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Stable charged heavy leptons and quarks can exist and hide in elusive atoms, bound by Coulomb attraction and playing the role of dark matter. However, in the expanding Universe it is not possible to recombine all the charged particles into…

Astrophysics · Physics 2008-11-26 K. M. Belotsky , M. Yu. Khlopov , K. I. Shibaev

Positive results of dark matter searches in DAMA/NaI and DAMA/LIBRA experiments, being put together with the results of other groups, can imply nontrivial particle physics solutions for cosmological dark matter. Stable particles with charge…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-18 Maxim Yu. Khlopov , Andrey G. Mayorov , Evgeny Yu. Soldatov

We reinterpret the results of the direct searches for dark matter in terms of composite dark matter, i.e. dark matter particles that form neutral bound states, generically called dark atoms, either with ordinary particles, or with other…

High Energy Physics - Phenomenology · Physics 2016-01-20 Quentin Wallemacq

The puzzles of direct dark matter searches can be solved in the scenario of dark atoms, which bind hypothetical, stable, lepton-like particles with charge $-2n$, where $n$ is any natural number, with $n$ nuclei of primordial helium. Avoid…

High Energy Physics - Phenomenology · Physics 2021-11-18 T. E. Bikbaev , M. Yu. Khlopov , A. G. Mayorov

In 2005 Sheldon Glashow has proposed his sinister model, opening the path to composite-dark-matter scenarios, in which heavy stable electrically charged particles bound in neutral atoms play the role of dark matter candidates. Though the…

High Energy Physics - Phenomenology · Physics 2015-12-04 M. Yu. Khlopov

The nonbaryonic dark matter of the Universe might consist of new stable charged species, bound by ordinary Coulomb interactions in various forms of heavy neutral "dark atoms". The existing models offer natural implementations for the…

High Energy Physics - Phenomenology · Physics 2015-06-10 Konstantin Belotsky , Maxim Khlopov , Maxim Laletin

Matter of subnuclear density in the inner crusts of neutron stars consists of neutron-rich atomic nuclei immersed in strongly degenerate relativistic gas of electrons and strongly nonideal liquid of neutrons. We give a brief account of…

Astrophysics · Physics 2007-05-23 D. G. Yakovlev , O. Y. Gnedin , A. Y. Potekhin

The nonbaryonic dark matter of the Universe is assumed to consist of new stable forms of matter. Their stability reflects symmetry of micro world and particle candidates for cosmological dark matter are the lightest particles that bear new…

High Energy Physics - Phenomenology · Physics 2015-06-18 M. Yu. Khlopov

We propose that dark matter is dominantly comprised of atomic bound states. We build a simple model and map the parameter space that results in the early universe formation of hydrogen-like dark atoms. We find that atomic dark matter has…

High Energy Physics - Phenomenology · Physics 2015-05-14 David E. Kaplan , Gordan Z. Krnjaic , Keith R. Rehermann , Christopher M. Wells

Positive results of dark matter searches in DAMA/NaI and DAMA/LIBRA experiments, being put together with negative results of other groups, can imply nontrivial particle physics solutions for cosmological dark matter. Stable particles with…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 Maxim Yu. Khlopov

A mechanism is identified whereby dark matter (DM) in protostellar halos dramatically alters the current theoretical framework for the formation of the first stars. Heat from neutralino DM annihilation is shown to overwhelm any cooling…

Astrophysics · Physics 2009-06-23 Douglas Spolyar , Katherine Freese , Paolo Gondolo

Extension of particle symmetry implies new conserved charges and the lightest particles, possessing such charges, should be stable. Created in early Universe, stable charged heavy leptons and quarks can exist and, hidden in elusive atoms…

Astrophysics · Physics 2007-05-23 Maxim Yu. Khlopov

Neutron stars contain a significant number of stable muons due to the large chemical potential and degenerate electrons. This makes them the unique vessel to capture muonphilic dark matter, which does not interact with other astrophysical…

High Energy Physics - Phenomenology · Physics 2019-09-04 Raghuveer Garani , Julian Heeck

The nonbaryonic dark matter of the Universe can consist of new stable charged species, bound in heavy neutral "atoms" by ordinary Coulomb interaction. Stable $\bar U$ (anti-$U$)quarks of 4th generation, bound in stable colorless ($\bar U…

High Energy Physics - Phenomenology · Physics 2014-02-04 M. Yu. Khlopov , R. M. Shibaev

Dark matter (DM) in protostellar halos can dramatically alter the current theoretical framework for the formation of the first stars. Heat from supersymmetric DM annihilation can overwhelm any cooling mechanism, consequently impeding the…

Astrophysics · Physics 2008-11-26 Katherine Freese , Paolo Gondolo , Douglas Spolyar

For a class of macroscopic dark matter with a large interaction strength with Standard Model particles, a nucleus could be captured by the dense, heavy dark matter as it traverses ordinary material. The radiated photon carries most of the…

High Energy Physics - Phenomenology · Physics 2021-12-23 Yang Bai , Joshua Berger

The dark atoms $XHe$ are the composite Thomson like atomic dark matter candidates. We address two cosmological problems of this model. The excess of new superheavy particles with even negative charge $X^{-2n}$ over the corresponding…

High Energy Physics - Phenomenology · Physics 2024-10-18 V. A. Beylin , M. Yu. Khlopov , D. O. Sopin

In this work, we study some aspects of the dark atom model. We consider a finite-size nucleus to find the wave functions of the bound state of a stable particle with a charge of $-2n$ and helium-4 $^4He^{++}$. Then we address the problem of…

High Energy Physics - Phenomenology · Physics 2025-12-11 M. I. Balino , J. Mwilima , D. O. Sopin , M. Yu. Khlopov

The hypothesis of composite $XHe$ dark atoms offers a compelling framework to address the challenges in direct dark matter particles detection, as their neutral, atom-like configuration evades conventional experimental signatures. A…

High Energy Physics - Phenomenology · Physics 2025-12-10 T. E. Bikbaev , M. Yu. Khlopov , A. G. Mayorov

Atomic dark matter is usually considered to be produced asymmetrically in the early Universe. In this work, we first propose that the symmetric atomic dark matter can be thermally produced through the freeze-out mechanism. The dominant atom…

High Energy Physics - Phenomenology · Physics 2026-03-31 Yu-Cheng Qiu , Jie Sheng , Liang Tan , Chuan-Yang Xing