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Abstract:

Within the framework of homogeneous models of the Universe, inflation provides the simplest explanation for the present cosmic isotropy, and a Bianchi type-IX (mixmaster) model is the least prejudiced guess we can make about the state of the Universe before the inflationary phase. However, a mixmaster model would not inflate unless either shear or the radiation energy density are large enough. Particle creation enhances the radiation energy density and therefore enlarges the set of inflating initial conditions for the Universe. © 1991 The American Physical Society.

Registro:

Documento: Artículo
Título:Particle creation, inflation, and cosmic isotropy
Autor:Calzetta, E.
Filiación:Instituto de Astronomía y Física del Espacio, Casilla de Correo 67, Sucursal 28, 1428 Buenos Aires, Argentina
Departamento de Física, Universidad de Buenos Aires, Ciudad Universitaria, 1428 Buenos Aires, Argentina
Año:1991
Volumen:44
Número:10
Página de inicio:3043
Página de fin:3051
DOI: http://dx.doi.org/10.1103/PhysRevD.44.3043
Título revista:Physical Review D
ISSN:05562821
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v44_n10_p3043_Calzetta

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Citas:

---------- APA ----------
(1991) . Particle creation, inflation, and cosmic isotropy. Physical Review D, 44(10), 3043-3051.
http://dx.doi.org/10.1103/PhysRevD.44.3043
---------- CHICAGO ----------
Calzetta, E. "Particle creation, inflation, and cosmic isotropy" . Physical Review D 44, no. 10 (1991) : 3043-3051.
http://dx.doi.org/10.1103/PhysRevD.44.3043
---------- MLA ----------
Calzetta, E. "Particle creation, inflation, and cosmic isotropy" . Physical Review D, vol. 44, no. 10, 1991, pp. 3043-3051.
http://dx.doi.org/10.1103/PhysRevD.44.3043
---------- VANCOUVER ----------
Calzetta, E. Particle creation, inflation, and cosmic isotropy. 1991;44(10):3043-3051.
http://dx.doi.org/10.1103/PhysRevD.44.3043