Exponential potential scalar field universes. 1. The Bianchi I models - INSPIRE

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Exponential potential scalar field universes. 1. The Bianchi I models

J.M. Aguirregabiria
(
- Basque U., Bilbao
)
,
A. Feinstein
(
- Basque U., Bilbao
)
,
J. Ibanez
(
- Basque U., Bilbao
)

Sep, 1993

17 pages

Published in:

Phys.Rev.D 48 (1993) 4662-4668

e-Print:

gr-qc/9309013 [gr-qc]

DOI:

10.1103/PhysRevD.48.4662

Report number:

PRINT-93-0694 (BASQUE)

View in:

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Abstract: (arXiv)

We obtain a general exact solution of the Einstein field equations for the anisotropic Bianchi type I universes filled with an exponential-potential scalar field and study their dynamics. It is shown, in agreement with previous studies, that for a wide range of initial conditions the late-time behaviour of the models is that of a power-law inflating FRW universe. This property, does not hold, in contrast, when some degree of inhomogeneity is introduced, as discussed in our following paper II.

general relativity
field theory: scalar
field equations: solution
cosmological model
asymptotic behavior
space-time: Bianchi
numerical calculations

References(12)

Figures(0)

Exact anisotropic scalar field cosmologies

A. Feinstein
(
- Basque U., Bilbao
)
,
J. Ibanez
(
- Basque U., Bilbao
)

- Class.Quant.Grav. 10 (1993) 93-98
•
DOI:
- 10.1088/0264-9381/10/1/011

Asymptotic behavior of homogeneous cosmological models in the presence of a positive cosmological constant

Robert M. Wald
(
- Chicago U., EFI
)

- Phys.Rev.D 28 (1983) 2118-2120
•
DOI:
- 10.1103/PhysRevD.28.2118

The Isotropy of the universe

Charles W. Misner
(
- Maryland U.
)

- Astrophys.J. 151 (1968) 431-457
•
DOI:
- 10.1086/149448

Inflation

Keith A. Olive
(
- Minnesota U.
)

- Phys.Rept. 190 (1990) 307-403
•
DOI:
- 10.1016/0370-1573(90)90144-Q

Scalar Fields in Cosmology with an Exponential Potential

J.J. Halliwell
(
- Cambridge U.
)

- Phys.Lett.B 185 (1987) 341
•
DOI:
- 10.1016/0370-2693(87)91011-2

Inflationary Models with Exponential Potentials

A.B. Burd
(
- Sussex U.
)
,
John D. Barrow
(
- Sussex U.
)

- Nucl.Phys.B 308 (1988) 929-945,
- Nucl.Phys.B 324 (1989) 276-276 (erratum)
•
DOI:
- 10.1016/0550-3213(88)90135-6

Homogeneous Cosmological Models and New Inflation

Michael S. Turner
(
- Fermilab and
- Chicago U., EFI
)
,
L.M. Widrow
(
- Fermilab and
- Chicago U., EFI
)

- Phys.Rev.Lett. 57 (1986) 2237-2240,
- Phys. Rev. Lett. 57 ( 1986) 2237-2240
•
DOI:
- 10.1103/PhysRevLett.57.2237

Cosmic no hair theorem in power law inflation

Yuichi Kitada
(
- Tokyo U.
)
,
Kei-ichi Maeda
(
- Waseda U.
)

- Phys.Rev.D 45 (1992) 1416-1419
•
DOI:
- 10.1103/PhysRevD.45.1416

Power law inflation as an attractor solution for inhomogeneous cosmological models

- Class.Quant.Grav. 7 (1990) 1163-1168
•
DOI:
- 10.1088/0264-9381/7/7/012

Cosmic no hair theorem in homogeneous space-times. 1. Bianchi models

Yuichi Kitada
(
- Tokyo U.
)
,
Kei-ichi Maeda
(
- Waseda U.
)

- Class.Quant.Grav. 10 (1993) 703-734
•
DOI:
- 10.1088/0264-9381/10/4/008

Why is the Universe isotropic?

C.B. Collins
(
- Cambridge U., DAMTP and
- Cambridge U.
)
,
S.W. Hawking
(
- Cambridge U., DAMTP and
- Cambridge U.
)

- Astrophys.J. 180 (1973) 317-334
•
DOI:
- 10.1086/151965

Exact scalar field cosmologies

G.F.R. Ellis
(
- SISSA, Trieste and
- Queen Mary, U. of London and
- Cape Town U.
)
,
M.S. Madsen
(
- Sussex U. and
- Cape Town U.
)

- Class.Quant.Grav. 8 (1991) 667-676
•
DOI:
- 10.1088/0264-9381/8/4/012