Advances in Astrophysics
Kantowski-Sachs Two Fluid Radiating Cosmological Model in Brans-Dicke Theory of Gravitation
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Author(s)
- V.U.M.Rao*
Department of Applied Mathematics, Andhra University, Visakhapatnam, India - G. Suryanarayana
Department of Applied Mathematics, Andhra University, Visakhapatnam, India - Y.Aditya
Department of Applied Mathematics, Andhra University, Visakhapatnam, India
Abstract
Keywords
References
[1] A. G. Reiss, et al., "Observational evidence from supernovae for an accelerating universe and a cosmological constant", Astron. J. 116, 1009-1038 (1998).
[2] A.G. Reiss, et al., "The case for an accelerating universe from supernovae", Publ. Astron. Soc. Pac. 114, 1284-1299 (2000).
[3] A.G. Reiss, et al., "Type-Ia supernova discoveries at from the Hubble space telescope: evidence for past deceleration and constraints and dark energy evolution", Astrophys. J. 607, 665-687 (2004).
[4] S. Perlmutter, et al. "Measurements1 Of The Cosmological Parameters and " From The First Seven Supernovae at ", Astrophys. J. 483, 565-581 (1997).
[5] S. Perlmutter, et al. "Discovery of a supernova explosion at half the age of the Universe", Nature 391, 51-54 (1998).
[6] S.Perlmutter, et al., "Measurements of Omega and Lambda from 42 High-Redshift Supernovae", Astrophys. J. 517, 565-586 (1999).
[7] R. K. Knop, et al. (Supernova Cosmology Project Collaboration) "New Constraints On and From an Independent Set of 11 High-Redshift Supernovae Observed With The Hubble Space Telescope", Astrophys. J. 598, 102-137 (2003) R. R. Caldwell, "A Phantom Menace? Cosmological con
[8] sequences of a dark energy component with super-negative equation of state", Phys. Lett. B 545, 23-29 (2002).
[9] Huange, et al., "Holographic explanation of wide-angle power correlation suppression in the cosmic microwave background radiation", J. Cosmol. Astropart. Phys., 05, 013 (2006).
[10] Daniel, et al., "Large scale structure as a probe of gravitational slip", Phys. Rev. D, 77, 103513 (2008).
[11] 11. O. Akarsu, C. B. Kilinc, "LRS Bianchi type I models with anisotropic dark energy and constant deceleration parameter", Gen. Relativ. Gravit. 42, 119-140 (2010).
[12] 12. O. Akarsu, C. B. Kilinc, "Bianchi type III models with anisotropic dark energy", Gen. Relativ. Gravit. 42, 763-775 (2010b).
[13] A.K.Yadav, "Some anisotropic dark energy models in Bianchi type-V space-time", Astrophys. Space Sci. 335, 565-575 (2011).
[14] A. K. Yadav, L. Yadav, "Bianchi type-III anisotropic dark energy models with constant deceleration parameter", Int. J. Theor. Phys. 50, 218-227 (2011).
[15] A. Pradhan, et al., "Bianchi Type-I anisotropic dark energy model with constant deceleration parameter", Int. J. Theor. Phys. 50, 2923-2938 (2011a).
[16] A. Pradhan, et al., "A new class of LRS Bianchi type-II dark energy models with variable EoS parameter", Astrophys. Space Sci. 334, 249-260 (2011b).
[17] A. Pradhan, A., H. Amirhashchi, B. Saha, "An interacting and non-interacting two-fluid scenario for dark energy in FRW universe with constant deceleration parameter", Astrophys. Space Sci. 333, 343-350 (2011).
[18] A. K. Yadav, et al., "Dark Energy Models with Variable Equation of State Parameter", Int. J. Theor. Phys. 50, 871-881 (2011).
[19] C.L Bennett, et al., "First year wilkinson microwave anisotropy probe observations: prelimi nary maps and basic results", Astrophys. J. Suppl. Ser. 148, 1-27 (2003).
[20] D.N.Spergel, et al. (WMAP Collaboration), "First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters", Astrophys. J. Suppl. Ser.148, 175-194 (2003).
[21] M.Tegmark, et al. (SDSS Collaboration), "Cosmological parameters from SDSS and WMAP" Phys. Rev. D 69, 103501 (2004).
[22] R. C. Tolman, "Relativity, thermodynamics, and cosmology. Oxford", Clarendon Press, London, Section 165 (1934).
[23] W. Davidson, "The Cosmological Implications of the Recent Counts of Radio Sources: II. An Evolutionary Model", Mon. Not. R. Astron. Soc. 124, 79-93 (1962).
[24] M. Cataldo, P. Mella, P. Minning, J. Saavedra, "Interacting cosmic fluids in power-law Friedmann–Robertson–Walker cosmological models", Phys. Lett. B, 662, 314-322 (2008).
[25] A. Pradhan, H. Amirhashchi, "Dark energy models in anisotropic Bianchi type-III space-time with variable EoS parameter", Astrophys. Space Sci. 332, 441-448 (2011).
[26] K.S. Adhav, M.V. Dawande, S. M.Borikar, "Interacting Cosmic Fluids in LRS Bianchi Type-I Cosmological Models", Bulg. Jour. Phys. 38, 371-379 (2011).
