Closed inflationary universe with tachyonic field. (English) Zbl 1189.83090
Summary: In this article we study closed inflationary universe models by using a tachyonic field theory. We determine and characterize the existence of a universe which has \(\Omega >1\) and which describes a period of inflation. We find that the considered models are less restrictive compared to the standard ones with a scalar field. We use recent astronomical observations to constrain the parameters appearing in the model. The results obtained are compared to those found in the standard scalar field inflationary universes.
MSC:
| 83F05 | Relativistic cosmology |
References:
| [1] | H.V. Peiris et al., Astrophys. J. Suppl. 148, 213 (2003) · doi:10.1086/377228 |
| [2] | WMAP Collaboration, D.N. Spergel et al., Astrophys. J. Suppl. 148, 175 (2003) · doi:10.1086/377226 |
| [3] | L. Page et al., astro-ph/0603449 |
| [4] | C.L. Bennett et al., Astrophys. J. Suppl. 148, 1 (2003) · doi:10.1086/377253 |
| [5] | G. Efstathiou, Mon. Not. R. Astron. Soc. 343, L95 (2003) · doi:10.1046/j.1365-8711.2003.06940.x |
| [6] | C. MacTavish et al., Astrophys. J. 647, 799 (2006) · doi:10.1086/505558 |
| [7] | D. Eisenstein et al., Astrophys. J. 633, 560 (2005) · doi:10.1086/466512 |
| [8] | J.P. Uzan, U. Kirchner, G.F.R. Ellis, Mon. Not. R. Astron. Soc. 344, L65 (2003) · doi:10.1046/j.1365-8711.2003.07043.x |
| [9] | A. Linde, JCAP 0305, 002 (2003) |
| [10] | M. Sasaki, T. Tanaka, K. Yamamoto, J. Yokoyama, Phys. Lett. B 317, 510 (1993) · doi:10.1016/0370-2693(93)91364-S |
| [11] | M. Bucher et al., Phys. Rev. D 52, 3314 (1995) · doi:10.1103/PhysRevD.52.3314 |
| [12] | M. Bucher, N. Turok, Phys. Rev. D 52, 5538 (1995) · doi:10.1103/PhysRevD.52.5538 |
| [13] | A. Linde, Phys. Lett. B 351, 99 (1995) · doi:10.1016/0370-2693(95)00370-Z |
| [14] | A. Linde, A. Mezhlumian, Phys. Rev. D 52, 6789 (1995) · doi:10.1103/PhysRevD.52.6789 |
| [15] | A. Linde, Phys. Rev. D 59, 023503 (1999) · doi:10.1103/PhysRevD.59.023503 |
| [16] | A. Linde, M. Sasaki, T. Tanaka, Phys. Rev. D 59, 123522 (1999) · doi:10.1103/PhysRevD.59.123522 |
| [17] | J.R. Gott, Nature 295, 304 (1982) · doi:10.1038/295304a0 |
| [18] | J.R. Gott, T.S. Statler, Phys. Lett. B 136, 157 (1984) · doi:10.1016/0370-2693(84)91171-7 |
| [19] | U. Moschella, R. Schaeffer, Phys. Rev. D 57, 2147 (1998) · doi:10.1103/PhysRevD.57.2147 |
| [20] | S. del Campo, R. Herrera, Phys. Rev. D 67, 063507 (2003) · Zbl 1222.83205 · doi:10.1103/PhysRevD.67.063507 |
| [21] | M. Bouchmadi, P.F. González-Días, Phys. Rev. D 65, 063510 (2002) · doi:10.1103/PhysRevD.65.063510 |
| [22] | S. del Campo, R. Herrera, J. Saavedra, Phys. Rev. D 70, 023507 (2004) · doi:10.1103/PhysRevD.70.023507 |
| [23] | M. White, D. Scott, Astrophys. J. 459, 415 (1996) · doi:10.1086/176904 |
| [24] | G. Ellis, W. Stoerger, P. McEwan, P. Dunsby, Gen. Relat. Grav. 34, 1445 (2002) · Zbl 1016.83045 · doi:10.1023/A:1020087004012 |
| [25] | G. Ellis, W. Stoerger, P. McEwan, P. Dunsby, Gen. Relat. Grav. 34, 1461 (2002) · Zbl 1039.83048 · doi:10.1023/A:1020039120851 |
| [26] | S. del Campo, R. Herrera, J. Saavedra, Int. J. Mod. Phys. D 14, 1 (2005) · Zbl 1071.83046 · doi:10.1142/S0218271805005931 |
| [27] | S. del Campo, R. Herrera, Class. Quantum Grav. 22, 2687 (2005) · Zbl 1074.83030 · doi:10.1088/0264-9381/22/13/012 |
| [28] | A. Sen, JHEP 9808, 012 (1998) · Zbl 0955.81038 · doi:10.1088/1126-6708/1998/08/012 |
| [29] | A. Sen, JHEP 9910, 008 (1999) · Zbl 0957.81038 · doi:10.1088/1126-6708/1999/10/008 |
| [30] | M.R. Garousi, Nucl. Phys. B 584, 284 (2000) · Zbl 0984.81123 · doi:10.1016/S0550-3213(00)00361-8 |
