Angular sizes in spherically symmetric Stephani cosmological models

作者: Jerzy Stelmach , Izabela Jakacka

DOI: 10.1088/0264-9381/23/23/003

关键词: Equation of stateCosmic microwave backgroundPhysicsQuantum mechanicsCircular symmetryRedshiftMathematical physicsContext (language use)Symmetry (physics)CosmologyUniverse

摘要: Spherically symmetric Stephani cosmological models are considered in the context of angular sizes compact as well expanding objects percepted by an observer placed at symmetry centre. We assume that matter filling up universe satisfies barotropic equation state centre p(r ≈ 0, t) = αρ(t). Angular examined a function parameter α, energy density Ωα0 and redshift z. Small angle anisotropies microwave background radiation connected with typical fluctuation mass corresponding to galaxy also calculated model. Finally horizon problem is discussed detail.

参考文章(28)
Jerzy Stelmach, Izabela Jakacka, Non-homogeneity-driven universe acceleration Classical and Quantum Gravity. ,vol. 18, pp. 2643- 2658 ,(2001) , 10.1088/0264-9381/18/14/303
Roberto A. Sussman, Towards a Physical Interpretation for the Stephani Universes General Relativity and Gravitation. ,vol. 32, pp. 1527- 1557 ,(2000) , 10.1023/A:1001934118532
Bahram Mashhoon, Is the Universe Homogeneous on a Large Scale? The Big Bang and Georges Lemaître. pp. 75- 81 ,(1984) , 10.1007/978-94-009-6487-7_6
Jayant Vishnu Narlikar, Introduction to Cosmology ,(1983)
R. Pain, M. S. Burns, E. Smith, D. Hardin, M. Sullivan, P. E. Nugent, J. Mendez, A. G. Kim, R. Ellis, L. Wang, B. C. Lee, K. Schahmaneche, N. Panagia, M. Doi, R. Gibbons, W. M. Wood-Vasey, N. Yasuda, A. S. Fruchter, R. A. Knop, D. A. Howell, G. Goldhaber, B. Schaefer, A. Goobar, C. Lidman, J. Raux, I. Hook, S. E. Deustua, A. L. Spadafora, G. Blanc, G. Folatelli, C. R. Pennypacker, N. A. Walton, D. E. Groom, K. Garton, S. Garmond, R. Quimby, A. Conley, G. Aldering, P. Astier, G. Sainton, G. Garavini, P. Ruiz-Lapuente, S. Fabbro, N. Regnault, S. Perlmutter, R. Amanullah, V. Stanishev, S. Nobili, New Constraints on $\Omega_M$, $\Omega_\Lambda$, and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST arXiv: Astrophysics. ,(2003) , 10.1086/378560
S. Perlmutter, G. Aldering, G. Goldhaber, R. A. Knop, P. Nugent, P. G. Castro, S. Deustua, S. Fabbro, A. Goobar, D. E. Groom, I. M. Hook, A. G. Kim, M. Y. Kim, J. C. Lee, N. J. Nunes, R. Pain, C. R. Pennypacker, R. Quimby, C. Lidman, R. S. Ellis, M. Irwin, R. G. McMahon, P. Ruiz‐Lapuente, N. Walton, B. Schaefer, B. J. Boyle, A. V. Filippenko, T. Matheson, A. S. Fruchter, N. Panagia, H. J. M. Newberg, W. J. Couch, The Supernova Cosmology Project, Measurements of $\Omega$ and $\Lambda$ from 42 high redshift supernovae The Astrophysical Journal. ,vol. 517, pp. 565- 586 ,(1999) , 10.1086/307221
J. Stelmach, VLBI data for compact radio sources versus exotic forms of matter in the universe The Astrophysical Journal. ,vol. 428, pp. 61- 64 ,(1994) , 10.1086/174220
H. Stephani, Konform flache Gravitationsfelder Communications in Mathematical Physics. ,vol. 5, pp. 337- 342 ,(1967) , 10.1007/BF01646448
Mariusz P. Dąbrowski, Martin A. Hendry, The Hubble Diagram of Type Ia Supernovae in Non-Uniform Pressure Universes The Astrophysical Journal. ,vol. 498, pp. 67- 76 ,(1998) , 10.1086/305546