Abstract
Two relativistic models for collapsing spheres at different stages of evolution, which include pre-relaxation processes, are presented. The influence of relaxation time on the outcome of evolution in both cases is exhibited and established. It is shown that relaxation processes can drastically change the final state of the collapsing system. In particular, there are cases in which the value of the relaxation time determines the bounce or the collapse of the sphere.
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REFERENCES
Peierls, R. (1955). Quantum Theory of Solids(Clarendon Press, Oxford).
Band, W., Meyer, L. (1948). Phys. Rev.73, 226.
Harwit, M. (1988). Astrophysical Concepts(Springer-Verlag, New York).
Flowers, E., Itoh, N. (1979). Astrophys. J.230, 847.
Flowers, E., Itoh N. (1981), Astrophys. J.250, 750.
Di Prisco, A., Herrera, L., Esculpi, M. (1996). Class. Quantum Grav.13, 1053.
Martínez, J. (1996). Phys. Rev. D53, 6921.
Herrera, L., Jiménez, J., Ruggeri, G. J. (1980). Phys. Rev. D22, 2305.
Cosenza, M., Herrera, L., Esculpi, M., Witten, L. (1982). Phys. Rev. D25, 2527.
Herrera, L., Jiménez, J., Esculpi, M. (1987). Phys. Rev. D36, 2986.
Tolman, R. (1939). Phys. Rev.55, 364.
Burrows, A., Lattimer, L. (1986). Astrophys. J.307, 178.
Bondi, H., van der Burg, M. G. J., Metzner, A. W. K. (1962). Proc. R. Soc. London A269, 21.
Vaidya, P. C. (1951). Proc. Ind. Acad. Sci. Sect. A33, 264.
Bondi, H. 1964. Proc. R. Soc. London A281, 39.
Herrera, L., Jiménez, J. (1983). Phys. Rev. D28, 2987.
Santos, N. O. (1985). Mon. Not. R. Astr. Soc.216, 403.
Cosenza, M., Herrera, L., Esculpi, M., Witten, L. (1981). J. Math. Phys.22, 118.
Barreto, W., Rojas, S. (1992). Astrophys. Space Sci.193, 201.
Kippenhahn, R., Weigert, A. (1994). Stellar Structure and Evolution(3rd printing, Springer-Verlag, Berlin).
Shapiro, S. L., Teukolsky, S. A. (1983). Black Holes, White Dwarfs and Neutron Stars(John Wiley & Sons, New York).
Hansen, C. J., Kawaler, S. D. (1994). Stellar Interiors Physical Principles, Structure, and Evolution(Springer-Verlag, New York).
Gokhroo, M. K., Mehra, A. L. (1994). Gen. Rel. Grav.26, 75.
Börner, G. (1973). On the properties of Matter in Neutron Stars(Springer Tracts in Physics, Springer-Verlag, Berlin).
Demiański M., 1985. Relativistic Astrophysics, International Series in Nat. Phyl. V110, D. Ter Haar, ed. (Pergamon Press, Oxford).
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Herrera, L., Martínez, J. Gravitational Collapse: A Case for Thermal Relaxation. General Relativity and Gravitation 30, 445–471 (1998). https://doi.org/10.1023/A:1018862910233
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DOI: https://doi.org/10.1023/A:1018862910233