Results 181 to 190 of about 176,413 (293)

Bubbles kick off primordial black holes to form more binaries

open access: yesPhysical Review Research
Primordial black holes (PBHs) may form before cosmological first-order phase transitions, leading to inevitable collisions between PBHs and bubble walls. In this paper, we have simulated the coevolution of an expanding scalar wall passing through a black
Zi-Yan Yuwen   +3 more
doaj   +1 more source

Structure of the Baryon Halo Around a Supermassive Primordial Black Hole

open access: yesParticles
According to some theoretical models, primordial black holes with masses of more than 108 solar masses could be born in the early universe, and their possible observational manifestations have been investigated in a number of works. Dense dark matter and
Boris Murygin   +2 more
doaj   +1 more source

Dark spiky primordial black holes

open access: yesPhysical Review D
11 pages, 1 figure; matches published ...
openaire   +2 more sources

Large fluctuations and primordial black holes

open access: yesPhysics Reports
In this paper, we review in detail different mechanisms of generation of large primordial fluctuations and their implications for the production of primordial black holes (PBHs) and scalar-induced secondary gravity waves (SIGW), with the ultimate aim of understanding the impact of loop correction on quantum correlations and the power spectrum.
Choudhury, Sayantan, Sami, M.
openaire   +2 more sources

NANOGrav Results and LIGO-Virgo Primordial Black Holes in Axionlike Curvaton Models [PDF]

open access: hybrid, 2021
Keisuke Inomata   +3 more
openalex   +1 more source

87th Annual Meeting of the Meteoritical Society 2025: Abstracts

open access: yes
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley   +1 more source

How open is the asteroid-mass primordial black hole window?

open access: yesSciPost Physics
Primordial black holes (PBHs) can make up all of the dark matter (DM) if their mass, $m$, is in the so-called "asteroid-mass window", $10^{17} g ≲ m ≲ 10^{22} g$. Observational constraints on the abundance of PBHs are usually calculated assuming they all
Matthew Gorton, Anne M. Green
doaj   +1 more source

Home - About - Disclaimer - Privacy