Constraining primordial non-Gaussianity and parity-violation through Scalar-Induced Gravitational Waves with next-generation ground-based interferometers
Ilaria Caporali, H. V. Ragavendra, Angelo Ricciardone, Nicola Bartolo
astro-ph.CO, gr-qc
Submitted: 2026-07-17
Comments: 13 pages, 5 figures, 2 Appendices
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- General Relativistic Dynamics of Irrotational Dust: Cosmological Implications
- The stochastic gravitational-wave background produced by non-linear cosmological perturbations
- Relativistic second-order perturbations of the Einstein-de Sitter Universe
- The cosmological gravitational wave background from primordial density perturbations
- Gravitational Wave Spectrum Induced by Primordial Scalar Perturbations
- The Maximal Amount of Gravitational Waves in the Curvaton Scenario
- Gravitational waves from inflation
- Semianalytic Calculation of Gravitational Wave Spectrum Nonlinearly Induced from Primordial Curvature Perturbations
- Scalar induced gravitational waves review
- New cosmological constraints on primordial black holes
- Primordial Black Holes as Dark Matter
- Science with the space-based interferometer LISA. IV: Probing inflation with gravitational waves
- Primordial black hole constraints for extended mass functions
- The Primordial Black Hole Dark Matter - LISA Serendipity
- Testing Primordial Black Holes as Dark Matter through LISA
- Constraints on Primordial Black Holes
- Primordial Black Holes as Dark Matter: Recent Developments
- Primordial black holes and their gravitational-wave signatures
- Inflation and Primordial Black Holes
- Observational imprints of enhanced scalar power on small scales in ultra slow roll inflation and associated non-Gaussianities
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