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We investigate the Q-ball decay in the gauge-mediated SUSY breaking. Q balls decay mainly into nucleons, and partially into gravitinos, while they are kinematically forbidden to decay into sparticles which would be cosmologically harmful.…

高能物理 - 唯象学 · 物理学 2015-05-28 Shinta Kasuya , Masahiro Kawasaki

The gauge-mediated model of supersymmetry breaking implies that stable non-topological solitons, Q-balls, could form in the early universe and comprise the dark matter. It is shown that the inclusion of the effects from gravity-mediation…

高能物理 - 唯象学 · 物理学 2009-09-02 Ian M. Shoemaker

We show that the recently reported anomalies in $b\to s\mu^+\mu^-$ transitions, as well as the long-standing $g_\mu-2$ discrepancy, can be addressed simultaneously by a new massive abelian gauge boson with loop-induced coupling to muons.…

高能物理 - 唯象学 · 物理学 2015-09-23 Geneviève Bélanger , Cédric Delaunay , Susanne Westhoff

Supersymmetric extensions of the Standard Model contain non-topological solitons, Q-balls, which can be stable and can be a form of cosmological dark matter. Understanding the interaction of SUSY Q-balls with matter fermions is important…

高能物理 - 唯象学 · 物理学 2009-11-10 Alexander Kusenko , Lee Loveridge , Mikhail Shaposhnikov

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…

宇宙学与河外天体物理 · 物理学 2015-05-18 Maxim Yu. Khlopov , Andrey G. Mayorov , Evgeny Yu. Soldatov

Supersymmetric extensions of the standard model predict the existence of non-topological solitons, $Q$-balls. Assuming the standard cosmological history preceded by inflation, $Q$-balls can form in the early universe and can make up the…

高能物理 - 唯象学 · 物理学 2017-01-04 Eric Cotner , Alexander Kusenko

Theories with low-energy supersymmetry predict the existence of stable non-topological solitons, Q-balls, that can contribute to dark matter. We discuss the experimental signatures, methods of detection, and the present limits on such dark…

高能物理 - 唯象学 · 物理学 2011-05-05 Alexander Kusenko , Vadim Kuzmin , Mikhail Shaposhnikov , P. G. Tinyakov

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

We report on the possibility that the Dark Matter particle is a stable, neutral, as-yet-undiscovered hadron in the standard model. The existence of a compact color-flavor-spin singlet sexaquark (S, uuddss) with mass ~2m_p, is compatible…

高能物理 - 唯象学 · 物理学 2022-01-17 Glennys R. Farrar , Zihui Wang , Xingchen Xu

We consider a model in which dark matter is a composite baryon of a dark sector governed by $SU(3)$ gauge theory, with vector-like quarks also charged under $U(1)_Y$. The model provides simple answer to the dark matter stability problem: it…

高能物理 - 唯象学 · 物理学 2016-10-21 Ran Huo , Shigeki Matsumoto , Yue-Lin Sming Tsai , Tsutomu T. Yanagida

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

Dark matter is postulated to be a neutral Dirac fermion, charged under a dark $U(1)_D$ gauge symmetry. Scalar partners of the quarks and leptons are also charged under $U(1)_D$. The dark gauge boson $Z_D$ and the dark Higgs boson $h_D$…

高能物理 - 唯象学 · 物理学 2022-07-06 Ernest Ma

We propose a model for dark matter and dark radiation, based on a strongly-coupled dark ${\rm SU}(5)$ gauge theory with fundamental and decuplet dark-quarks. The model supports light dark-baryons, respecting the chiral symmetry, which are…

高能物理 - 唯象学 · 物理学 2020-11-13 Deog Ki Hong

If dark matter (DM) contains equal numbers of u,d,s quarks, the ratio of DM and ordinary matter densities is shown to follow from the Boltzmann distribution in the Quark Gluon Plasma. For sexaquark DM in the 1860-1880 MeV mass range…

高能物理 - 唯象学 · 物理学 2022-01-17 Glennys R. Farrar

We revisit constraints on dark matter that is charged under a $U(1)$ gauge group in the dark sector, decoupled from Standard Model forces. We find that the strongest constraints in the literature are subject to a number of mitigating…

高能物理 - 唯象学 · 物理学 2017-08-08 Prateek Agrawal , Francis-Yan Cyr-Racine , Lisa Randall , Jakub Scholtz

If dark matter particles have an electric charge, as in models of millicharged dark matter, such particles should be accelerated in the same astrophysical accelerators that produce ordinary cosmic rays, and their spectra should have a…

高能物理 - 唯象学 · 物理学 2017-03-02 Ping-Kai Hu , Alexander Kusenko , Volodymyr Takhistov

The origin and composition of the cosmological dark matter remain a mystery. However, upcoming 21-cm measurements during cosmic dawn, the period of the first stellar formation, can provide new clues on the nature of dark matter. During this…

宇宙学与河外天体物理 · 物理学 2018-06-05 Julian B. Muñoz , Abraham Loeb

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

Though widely accepted, it is not proven that supermassive compact objects (SMCOs) residing in galactic centers are black holes. In particular, the Milky Way's SMCO can be a giant nontopological soliton, Q-ball, made of a scalar field: this…

高能物理 - 唯象学 · 物理学 2016-11-15 Sergey Troitsky

Dark matter (DM) could be a relic of freeze-in through a light mediator, where the DM is produced by extremely feeble, IR-dominated processes in the thermal Standard Model plasma. In the simplest viable models with the DM mass below the MeV…

宇宙学与河外天体物理 · 物理学 2021-09-15 Cora Dvorkin , Tongyan Lin , Katelin Schutz