[27] B. Saha, H. Amirhashchi, A. Pradhan, "Two-fluid scenario for dark energy models in an FRW universe-revisited", Astrophys. Space Sci. 342, 257-267 (2012).
[28] H. Amirhashchi, A. Pradhan, B. Saha, "An interacting two-fluid scenario for dark energy in an FRW universe", Chin. Phys. Lett. 28, 039801 (2011).
[29] K. S. Adhav, M. V. Dawande, S. M. Borikar, "Kaluza-Klein interacting cosmic fluid cosmological model", Jour. of Theo. and Applied Phys. 6, 33 (2012).
[30] D. R. K. Reddy, R. Santhi Kumar, "Two fluid scenario for dark energy model in a scalar-tensor theory of gravitation", Int. J. Theor. Phys. 52, 1362-1369 (2013).
[31] H. Amirhashchi, A. Pradhan, Hishamuddin Zainuddin, "Interacting two-fluid viscous dark energy models in a non-flat universe", Research in Astron. Astrophysics 13, 129-138 (2013).
[32] C. H. Brans, R. H. Dicke, "Mach's principle and a relativistic theory of gravitation", Phys.Rev.124, 925-935(1961).
[33] T. Singh, L. N. Rai, "Scalar-tensor theories of gravitation: Foundations and prospects" Gen.Rel.Grav 15, 875- 902 (1983).
[34] D. R. K.Reddy, V. U. M.Rao, "Field of a charged particle in Brans-Dicke theory of gravitation", J. Phys. A: Math. Gen., 14, 1973-1976 (1981).
[35] A. Banerjee, N. O. Santos, "Bianchi type-II cosmological models in Brans-Dicke theory", Nuovo Cimento, 67B, 31-40 (1982).
[36] Shri Ram." Spatially homogeneous and anisotropic cosmological solution in Brans-Dicke theory", Gen. Relativ. Gravit., 15, 635-640 (1983).
[37] Shri Ram, D. K Singh, "Exact Bianchi type VI0 cosmological solutions with matter in Brans-Dicke theory", Astrophys. Space Sci., 103, 21-26 (1984).
[38] M. S. Berman, et al." Brans-Dicke static universes", Gen. Relativ. Gravit. 21, 287-292 (1989).
[39] D. R. K. Reddy,"A String cosmological model in Brans-Dicke theory of gravitation", Astrophys. Space Sci., 286, 365-371 (2003).
[40] D. R. K. Reddy, R. L. Naidu, "Five dimensional string cosmological models in a scalar-tensor theory of gravitation", Astrophys. Space Sci., 307, 395-398 (2007).
[41] K.S. Adhav, A. S. Nimkar, M. R. Ugale, M.V. Dawande, "N-dimensional string cosmological model in Brans–Dicke theory of gravitation", Astrophys. Space Sci., 310, 231-235 (2007).
[42] V. U. M. Rao, M. Vijaya Santhi, "Bianchi Type-II, VIII & IX Perfect fluid cosmological models in Brans Dicke theory of gravitation", J. Mod. Phys., 2, 1222-1228 (2011).
[43] V.U.M.Rao, M. Vijaya Santhi, "Bianchi type-II, VIII & IX perfect fluid magnetized cosmological models in Brans-Dicke theory of gravitation", Astrophys. Space Sci., 337, 387-392 (2012).
[44] V.U.M.Rao, M. Vijaya Santhi, "Bianchi Types II, VIII, and IX String cosmological models in Brans-Dicke theory of gravitation", ISRN Math. Phys., doi:10.5402/2012/573967 (2012).
[45] R. L. Naidu, K. Dasu Naidu, K. Shobhan Babu, D.R.K. Reddy, "A five dimensional Kaluza-Klein bulk viscous string cosmological model in Brans-Dicke scalar-tensor theory of gravitation", Astrophys. Space Sci., 347, 197-201 (2013).
[46] T. Vidya Sagar, et al., "A five dimensional Kaluza-Klein bulk viscous string cosmological model in Brans-Dicke scalar-tensor theory of gravitation", Astrophys. Space Sci., 349, 479-483 (2014).
[47] S. Das, A.M. Abdulla, "An Interacting Model of Dark Energy in Brans-Dicke Theory", Astrophys. Space Sci.,351, 651-660 (2014).
[48] D. D.Pawar, Y.S. Solanke, "Exact Kantowski-Sachs Anisotropic Dark Energy Cosmological Models in Brans Dicke Theory of Gravitation", Int. J. Theor. Phys., 53, 3052-3065 (2014).
[49] D. Pavon, B. Wang, "Le Chatelier–Braun principle in cosmological physics", Gen. Relativ. Gravit. 41, 1-5(2009).
[50] L. Amendola, G. Camargo Campos, R. Rosenfeld, "Consequences of dark matter-dark energy interaction on cosmological parameters derived from type Ia supernova data", Phys. Rev. D 75, 083506 (2007).
[51] Z. K. Guo, N. Ohta, S. Tsujikawa, "Probing the coupling between dark components of the universe", Phys. Rev.D, 76, 023508 (2007).