On the Gauge Invariance of Scalar Induced Gravitational Waves: Gauge Fixings Considered
arXiv:2010.01487
Abstract
The energy density spectrum is an observable of gravitational waves. Divergence has appeared in the energy density spectra of the scalar induced gravitational waves for different gauge fixings. To resolve the discrepancy, we investigate the gauge invariance of the scalar induced gravitational waves. It is shown that the gauge invariant induced gravitational waves can be obtained by subtracting the fictitious tensor perturbations via introducing the counter term composed of the first order scalar perturbations. The kernel function uniquely determines the energy density spectrum of the scalar induced gravitational waves. We explicitly calculate the gauge invariant kernel functions in the Newtonian gauge and the uniform density gauge, respectively. The discrepancy between the energy density spectra upon the Newtonian gauge and the uniform density gauge is shown to be eliminated in the gauge invariant framework. In fact, the gauge invariant approach is also available to other kinds of gauge fixings.
arXiv comment9 pages, 5 figures, sequal to arXiv: 2009.11994 [gr-qc]
References in corpus (17)
- Gravitational Wave Spectrum Induced by Primordial Scalar Perturbations
- Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities
- The cosmological gravitational wave background from primordial density perturbations
- Cosmological perturbations
- Semianalytic Calculation of Gravitational Wave Spectrum Nonlinearly Induced from Primordial Curvature Perturbations
- Perturbations of spacetime: gauge transformations and gauge invariance at second order and beyond
- CMB polarization from secondary vector and tensor modes
- Gauge Independence of Induced Gravitational Waves
- Scalar Induced Gravitational Waves in Different Gauges
- Constraints on primordial density perturbations from induced gravitational waves
- Gauge dependence of gravitational waves generated from scalar perturbations
- On the gauge dependence of gravitational waves generated at second order from scalar perturbations
- Gauge-invariant Formulation of the Second-order Cosmological Perturbations
- Hamiltonian approach to 2nd order gauge invariant cosmological perturbations
- Gauge transformation of scalar induced gravitational waves
- Gauge transformation of scalar induced tensor perturbation during matter domination
- Gauge Invariant Second Order Gravitational Waves
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