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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

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…

Cosmology and Nongalactic Astrophysics · Physics 2017-08-23 Maxim Yu. Khlopov

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…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-20 Maxim Yu. Khlopov

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…

High Energy Physics - Phenomenology · Physics 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…

Astrophysics · Physics 2008-01-03 M. Yu. Khlopov

A widely accepted viewpoint is to consider candidates for cosmological dark matter as neutral and weakly interacting particles, as well as to consider only light elements in the pregalactic chemical composition. It is shown that stable…

Astrophysics · Physics 2008-01-03 M. 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…

Cosmology and Nongalactic Astrophysics · Physics 2011-12-06 Maxim Yu. Khlopov

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…

High Energy Physics - Phenomenology · Physics 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…

High Energy Physics - Phenomenology · Physics 2017-11-30 O. V. Bulekov , M. Yu. Khlopov , A. S. Romaniouk , Yu. S. Smirnov

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

It was recently proposed that stable particles of charge $-2$, $O^{--}$, can exist and constitute dark matter after they bind with primordial helium in O-helium (OHe) atoms. We study here in details the possibility that this model provides…

High Energy Physics - Phenomenology · Physics 2014-01-22 Jean-René Cudell , Maxim Yu. 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…

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

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

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…

High Energy Physics - Phenomenology · Physics 2016-11-18 Jean-René Cudell , Maxim Khlopov , 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…

High Energy Astrophysical Phenomena · Physics 2014-12-01 Jean-René Cudell , Maxim Yu. Khlopov , Quentin Wallemacq

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…

High Energy Physics - Experiment · Physics 2011-11-16 Konstantin M. Belostky , Maxim Yu. Khlopov , Konstantin I. Shibaev

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

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

Composite dark matter is a natural setting for implementing inelastic dark matter - the O(100 keV) mass splitting arises from spin-spin interactions of constituent fermions. In models where the constituents are charged under an axial U(1)…

High Energy Physics - Phenomenology · Physics 2014-11-20 Daniele S. M. Alves , Siavosh R. Behbahani , Philip Schuster , Jay G. Wacker

We present a scenario where dark matter is in the form of dark atoms that can accomodate the experimentally observed excess of positrons in PAMELA and AMS-02 while being compatible with the constraints imposed on the gamma-ray flux from…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-12 Konstantin Belotsky , Maxim Khlopov , Chris Kouvaris , Maxim Laletin
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