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    Scalar-induced gravitational waves from coherent initial states

    Dipayan Mukherjee1,*, H. V. Ragavendra2,3,†, and Shiv K. Sethi1,‡

    • *Contact author: dipayanmkh@gmail.com
    • †Contact author: ragavendra.hv@pd.infn.it
    • ‡Contact author: sethi@rri.res.in

    Phys. Rev. D 113, 023533 – Published 21 January, 2026

    DOI: https://doi.org/10.1103/qd1s-9fxl

    Abstract

    We investigate the impact of statistical inhomogeneity and anisotropy in primordial scalar perturbations on the scalar-induced gravitational waves (SIGWs). Assuming inflationary quantum fluctuations originate from a coherent state, the resulting primordial scalar perturbations acquire a nonzero space-dependent mean, violating statistical homogeneity, statistical isotropy, and parity. As a consequence of statistical inhomogeneities, the SIGW acquires distinct scale-dependent features in its correlation function. Statistical anisotropies further lead to possible parity violation and correlation between different polarization modes in the tensor perturbations. Therefore, detection of these signatures in the stochastic gravitational wave background would offer probes to the statistical nature of primordial scalar perturbations beyond the scales accessible to cosmic microwave background observations.

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    See Also

    Cosmological consequences of statistical inhomogeneity

    H. V. Ragavendra, Dipayan Mukherjee, and Shiv K. Sethi
    Phys. Rev. D 111, 023541 (2025)

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