Stability of inflationary solutions driven by a changing dissipative fluid

Luis P. Chimento; Alejandro S. Jakubi; Diego Pavón

doi:https://doi.org/10.1088/0264-9381/16/5/312

Stability of inflationary solutions driven by a changing dissipative fluid

Luis P. Chimento, Alejandro S. Jakubi, Diego Pavón

Department of Physics

Research output: Contribution to journal › Article › Research › peer-review

11 Citations (Scopus)

Abstract

In this paper the second Lyapunov method is used to study the stability of the de Sitter phase of cosmic expansion when the source of the gravitational field is a viscous fluid. Different inflationary scenarios related to reheating and decay of mini-black holes into radiation are investigated using an effective fluid described by time-varying thermodynamical quantities.

Original language	English
Pages (from-to)	1625-1635
Journal	Classical and Quantum Gravity
Volume	16
DOIs	https://doi.org/10.1088/0264-9381/16/5/312
Publication status	Published - 1 May 1999

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title = "Stability of inflationary solutions driven by a changing dissipative fluid",

abstract = "In this paper the second Lyapunov method is used to study the stability of the de Sitter phase of cosmic expansion when the source of the gravitational field is a viscous fluid. Different inflationary scenarios related to reheating and decay of mini-black holes into radiation are investigated using an effective fluid described by time-varying thermodynamical quantities.",

author = "Chimento, {Luis P.} and Jakubi, {Alejandro S.} and Diego Pav{\'o}n",

year = "1999",

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T1 - Stability of inflationary solutions driven by a changing dissipative fluid

AU - Chimento, Luis P.

AU - Jakubi, Alejandro S.

AU - Pavón, Diego

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Y1 - 1999/5/1

N2 - In this paper the second Lyapunov method is used to study the stability of the de Sitter phase of cosmic expansion when the source of the gravitational field is a viscous fluid. Different inflationary scenarios related to reheating and decay of mini-black holes into radiation are investigated using an effective fluid described by time-varying thermodynamical quantities.

AB - In this paper the second Lyapunov method is used to study the stability of the de Sitter phase of cosmic expansion when the source of the gravitational field is a viscous fluid. Different inflationary scenarios related to reheating and decay of mini-black holes into radiation are investigated using an effective fluid described by time-varying thermodynamical quantities.

U2 - https://doi.org/10.1088/0264-9381/16/5/312

DO - https://doi.org/10.1088/0264-9381/16/5/312

M3 - Article

SN - 0264-9381

VL - 16

SP - 1625

EP - 1635

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

ER -

Stability of inflationary solutions driven by a changing dissipative fluid

Abstract

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