On coincidence problem and attractor solutions in ELKO dark energy model

S. Weinberg, Rev. Mod. Phys. 61, 1 (1989)

1989

Earlier work this paper cites.

E. J Copeland, A. R. Liddle, and D. Wands Phys. Rev. D 57, 4686 (1998); L. Amendola, Phys. Rev. D 60, 043501 (1999); L. Amendola, C. Quercellini, D. Tocchini-Valentini, and A. Pasqui, Astrophys. J. 583, L53 (2003); M. Alimohammadi and H. M. Sadjadi, Phys. Rev. D 73,083527 (2006)

2006

Earlier work this paper cites.

X. Zhang, H. Li, Y. Piao, and X. Zhang, Mod. Phys. Lett. A 21, 231 (2006); C. G. Boehmer, AnnalenPhys. 16, 325 (2007); Y. Cai and J. Wang, Class. Quant. Grav. 25, 165014 (2008); B. Saha, arXiv:1103.2890v1 [gr-qc]; C. G. Boehmer and J. Burnett, Mod. Phys. Lett. A 25, 101 (2010)

Original

2010

Earlier work this paper cites.

Ch. G. Boehmer, Phys. Rev. D77, 123535 (2008); D. Gredat and S. Shankaranarayanan, JCAP 1001, 008 (2010), arXiv:0807.3336v2 [astro-ph]

Original

2010

Earlier work this paper cites.

C. G. Boehmer and J. Burnett, Mod. Phys. Lett. A 25, 101 (2010), arXiv:0906.1351v1 [gr-qc]

Original

2010

Cited alongside, same era.

P. J. Steinhardt, in Critical Problems in Physics, Eds. V.L. Fitch, D. R. Marlow, and. M. A. E. Dementi, Princeton University Press, 1997; N. Straumann, arXiv:astro-ph/0009386v1; D. T. Valentini, L. Amendola, Phys. Rev. D 65, 063508 (2002); V. Sahni, Lect. NotesPhys. 653, 141 (2004); S. Nojiri and S. D. Odintsov, Gen. Rel. Grav. 38, 1285 (2006); L. Amendola, S. Tsujikawa, and M. Sami, Phys. Lett. B 632, 155 (2006); S. Nojiri and S. D. Odintsov, Phys. Lett. B 637, 139 (2006); H. M. Sadjadi and M. Alimohammadi, Phys. Rev. D 74, 103007 (2006); H. M. Sadjadi and M. Honardoost, Phys. Lett. B 647, 231 (2007); E. V. Linder and R. J. Scherrer, arXiv:0811.2797v1 [astro-ph]; M. Jamil, F. Rahaman and M. Kalam, Eur. Phys. J. C 60, 149 (2009); N. Cruz, S. Lepe, and F. Pena, Phys. Lett. B 699, 135 (2011); Ch. G. Boehmer, G Caldera-Cabral, N. Chan, R. Lazkoz, and R. Maartens, Phys. Rev. D 81, 083003 (2010); Ch. Ahn, Ch. Kim, and E. V. Linder, arXiv:1106.1435v1 [astro-ph.CO]

Original

2010

Cited alongside, same era.

S. Perlmutter et al., Nature (London) 391, 51 (1998); A. G. Riess et al. (Supernova Search Team Collaboration), Astron. J. 116, 1009 (1998); Astron. J. 117, 707 (1999); S. Perlmutter et al. (Supernova Cosmology Project Collaboration), Astrophys. J. 517, 565 (1999); E. V. Linder, arXiv:1009.1411v2 [astro-ph.CO]; E. Elizalde, S. Nojiri, S. D. Odintsov, L. Sebastiani, and S. Zerbini, Phys. Rev. D 83, 086006 (2011); Y. L. Bolotin, O. A. Lemets, and D. A. Yerokhin, arXiv:1108.0203v3 [astro-ph.CO]; A. Barreira and P.P. Avelino, Phys. Rev. D 83, 103001 (2011)

Original

2011

Cited alongside, same era.

D. V. Ahluwalia, and D. Grumiller, JCAP 07 (2005) 012, arXiv:hep-th/0412080v3; D. V. Ahluwalia and D. Grumiller, Phys. Rev. D 72, 0677701 (2005), arXiv:hep-th/0410192v2; D. V. Ahluwalia, Ch. Lee, and D. Schritt, Phys. Lett. B 687, 248 (2010); D. V. Ahluwalia, Ch. Lee, and D. Schritt, Phys. Rev. D 83, 065017 (2011)

2011

Closest in time.

H. Wei, Phys. Lett. B 695, 307 (2011), arXiv:1002.4230v3 [gr-qc]

Original

2011

Closest in time.

Ch. G. Boehmer, J. Burnett, D. F. Mota, and D. J. Shaw, JHEP 07(2010)053, arXiv:1003.3858v2 [hep-th]; L. Fabbri, Phys. Rev. D 85, 047502 (2012); L. Fabbri and S. Vignolo, Annalen Phys. 524, 77 (2012); G. Chee, arXiv:1007.0554v1 [gr-qc]

Original

2012

Closest in time.