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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

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

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

宇宙学与河外天体物理 · 物理学 2009-12-01 Maxim Yu. Khlopov , Andrey G. Mayorov , Evgeniy Yu. Soldatov

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

Direct searches for dark matter lead to serious problems for simple models with stable neutral Weakly Interacting Massive Particles (WIMPs) as candidates for dark matter. A possibility is discussed that new stable quarks and charged leptons…

宇宙学与河外天体物理 · 物理学 2011-12-06 Maxim Yu. Khlopov

Direct searches for dark matter lead to serious problems for simple models with stable neutral Weakly Interacting Massive Particles (WIMPs) as candidates for dark matter. A possibility is discussed that new stable quarks and charged leptons…

宇宙学与河外天体物理 · 物理学 2017-08-23 Maxim Yu. Khlopov

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

The nonbaryonic dark matter of the Universe can consist of new stable charged leptons and quarks, if they are hidden in elusive "dark atoms" of composite dark matter. Such possibility can be compatible with the severe constraints on…

宇宙学与河外天体物理 · 物理学 2015-05-20 Maxim Yu. Khlopov

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

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

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…

高能物理 - 唯象学 · 物理学 2015-06-18 M. Yu. Khlopov

Heavy stable charged particles can exist, hidden from us in bound atomlike states. Models with new stable charged leptons and quarks give rise to realistic composite dark matter scenarios. Significant or even dominant component of O-helium…

天体物理学 · 物理学 2008-06-25 Maxim Yu. Khlopov

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

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…

高能物理 - 唯象学 · 物理学 2016-01-20 Quentin Wallemacq

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

We consider the model of composite dark matter assuming stable particles of charge $-2$ bound with primordial helium nuclei by Coulomb force in $O$He atoms. We study capture of such dark atoms in matter and propose a possibility of…

高能物理 - 唯象学 · 物理学 2019-01-18 Vakhid A. Gani , Maxim Yu. Khlopov , Dmitry N. Voskresensky

The nonbaryonic dark matter of the Universe is assumed to consist of new stable particles. Stable particle candidates for cosmological dark matter are usually considered as neutral and weakly interacting. However stable charged leptons and…

高能物理 - 唯象学 · 物理学 2017-11-30 O. V. Bulekov , M. Yu. Khlopov , A. S. Romaniouk , Yu. S. Smirnov

The nonbaryonic dark matter of the Universe can consist of new stable double charged particles $O^{--}$, bound with primordial helium in heavy neutral O-helium (OHe)"atoms" by ordinary Coulomb interaction. O-helium dark atoms can play the…

高能物理 - 实验 · 物理学 2011-11-16 Konstantin M. Belostky , Maxim Yu. Khlopov , Konstantin I. Shibaev

The existence of cosmological dark matter is in the bedrock of the modern cosmology. The dark matter is assumed to be nonbaryonic and to consist of new stable particles. However if composite dark matter contains stable electrically charged…

高能物理 - 唯象学 · 物理学 2018-05-02 Maxim Yu. Khlopov

Particle physics candidates for cosmological dark matter are usually considered as neutral and weakly interacting. However stable charged leptons and quarks can also exist and, hidden in elusive atoms, play the role of dark matter. The…

天体物理学 · 物理学 2008-01-03 M. Yu. Khlopov
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