Cosmology of the Nambu-Jona-Lasinio Model
- 1 Instituto de Fisica, Universidad Nacional Autonoma de Mexico, A.P. 20-364, 01000, Mexico D.F., Mexico
- 2 Instituto de Fisica, Universidad Nacional Autonoma de Mexico, A.P. 20-364, 01000, Mexico D.F., Mexico
Abstract
We review the Nambu and Jona-Lasinio model (NJL), proposed long time ago, in the sixties, as a fermion interaction theory with chiral symmetry. The theory is not renormalizable and presents a symmetry breaking due to quantum effects which depends on the strength of the coupling constant. We may associate a phase transition with this symmetry breaking, leading from fermion states to a fermion condensate which can be described effectively by a scalar field. Our purpose in this paper is to exploit the interesting properties of NJL in a different context other than particle physics by studying its cosmological dynamics. We are interested in finding whether possibly the NJL model could be used to describe the still unknown dark energy and/or dark matter, from up to 95% of the energy content of the universe at present time.
- Perlmutter, S., et al. (1999) Astrophysical Journal, 517, 565-586. http://dx.doi.org/10.1086/307221
- Riess, A.G., et al. (1998) Astronomical Journal, 116, 1009-1038. http://dx.doi.org/10.1086/300499
- Amanullah, R., et al. (2010) Astrophysical Journal, 716, 712-738. http://dx.doi.org/10.1088/0004-637X/716/1/712
- Carlos, C., et al. (2010) Astronomical Journal, 139, 519-539. http://dx.doi.org/10.1088/0004-6256/139/2/519
- Hicken, M., et al. (2009) Astrophysical Journal, 700, 331-357. http://dx.doi.org/10.1088/0004-637X/700/1/331
- Riess, A.G., et al. (2007) Astrophysical Journal, 659, 98-121. http://dx.doi.org/10.1086/510378
- Sakharov, A.D. (1966) Soviet Physics—JETP, 22, 241.
- Peebles, P.J.E. and Yu, J.T. (1970) Astrophysical Journal, 162, 815-836. http://dx.doi.org/10.1086/150713
- Sunyaev, R.A., et al. (1970) Astrophysics and Space Science, 7, 3-19.
- Blake, C. and Glazebrook, K. (2003) Astrophysical Journal, 594, 665-673. http://dx.doi.org/10.1086/376983
- Bennett, C.L., et al. (2013) Astrophysical Journal Supplement, 208, 20. http://dx.doi.org/10.1088/0067-0049/208/2/20
- Ade, P.A.R., et al. (2015) arXiv:1502.01589.
- Reid, B.A., Chengalur, J.N., Begum, A. and Karachentsev, I.D. (2010) Monthly Notices of the Royal Astronomical Society, 404, L60-L63. http://dx.doi.org/10.1111/j.1745-3933.2010.00835.x
- Percival, W.J., et al. (2001) Monthly Notices of the Royal Astronomical Society, 327, 1297-1306. http://dx.doi.org/10.1046/j.1365-8711.2001.04827.x
- Tegmark, M., et al. (2001) Monthly Notices of the Royal Astronomical Society, 328, 1039-1063. http://dx.doi.org/10.1046/j.1365-8711.2001.04902.x
- Padmanabhan, N., et al. (2012) Monthly Notices of the Royal Astronomical Society, 427, 2132-2145. http://dx.doi.org/10.1111/j.1365-2966.2012.21888.x
- Anderson, L., et al. (2014) Monthly Notices of the Royal Astronomical Society, 441, 24-62. http://dx.doi.org/10.1093/mnras/stu523
- Eisenstein, D.J., et al. (2005) Astrophysical Journal, 633, 560-574. http://dx.doi.org/10.1086/466512
- Tojeiro, R., et al. (2014) Monthly Notices of the Royal Astronomical Society, 440, 2222-2237. http://dx.doi.org/10.1093/mnras/stu371