Katore, S. D.; Rane, R. S.; Wankhade, K. S. Domain walls strange quark matter in Einstein-Rosen space-time with cosmological constant and heat flow. (English) Zbl 1200.83034 Int. J. Theor. Phys. 49, No. 8, 1929-1935 (2010). Summary: We study the solutions of Einstein field equations for domain walls with cosmological constant and heat flow in Einstein-Rosen cylindrical symmetric space-time when strange quark matter and normal matter attached to the domain walls. Some physical and kinematical features of the obtained cosmological model are studied and discussed. Cited in 6 Documents MSC: 83C15 Exact solutions to problems in general relativity and gravitational theory 83F05 Relativistic cosmology 83C55 Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) 81V05 Strong interaction, including quantum chromodynamics 80A10 Classical and relativistic thermodynamics Keywords:strange quark matter; domain wall; cylindrical symmetric space-time; cosmological constant and heat flow PDFBibTeX XMLCite \textit{S. D. Katore} et al., Int. J. Theor. Phys. 49, No. 8, 1929--1935 (2010; Zbl 1200.83034) Full Text: DOI References: [1] Alcock, C., Farthi, E., Olinto, A.: Astrophys. J. 310, 261 (1986) · doi:10.1086/164679 [2] Banerjee, A., Sanyal, A.K.: Gen. Relativ. Gravit. 20, 103 (1988) · doi:10.1007/BF00759320 [3] Bergmann, P.G.: Int. J. Theor. Phys. 1, 25 (1968) · doi:10.1007/BF00668828 [4] Bergmann, O.: Phys. Lett. A 82, 383 (1981) · doi:10.1016/0375-9601(81)90782-9 [5] Bodmar, A.R.: Phys. Rev. D 4, 1601 (1971) · doi:10.1103/PhysRevD.4.1601 [6] Bradley, J.M., Sviestins, E.: Gen. Relativ. Gravit. 16, 1119 (1984) · doi:10.1007/BF00760236 [7] Coley, A.A., Dunn, K.: J. Math. Phys. 33, 1772 (1992) · Zbl 0753.76202 · doi:10.1063/1.529654 [8] Collins, C.B., Glass, E.N., Wilkinson, D.A.: Gen. Relativ. Gravit. 12, 805 (1980) · Zbl 0453.53046 · doi:10.1007/BF00763057 [9] Deng, Y.: Gen. Relativ. Gravit. 21, 503 (1989) · doi:10.1007/BF00904501 [10] Deng, Y., Mannheim, P.D.: Phys. Rev. D 42, 371 (1990) · doi:10.1103/PhysRevD.42.371 [11] Farthi, E., Jaffe, R.L.: Phys. Rev. D 30, 2379 (1984) · doi:10.1103/PhysRevD.30.2379 [12] Fulling, S.A., Parker, L., Hu, B.L.: Phys. Rev. D 10, 3905 (1974) · doi:10.1103/PhysRevD.10.3905 [13] Godel, K.: Rev. Mod. Phys. 21, 447 (1949) · Zbl 0041.56701 · doi:10.1103/RevModPhys.21.447 [14] Haensal, P., Zdunik, J.L., Schaeffer, R.: Astron. Astrophys. 160, 121 (1986) [15] Itoch, N.: Prog. Theor. Phys. 44, 291 (1970) · doi:10.1143/PTP.44.291 [16] Kibble, T.W.B.: J. Phys. A 9, 1387 (1976) · Zbl 0333.57005 · doi:10.1088/0305-4470/9/8/029 [17] Linde, A.D.: Sov. Phys. JETP Lett. 19, 183 (1974) [18] Mukherjee, G.: J. Astrophys. Astron. 7, 259 (1986) · doi:10.1007/BF02714214 [19] Novello, M., Reboucas, M.J.: Astrophys. J. 225, 719 (1978) · doi:10.1086/156533 [20] Okuyama, N., Maeda, K.: Phys. Rev. D 70, 064030 (2004) · doi:10.1103/PhysRevD.70.064030 [21] Perlmutter, et al.: Nature (Lond.) 391, 51 (1998) · doi:10.1038/34124 [22] Riess, A.G., et al.: Astron. J. 116, 1009 (1998) · doi:10.1086/300499 [23] Singh, J.K.: Astrophys. Space Sci. 310, 241 (2007) · Zbl 1162.83315 · doi:10.1007/s10509-007-9505-9 [24] Witten, E.: Phys. Rev. D 30, 272 (1984) · doi:10.1103/PhysRevD.30.272 [25] Yavuz, I., Yilmaz, I., Baysal, H.: Int. J. Mod. Phys. D 14, 1365 (2005) · Zbl 1084.83034 · doi:10.1142/S0218271805007061 [26] Yilmaz, I.: Phys. Rev. D 71, 103503 (2005) · doi:10.1103/PhysRevD.71.103503 [27] Yilmaz, I.: Gen. Relativ. Gravit. 38, 1397 (2006) · Zbl 1104.83035 · doi:10.1007/s10714-006-0322-1 [28] Zeldovich, Y.B.: Sov. Phys. JETP Lett. 6, 316 (1967) [29] Zeldovich, Y.B.: Sov. Phys. JETP Lett. 14, 1143 (1968) 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.