CrossRef Open Access 2025

Dark Matter Around Primordial Black Holes

Yu. N. Eroshenko

Abstrak

Abstract Massive primordial black holes may have formed in the early universe, accounting for a small fraction of dark matter. Most of dark matter, however, may be composed of elementary particles or black holes with smaller masses. These objects could form dense spikes around the large black holes during the radiation-dominated phase of the universe’s evolution. Dark matter particles can annihilate in the spikes. In this study, we discuss the structure and properties of the spikes, considering their transformation due to annihilation. In the hybrid scenario involving black holes of various masses, small black holes can collide and merge in the central regions around larger black holes.

Penulis (1)

Y

Yu. N. Eroshenko

Format Sitasi

Eroshenko, Y.N. (2025). Dark Matter Around Primordial Black Holes. https://doi.org/10.1134/s106377882560054x

Akses Cepat

Lihat di Sumber doi.org/10.1134/s106377882560054x
Informasi Jurnal
Tahun Terbit
2025
Bahasa
en
Sumber Database
CrossRef
DOI
10.1134/s106377882560054x
Akses
Open Access ✓