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The particle origin of dark matter (DM) remains elusive despite decades of direct, indirect, and collider searches. Several groups have reported a $\gamma$-ray excess toward the Galactic Centre, commonly referred to as the Galactic Centre…

高能物理 - 唯象学 · 物理学 2025-12-01 Jordan Koechler , Mattia Di Mauro

Motivated by the very recent cosmic-ray electron+positron excess observed by DAMPE collaboration, we investigate a Dirac fermion dark matter (DM) in the gauged $L_e - L_\mu$ model. DM interacts with the electron and muon via the…

高能物理 - 唯象学 · 物理学 2018-05-09 Guang Hua Duan , Xiao-Gang He , Lei Wu , Jin Min Yang

We describe a simple model of Dark Matter, which explains the PAMELA/ATIC excesses while being consistent with all present constraints. The DAMA annual modulation signal can also be explained for some values of the parameters. The model…

高能物理 - 唯象学 · 物理学 2010-02-22 Patrick J. Fox , Erich Poppitz

Dark matter annihilation is one of the leading explanations for the recently observed $e^\pm$ excesses in cosmic rays by PAMELA, ATIC, FERMI-LAT and HESS. Any dark matter annihilation model proposed to explain these data must also explain…

高能物理 - 唯象学 · 物理学 2010-04-29 Xiao-Jun Bi , Xiao-Gang He , Ernest Ma , Juan Zhang

Recent data on $e^+/e^-$ and $\bar{p}$ cosmic rays suggest that dark matter annihilate into the standard model (SM) particles through new leptophilic interaction. In this paper, we consider a standard model extension with the gauged…

高能物理 - 唯象学 · 物理学 2011-01-05 Seungwon Baek , Pyungwon Ko

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

Positron excess upto energies $\sim$350 GeV has been observed by AMS-02 result and it is consistent with the positron excess observed by PAMELA upto 100 GeV. There is no observed excess of anti-protons over the expected CR background. We…

高能物理 - 唯象学 · 物理学 2015-06-16 Moumita Das , Subhendra Mohanty

We consider a supersymmetric model with extra $U(1)_B \times U(1)_L$ gauge symmetry that are broken spontaneously. Salient features of this model are that there are three different types of cold dark matter (CDM) candidates, and neutral…

高能物理 - 唯象学 · 物理学 2011-06-28 Pyungwon Ko , Yuji Omura

We present a supersymmetric model with two dark matter (DM) components explaining the galactic positron excess observed by PAMELA/HEAT and ATIC/PPB-BETS: One is the conventional (bino-like) lightest supersymmetric particle (LSP) \chi, and…

高能物理 - 唯象学 · 物理学 2009-08-01 Bumseok Kyae

In this letter, we study the possibility that Kaluza-Klein dark matter in a model with one universal extra dimension is responsible for the recent observations of the PAMELA and ATIC experiments. In this model, the dark matter particles…

高能物理 - 唯象学 · 物理学 2010-04-21 Dan Hooper , Kathryn Zurek

We propose a dark matter model in which the dark sector is gauged under a new SU(2) group. The dark sector consists of SU(2) dark gauge fields, two triplet dark Higgs fields, and two dark fermion doublets (dark matter candidates in this…

高能物理 - 唯象学 · 物理学 2014-11-20 Hao Zhang , Chong Sheng Li , Qing-Hong Cao , Zhao Li

Recently, new data on antiprotons and positrons from PAMELA, e- + e+ spectra from ATIC, FERMI and HESS up to TeV energies all indicate deviations from expectations, which has caused an interesting mix of new explanations, ranging from…

宇宙学与河外天体物理 · 物理学 2014-11-20 Wim de Boer

We propose two supersymmetric Standard Models (SMs) with decaying and stable dark matter (DM) particles. To explain the SM fermion masses and mixings and have a heavy decay DM particle S, we consider the Froggatt-Nielsen mechanism by…

高能物理 - 唯象学 · 物理学 2014-11-20 Xin Gao , Zhaofeng Kang , Tianjun Li

In this work, we have considered a gauged $U(1)_{\rm B-L}$ extension of the Standard Model (SM) with three right handed neutrinos for anomaly cancellation and two additional SM singlet complex scalars with non-trivial B-L charges. One of…

高能物理 - 唯象学 · 物理学 2016-08-23 Anirban Biswas , Sandhya Choubey , Sarif Khan

Either ATIC or Fermi-LAT data can be fitted together with the PAMELA data by three components: primary background ~ E^{-3.3}, secondary background ~ E^{-3.6}, and an additional source of electrons ~ E^{-g_a} Exp(-E/E_{cut}). We find that…

高能天体物理现象 · 物理学 2009-07-30 Dmitry Malyshev

By extending the lepton sector of standard model to include one sterile neutrino and two sets of new Higgs doublets and right-handed neutrinos, denoted by $(\eta_1, N_1, N_3)$ and $(\eta_2, N_2, N_4)$, with two $Z_2$ symmetries, the puzzles…

高能物理 - 唯象学 · 物理学 2009-05-26 Chuan-Hung Chen

We propose a simple model of supersymmetric dark matter that can explain recent results from PAMELA and ATIC experiments. It is based on a U(1)_B-L extension of the minimal supersymmetric standard model. The dark matter particle is a linear…

高能物理 - 唯象学 · 物理学 2011-03-23 Rouzbeh Allahverdi , Bhaskar Dutta , Katherine Richardson-McDaniel , Yudi Santoso

The PAMELA and ATIC collaborations have recently reported an excess in the cosmic ray positron and electron fluxes. These lepton anomalies might be related to cold dark matter (CDM) particles annihilating within a nearby dark matter clump.…

高能天体物理现象 · 物理学 2009-09-01 Pierre Brun , Timur Delahaye , Juerg Diemand , Stefano Profumo , Pierre Salati

In this work, we explore an extension of the Standard Model designed to elucidate the fermion mass hierarchy, account for the dark matter relic abundance, and explain the observed matter-antimatter asymmetry in the universe. Beyond the…

Recently the ATIC and PAMELA collaborations released their results which show the abundant e^\pm excess in cosmic rays well above the background, but not for the \bar{p}. Their data if interpreted as the dark matter particles' annihilation…

高能物理 - 唯象学 · 物理学 2009-06-02 Xiao-Jun Bi , Pei-Hong Gu , Tianjun Li , Xinmin Zhang
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