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相关论文: White dwarf axions, PAMELA data, and flipped-SU(5)

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We are inspired by the facts that M-theory may reconcile the supersymmetric GUT scale with that of quantum gravity, and that it provides new avenues for low-energy supersymmetry breaking, to re-examine a flipped SU(5) model that has been…

高能物理 - 唯象学 · 物理学 2009-09-11 J. Ellis , G. K. Leontaris , S. Lola , D. V. Nanopoulos

The radiatively induced neutrino mass matrix is investigated on the basis of an SU(5) SUSY model. In order to evade the proton decay, an ansatz based on a discrete symmetry $Z_2$ is assumed: although, at the unification scale, we have two…

高能物理 - 唯象学 · 物理学 2007-05-23 Yoshio Koide , Joe Sato

We apply a recently proposed mechanism -- in which an SU(3) symmetry predicts the weak mixing angle -- to construct realistic theories with composite quarks and leptons at a TeV. Although the models are strongly coupled, they are reliably…

高能物理 - 唯象学 · 物理学 2007-05-23 Savas Dimopoulos , David Elazzar Kaplan

The positron excess observed by the PAMELA experiment may come from dark matter annihilation, if the annihilation cross section is large enough. We show that the dark matter annihilation scenarios to explain the positron excess may also be…

高能物理 - 唯象学 · 物理学 2014-11-18 Junji Hisano , Masahiro Kawasaki , Kazunori Kohri , Kazunori Nakayama

We consider the Z5 two-component dark matter model within the framework of the Type-II seesaw mechanism. Due to the new annihilation processes related to triplets, the light component cannot necessarily be dominant in the dark matter relic…

高能物理 - 唯象学 · 物理学 2024-11-19 XinXin Qi , Hao Sun

An extended seesaw model proposed to achieve low scale leptogenesis can resolve the excess positron and electron fluxes observed from PAMELA, ATIC and/or Fermi-LAT, and simultaneously accommodate some of recent experimental results for dark…

高能物理 - 唯象学 · 物理学 2011-06-27 H. S. Cheon , Sin Kyu Kang , C. S. Kim

We propose a simple $SU(5)$ model that connects the neutrino mass generation mechanism to the observed disparity between the masses of charged leptons and down-type quarks. The model is built out of $5$-, $10$-, $15$-, $24$-, and…

高能物理 - 唯象学 · 物理学 2020-01-22 Ilja Doršner , Shaikh Saad

The recent observation by the PAMELA satellite of a rising positron fraction up to $\sim$ 100 GeV has triggered a considerable amount of putative interpretations in terms of dark matter (DM) annihilation or decay. Here, we make a critical…

星系天体物理 · 物理学 2014-11-20 Julien Lavalle

The Pentagon Model is an explicit supersymmetric extension of the Standard Model, which involves a new strongly-interacting SU(5) gauge theory at TeV-scale energies. We show that the Pentagon can be embedded into an SU(5) x SU(5) x SU(5)…

高能物理 - 理论 · 物理学 2009-11-18 T. Banks , S. Echols , J. L. Jones

We investigate the requirement of the existence of two degenerate vacua of the effective potential as a function of the Weinberg-Salam Higgs scalar field norm, as suggested by the multiple point principle, in an extension of the Standard…

高能物理 - 唯象学 · 物理学 2009-11-11 C. R. Das , C. D. Froggatt , L. V. Laperashvili , H. B. Nielsen

Fermion masses and mixing angles including that of neutrinos are studied in a model with symmetry group SUSY $SO(10)\times \Delta (48) \times U(1)$. Universality of Yukawa coupling of superfields is assumed. The resulting texture of mass…

高能物理 - 唯象学 · 物理学 2007-05-23 K. C. Chou , Y. L. Wu

It is pointed out that a class of flipped SU(5) models based on F-theory naturally explains the gauge coupling unification. It is because the group SU(5) x U(1)_X is embedded in SO(10) and E_8. To prohibit the dimension 4 and 5 proton decay…

高能物理 - 理论 · 物理学 2015-05-27 Kang-Sin Choi , Bumseok Kyae

In anomaly-mediated supersymmetry breaking, superpartners in a hidden sector have masses that are proportional to couplings squared, and so naturally freeze out with the desired dark matter relic density for a large range of masses. We…

高能物理 - 唯象学 · 物理学 2014-10-03 Jonathan L. Feng , Vikram Rentala , Ze'ev Surujon

We show that judiciously chosen R-parity violating terms in the minimal renormalizable supersymmetric SU(5) are able to correct all the phenomenologically wrong mass relations between down quarks and charged leptons. The model can…

高能物理 - 唯象学 · 物理学 2015-07-22 Borut Bajc , Luca Di Luzio

A dark matter model which is called w-matter or mirror dark matter is concretely constructed based on (f-SU(5))X(w-SU(5)) symmetry. There is no Higgs field and all masses originate from interactions in the present model. W-matter is dark…

综合物理 · 物理学 2009-12-15 Shi-Hao Chen

We propose a model which unifies the Left-Right symmetry with the $SU(3)_L$ gauge group, called flipped trinification, and based on the $SU(3)_C\otimes SU(3)_L\otimes SU(3)_R\otimes U(1)_X$ gauge group. The model inherits the interesting…

高能物理 - 唯象学 · 物理学 2018-05-23 P. V. Dong , D. T. Huong , Farinaldo S. Queiroz , José W. F. Valle , C. A. Vaquera-Araujo

We use linear response analysis and the fluctuation-dissipation theorem to derive the energy loss of a heavy quark in the SU(2) classical Coulomb plasma in terms of the $l=1$ monopole and non-static structure factor. The result is valid for…

核理论 · 物理学 2011-01-28 Sungtae Cho , Ismail Zahed

We propose a scalar dark matter model featuring a hidden gauge symmetry, denoted as U(1)_X, with two complex scalars, Phi and S. In this framework, Phi spontaneously breaks the U(1)_X gauge symmetry, while S serves as a viable dark matter…

高能物理 - 唯象学 · 物理学 2025-05-20 Yu-Hang Su , Chengfeng Cai , Yu-Pan Zeng , Hong-Hao Zhang

Nonsupersymmetric minimal SU(5) with Higgs representations ${24}_H$ and $5_H$ and standard fermions in ${\bar 5}_F\oplus {10}_F$ is well known for its failure in unification of gauge couplings and lack of predicting neutrino masses. Like…

高能物理 - 唯象学 · 物理学 2018-08-09 Biswonath Sahoo , Mainak Chakraborty , M. K. Parida

The axion, a well-motivated hypothetical particle arising in extensions of the Standard Model, can be produced copiously within the hot, compact cores of white dwarf stars. The shape of the white dwarf luminosity function (WDLF) is a…

太阳与恒星天体物理 · 物理学 2026-03-10 Martín L. Alberino , Marcelo M. Miller Bertolami , María E. Camisassa , Andrea Caputo , Santiago Torres