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Tachyon potential in Bianchi type-V universe. (English) Zbl 1252.83030

Summary: The solution for a tachyon potential has been obtained for a Bianchi type-V universe in two forms (power-law and exponential type).

MSC:

83C15 Exact solutions to problems in general relativity and gravitational theory
83F05 Relativistic cosmology
83D05 Relativistic gravitational theories other than Einstein’s, including asymmetric field theories
Full Text: DOI

References:

[1] G. W. Gibbons, Phys. Lett. B 537, 1 (2002). · Zbl 0995.83084 · doi:10.1016/S0370-2693(02)01881-6
[2] M. Fairbairn and M. H. G. Tytgat, Phys. Lett. B 546, 1 (2002). · Zbl 0998.83514 · doi:10.1016/S0370-2693(02)02638-2
[3] E. Recami, Rivista Nuovo Cim. 9, 1 (1986). · doi:10.1007/BF02724327
[4] A. Sen, JHEP 0204, 048 (2002); 0202, 065 (2002). · doi:10.1088/1126-6708/2002/04/048
[5] A. Feinstein, Phys. Rev. D 66, 063511 (2002). · doi:10.1103/PhysRevD.66.063511
[6] T. Padmanabhan, Phys. Rev. D 66, 021301 (2002). · doi:10.1103/PhysRevD.66.021301
[7] A. Sen, JHEP 0207, 065 (2002). · doi:10.1088/1126-6708/2002/07/065
[8] C. W. Misner, K. S. Thorne, and J. A. Wheeler, Gravitation (W. H. Freeman, New York, 1973).
[9] C. W. Misner, Astroph. J. 151, 431 (1968). · doi:10.1086/149448
[10] B. L. Hu and L. Parker, Phys. Rev. D 17, 933 (1978). · doi:10.1103/PhysRevD.17.933
[11] P. K. Suresh, JCAP 04, 023 (2008). · doi:10.1088/1475-7516/2008/04/023
[12] S. Mukahyama, Phys. Rev. D 66, 024009 (2002). · doi:10.1103/PhysRevD.66.024009
[13] T. Singh and R. Chaubey, Pramana J. Phys. 71, 447 (2008). · doi:10.1007/s12043-008-0124-y
[14] R. Chaubey, Astrophys. Space Sci. 321, 241 (2009). · doi:10.1007/s10509-009-0027-5
[15] T. Singh and R. Chaubey, Pramana J. Phys. 68, 721 (2007). · doi:10.1007/s12043-007-0072-y
[16] T. Singh and R. Chaubey, Int. J. Mod. Phys. D 15, 111 (2006).
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