| [31] | E.A. Bergshoeff, M. de Roo, T.C. de Wit, E. Eyras, S. Panda, JHEP 0005, 009 (2000) · Zbl 0990.81618 · doi:10.1088/1126-6708/2000/05/009 |
| [32] | J. Kluson, Phys. Rev. D 62, 126003 (2000) · doi:10.1103/PhysRevD.62.126003 |
| [33] | D. Kutasov, V. Niarchos, Nucl. Phys. B 666, 56 (2003) · Zbl 1057.81547 · doi:10.1016/S0550-3213(03)00498-X |
| [34] | G.W. Gibbons, Phys. Lett. B 537, 1 (2002) · Zbl 0995.83084 · doi:10.1016/S0370-2693(02)01881-6 |
| [35] | M. Fairbairn, M.H.G. Tytgat, Phys. Lett. B 546, 1 (2002) · Zbl 0998.83514 · doi:10.1016/S0370-2693(02)02638-2 |
| [36] | D. Choudhury, D. Ghoshal, D.P. Jatkar, S. Panda, Phys. Lett. B 544, 231 (2002) · Zbl 0998.83064 · doi:10.1016/S0370-2693(02)02512-1 |
| [37] | L. Kofman, A. Linde, JHEP 0207, 004 (2002) · doi:10.1088/1126-6708/2002/07/004 |
| [38] | X.Z. Li, J.G. Hao, D.J. Liu, Chin. Phys. Lett. 19, 1584 (2002) · doi:10.1088/0256-307X/19/11/305 |
| [39] | F. Leblond, A.W. Peet, JHEP 0304, 048 (2003) · doi:10.1088/1126-6708/2003/04/048 |
| [40] | S. Nojiri, S.D. Odintsov, Phys. Lett. B 571, 1 (2003) · Zbl 1031.83016 · doi:10.1016/j.physletb.2003.08.013 |
| [41] | S. Kachru, R. Kallosh, A. Linde, J.M. Maldacena, L. McAllister, S.P. Trivedi, JCAP 0310, 013 (2003) |
| [42] | Z.K. Guo, Y.Z. Zhang, JCAP 0408, 010 (2004) |
| [43] | D.J. Liu, X.Z. Li, Phys. Rev. D 70, 123504 (2004) · doi:10.1103/PhysRevD.70.123504 |
| [44] | J.M. Aguirregabiria, R. Lazkoz, Phys. Rev. D 69, 123502 (2004) · doi:10.1103/PhysRevD.69.123502 |
| [45] | J.M. Aguirregabiria, R. Lazkoz, Mod. Phys. Lett. A 19, 927 (2004) · Zbl 1075.83549 · doi:10.1142/S021773230401391X |
| [46] | G. Calcagni, Phys. Rev. D 69, 103508 (2004) · doi:10.1103/PhysRevD.69.103508 |
| [47] | X.H. Meng, P. Wang, Class. Quantum Grav. 21, 2527 (2004) · Zbl 1049.83040 · doi:10.1088/0264-9381/21/11/001 |
| [48] | K. Hotta, Prog. Theor. Phys. 112, 653 (2004) · Zbl 1061.81060 · doi:10.1143/PTP.112.653 |
| [49] | K. Hotta, JHEP 0603, 070 (2006) · Zbl 1226.83063 · doi:10.1088/1126-6708/2006/03/070 |
| [50] | L. Balart, S. del Campo, R. Herrera, P. Labraña, J. Saavedra, Phys. Lett. B 647, 313 (2007) · doi:10.1016/j.physletb.2007.02.011 |
| [51] | A. Sen, JHEP 0204, 048 (2002) · doi:10.1088/1126-6708/2002/04/048 |
| [52] | A. Sen, JHEP 0207, 065 (2002) · doi:10.1088/1126-6708/2002/07/065 |
| [53] | K. Koyama, J. Soda, Phys. Lett. B 483, 432 (2000) · Zbl 0961.83054 · doi:10.1016/S0370-2693(00)00545-1 |
| [54] | M. Sami, P. Chingangbam, T. Qureshi, Phys. Rev. D 66, 043530 (2002) · doi:10.1103/PhysRevD.66.043530 |
| [55] | Z. Guo, Y. Piao, R. Cai, Y. Zhang, Phys. Rev. D 68, 043508 (2003) · doi:10.1103/PhysRevD.68.043508 |
| [56] | D.J. Schwarz, C.A. Terrero-Escalante, A.A. Garcia, Phys. Lett. B 517, 243 (2001) · doi:10.1016/S0370-2693(01)01036-X |
| [57] | D.A. Steer, F. Vernizzi, Phys. Rev. D 70, 043527 (2004) · doi:10.1103/PhysRevD.70.043527 |
| [58] | G. Ballesteros, J.A. Casas, J.R. Espinosa, JCAP 0603, 001 (2006) |
| [59] | K. Bhattacharya, S. Mohanty, A. Nautiyal, astro-ph/0607049 |
| [60] | M. Tegmark et al., Phys. Rev. D 69, 103501 (2004) · doi:10.1103/PhysRevD.69.103501 |
| [61] | E.R. Harrison, Phys. Rev. D 1, 2726 (1970) · doi:10.1103/PhysRevD.1.2726 |
| [62] | Y.B. Zel’dovich, Mon. Not. R. Astron. Soc. 160, 1 (1972) |
This reference list is based on information provided by the publisher or from digital mathematics libraries. Its items are heuristically matched to zbMATH identifiers and may contain data conversion errors. In some cases that data have been complemented/enhanced by data from zbMATH Open. This attempts to reflect the references listed in the original paper as accurately as possible without claiming completeness or a perfect matching.
