Abstract
Irreversible matter creation is investigated in a two-component (scalar field and ordinary matter) cosmological fluid in a homogeneous spatially flat and isotropic Friedmann-Robertson-Walker (FRW) inflationary Universe during its reheating era. The thermodynamics of open systems as applied together with the gravitational field equations to the two-component cosmological fluid leads to a generalisation of the elementary reheating theory in which the decay (creation) pressures are explicitly considered as parts of the fluid stress-energy tensor. Particular models describing coherently oscillating scalar waves and leading to a high particle production at the beginning of the oscillatory period are considered too.
Similar content being viewed by others
References
Abramo, L.R.W. and Lima, J.A.S.: 1996, Class. Quantum Grav. 13, 2593.
Albrecht, A., Steinhardt, P.J., Turner, M.S. and Wilezek, F.: 1982, Phys. Rev. Lett. 48, 1437.
Barrow, J.D. and Saich, P.: 1993, Class. Quantum Grav. 10, 279.
Boyanovski, D., de Vega, H.J. and Holman, R.: 1997, hep-ph/9701304.
Calvao, M.O., Lima, J.A.S. and Waga, I.: 1992, Phys. Lett. A 162, 223.
Kofman, L., Linde, A. and Starobinsky, A.A.: 1997, hep-ph/9704452.
Kolb, E.W. and Riotto, A.: 1997, Phys. Rev. D 55,6, 3313.
Kolb, E.W. and Turner, M.S.: 1990, The Early Universe, Addison-Wesley, Redwood City.
Lima, J.A.S., Germano, A.S.M. and Abramo, L.R.W.: 1996, Phys. Rev. D 53,8, 4278.
Linde, A.: 1992, Particle Physics and Inflationary Cosmology, Harwood Academic Publishers.
Prigogine, I., Geheniau, J., Gunzig, E. and Nardone, P.: 1988, Proc. Natl. Acad. Sci. U.S.A. 85, 7428.
Sudharshan, R. and Johri, V.B.: 1994, Gen. Rel. Grav. 26,1, 41.
Zimdahl, W., Pavon, D. and Maartens, R.: 1996, astro-ph/9611147.
Rights and permissions
About this article
Cite this article
Harko, T., Mak, M. Irreversible Matter Creation in Inflationary Cosmology. Astrophysics and Space Science 253, 161–175 (1997). https://doi.org/10.1023/A:1000699922344
Issue Date:
DOI: https://doi.org/10.1023/A:1000699922344