scholarly journals When primordial black holes from sound speed resonance meet a stochastic background of gravitational waves

2019 ◽  
Vol 100 (4) ◽  
Author(s):  
Yi-Fu Cai ◽  
Chao Chen ◽  
Xi Tong ◽  
Dong-Gang Wang ◽  
Sheng-Feng Yan
Keyword(s):  
Black Holes ◽  
Gravitational Waves ◽  
Sound Speed ◽  
Primordial Black Holes ◽  
Stochastic Background

scholarly journals Probing planetary-mass primordial black holes with continuous gravitational waves

2021 ◽  
pp. 100836
Author(s):  
Andrew L. Miller ◽  
Sébastien Clesse ◽  
Federico De Lillo ◽  
Giacomo Bruno ◽  
Antoine Depasse ◽  
...  
Keyword(s):  
Black Holes ◽  
Gravitational Waves ◽  
Primordial Black Holes ◽  
Planetary Mass

On Primordial Black Holes and secondary gravitational waves generated from inflation with solo/multi-bumpy potential

2021 ◽  
Author(s):  
Rui feng Zheng ◽  
Jia ming Shi ◽  
Taotao Qiu
Keyword(s):  
Black Holes ◽  
Black Hole ◽  
Gravitational Waves ◽  
Power Spectra ◽  
Small Scale ◽  
Primordial Black Hole ◽  
Primordial Black Holes ◽  
Slow Roll ◽  
Spherical Collapse ◽  
Scalar Perturbations

Abstract It is well known that primordial black hole (PBH) can be generated in inflation process of the early universe, especially when the inflaton field has some non-trivial features that could break the slow-roll condition. In this paper, we investigate a toy model of inflation with bumpy potential, which has one or several bumps. We found that potential with multi-bump can give rise to power spectra with multi peaks in small-scale region, which can in turn predict the generation of primordial black holes in various mass ranges. We also consider the two possibilities of PBH formation by spherical collapse and elliptical collapse. And discusses the scalar-induced gravitational waves (SIGWs) generated by the second-order scalar perturbations.

scholarly journals Gravity waves and primordial black holes in scalar warm little inflation

2021 ◽  
Vol 2021 (12) ◽  
pp. 052
Author(s):  
Mar Bastero-Gil ◽  
Marta Subías Díaz-Blanco
Keyword(s):  
Black Holes ◽  
Spectral Density ◽  
Gravitational Waves ◽  
Gravity Waves ◽  
High Frequency ◽  
Degrees Of Freedom ◽  
Primordial Black Holes ◽  
Frequency Range ◽  
Warm Inflation ◽  
Large Fluctuations

Abstract In warm inflation, dissipation due to the interactions of the inflaton field to other light degrees of freedom leads naturally to the enhancement of the primordial spectrum during the last 10-20 efolds of inflation. We study this effect in a variant of the Warm Little Inflaton model, where the inflaton couples to light scalars, with a quartic chaotic potential. These large fluctuations on re-entry will form light, evaporating Primordial Black Holes, with masses lighter than 106 g. But at the same time they will act as a source for the tensors at second order. The enhancement is maximal near the end of inflation, which result in a spectral density of Gravitational Waves (GW) peaked at frequencies f ∼ O(105-106) Hz today, and with an amplitude ΩGW ∼ 10-9. Although the frequency range is outside the reach of present and planned GW detectors, it might be reached in future high-frequency gravitational waves detectors, designed to search for cosmological stochastic GW backgrounds above MHz frequencies.

Sign in / Sign up

Export Citation Format

Share Document