Black Holes and Neutron Stars in an Oscillating Universe
arXiv:2110.11897 · doi:10.1134/S199034132103007X
Abstract
One of the problems for the cyclic Universe will be its compatibility with a vast population of indestructible black holes that accumulate from cycle to cycle. The article considers a simple iterative model of the evolution of black holes in a cyclic Universe, independent of specific cosmological theories. The model has two free parameters that determine the iterative decrease in the number of black holes and the increase in their individual mass. It is shown that this model, with wide variations in the parameters, explains the observed number of supermassive black holes at the centers of galaxies, as well as the relationships between different classes of black holes. The mechanism of accumulation of relict black holes during repeated pulsations of the Universe may be responsible for the black hole population detected by LIGO observations and probably responsible for the dark matter phenomenon. The number of black holes of intermediate masses corresponds to the number of globular clusters and dwarf satellite galaxies. These results argue for models of the oscillating Universe, and at the same time impose substantial requirements on them. Models of a pulsating Universe should be characterized by a high level of relict gravitational radiation generated at the time of maximum compression of the Universe and mass mergers of black holes, as well as solve the problem of the existence of the largest black hole that is formed during this merger. It has been hypothesized that some neutron stars can survive from past cycles of the Universe and contribute to dark matter. These relict neutron stars will have a set of features by which they can be distinguished from neutron stars born in the current cycle of the birth of the Universe. The observational signs of relict neutron stars and the possibility of their search in different wavelength ranges are discussed.
Astrophysical Bulletin, 76, 229-247, 2021; 16 pages, 2 figures
References in corpus (12)
- Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
- First M87 Event Horizon Telescope Results. V. Physical Origin of the Asymmetric Ring
- Planck evidence for a closed Universe and a possible crisis for cosmology
- The Expansion of the Universe is Faster than Expected
- Pulsar braking and the P-Pdot diagram
- Understanding the "anti-kick" in the merger of binary black holes
- Observational Evidence for a Dark Side to NGC5128's Globular Cluster System
- Rapid Black Hole Growth at the Dawn of the Universe: A Super-Eddington Quasar at z=6.6
- Structural Parameters of Mayall II = G1 in M31
- A repulsive force in the Einstein theory
- Statistics of interpulse radio pulsars - the key to solving the alignment/counter-alignment problem
- Gravitational wave background discovered by NANOGrav as evidence of a cyclic universe
Cited by in corpus (6)
- Spin of primordial black holes in the model with collapsing domain walls
- Evolution of black holes through a nonsingular cosmological bounce
- Gravitational wave background discovered by NANOGrav as evidence of a cyclic universe
- Survival of black holes through a cosmological bounce
- Accretion of Galaxies around Supermassive Black Holes and a Theoretical Model of the Tully-Fisher and M-Sigma Relations
- The Metron Project -- I. The Metron Project Science Program