(r) gravity Viability condi
- Page 11 and 12: 3 Cosmological evolution in viable
- Page 13 and 14: Cosmological evolution in viable f(
- Page 15 and 16: Cosmological evolution in viable f(
- Page 17 and 18: 8 − 3H 2 − 2Ḣ = 1 κ 2 p m +
- Page 19 and 20: (z = 0) = H 0 = 100 hkms −1 Mpc
- Page 21 and 22: (z = 0) = H 0 = 100 hkms −1 Mpc
- Page 23 and 24: effective repulsive force 12h R ∼
- Page 25 and 26: Testing F(R) gravity with Sne Ia da
- Page 27 and 28: Testing F(R) gravity with Sne Ia da
- Page 29 and 30: ere right lethand us remind side (r
- Page 31 and 32: e previous section, we study two pa
- Page 33 and 34: en at redshift z = 1000 where δ is
Brief Article<br />
The Author<br />
April 6, 2012<br />
FLRW cosmologies<br />
1<br />
w>−1, quintessence fluid ,<br />
w = −1, cosmological constant ,<br />
Cosmological Principle: assumes that the Universe is the same in every point (at large<br />
scales), what from w
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