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The hypothesis that dark matter is converted into visible particles in active galactic nuclei is investigated. If dark matter consists of stable superheavy neutral particles and active galactic nuclei are rotating black holes, then, due to…

General Relativity and Quantum Cosmology · Physics 2009-03-19 A. A. Grib , Yu. V. Pavlov

The hypothesis that cold dark matter consists of primordial superheavy particles, the decay of short lifetime component of which led to the observable mass of matter while long living component survived up to modern times manifesting its…

General Relativity and Quantum Cosmology · Physics 2009-11-07 A. A. Grib , Yu. V. Pavlov

One of the greatest mysteries in astrophysics and cosmology is the nature and the origin of cold dark matter, which represents more than 84% of the mass in the universe. Dark matter reacts on and produces gravitational forces and governs…

General Physics · Physics 2021-10-11 Roman Schnabel

The model of creation of observable particles and particles of the dark matter, considered to be superheavy particles, due to particle creation by the gravitational field of the Friedmann model of the early Universe is given. Estimates on…

High Energy Physics - Phenomenology · Physics 2009-10-31 A. A. Grib , Yu. V. Pavlov

Ordinary baryonic particles (such as protons and neutrons) account for only one-sixth of the total matter in the Universe. The remainder is a mysterious "dark matter" component, which does not interact via electromagnetism and thus neither…

We study the formation and properties of dark neutron stars in a scenario where dark matter is made up of (heavy) dark baryons in a sequestered copy of the MSSM. This scenario naturally explains the coincidence of baryonic and dark matter…

High Energy Physics - Phenomenology · Physics 2025-11-05 Jacob A. Litterer , João G. Rosa

Results on particle creation from vacuum by the gravitational field of the expanding Friedmann Universe are presented. Finite results for the density of particles and the energy density for created particles are given for different exact…

General Relativity and Quantum Cosmology · Physics 2016-11-02 A. A. Grib , Yu. V. Pavlov

The recently observed Deuterium abundance in a low- metallicity high-redshift hydrogen cloud, which is about ten times larger than that observed in the near interstellar medium, is that expected from the Standard Big Bang Nucleosynthesis…

Astrophysics · Physics 2009-10-28 Arnon Dar

Multidimensional modification of gravity with a smaller mass scale of the gravitational interaction is considered. Stable by assumption dark matter particles could decay via interactions with virtual black holes. The decay rates of such…

High Energy Physics - Phenomenology · Physics 2023-12-12 E. V. Arbuzova , A. D. Dolgov , A. A. Nikitenko

It is now widely accepted that most of mass--energy in the universe is unobserved except by its gravitational effects. Baryons make only about 4% of the total, with "dark matter" making up about 23% and the "dark energy" responsible for the…

Astrophysics · Physics 2007-05-23 Edward A. Baltz

The nonbaryonic dark matter of the Universe is assumed to consist of new stable particles. A specific case is possible, when new stable particles bear ordinary electric charge and bind in heavy "atoms" by ordinary Coulomb interaction. Such…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-17 Maxim Yu. Khlopov , Andrey G. Mayorov , Evgeny Yu. Soldatov

Neutron stars offer powerful astrophysical laboratories to probe the properties of dark matter. Gradual accumulation of heavy, non-annihilating dark matter in neutron stars can lead to the formation of comparable-mass black holes, and…

High Energy Physics - Phenomenology · Physics 2025-04-23 Anupam Ray

We investigate the possibility that galactic dark matter could be interacting fermions in the neutrino mass range. Assuming that galactic halos behave like a fluid in hydrostatic and thermal equilibrium, we employ the equation of state for…

Astrophysics of Galaxies · Physics 2024-10-01 Andrés Aceña

Assuming existence of (very) heavy fourth generation of quarks and antiquarks we argue that antibaryon composed of the three heavy antiquarks can be light, stable and invisible, hence a good candidate for the Dark matter particle. Such…

High Energy Physics - Phenomenology · Physics 2013-03-26 D. Gorbunov , P. Pakhlov

The astronomical dark matter is an essential component of the Universe and yet its nature is still unresolved. It could be made of neutral and massive elementary particles which are their own antimatter partners. These dark matter species…

High Energy Astrophysical Phenomena · Physics 2015-06-19 Pierre Salati

We review progress in understanding dark matter by astrophysics, and particularly via the effect of gravitational lensing. Evidence from many different directions now all imply that five sixths of the material content of the universe is in…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 Richard Massey , Thomas Kitching , Johan Richard

Astronomical and cosmological observations of the past 80 years build solid evidence that atomic matter makes up only a small fraction of the matter in the universe. The dominant fraction does not interact with electromagnetic radiation,…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 Wolfgang Rau

Dark matter has been recognized as an essential part of matter for over 70 years now, and many suggestions have been made, what it could be. Most of these ideas have centered on Cold Dark Matter, particles that are predicted in extensions…

Astrophysics · Physics 2016-11-15 Peter L. Biermann , Faustin Munyaneza

The dark matter problem is almost a century old. Since the 1930s evidence has been growing that our cosmos is dominated by a new form of non-baryonic matter, that holds galaxies and clusters together and influences cosmic structures up to…

Cosmology and Nongalactic Astrophysics · Physics 2018-01-25 Laura Baudis

We propose that dark matter consists of collections of atoms encapsulated inside pieces of an alternative vacuum, in which the Higgs field vacuum expectation value is appreciably smaller than in the usual vacuum. The alternative vacuum is…

Astrophysics · Physics 2007-05-23 C. D. Froggatt , H. B. Nielsen
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