Abstract:
A new model of warm inflation without slow-roll conditions for the scalar field is studied. Classicality conditions that must be satisfied to have an effective stochastic approach in the warm inflation scenario are analyzed for a general coarse-grained field, defined with a function that describes the long wavelength suppression. The theory can predict the spectral density of the fluctuations of the field which can be compared with the COBE data.
Registro:
Documento: |
Artículo
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Título: | Power spectrum of the primordial scalar field fluctuations in the warm inflation scenario |
Autor: | Bellini, M. |
Filiación: | Departamento de Física, Fac. de Ciencias Exactas y Naturales, Univ. Nacional de Mar del Plata, Funes 3350, (7600) Mar del Plata, Buenos Aires, Argentina Inst. de Fis. y Matematicas, Univ. Michoacana S. Nicolas Hidalgo, 58060 Morelia, Michoacán, Mexico
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Idioma: |
Inglés
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Año: | 1998
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Volumen: | 58
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Número: | 10
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Número de artículo: | 103518
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Página de inicio: | 1035181
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Página de fin: | 1035185
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Título revista: | Physical Review D - Particles, Fields, Gravitation and Cosmology
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Título revista abreviado: | Phys Rev D Part Fields Gravit Cosmol
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ISSN: | 05562821
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CODEN: | PRVDA
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Registro: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v58_n10_p1035181_Bellini |
Referencias:
- Berera, A., Fang, L.-Z., (1995) Phys. Rev. Lett., 74, p. 1912
- Berera, A., (1995) Phys. Rev. Lett., 75, p. 3218
- Berera, A., (1996) Phys. Rev. D, 54, p. 2519
- Bellini, M., Inflation with finite temperature (1998) Phys. Lett. B, 428, p. 31
- Bellini, M., Casini, H., Montemayor, R., Sisterna, P., (1996) Phys. Rev. D, 54, p. 7172
- Casini, H., Montemayor, R., Sisterna, P., unpublishedStratonovich, R.L., (1963) Topics in the Theory of Random Noise, 1. , Gordon and Breach, New York
- Berera, A., (1997) Phys. Rev. D, 55, p. 3346
- Hu, B.L., Paz, J.P., Zhang, Y., (1992) Phys. Rev. D, 45, p. 2843
- Smoot, R.L., (1992) Astrophys. J., 396, pp. L1
Citas:
---------- APA ----------
(1998)
. Power spectrum of the primordial scalar field fluctuations in the warm inflation scenario. Physical Review D - Particles, Fields, Gravitation and Cosmology, 58(10), 1035181-1035185.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v58_n10_p1035181_Bellini [ ]
---------- CHICAGO ----------
Bellini, M.
"Power spectrum of the primordial scalar field fluctuations in the warm inflation scenario"
. Physical Review D - Particles, Fields, Gravitation and Cosmology 58, no. 10
(1998) : 1035181-1035185.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v58_n10_p1035181_Bellini [ ]
---------- MLA ----------
Bellini, M.
"Power spectrum of the primordial scalar field fluctuations in the warm inflation scenario"
. Physical Review D - Particles, Fields, Gravitation and Cosmology, vol. 58, no. 10, 1998, pp. 1035181-1035185.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v58_n10_p1035181_Bellini [ ]
---------- VANCOUVER ----------
Bellini, M. Power spectrum of the primordial scalar field fluctuations in the warm inflation scenario. Phys Rev D Part Fields Gravit Cosmol. 1998;58(10):1035181-1035185.
Available from: https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v58_n10_p1035181_Bellini [ ]