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On the Gauge Invariance of Scalar Induced Gravitational Waves: Gauge Fixings Considered

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arxiv 2010.01487 v1 pith:ZL4GIKFT submitted 2020-10-04 gr-qc astro-ph.CO

On the Gauge Invariance of Scalar Induced Gravitational Waves: Gauge Fixings Considered

classification gr-qc astro-ph.CO
keywords gaugedensitygravitationalwavesinducedscalarenergyinvariant
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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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.

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Cited by 2 Pith papers

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    A gauge-invariant source term for scalar-induced gravitational waves is derived for smooth reheating with an inflaton field transitioning into fluids.

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    A review that unifies analytical expressions for scalar-induced gravitational waves and emphasizes calculations for non-radiation-dominated cosmologies.