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Abstract:

We discuss the onset of inflation in an inhomogeneous, asymptotically Friedmann-Robertson-Walker universe coupled to a scalar inflaton field. We consider a three-parameter family of inhomogeneous Cauchy data, for which we can solve analytically the constraint equations. Inflation only occurs if the Cauchy data are homogeneous over several horizon lengths. © 1992 The American Physical Society.

Registro:

Documento: Artículo
Título:Inflation in inhomogeneous cosmology
Autor:Calzetta, E.; Sakellariadou, M.
Filiación:Instituto de Astronomía Y Física del Espacio, Casilla de Correo 67-Sucursal 28, Universidad de Buenos Aires, 1428 Buenos Aires, 1428 Buenos Aires, Argentina
Research Group in General Relativity, Faculté des Sciences, Boulevard du Triomphe, 1050 Bruxelles, Belgium
Año:1992
Volumen:45
Número:8
Página de inicio:2802
Página de fin:2805
DOI: http://dx.doi.org/10.1103/PhysRevD.45.2802
Título revista:Physical Review D
ISSN:05562821
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v45_n8_p2802_Calzetta

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Citas:

---------- APA ----------
Calzetta, E. & Sakellariadou, M. (1992) . Inflation in inhomogeneous cosmology. Physical Review D, 45(8), 2802-2805.
http://dx.doi.org/10.1103/PhysRevD.45.2802
---------- CHICAGO ----------
Calzetta, E., Sakellariadou, M. "Inflation in inhomogeneous cosmology" . Physical Review D 45, no. 8 (1992) : 2802-2805.
http://dx.doi.org/10.1103/PhysRevD.45.2802
---------- MLA ----------
Calzetta, E., Sakellariadou, M. "Inflation in inhomogeneous cosmology" . Physical Review D, vol. 45, no. 8, 1992, pp. 2802-2805.
http://dx.doi.org/10.1103/PhysRevD.45.2802
---------- VANCOUVER ----------
Calzetta, E., Sakellariadou, M. Inflation in inhomogeneous cosmology. 1992;45(8):2802-2805.
http://dx.doi.org/10.1103/PhysRevD.45.2802