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相关论文: SU(5) Grand Unified Model and Dark Matter

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We now know firmly that neutrinos have tiny masses, but in the minimal Standard Model there is no natural sources for such tiny masses. On the other hand, the extra heavy Z^{\prime 0} requires the extra Higgs field, the particle generating…

高能物理 - 唯象学 · 物理学 2011-05-30 W-Y. Pauchy Hwang

In this work we investigate the possibility that a simple extension of the Standard Model (SM) can be the dark matter of the universe. We postulate the existence of a scalar field singlet like the Higgs as an extra term in the SM…

广义相对论与量子宇宙学 · 物理学 2014-03-21 Tonatiuh Matos , Ricardo Lopez-Fernandez

We explore the parameter space of a U(1) extension of the standard model -- also called the super-weak model -- from the point of view of explaining the observed dark matter energy density in the Universe. The new particle spectrum contains…

高能物理 - 唯象学 · 物理学 2022-01-25 Sho Iwamoto , Károly Seller , Zoltán Trócsányi

The present matter content of our universe may be governed by a $U(1)_{B-L}$ symmetry -- the simplest gauge completion of the seesaw mechanism which produces small neutrino masses. The matter parity results as a residual gauge symmetry,…

高能物理 - 唯象学 · 物理学 2020-12-15 Phung Van Dong , Duong Van Loi

We construct a model of phantom energy using the graded Lie algebra SU(2/1). The negative kinetic energy of the phantom field emerges naturally from the graded Lie algebra, resulting in an equation of state with w<-1. The model also…

高能物理 - 理论 · 物理学 2008-11-26 Max Chaves , Douglas Singleton

The similar cosmological abundances observed for visible and dark matter suggest a common origin for both. By viewing the dark matter density as a dark-sector asymmetry, mirroring the situation in the visible sector, we show that the…

高能物理 - 唯象学 · 物理学 2012-03-01 Kalliopi Petraki , Mark Trodden , Raymond R. Volkas

One of the most puzzling problems of modern physics is the identification of the nature a non-relativistic matter component present in the universe, contributing to more than 25$\%$ of the total energy budget, known as Dark Matter. Weakly…

高能物理 - 唯象学 · 物理学 2019-01-18 Mathias Pierre

Gauge coupling unification and the success of TeV-scale weakly interacting dark matter are usually taken as evidence of low energy supersymmetry (SUSY). However, if we assume that the tuning of the higgs can be explained in some unnatural…

高能物理 - 唯象学 · 物理学 2009-11-11 Rakhi Mahbubani , Leonardo Senatore

We study a scale invariant $SU(2)\times U(1)_Y \times U(1)_s$ model which has only dimensionless couplings. The shadow $U(1)_s$ is hidden, and it interacts with the Standard Model (SM) solely through mixing in the scalar sector and kinetic…

高能物理 - 唯象学 · 物理学 2008-11-26 We-Fu Chang , John N. Ng , Jackson M. S. Wu

Self-interacting dark matter has been suggested in order to overcome the difficulties of the Cold Dark Matter model on galactic scales. We argue that a scalar gauge singlet coupled to the Higgs boson, leading to an invisibly decaying Higgs,…

天体物理学 · 物理学 2007-05-23 M. C. Bento , O. Bertolami , R. Rosenfeld , L. Teodoro

Scalar fields are favorite among the possible candidates for the dark energy. Most frequently discussed are those with degenerate minima at $\pm \phi_{min}$. In this paper, a slightly modified two-Higgs doublet model is taken to contain the…

高能物理 - 唯象学 · 物理学 2024-07-26 Muhammad Usman , Asghar Qadir

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

We investigate a new type of dark matter with couplings to ordinary matter naturally suppressed by at least one order of magnitude compared to weak interactions. Despite the extra-weak interactions massive particles of this type (XWIMPs)…

高能物理 - 唯象学 · 物理学 2008-11-26 Daniel Feldman , Boris Kors , Pran Nath

A simple model of dark matter contains a light Dirac field charged under a hidden U(1) gauge symmetry. When a chiral matter content in a strong dynamics satisfies the t'Hooft anomaly matching condition, a massless baryon is a natural…

高能物理 - 唯象学 · 物理学 2019-09-04 Ayuki Kamada , Masaki Yamada , Tsutomu T. Yanagida

We study scenarios where Dark Matter is a weakly interacting particle (WIMP) embedded in an ElectroWeak multiplet. In particular, we consider real SU(2) representations with zero hypercharge, that automatically avoid direct detection…

It has recently been pointed out that the 511 keV emission line detected by INTEGRAL/SPI from the bulge of our galaxy could be explained by annihilations of light dark matter particles into $e^+ e^-$. We present the possibility that dark…

高能物理 - 唯象学 · 物理学 2007-05-23 H. N. long , N. Q. Lan , D. V. Soa , L. N. Thuc

Given the lack of empirical evidence of weakly interacting dark matter, it is reasonable to look to other candidates such as a confining dark sector with a similar number of particles as the standard model. Twin Higgs mirror matter is one…

Why matter and dark matter contents of the universe are of the same order of magnitude, is one of the puzzles of modern cosmology. At the face of it, this would seem to point towards a basic similarity between matter and dark matter,…

高能物理 - 唯象学 · 物理学 2025-02-24 Rabindra N. Mohapatra , Nobuchika Okada

We construct a model based on an extra gauge symmetry, SU(2)_X x U(1)_{B-L}, which can provide gauge bosons to serve as weakly-interacting massive particle dark matter. The stability of the dark matter is naturally guaranteed by a discrete…

高能物理 - 唯象学 · 物理学 2014-03-07 Cheng-Wei Chiang , Takaaki Nomura , Jusak Tandean

Dark matter in the universe seems to be one of the most important puzzles science has to face in this moment. In this essay we point out that dark matter could be a spin-0 fundamental interaction of Nature rather than a simple particle.…

天体物理学 · 物理学 2010-12-09 T. Matos , L. A. Urena-Lopez
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