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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…

高能物理 - 唯象学 · 物理学 2025-12-10 T. E. Bikbaev , M. Yu. Khlopov , A. G. Mayorov

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…

高能物理 - 唯象学 · 物理学 2021-11-18 T. E. Bikbaev , M. Yu. Khlopov , A. G. Mayorov

The old and still not solved problem of dark atom solution for the puzzles of direct dark matter searches is related with rigorous prove of the existence of a low energy bound state in the dark atom interaction with nuclei. Such prove must…

高能物理 - 唯象学 · 物理学 2020-11-06 T. E. Bikbaev , M. Yu. Khlopov , A. G. Mayorov

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…

高能物理 - 唯象学 · 物理学 2024-10-18 V. A. Beylin , M. Yu. Khlopov , D. O. Sopin

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…

宇宙学与河外天体物理 · 物理学 2010-11-23 Maxim Yu. Khlopov , Andrey G. Mayorov , Evgeny Yu. Soldatov

The nonbaryonic dark matter of the Universe can consist of new stable charged particles, bound in heavy "atoms" by ordinary Coulomb interaction. If stable particles $O^{--}$ with charge -2 are in excess over their antiparticles (with charge…

高能物理 - 唯象学 · 物理学 2011-11-16 Maxim Yu. Khlopov , Andrey G. Mayorov , Evgeny Yu. Soldatov

Among composite-dark-matter scenarios, one of the simplest and most predictive is that of O-helium (OHe) dark atoms, in which a lepton-like doubly charged particle O is bound with a primordial helium nucleus, and is the main constituent of…

高能物理 - 唯象学 · 物理学 2016-11-18 Jean-René Cudell , Maxim Khlopov , Quentin Wallemacq

A recent composite-dark-matter scenario assumes that the dominant fraction of dark matter consists of O-helium (OHe) dark atoms, in which a lepton-like doubly charged particle O is bound with a primordial helium nucleus. It liberates the…

宇宙学与河外天体物理 · 物理学 2014-01-16 J. R. Cudell , M. Khlopov , Q. Wallemacq

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…

宇宙学与河外天体物理 · 物理学 2015-03-17 Maxim Yu. Khlopov , Andrey G. Mayorov , Evgeny Yu. Soldatov

Minimal walking technicolor models can provide a nontrivial solution for cosmological dark matter, if the lightest technibaryon is doubly charged. Technibaryon asymmetry generated in the early Universe is related to baryon asymmetry and it…

天体物理学 · 物理学 2008-11-26 Maxim Yu. Khlopov , Chris Kouvaris

While the behavior of the dominant component of the dark matter is reasonably well established by cosmological observables, its particle nature and interactions with the rest of the matter are not known. We consider three dark matter models…

宇宙学与河外天体物理 · 物理学 2020-03-24 Gautham A P , Shiv Sethi

The small-scale structure problems of the universe can be solved by self-interacting dark matter that becomes strongly interacting at low energies. A particularly predictive model is resonant short-range self-interactions, with a…

高能物理 - 唯象学 · 物理学 2019-05-14 Eric Braaten , Daekyoung Kang , Ranjan Laha

We investigate the classical motion of three charged particles with both attractive and repulsive interaction.The triple collision is a main source of chaos in such three body Coulomb problems.By employing the McGehee scaling technique, we…

混沌动力学 · 物理学 2009-11-10 Nark Nyul Choi , Min-Ho Lee , Gregor Tanner

Recently it was argued that it might be possible treat the conventional nuclear structure problem -- nonrelativistic point nucleons interacting through a static and rather singular potential -- as an effective theory in a shell-model basis.…

核理论 · 物理学 2009-11-07 W. C. Haxton , T. Luu

We study neutron matter and symmetric nuclear matter with the quark-meson model for the two-nucleon interaction. The Bethe-Bruckner-Goldstone many-body theory is used to describe the correlations up to the three hole-line approximation with…

核理论 · 物理学 2014-12-11 M. Baldo , K. Fukukawa

Positive results of dark matter searches in experiments DAMA/NaI and DAMA/LIBRA confronted with results of other groups can imply nontrivial particle physics solutions for cosmological dark matter. Stable particles with charge -2, bound…

高能物理 - 唯象学 · 物理学 2015-05-20 Maxim Yu. Khlopov , Andrey G. Mayorov , Evgeny Yu. Soldatov

New stable quarks and charged leptons may exist and be hidden from detection, as they are bound by Coulomb interaction in neutral dark atoms of composite dark matter. This possibility leads to fundamentally new types of indirect effects…

高能天体物理现象 · 物理学 2014-12-01 Jean-René Cudell , Maxim Yu. Khlopov , Quentin Wallemacq

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…

宇宙学与河外天体物理 · 物理学 2014-11-20 Maxim Yu. Khlopov

Cold dark matter (DM) scenario may be cured of several problems by involving self-interaction of dark matter. Viability of the models of long-range interacting DM crucially depends on the effectiveness of recombination of the DM particles,…

宇宙学与河外天体物理 · 物理学 2016-09-06 K. M. Belotsky , E. A. Esipova , A. A. Kirillov

This work describes a few-body dynamics method based on the Faddeev integral equations in momentum space for determining the total cross sections of fusion and breakup reactions with two- and three-body final channels in the continuum,…

核理论 · 物理学 2026-04-27 Mikhail Egorov
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