Gravitational-wave constraints on abundance of primordial black holes

By R. Saito, J. Yokoyama. 2010

190 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Oceanography

View Paper: https://www.semanticscholar.org/paper/447236ab85b8d076d42404a0c3d316f24cc45974

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. K. Kohri
2. Florian Kuhnel
3. T. Terada
4. B. Carr
5. T. Nakama
6. Keisuke Inomata
7. Guillem Domènech
8. Misao Sasaki

In Oceanography

1. Keisuke Inomata
2. T. Nakama
3. K. Kohri
4. T. Terada
5. Florian Kuhnel
6. B. Carr
7. Guillem Domènech
8. Shi Pi

Citations in the corpus

• Primordial Black Holes from Polynomial Potentials in Single Field Inflation (2017, unknown): “A large scalar perturbation can generate gravitational waves via secondorder effects, which would affect pulsar timing [33, 34].”
• Gravitational waves induced by scalar perturbations during a gradual transition from an early matter era to the radiation era (2019, background): “ely rare peaks during the radiation-dominated (RD) era. In such scenarios, the scalar perturbations may simultaneously induce stochastic GWs that can be detected by current and future GW observations [4,5,23,24]. Even if no sizable amount of primordial black holes was produced, the induced GWs can b”
• Primordial Black Holes as Dark Matter: Recent Developments (2020, background): “The associated frequency was originally given as 10−8 (M/10M ) Hz but this estimate contained a numerical error [232] and was later reduced by a factor of 10 [233].”