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相关论文: Gamma-ray signatures for Kaluza-Klein dark matter

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A leading hypothesis for the nature of the elusive dark matter are thermally produced, weakly interacting massive particles that arise in many theories beyond the standard model of particle physics. Their self-annihilation in astrophysical…

高能物理 - 唯象学 · 物理学 2017-08-23 Torsten Bringmann

Monochromatic gamma ray lines have long been known to provide potential smoking gun signals for annihilating dark matter. Here, we demonstrate that the situation is particularly interesting for Kaluza-Klein dark matter because resonant…

高能物理 - 唯象学 · 物理学 2014-10-13 Chiara Arina , Torsten Bringmann , Joseph Silk , Martin Vollmann

Indirect Dark Matter searches are based on the observation of secondary particles produced by the annihilation or decay of Dark Matter. Among them, gamma-rays are perhaps the most promising messengers, as they do not suffer deflection or…

高能天体物理现象 · 物理学 2013-08-07 Gianfranco Bertone , C. B. Jackson , Gabe Shaughnessy , Tim M. P. Tait , Alberto Vallinotto

High energy gamma-rays and neutrinos can be produced both by the annihilation and by the possible slow decay of dark matter particles. We discuss the fluxes and spectra of such secondaries produced by dark matter particles in the universe…

天体物理学 · 物理学 2009-10-28 F. W. Stecker

Recent studies have suggested the possibility that the lightest supersymmetric particle is a suitable dark matter candidate. In this theoretical framework, annihilations in high density environments like the center of dark matter haloes may…

天体物理学 · 物理学 2007-05-23 Lidia Pieri , Enzo Branchini

With the growing interest in indirect detection for dark matter signature, the thesis aims to investigate the signal originating from the self-annihilation of dark matter candidates. The methods for targeting the dark matter signal are…

高能天体物理现象 · 物理学 2022-09-01 Pooja Bhattacharjee

We describe cosmic gamma-ray and neutrino signals of dark matter annihilation, explaining how the complementarity of these signals provides additional information that, if observable, can enlighten the particle nature of dark matter. This…

高能物理 - 唯象学 · 物理学 2013-05-30 Rouzbeh Allahverdi , Sheldon Campbell , Bhaskar Dutta

Neutralino dark matter can be indirectly detected by observing the gamma ray lines from the annihilation processes XX-->gg and XX-->gZ. In this paper we study the implications that the observation of these two lines could have for the…

高能物理 - 唯象学 · 物理学 2010-01-08 Carlos E. Yaguna

Dark matter candidates such as weakly-interacting massive particles are predicted to annihilate or decay into Standard Model particles leaving behind distinctive signatures in gamma rays, neutrinos, positrons, antiprotons, or even…

高能天体物理现象 · 物理学 2017-06-01 Jan Conrad , Olaf Reimer

We propose a new signature for weakly interacting massive particle (WIMP) dark matter, a spectral feature in the diffuse extragalactic gamma-ray radiation. This feature, a sudden drop of the gamma-ray intensity at an energy corresponding to…

天体物理学 · 物理学 2010-04-06 Lars Bergstrom , Joakim Edsjo , Piero Ullio

We propose that cold dark matter is made of Kaluza-Klein particles and explore avenues for its detection. The lightest Kaluza-Klein state is an excellent dark matter candidate if standard model particles propagate in extra dimensions and…

高能物理 - 唯象学 · 物理学 2009-10-09 Hsin-Chia Cheng , Jonathan L. Feng , Konstantin T. Matchev

We consider neutralino annihilation in dense extragalactic systems known to be dominated by dark matter, in particular M87 and several local dwarf spheroidal galaxies. These annihilations can produce energetic gamma rays which may be…

天体物理学 · 物理学 2008-11-26 E. A. Baltz , C. Briot , P. Salati , R. Taillet , J. Silk

The lightest Kaluza-Klein particle (LKP), which appears in the theory of universal extra dimensions, is one of the good candidates for cold dark matter. The gamma-ray spectrum from annihilation of LKP dark matter shows a characteristic peak…

高能天体物理现象 · 物理学 2015-02-10 Satoshi Tsuchida , Masaki Mori

We use high resolution numerical simulations of the formation of cold dark matter halos to simulate the background of decay products from neutralino annihilation, such as gamma-rays or neutrinos. Halos are non-spherical, have steep singular…

天体物理学 · 物理学 2008-11-26 Carlos Calcaneo-Roldan , Ben Moore

The instability of dark matter may produce visible signals in the spectrum of cosmic gamma-rays. We consider this possibility in frameworks with additional spatial dimensions and supersymmetry. Examples of particles include…

天体物理学 · 物理学 2011-11-10 Jose A. R. Cembranos , Jonathan L. Feng , Louis E. Strigari

In this talk I contrast three different particle dark matter candidates, all motivated by new physics beyond the Standard Model: supersymmetric dark matter, Kaluza-Klein dark matter, and scalar dark matter. I then discuss the prospects for…

高能物理 - 唯象学 · 物理学 2009-10-09 Konstantin Matchev

High resolution simulations reveal that in the cold dark matter scenario the structures form hierarchically and a large number of substructures survive in the galactic halos. The substructures can be probed if they emit gamma rays via dark…

天体物理学 · 物理学 2009-11-13 Xiao-Jun Bi

If dark matter (DM), which is considered to constitute most of the mass of galaxies, is made of supersymmetric (SUSY) particles, the centers of galaxies should emit gamma-rays produced by their self-annihilation. We present accurate…

天体物理学 · 物理学 2008-11-26 Francisco Prada , Anatoly Klypin , J. Flix , M. Martinez , E. Simonneau

We discuss a simple theory for physics beyond the Standard Model where a Majorana dark matter is predicted from anomaly cancellation. We discuss in detail the minimal theory where the baryon number is a local symmetry spontaneously broken…

高能物理 - 唯象学 · 物理学 2025-04-01 Hridoy Debnath , Pavel Fileviez Perez , Kevin Gonzalez-Quesada

We consider the gamma-ray spectrum from neutralino dark matter annihilations and show that internal bremsstrahlung of W pair final states gives a previously neglected source of photons at energies near the mass of the neutralino. For masses…

高能物理 - 唯象学 · 物理学 2009-11-11 Lars Bergstrom , Torsten Bringmann , Martin Eriksson , Michael Gustafsson
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