Built on

S. D. Odintsov and V. K. Oikonomou, Phys. Rev. D 99
Original
1901
Earlier work this paper cites.
A. Caputo, arXiv:1902.02666 [hep-ph]
Original
1902
Earlier work this paper cites.
A. Caputo, L. Sberna, M. Frias, D. Blas, P. Pani, L. Shao and W. Yan, Phys. Rev. D 100
Original
1902
Earlier work this paper cites.
M. Cicoli, V. Guidetti and F. G. Pedro, arXiv:1903.01497 [hep-th]
Original
1903
Earlier work this paper cites.
H. Fukunaga, N. Kitajima and Y. Urakawa, arXiv:1903.02119 [astro-ph.CO]
Original
1903
Earlier work this paper cites.
D. Croon, R. Houtz and V. Sanz, JHEP 1907
Original
1904
Earlier work this paper cites.
F. V. Day and J. I. McDonald, JCAP 1910
Original
1904
Earlier work this paper cites.
M. Rozner, E. Grishin, Y. B. Ginat, A. P. Igoshev and V. Desjacques, arXiv:1904.01958 [gr-qc]
Original
1904
Earlier work this paper cites.
M. Lawson, A. J. Millar, M. Pancaldi, E. Vitagliano and F. Wilczek, arXiv:1904.11872 [hep-ph]
Original
1904
Earlier work this paper cites.
S. D. Odintsov and V. K. Oikonomou, Phys. Rev. D 99
Original
1905
Earlier work this paper cites.
G. Y. Huang and S. Zhou, Phys. Rev. D 100
Original
1905
Earlier work this paper cites.
T. Tenkanen and L. Visinelli, JCAP 1908
Original
1906
Earlier work this paper cites.
S. Nojiri, S. D. Odintsov and V. K. Oikonomou, arXiv:1907.01625 [gr-qc]
Original
1907
Earlier work this paper cites.
S. Nojiri, S. D. Odintsov, V. K. Oikonomou and A. A. Popov, Phys. Rev. D 100
Original
1909
Earlier work this paper cites.
E. Masaki, A. Aoki and J. Soda, arXiv:1909.11470 [hep-ph]
Original
1909
Earlier work this paper cites.
A. Arvanitaki, S. Dimopoulos, M. Galanis, L. Lehner, J. O. Thompson and K. Van Tilburg, arXiv:1909.11665 [astro-ph.CO]
Original
1909
Earlier work this paper cites.
D. Guerra, C. F. B. Macedo and P. Pani, JCAP 1909
Original
1909
Earlier work this paper cites.
M. Benetti and S. Capozziello, arXiv:1910.09975 [astro-ph.CO]
Original
1910
Earlier work this paper cites.
M. Kavic, S. L. Liebling, M. Lippert and J. H. Simonetti, arXiv:1910.06977 [astro-ph.HE]
Original
1910
Earlier work this paper cites.
D. Blas, A. Caputo, M. M. Ivanov and L. Sberna, arXiv:1910.06128 [hep-ph]
Original
1910
Earlier work this paper cites.
A. Korochkin, A. Neronov and D. Semikoz, arXiv:1911.13291 [hep-ph]
Original
1911
Earlier work this paper cites.
C. F. Chang and Y. Cui, arXiv:1911.11885 [hep-ph]
Original
1911
Earlier work this paper cites.
N. Crisosto, G. Rybka, P. Sikivie, N. S. Sullivan, D. B. Tanner and J. Yang, arXiv:1911.05772 [astro-ph.CO]
Original
1911
Earlier work this paper cites.
K. Choi, H. Seong and S. Yun, arXiv:1911.00532 [hep-ph]
Original
1911
Earlier work this paper cites.
C. S. Machado, W. Ratzinger, P. Schwaller and B. A. Stefanek, arXiv:1912.01007 [hep-ph]
Original
1912
Earlier work this paper cites.
S. Nojiri and S. D. Odintsov, Phys. Lett. B 657
Original
1941
Earlier work this paper cites.
A. D. Linde, Phys. Lett. B 259
1991
Earlier work this paper cites.
A. G. Riess et al
1998
Earlier work this paper cites.
A.S.Sakharov and M.Yu.Khlopov, Yadernaya Fizika (1994) V. 57, PP. 514- 516. ( Phys.Atom.Nucl. (1994) V. 57, PP. 485-487); A.S.Sakharov, D.D.Sokoloff and M.Yu.Khlopov, Yadernaya Fizika (1996) V. 59, PP. 1050-1055. (Phys.Atom.Nucl. (1996) V. 59, PP. 1005-1010); M .Yu.Khlopov, A.S.Sakharov and D.D.Sokoloff, Nucl.Phys. B (Proc. Suppl.) (1999) V. 72, 105-109
1999
Earlier work this paper cites.
K. Choi, J. c. Hwang and K. W. Hwang, Phys. Rev. D 61
2000
Earlier work this paper cites.
M. Kamionkowski and A. H. Jaffe, Int. J. Mod. Phys. A 16S1A
2001
Earlier work this paper cites.

Similar

S. Capozziello, Int. J. Mod. Phys. D 11
2002
Cited alongside, same era.
S. Nojiri and S. D. Odintsov, Phys. Rev. D 68
2003
Cited alongside, same era.
V. Sahni, T. D. Saini, A. A. Starobinsky and U. Alam, JETP Lett. 77
2003
Cited alongside, same era.
S. M. Carroll, V. Duvvuri, M. Trodden and M. S. Turner, Phys. Rev. D 70
2004
Cited alongside, same era.
M. Dine and A. Anisimov, JCAP 0507
2005
Cited alongside, same era.
S. Nojiri and S. D. Odintsov, Phys. Rev. D 74
2006
Cited alongside, same era.
S. Nojiri, S.D. Odintsov, eConf C0602061
2007
Cited alongside, same era.

Then

P. Sikivie, Phys. Rev. Lett. 113
Original
2014
Later among the works it cites.
A. Arvanitaki and A. A. Geraci, Phys. Rev. Lett. 113
Original
2014
Later among the works it cites.
H. Yoshino and H. Kodama, PTEP 2014
Original
2014
Later among the works it cites.
A. B. Balakin, R. K. Muharlyamov and A. E. Zayats, Eur. Phys. J. D 68
Original
2014
Later among the works it cites.
A. Arvanitaki, M. Baryakhtar and X. Huang, Phys. Rev. D 91
Original
2015
Later among the works it cites.

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

Reading the bibliography…

2020

Geometric Inflation and Dark Energy with Axion $F(R)$ Gravity

Odintsov, S. D., Oikonomou, V. K.

Understand

We present a model of $F(R)$ gravity in the presence of a string theory motivated misalignment axion like particle materialized in terms of a canonical scalar field minimally coupled with gravity, and we study the cosmological phenomenology of the model, emphasizing mainly on the late-time era.

The main result of the paper is that inflation and the dark energy era may be realized in a geometric way by an $F(R)$ gravity, while the axion is the dark matter constituent of the Universe.
The $F(R)$ gravity model consists of an $R^2$ term, which as we show dominates the evolution during the early time, thus producing a viable inflationary phenomenology, and a power law term $\sim R^{\delta}$ with $\delta\ll 1 $ and positive, which eventually controls the late-time era.
The axion field remains frozen during the inflationary era, which is an effect known for misalignment axions, but as the Universe expands, the axion starts to oscillate, and its energy density scales eventually as we show, as $\rho_a\sim a^{-3}$.