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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…

高能物理 - 唯象学 · 物理学 2015-06-10 Konstantin Belotsky , Maxim Khlopov , Maxim Laletin

We suggest a new left-right symmetric grand unified model by extending Pati-Salam group to contain an isospin SU(2) and a flavor SO(3) subgroup, where the superheavy fermions are introduced as a mirror to the low-energy standard model…

高能物理 - 唯象学 · 物理学 2009-07-22 Wei-Min Yang , Hong-Huan Liu

This Letter proposes a new search for confining dark sectors at the Large Hadron Collider. As a result of the strong dynamics in the hidden sector, dark matter could manifest in proton-proton collisions at the Large Hadron Collider in form…

高能物理 - 唯象学 · 物理学 2022-09-07 Cesare Cazzaniga , Annapaola de Cosa

We consider a simple extension of the Standard Model that can account for the dark matter and explain the existence of neutrino masses. The model includes a vector-like doublet of SU(2), a singlet fermion, and two scalar singlets, all of…

高能物理 - 唯象学 · 物理学 2016-02-17 Michael Klasen , David R. Lamprea , Carlos E. Yaguna

We discuss a simple non-supersymmetric model based on the electroweak gauge group $SU(2)_L\times SU(2)^\prime\times U(1)_{B-L}$ where the lightest of the right-handed neutrinos, which are part of the leptonic doublet of $SU(2)^\prime$, play…

高能物理 - 唯象学 · 物理学 2016-08-22 P. S. Bhupal Dev , D. Kazanas , R. N. Mohapatra , V. L. Teplitz , Yongchao Zhang

We present a model based on the $SU(3)_C\otimes SU(3)_L\otimes U(1)_X$ gauge symmetry that relates the mass hierarchy of the fermions with the solution to the strong CP problem through the $U(1)_{PQ}$ Peccei-Quinn symmetry. This last…

高能物理 - 唯象学 · 物理学 2018-12-19 A. G. Dias , J. Leite , D. D. Lopes , C. C. Nishi

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

All pieces of concrete evidence for phenomena outside the standard model (SM) - neutrino masses and dark matter - are consistent with the existence of new degrees of freedom that interact very weakly, if at all, with those in the SM. We…

高能物理 - 唯象学 · 物理学 2017-10-18 Jeffrey M. Berryman , André de Gouvêa , Kevin J. Kelly , Yue Zhang

The Large Hadron electron Collider (LHeC) has been designed to push the field of deep inelastic scattering to the high energy and intensity frontier using an intense electron beam with a proton beam from the High Luminosity-Large Hadron…

高能物理 - 唯象学 · 物理学 2023-05-17 Guo-yuan Huang , Sudip Jana , Alvaro S. de Jesus , Farinaldo S. Queiroz , Werner Rodejohann

While the SUSY flavor, CP and gravitino problems seem to favor a very heavy spectrum of matter scalars, fine-tuning in the electroweak sector prefers low values of superpotential mass \mu. In the limit of low \mu, the two lightest…

高能物理 - 唯象学 · 物理学 2015-05-28 Howard Baer , Vernon Barger , Peisi Huang

One of the great attractions of minimal super-unified supersymmetric models is the prediction of a massive, stable, weakly interacting particle (the lightest supersymmetric partner, LSP) which can have the right relic abundance to be a cold…

高能物理 - 唯象学 · 物理学 2016-09-01 E. Diehl , G. Kane , C. Kolda , J. Wells

We propose a new physics model which has a cold dark matter candidate and can explain the $b \to s \mu^+\mu^-$ anomaly at the same time. Our model includes a scalar quark $\widetilde{q}$ and a scalar lepton $\widetilde{\ell}$ which are…

高能物理 - 唯象学 · 物理学 2018-11-12 Seungwon Baek , Chaehyun Yu

We give a model for composite quarks and leptons based on the semisimple gauge group SU(4), with the preons in the 10 representation; this choice of gauge gluon and preon multiplets is motivated by the possibility of embedding them in an…

高能物理 - 理论 · 物理学 2016-09-06 Stephen L. Adler

We show that models with exotic leptons transforming as E ~ (1,3,-1) under the standard model gauge symmetry are well suited for generating neutrino mass via a radiative inverse seesaw. This approach realizes natural neutrino masses and…

高能物理 - 唯象学 · 物理学 2015-06-04 Sandy S. C. Law , Kristian L. McDonald

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…

天体物理学 · 物理学 2007-05-23 Maxim Yu. Khlopov

Since there are dark matter particles (neutrino) with mass about 10^(-1)eV in the universe, the superstructures with a scale of 10^(19) solar mass [large number A is about 10^(19)] appeared around the era of the hydrogen recombination. The…

天体物理学 · 物理学 2016-09-14 Wuliang Huang , Xiaodong Huang

A recent study of gamma-ray data from the Galactic Center motivates the investigation of light (~7-10 GeV) particle dark matter models featuring tau lepton pairs as dominant annihilation final state. The Lepton-Specific two-Higgs-doublet…

高能物理 - 唯象学 · 物理学 2015-05-28 M. S. Boucenna , S. Profumo

We report a recent study on lepton masses within a beyond standard model with a SU(3) family symmetry model. In this scenario ordinary heavy fermions, top and bottom quarks and tau lepton become massive at tree level from Dirac See-saw…

高能物理 - 唯象学 · 物理学 2012-12-20 Albino Hernandez-Galeana

The significant excess of events recently found by the H1 and ZEUS Collaborations at HERA in the deep-inelastic e^+ p scattering for high momentum-transfers squared Q^2>15000 GeV^2 over the expectation of the standard model can be explained…

高能物理 - 唯象学 · 物理学 2009-12-30 Keiichi Akama , Kazuo Katsuura , Hidezumi Terazawa

SO(10) grand unified theories can ensure the stability of new particles in terms of the gauge group structure itself, and in this respect are well suited to accommodate dark matter (DM) candidates in the form of new stable massive…

高能物理 - 唯象学 · 物理学 2016-03-23 Sofiane M. Boucenna , Martin B. Krauss , Enrico Nardi