A strong dissipative inflationary model

The dynamics of a single scalar field which describes a second-order phase transition is considered taking into account the thermal effects in the high temperature limit. I conclude that thermal effects play a very important role during inflation and must not be ignored in models for the early unive...

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Autor principal: Bellini, Mauricio
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: 2003
Acceso en línea:Registro en Scopus
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100 1 |a Bellini, Mauricio 
245 1 2 |a A strong dissipative inflationary model 
260 |c 2003 
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 Guth, A.H., (1981) Phys. Rev. D, 23, p. 347 
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504 |a Erratum (1999) Phys. Rev. D, 60, p. 089901 
504 |a Maia, J.M.F., Lima, J.A.S., (1999) Phys. Rev. D, 60, p. 101301 
504 |a Berera, A., Gleiser, M., Ramos, R.O., (1998) Phys. Rev. D, 58, p. 123508 
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504 |a Bellini, M., (2001) Phys. Rev. D, 63, p. 123510 
504 |a (2003) Gen. Rel. Grav., 35, p. 41 
504 |a (2001) Phys. Rev. D, 64, p. 123508 
504 |a (2003) Phys. Rev. D, 67, p. 027303 
506 |2 openaire  |e Política editorial 
520 3 |a The dynamics of a single scalar field which describes a second-order phase transition is considered taking into account the thermal effects in the high temperature limit. I conclude that thermal effects play a very important role during inflation and must not be ignored in models for the early universe. At the end of inflation thermal fluctuations are more important than quantum fluctuations, due to the fact that T > Hc.  |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 
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