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We calculate the baryon asymmetry created by the decay of a pseudo Nambu-Goldstone boson whose interactions violate baryon number conservation. Our results are in disagreement with previous results in the original spontaneous baryogenesis…

高能物理 - 唯象学 · 物理学 2009-10-30 Alexandre Dolgov , Katherine Freese , Raghavan Rangarajan , Mark Srednicki

We first suggested a scenario in which a generic, dark chiral gauge group undergoes a first order phase transition in order to generate the observed baryon asymmetry in the universe, provide a viable dark matter candidate and explain the…

高能物理 - 唯象学 · 物理学 2012-02-15 Devin G. E. Walker

The radiative neutrino mass model with an inert doublet scalar has been considered as a promising candidate which can explain neutrino masses, dark matter abundance and baryon number asymmetry if dark matter is identified with the lightest…

高能物理 - 唯象学 · 物理学 2015-06-05 Shoichi Kashiwase , Daijiro Suematsu

If there are a plethora of axions in nature, they may have a complicated potential and create an axion landscape. We study a possibility that one of the axions is so light that it is cosmologically stable, explaining the observed dark…

高能物理 - 唯象学 · 物理学 2017-03-03 Ryuji Daido , Takeshi Kobayashi , Fuminobu Takahashi

Effect of the electroweak non-conservation of the baryon number could be a key ingredient to explain the ratio of dark and baryonic densities. If dark matter is explained by dark atoms, in which stable -2n charged particles are bound with n…

高能物理 - 唯象学 · 物理学 2024-01-15 V. A. Beylin , M. Yu. Khlopov , D. O. Sopin

We investigate a theory of $SU(9)$ dark grand unification, where dark matter consists of asymmetric dark baryons from the $Sp(4)_D$ dark QCD sector. By unifying the dark color gauge group with the Standard Model gauge group, the asymmetry…

高能物理 - 唯象学 · 物理学 2026-02-03 Yi Chung

The majoron is a well-motivated light (pseudo-Nambu-Goldstone) boson associated with the spontaneous breaking of a global lepton-number symmetry. In this {\it letter}, we relate the spontaneous breaking scale and its soft-breaking mass by…

高能物理 - 唯象学 · 物理学 2024-06-28 Qiuyue Liang , Xavier Ponce Díaz , Tsutomu T. Yanagida

In supergravity models (such as standard superstring constructions) that possess a Heisenberg symmetry, supersymmetry breaking by the inflationary vacuum energy does not lift flat directions at tree level. One-loop corrections give small…

高能物理 - 唯象学 · 物理学 2009-09-15 Bruce A. Campbell , Mary K. Gaillard , Hitoshi Murayama , Keith A. Olive

The existence of dark matter (DM) and the origin of the baryon asymmetry are persistent indications that the SM is incomplete. More recently, the ATLAS and CMS experiments have observed an excess of diphoton events with invariant mass of…

高能物理 - 唯象学 · 物理学 2016-06-08 Mads T. Frandsen , Ian M. Shoemaker

The available data on large scale structures seem to favour models with mixed dark matter (MDM), i.e. with a hot and cold component in a rather well--defined amount, or with some form of ``warm" dark matter. I discuss some prospects for…

高能物理 - 唯象学 · 物理学 2016-09-01 A. Masiero

Dark and baryonic matter contribute comparable energy density to the present Universe. The dark matter may also be responsible for the cosmic positron/electron excesses. We connect these phenomena with Dirac seesaw for neutrino masses. In…

高能物理 - 唯象学 · 物理学 2009-10-29 Pei-Hong Gu , Utpal Sarkar , Xinmin Zhang

We propose a simple model in which the baryon asymmetry and dark matter are created via the decays and inverse decays of QCD-triplet scalars, at least one of which must be in the TeV mass range. Singlet fermions produced in these decays…

高能物理 - 唯象学 · 物理学 2020-07-01 Brian Shuve , David Tucker-Smith

We consider a model with a small explicit breaking of a global symmetry, as suggested by gravitational arguments. Our model has one scalar field transforming under a non-anomalous U(1) symmetry, and coupled lo matter and to gauge bosons.…

高能物理 - 唯象学 · 物理学 2009-11-10 Eduard Masso , Francesc Rota , Gabriel Zsembinszki

We propose a scenario in which dark energy and dark matter are described in a unified manner. The ultralight pseudo-Nambu-Goldstone (pNG) boson, A, naturally explains the observed magnitude of dark energy, while the bosonic supersymmetry…

高能物理 - 唯象学 · 物理学 2010-11-05 Fuminobu Takahashi , T. T. Yanagida

We study a scenario in which the baryon asymmetry of the universe arises from a cosmological phase transition where lepton-number is spontaneously broken. If the phase transition is first order, a lepton-number asymmetry can arise at the…

高能物理 - 唯象学 · 物理学 2017-11-22 Andrew J. Long , Andrea Tesi , Lian-Tao Wang

The nature of dark matter (DM) particles and the mechanism that provides their measured relic abundance are currently unknown. In this paper we investigate inert scalar and vector like fermion doublet DM candidates with a charge asymmetry…

高能物理 - 唯象学 · 物理学 2015-05-30 Chiara Arina , Narendra Sahu

We consider a supersymmetric model of dark energy coupled to cold dark matter: the supersymmetron. In the absence of cold dark matter, the supersymmetron converges to a supersymmetric minimum with a vanishing cosmological constant. When…

高能物理 - 唯象学 · 物理学 2015-05-30 Philippe Brax , Anne-Christine Davis

We propose a low scale leptogenesis scenario in the framework of composite Higgs models supplemented with singlet heavy neutrinos. One of the neutrinos can also be considered as a dark matter candidate whose stability is guaranteed by a…

高能物理 - 唯象学 · 物理学 2021-04-28 M. Ahmadvand

We discuss a new mechanism for baryogenesis, in which the baryon asymmetry is generated by the lightest particle in another sector, for example the supersymmetric particle (LSP), decaying to quarks via baryonic-number-violating…

高能物理 - 唯象学 · 物理学 2015-05-27 Angelo Monteux , Chang Sub Shin

A novel mechanism for explaining the matter-antimatter asymmetry of the universe is considered. We assume that the universe starts from completely symmetric state and then, as it cools down, it undergoes a quantum-phase transition which in…

宇宙学与河外天体物理 · 物理学 2011-05-31 V. R. Shaginyan , G. S. Japaridze , M. Ya. Amusia , A. Z. Msezane , K. G. Popov
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