2008
DOI: 10.1103/physrevd.77.064002
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Parametric resonance and cosmological gravitational waves

Abstract: We investigate the production of gravitational waves due to quantum fluctuations of the vacuum during the transition from the inflationary to the radiation-dominated eras of the universe, assuming this transition to be dominated by the phenomenon of parametric resonance. The energy spectrum of the gravitational waves is calculated using the method of continuous Bogoliubov coefficients, which avoids the problem of overproduction of gravitons at large frequencies. We found, on the sole basis of the mechanism of … Show more

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Cited by 19 publications
(23 citation statements)
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“…This method has been used by us in previous works to investigate the generation of gravitational waves in different cosmological models [19,22,34]. Upon the redefinition…”
Section: Gravitational-wave Spectrummentioning
confidence: 97%
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“…This method has been used by us in previous works to investigate the generation of gravitational waves in different cosmological models [19,22,34]. Upon the redefinition…”
Section: Gravitational-wave Spectrummentioning
confidence: 97%
“…Having determined the time evolution of a /a from Eqs. (16)- (19), we then solve Eqs. (26) and (27) (again with a Runge-Kutte method) for different values of ω(η 0 ) = k/a(η 0 ) and with initial conditions (32) and (33).…”
Section: Numerical Simulationsmentioning
confidence: 99%
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“…The gravitational waves energy density is given by [42] 1) where N k (τ ) is the number of gravitons created for a given mode k in a different vacuum state as the universe expands. Then the dimensionless relative logarithmic energy spectrum Ω GW at the present time τ 0 can be defined as [42] Ω…”
Section: A Formalismmentioning
confidence: 99%
“…Then the dimensionless relative logarithmic energy spectrum Ω GW at the present time τ 0 can be defined as [42] Ω…”
Section: A Formalismmentioning
confidence: 99%