General solution to two-scalar field cosmologies with exponential potentials

We find the exact general solution for cosmological models arising from the interaction of the gravitational field with two scalar fields in both flat Robertson-Walker and the locally rotationally symmetric Bianchi I spacetime filled with an exponential potential. One scalar field self-interacts wit...

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Autor principal: Chimento, L.P
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: 1998
Acceso en línea:Registro en Scopus
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Registro en la Biblioteca Digital
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100 1 |a Chimento, L.P. 
245 1 0 |a General solution to two-scalar field cosmologies with exponential potentials 
260 |c 1998 
270 1 0 |m Chimento, L.P.; Departamento de Física, Universidad de Buenos Aires, Ciudad Universitaria, 1428 Buenos Aires, Argentina; email: chimento@df.uba.ar 
506 |2 openaire  |e Política editorial 
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520 3 |a We find the exact general solution for cosmological models arising from the interaction of the gravitational field with two scalar fields in both flat Robertson-Walker and the locally rotationally symmetric Bianchi I spacetime filled with an exponential potential. One scalar field self-interacts with this potential and the other is a free massless scalar field. The solutions have a singularity and a set of these exhibit the transition to power-law inflation for both metrics.  |l eng 
593 |a Departamento de Física, Universidad de Buenos Aires, Ciudad Universitaria, 1428 Buenos Aires, Argentina 
773 0 |d 1998  |g v. 15  |h pp. 965-974  |k n. 4  |p Classical Quantum Gravity  |x 02649381  |w (AR-BaUEN)CENRE-326  |t Classical and Quantum Gravity 
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856 4 0 |u https://doi.org/10.1088/0264-9381/15/4/017  |y DOI 
856 4 0 |u https://hdl.handle.net/20.500.12110/paper_02649381_v15_n4_p965_Chimento  |y Handle 
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