Gravitational waves from primordial black hole isocurvature: the effect of non-Gaussianities
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Publication:6670454
DOI10.1088/1475-7516/2024/12/039MaRDI QIDQ6670454
Theodoros Papanikolaou, Xiao-Han Ma, Xin-Chen He, Emmanuel N. Saridakis, Yi-Fu Cai, Misao Sasaki
Publication date: 23 January 2025
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Cites Work
- One small step for an inflaton, one giant leap for inflation: \textit{a novel non-Gaussian tail and primordial black holes}
- A new type of isotropic cosmological models without singularity
- Baryon asymmetry from primordial black holes
- General relativistic dynamics of irrotational dust: Cosmological implications
- Primordial black holes—perspectives in gravitational wave astronomy
- Quantum diffusion during inflation and primordial black holes
- Primordial black holes from inflation and non-Gaussianity
- A cosmological signature of the SM Higgs instability: gravitational waves
- Scalaron from R2-gravity as a heavy field
- Gravitational waves from a universe filled with primordial black holes
- GUT-scale primordial black holes: mergers and gravitational waves
- Gravitational waves induced from primordial black hole fluctuations: the effect of an extended mass function
- Non-Gaussianity effects on the primordial black hole abundance for sharply-peaked primordial spectrum
- Primordial black holes in peak theory with a non-Gaussian tail
- The exponential tail of inflationary fluctuations: consequences for primordial black holes
- Metric preheating and radiative decay in single-field inflation
- Clustering of primordial black holes with non-Gaussian initial fluctuations
- Inflationary universe: A possible solution to the horizon and flatness problems
- Laser interferometry for the Big Bang Observer
- Primordial black hole formation in the radiative era: investigation of the critical nature of the collapse
- Ultra-slow-roll inflation with quantum diffusion
- Highly non-Gaussian tails and primordial black holes from single-field inflation
- Induced gravitational waves from flipped SU(5) superstring theory at nhz
- Primordial black holes in loop quantum cosmology: the effect on the threshold
- Primordial black holes from sound speed resonance in the inflaton-curvaton mixed scenario
- Enhanced curvature perturbation and primordial black hole formation in two-stage inflation with a break
- Clustering of primordial black holes from quantum diffusion during inflation
- Gravitational waves from primordial black hole evaporation with large extra dimensions
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