Pradhan, Anirudh; Singh, Sanjay Kumar Bianchi type I magnetofluid cosmological models with variable cosmological constant revisited. (English) Zbl 1051.83024 Int. J. Mod. Phys. D 13, No. 3, 503-516 (2004). A Bianchi-type-I cosmological model with a bulk viscous matter and a magnetic field is investigated. It is shown that the model does not approach isotropy for large times. The behavior of the cosmological constant is also investigated. Reviewer: Mohammad Khorrami (Tehran) Cited in 41 Documents MSC: 83F05 Relativistic cosmology 83C55 Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) Keywords:cosmology; Bianchi type I universe; magnetofluid models PDF BibTeX XML Cite \textit{A. Pradhan} and \textit{S. K. Singh}, Int. J. Mod. Phys. D 13, No. 3, 503--516 (2004; Zbl 1051.83024) Full Text: DOI arXiv References: [1] DOI: 10.1086/149694 [2] Shikin I. S., Dokl. Akad. Nauk SSSR 171 pp 73– (1966) [3] Robertson H. P., Proc. London Math. Soc. 42 pp 90– (1936) [4] DOI: 10.1103/PhysRevLett.30.188 [5] Asseo E., Phys. Rep. 6 pp 148– (1987) [6] DOI: 10.1111/j.1749-6632.1975.tb31440.x [7] DOI: 10.1086/167625 [8] DOI: 10.1086/170484 [9] Perley R., Astrophys. J. 101 pp 1623– (1991) [10] DOI: 10.1086/171104 [11] DOI: 10.1086/171125 [12] DOI: 10.1086/303987 [13] DOI: 10.1038/385131a0 [14] Barrow J. D., Phys. Rev. 55 pp 7451– (1997) [15] Zeldovich Ya. A., Sov. Astron. 13 pp 608– (1970) [16] Turner M. S., Phys. Rev. 30 pp 2743– (1988) [17] DOI: 10.1086/185528 [18] DOI: 10.1086/186384 [19] Dolgov A. D., Phys. Rev. 47 pp 3144– (1993) [20] Dolgov A. D., Phys. Rev. 48 pp 2499– (1993) [21] Bali R., Int. J. Theor. Phys. 47 pp 7– (1986) [22] DOI: 10.1142/S0218271803003761 · Zbl 1079.83578 [23] DOI: 10.1086/149694 [24] DOI: 10.1086/149875 [25] DOI: 10.1071/PH850239 [26] DOI: 10.1007/BF02755172 [27] Klimek Z., Post. Astron. 19 pp 165– (1971) [28] DOI: 10.1007/BF00643930 · Zbl 0714.76120 [29] DOI: 10.1086/151073 [30] DOI: 10.1088/0264-9381/8/2/014 [31] DOI: 10.1088/0264-9381/12/6/011 · Zbl 0825.83004 [32] Zimdahl W., Phys. Rev. 53 pp 5483– (1996) [33] DOI: 10.1063/1.526582 · Zbl 0562.76124 [34] DOI: 10.1016/0375-9601(87)90104-6 [35] DOI: 10.1016/0375-9601(88)90860-2 [36] Pradhan A., Astr. Lett. Commun. 35 pp 283– (1997) [37] DOI: 10.1142/S0218271801000767 [38] DOI: 10.1142/S021827180100086X [39] Pradhan A., Int. J. Mod. Phys. 11 pp 839– (2002) [40] DOI: 10.1142/S0218271802002402 · Zbl 1062.83575 [41] DOI: 10.1142/S0218271803003359 [42] DOI: 10.1007/BF02728301 [43] Ratra B., Phys. Rev. 37 pp 3406– (1988) [44] Dolgov A. D., Phys. Rev. 55 pp 5881– (1997) [45] Sahni V., Int. J. Mod. Phys. 9 pp 373– (2000) [46] DOI: 10.1016/S0370-1573(03)00120-0 · Zbl 1027.83544 [47] DOI: 10.1088/0264-9381/17/18/317 · Zbl 0971.83086 [48] DOI: 10.1086/304265 [49] DOI: 10.1086/300499 [50] DOI: 10.1016/0370-1573(85)90033-X · Zbl 0966.83541 [51] DOI: 10.1086/311140 [52] DOI: 10.1023/A:1013229818403 · Zbl 0992.83060 [53] DOI: 10.1023/A:1003651222960 · Zbl 0959.83040 [54] DOI: 10.1086/306308 [55] DOI: 10.1023/A:1001835420565 · Zbl 0965.83042 [56] DOI: 10.1098/rspa.1958.0111 [57] DOI: 10.1086/149127 [58] DOI: 10.1063/1.1704952 [59] DOI: 10.1086/148522 [60] DOI: 10.1007/BF01646733 [61] Islam J. N., New York 199 pp 86– [62] DOI: 10.1007/BF00668721 · Zbl 0597.76128 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. It attempts to reflect the references listed in the original paper as accurately as possible without claiming the completeness or perfect precision of the matching.