A Brief Review of the Dynamical Universe in the Early and Late Stages
Keywords:
Expanding Universe, Inflation, Friedman Equations, Cosmological Singularities, Phantom Energy Era.Abstract
A dynamical study of the universe is briefly reviewed in the early stage (inflation) as well as in the late era (cosmic doomsday). The cosmological model of the expanding universe, governed by the Friedman equations, is explored. It is indicated that the expansion is proved to be accelerated experimentally. In the early phase, just after the big bang, the expansion of the universe is rapid and approximately exponential, which is termed as inflation. The mathematical formulation and physical significance of the inflation is discussed briefly. A number of inflationary models are also listed. The ultimate fate of the universe is briefed in the scenario of dark energy and phantom energy. The possible singularities, arising in the phantom energy era, are also discussed.
References
- Friedmann AA. On space curvature. Z. Physik. 1922; 10: 377-386
- Hubble EA relation between distance and radial velocity among extra-galactic nebulae. Proc. Nat. Acad. Sc. 1929; 15: 168-173
- Lemaitre G. The Evolution of the Universe: Discussion Nature. 1931; 128: 699-700
- Alpher RA, Herman H and Gamow R. Evolution of the Universe.? Nature. 1948; 162: 774
- Alpher RA, Bethe H and Gammow G. The origin of chemical elements.? Phys. Rev. 1948; 73: 803
- Perlmutter S et al. Measurements of ? and ? from 42 High-Redshift Supernovae. Astrophys. J. 1999; 517: 565-586? and Discovery of a supernova explosion at half the age of the Universe. Nature. 1998; 391: 51-53
- Riess AG et al. Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant.? Astron. J. 1998; 116: 1009-1038
- Schmidt B et al. The High-Z Supernova Search: Measuring Cosmic Deceleration and Global Curvature of the Universe Using Type IA Supernovae. Astron. J. 1998; 507: 46-63
- Guth A. The Inflationary Universe. Reading, Massachusetts: Persian Books. 1997
- Guth A. Inflationary universe: A possible solution to the horizon and flatness problems. Phys. Rev. D. 1981; 23: 347-356
- Kazanas D. Dynamics of the universe and spontaneous symmetry breaking. Astrophys. J. 1980; 241: L59-L63
- Sato K. Cosmological baryon-number domain structure and the first order phase transition of a vacuum. Phys. Lett. B 1981; 99: 66-70
- Einhorn BM and Sato K. Monopole production in the very early universe in a first-order phase transition. Nucl. Phys. B. 1981; 180: 385-404
- Hawking SW, Moss IG and Stewart JM. Bubble collisions in the very early universe. Phys. Rev. D. 1982; 26: 2681-2693
- Guth AH and Weinberg EJ. Could the universe have recovered from a slow first-order phase transition?. Nucl. Phys. B. 1983; 212: 321-364
- Linde AD. A new inflationary universe scenario: A possible solution of the horizon, flatness, homogeneity, isotropy and primordial monopole problems. Phys. Lett. B. 1982; 108: 389-393 and Coleman-Weinberg theory and the new inflationary universe scenario. Phys. Lett. B. 1982; 114: 431-435
- Linde AD. Scalar field fluctuations in the expanding universe and the new inflationary universe scenario. Phys. Lett. B. 1982; 116: 335-339
- Albert A and Steinhardt P. Cosmology for Grand Unified Theories with Radiatively Induced Symmetry Breaking.? Phys. Rev. Lett. 1982; 48: 1220-1223
- Coleman S and Weinberg E. Radiative Corrections as the Origin of Spontaneous Symmetry Breaking. Phys. Rev. D. 1973; 7: 1888-1910
- Linde AD. Chaotic Inflation. Phys. Lett. B. 1983; 129: 177-181
- Linde AD. Axions in inflationary cosmology. Phys. Lett. B. 1991; 259: 38-47
- Linde AD. Hybrid inflation. Phys. Rev. D. 1994; 49: 748-755
- Weinberg S. Cosmology (Chapter-4) Oxford University Press, New York. 2008
- Islam J. Possible ultimate fate of the universe. Quart. J. Roy. Astron. Soc. 1977; 18: 3-8
- Dyson FJ. Time without end: Physics and biology in an open universe. Rev. Mod. Phys. 1979; 51: 447-460
- Padmanabhan T. Dark Energy: Mystery of the Millennium. AIP Conf. Proc. 2006; 861: 179-196
- Sahani V and Starobinsky A. Reconstructing dark energy. Int. J. Mod. Phys. D. 2006; 15: 2105-2132
- Caldwell RR. A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state. Phys. Lett. B. 2002; 545: 23-29
- Caldwell RR, Kamionkowski M and Weinberg NN. Phantom Energy: Dark Energy with w < ?1 causes a Cosmic Doomsday. Phys. Rev. Lett. 2003; 91: 071301
- Hawking SW and Ellis GFR. The Large Scale Structure of Space-Time (Cambridge University Press, Cambridge) 1973
- Carroll SM, Homan M and Trodden M. ‘Can the dark energy equation-of-state parameter w be less than ?1? Phys. Rev. D. 2003; 68: 023509
- Jambrina LF. Grand Rip and Grand Bang/Crunch cosmological singularities. Phys. Rev D. 2014; 90: 064094
Downloads
Published
Issue
Section
License
Copyright (c) IJSRST

This work is licensed under a Creative Commons Attribution 4.0 International License.