Abstract:
As the red shift shows no sign of oscillatory behavior in an expanding universe we postulate that the energy ωk of a scalar field does not oscillate in such a universe. In the massive case, expanding the differential equation for ωk in mass powers, we find that the nonoscillatory solution coincides with the adiabatic solution up to the m6 order. We also demonstrate that this solution is unique for all the evolution of the universe with cosmological interest. Using the nonoscillatory solution as the one that defines the good vacuum state, we compute the particle and energy creation for a simple model of expanding universe. Both quantities turn out to be finite. © 1986 Plenum Publishing Corporation.
Registro:
Documento: |
Artículo
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Título: | A physical characterization of the adiabatic vacuum in Robertson-Walker universe |
Autor: | Castagnino, M.; Chimento, L. |
Filiación: | Instituto de Física Rosario, Av. Pellegrini 250, Rosario, 2000, Argentina Instituto de Astronomía y Física del Espacio, Casilla de Correos 67, Sucursal 28, Buenos Aires, 1428, Argentina Departamento de Física, Facultad de Ciencias Exactas y Naturales, Ciudad Universitaria, Pabellón 1, Buenos Aires, 1428, Argentina
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Año: | 1986
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Volumen: | 18
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Número: | 2
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Página de inicio: | 193
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Página de fin: | 205
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DOI: |
http://dx.doi.org/10.1007/BF00766485 |
Título revista: | General Relativity and Gravitation
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Título revista abreviado: | Gen Relat Gravit
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ISSN: | 00017701
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Registro: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00017701_v18_n2_p193_Castagnino |
Referencias:
- Parker, L., (1969) Phys. Rev., 183, p. 1057
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- Mamaev, S.G., Mostepanenko, V.M., Starobinski, A.A., (1976) Sov. Phys. JETP, 43, p. 823
- Castagnino, M., Chimento, L., Harari, D., (1981) Phys. Rev. D, 24, p. 290
- Castagnino, M., Chimento, L., Laciana, C., On Three Equivalent Definitions for the Spin 1 Massive Particles in Robertson-Walker Universe (1984) Progress of Theoretical Physics, 71, p. 309
- Castagnino, M., (1978) Gen. Rel. Grav., 9, p. 101
- Castagnino, M., Chimento, L., Harari, D., Nuñez, C., (1984) J. Math. Phys., 25, p. 360
- Parker, L., Fulling, S.A., (1974) Phys. Rev. D, 9, p. 341
- Fulling, S.A., Parker, L., Hu, B.L., (1974) Phys. Rev. D, 10, p. 3905
- Christensen, S.M., (1976) Phys. Rev. D, 14, p. 2490
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- Fulling, S.A., (1979) Gen. Rel. Grav., 10, p. 807
- Castagnino, M., (1983) Gen. Rel. Grav., 15, p. 1149
- Castagnino, M., Chimento, L., and Laciana, C. (1986) to be published; Waterman, P.C., Energy Conservation and WKB Methods (1973) American Journal of Physics, 41, p. 373
- Birrell, N.D., Davies, P.C.W., (1982) Quantum Fields in Curved Space, , Cambridge University Press, Cambridge
Citas:
---------- APA ----------
Castagnino, M. & Chimento, L.
(1986)
. A physical characterization of the adiabatic vacuum in Robertson-Walker universe. General Relativity and Gravitation, 18(2), 193-205.
http://dx.doi.org/10.1007/BF00766485---------- CHICAGO ----------
Castagnino, M., Chimento, L.
"A physical characterization of the adiabatic vacuum in Robertson-Walker universe"
. General Relativity and Gravitation 18, no. 2
(1986) : 193-205.
http://dx.doi.org/10.1007/BF00766485---------- MLA ----------
Castagnino, M., Chimento, L.
"A physical characterization of the adiabatic vacuum in Robertson-Walker universe"
. General Relativity and Gravitation, vol. 18, no. 2, 1986, pp. 193-205.
http://dx.doi.org/10.1007/BF00766485---------- VANCOUVER ----------
Castagnino, M., Chimento, L. A physical characterization of the adiabatic vacuum in Robertson-Walker universe. Gen Relat Gravit. 1986;18(2):193-205.
http://dx.doi.org/10.1007/BF00766485