Improved calculation of relic gravitational waves
arXiv:gr-qc/0612041 · doi:10.1088/1009-1963/16/10/012
Abstract
In this paper, we improve the calculation of the relic gravitational waves (RGW) in two aspects: First, we investigate the transfer function after considering the redshift-suppression effect, the accelerating expansion effect, the damping effect of free-streaming relativistic particles, and the damping effect of cosmic phase transition, and give a simple approximate analytic expression, which clearly illustrates the dependent relations on the cosmological parameters. Second, we develop a numerical method to calculate the primordial power spectrum of RGW at a very wide frequency range, where the observed constraints on (the scalar spectral index) and (the amplitude of primordial scalar spectrum) and the Hamilton-Jacobi equation are used. This method is applied to two kinds of inflationary models, which all satisfy the current constraints on , (the running of ) and (the tensor-scalar ratio). We plot them in the diagram, where is the strength of RGW, and study their detection by the CMB experiments and laser interferometers.
17 pages, 3 figures, minor typos corrected
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- Amplification of the Primordial Gravitational Waves Energy Spectrum by a Kinetic Scalar in Gravity
- Amplification of Primordial Gravitational Waves by a Geometrically Driven non-canonical Reheating Era
- -Gravity Generated Post-inflationary Eras and their Effect on Primordial Gravitational Waves
- Reconstructing Dark Energy Potentials From Parameterized Deceleration Parameters
- Effects of a Pre-inflationary de Sitter Bounce on the Primordial Gravitational Waves in Gravity Theories
- Detecting Relic Gravitational Waves in the CMB: Comparison of Planck and Ground-based Experiments
- Propagation of gravitational waves in an expanding background in the presence of a point mass
- Exact solutions of primordial gravitational waves
- Primordial gravitational waves from the space-condensate inflation model