Power spectrum of the primordial scalar field fluctuations in the warm inflation scenario
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 t...
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| Formato: | Capítulo de libro |
| Lenguaje: | Inglés |
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1998
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| Acceso en línea: | Registro en Scopus Handle Registro en la Biblioteca Digital |
| Aporte de: | Registro referencial: Solicitar el recurso aquí |
| LEADER | 03079caa a22003977a 4500 | ||
|---|---|---|---|
| 001 | PAPER-2839 | ||
| 003 | AR-BaUEN | ||
| 005 | 20241008082446.0 | ||
| 008 | 140217s1998 xx ||||fo|||| 00| 0 eng|d | ||
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| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Bellini, Mauricio | |
| 245 | 1 | 0 | |a Power spectrum of the primordial scalar field fluctuations in the warm inflation scenario |
| 260 | |c 1998 | ||
| 270 | 1 | 0 | |m Bellini, M.; Departamento de Física, Fac. de Ciencias Exactas y Naturales, Univ. Nacional de Mar del Plata, Funes 3350, (7600) Mar del Plata, Buenos Aires, Argentina; email: mbellini@mdp.edu.ar |
| 504 | |a Berera, A., Fang, L.-Z., (1995) Phys. Rev. Lett., 74, p. 1912 | ||
| 504 | |a Berera, A., (1995) Phys. Rev. Lett., 75, p. 3218 | ||
| 504 | |a Berera, A., (1996) Phys. Rev. D, 54, p. 2519 | ||
| 504 | |a Bellini, M., Inflation with finite temperature (1998) Phys. Lett. B, 428, p. 31 | ||
| 504 | |a Bellini, M., Casini, H., Montemayor, R., Sisterna, P., (1996) Phys. Rev. D, 54, p. 7172 | ||
| 504 | |a Casini, H., Montemayor, R., Sisterna, P., unpublishedStratonovich, R.L., (1963) Topics in the Theory of Random Noise, 1. , Gordon and Breach, New York | ||
| 504 | |a Berera, A., (1997) Phys. Rev. D, 55, p. 3346 | ||
| 504 | |a Hu, B.L., Paz, J.P., Zhang, Y., (1992) Phys. Rev. D, 45, p. 2843 | ||
| 504 | |a Smoot, R.L., (1992) Astrophys. J., 396, pp. L1 | ||
| 506 | |2 openaire |e Política editorial | ||
| 520 | 3 | |a 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. |l eng | |
| 593 | |a Departamento de Física, Fac. de Ciencias Exactas y Naturales, Univ. Nacional de Mar del Plata, Funes 3350, (7600) Mar del Plata, Buenos Aires, Argentina | ||
| 593 | |a Inst. de Fis. y Matematicas, Univ. Michoacana S. Nicolas Hidalgo, 58060 Morelia, Michoacán, Mexico | ||
| 773 | 0 | |d 1998 |g v. 58 |h pp. 1035181-1035185 |k n. 10 |p Phys Rev D Part Fields Gravit Cosmol |o Nro. del artículo: 103518 |x 05562821 |w (AR-BaUEN)CENRE-394 |t Physical Review D - Particles, Fields, Gravitation and Cosmology | |
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| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_05562821_v58_n10_p1035181_Bellini |x handle |y Handle |
| 856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v58_n10_p1035181_Bellini |x registro |y Registro en la Biblioteca Digital |
| 961 | |a paper_05562821_v58_n10_p1035181_Bellini |b paper |c PE | ||
| 962 | |a info:eu-repo/semantics/article |a info:ar-repo/semantics/artículo |b info:eu-repo/semantics/publishedVersion | ||
| 963 | |a VARI | ||