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Related papers: Soft Gamma Rays from Heavy WIMPs

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We consider a twin WIMP scenario whose twin sector contains a full dark copy of the SM hadrons, where the lightest twin particles are twin pions. By analogy to the standard WIMP paradigm, the dark matter (DM) freezes out through twin…

High Energy Physics - Phenomenology · Physics 2016-05-25 Marat Freytsis , Simon Knapen , Dean J. Robinson , Yuhsin Tsai

Recently the study of anomalous gamma-ray emission in the regions surrounding the galactic center has drawn a lot of attention as it points out that the excess of $\sim 1-3$ GeV gamma-ray in the low latitude is consistent with the emission…

High Energy Physics - Phenomenology · Physics 2015-04-09 Tanushree Basak , Tanmoy Mondal

The recently observed excess in gamma-ray signal near the Galactic center suggests that dark matter particles may annihilate into charged fermions that produce gamma-ray to be observed. In this paper, we consider a leptonic dark matter,…

High Energy Physics - Phenomenology · Physics 2016-09-29 Jongkuk Kim , Jong-Chul Park , Seong Chan Park

It has been recently pointed out that the excess of the gamma ray spectrum in the Fermi Bubbles at low latitude can be well explained by the annihilation of dark matter particles. The best-fit candidate corresponds to the annihilation of a…

High Energy Physics - Phenomenology · Physics 2015-06-17 Nobuchika Okada , Osamu Seto

Motivated by the absence, so far, of any direct signal of conventional low-energy supersymmetry, we explore the consequences of making the lightest Higgs boson in supersymmetry relatively heavy, up to about 300 GeV, in the most…

High Energy Physics - Phenomenology · Physics 2008-11-26 Riccardo Barbieri , Lawrence J. Hall , Yasunori Nomura , Vyacheslav S. Rychkov

We propose a comprehensive theory of dark matter that explains the recent proliferation of unexpected observations in high-energy astrophysics. Cosmic ray spectra from ATIC and PAMELA require a WIMP with mass M_chi ~ 500 - 800 GeV that…

High Energy Physics - Phenomenology · Physics 2009-02-26 Nima Arkani-Hamed , Douglas P. Finkbeiner , Tracy R. Slatyer , Neal Weiner

Current cosmological models and data suggest the existence of a cold Dark Matter (DM) component, however the nature of DM particles remains unknown. A favored candidate for DM is a Weakly Interacting Massive Particle (WIMP) in the mass…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Benjamin Zitzer

We study the decay of a heavy CP-even neutral Higgs into an on-shell Standard Model-like Higgs boson and two photons, $H\to h\gamma\gamma$, in the two-Higgs doublet model. We argue that the decay channel $H\to h\gamma\gamma$, followed by…

High Energy Physics - Phenomenology · Physics 2025-07-10 M. A. Arroyo-Ureña , Alejandro Ibarra , Pablo Roig , T. Valencia-Pérez

We explore modifications to the loop-induced Higgs couplings h\gamma\gamma\ and h\gamma Z from light charginos in the Minimal Supersymmetric Standard Model. When the lightest chargino mass is above the naive LEP bound of order 100 GeV the…

High Energy Physics - Phenomenology · Physics 2015-06-17 Brian Batell , Sunghoon Jung , Carlos E. M. Wagner

Dark matter particles annihilating into Standard Model fermions may be able to explain the recent observation of a gamma-ray excess in the direction of the Galactic Center. Recently, a hidden photon model has been proposed to explain this…

High Energy Physics - Phenomenology · Physics 2015-06-04 Samuel D. McDermott

The possibility of a light charged Higgs boson $H^\pm$ that decays predominantly to quarks ($cs$ and/or $cb$) and with a mass in the range 80 GeV $\le m_{H^\pm} \le 90$ GeV is studied in the context of Three-Higgs-Doublet Models (3HDMs). At…

High Energy Physics - Phenomenology · Physics 2018-12-26 A. G. Akeroyd , Stefano Moretti , Muyuan Song

Natural models of supersymmetry with a gravitino LSP provide distinctive signatures at the LHC. For a neutralino NLSP, sparticles can decay to two high energy photons plus missing energy. We use the ATLAS diphoton search with 4.8 fb^{-1} of…

High Energy Physics - Phenomenology · Physics 2013-05-30 James Barnard , Benjamin Farmer , Tony Gherghetta , Martin White

The spontaneous breaking of B-L symmetry naturally accounts for the small observed neutrino masses via the seesaw mechanism. We have recently shown that the cosmological realization of B-L breaking in a supersymmetric theory can…

High Energy Physics - Phenomenology · Physics 2012-07-19 Wilfried Buchmüller , Valerie Domcke , Kai Schmitz

Taking a bottom-up point of view and focussing on the lack of signals so far in the Higgs and in the flavour sectors, we argue in favour of giving consideration to supersymmetric extensions of the Standard Model where the lightest Higgs…

High Energy Physics - Phenomenology · Physics 2010-09-02 Riccardo Barbieri , Enrico Bertuzzo , Marco Farina , Paolo Lodone , Duccio Pappadopulo

The EGRET telescope has identified a gamma-ray source at the Galactic center. We point out here that the spectral features of this source are compatible with the gamma-ray flux induced by pair annihilations of dark matter weakly interacting…

A numerical calculation of properties of finite absorbers and of intergalactic medium based on photoionization equilibrium is performed to confront alternative UV sources in addition to quasars. It is seen that a spectrum including a large…

Astrophysics · Physics 2010-11-30 L. Masperi , S. Savaglio

Recently, the CoGeNT collaboration reported the WIMP candidate signal events exceeding the known backgrounds where the light WIMP with large cross section is supported. Motivated by this issue, we analyze a light neutralino dark matter…

High Energy Physics - Phenomenology · Physics 2010-12-30 Kyu Jung Bae , Hyung Do Kim , Seodong Shin

Excesses of Galactic gamma rays in the 1-100 GeV region observed by EGRET and by WMAP have been interpreted as signals of dark matter (LSP) annihilation. We argue that the excess of TeV gamma rays from the Galactic center observed by…

Astrophysics · Physics 2007-05-23 Matts Roos

Galactic weakly interacting massive particles (WIMPs) may scatter off solar nuclei to orbits gravitationally bound to the Sun. Once bound, the WIMPs continue to lose energy by repeated scatters in the Sun, eventually leading to complete…

High Energy Astrophysical Phenomena · Physics 2010-04-29 Sofia Sivertsson , Joakim Edsjo

The diffuse galactic EGRET gamma ray data show a clear excess for energies above 1 GeV in comparison with the expectations from conventional galactic models. The excess is seen with the same spectrum in all sky directions, as expected for…

High Energy Physics - Phenomenology · Physics 2009-11-10 W. de Boer
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