Impact of Scale-dependent Primordial Non-Gaussianity on Scalar-induced Gravitational Waves
astro-ph.CO, hep-ph, hep-th
Submitted: 2026-08-25
Updated: 2026-08-25
Comments: 47 pages, 27 figures + References
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Semianalytic Calculation of Gravitational Wave Spectrum Nonlinearly Induced from Primordial Curvature Perturbations
- A Cosmological Signature of the SM Higgs Instability: Gravitational Waves
- Scalar induced gravitational waves review
- The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background
- The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals
- Cosmology with the Laser Interferometer Space Antenna
- Sensitivity Studies for Third-Generation Gravitational Wave Observatories
- The Science of the Einstein Telescope
- Non-Gaussianity and the induced gravitational wave background
- Primordial Non-Gaussianity $f_{\mathrm{NL}}$ and Anisotropies in Scalar-Induced Gravitational Waves
- Gravitational waves induced by the local-type non-Gaussian curvature perturbations
- Primordial black holes in non-Gaussian regimes
- Primordial Black Holes from Inflation and non-Gaussianity
- Primordial black hole formation with non-Gaussian curvature perturbations
- Peaks and primordial black holes: the effect of non-Gaussianity
- Primordial non-gaussianity up to all orders: theoretical aspects and implications for primordial black hole models
- Non-Gaussianity effects on the primordial black hole abundance for sharply-peaked primordial spectrum
- The Sign of non-Gaussianity and the Primordial Black Holes Abundance
- Quantum diffusion beyond slow-roll: implications for primordial black-hole production
- Primordial Black Holes and Local Non-Gaussianity in Canonical Inflation
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