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相关论文: Neutralino Annihilation into Two Photons

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A full one-loop calculation of neutralino S-wave annihilation into the $Z\gamma$ final state is performed in the minimal supersymmetric extension of the Standard Model. This process, like the similar one with two photons in the final state,…

高能物理 - 唯象学 · 物理学 2010-11-30 P. Ullio , L. Bergstrom

We calculate the flux of cosmic gamma rays expected {}from the annihilation of neutralinos in the Galactic halo. Our calculation of the annihilation cross section to two photons improves the existing calculations by inclusion of exact…

高能物理 - 唯象学 · 物理学 2016-09-01 Gerard Jungman , Marc Kamionkowski

The neutralino pair annihilation into two photons in our galactic halo gives a robust dark matter signal, since it would give a quasi-monotonic gamma ray. This process is radiatively-induced, and the full-one loop calculation was done…

高能物理 - 唯象学 · 物理学 2009-11-07 Junji Hisano , Sh. Matsumoto , Mihoko M. Nojiri

We revisit the one-loop calculation of the annihilation of a pair of the lightest neutralinos into a pair of photons, a pair of gluons and also a Z photon final state. For the latter we have identified a new contribution that may not always…

高能物理 - 唯象学 · 物理学 2011-07-19 F. Boudjema , A. Semenov , D. Temes

We present a complete calculation of the cross section for neutralino annihilation into the two-gluon final state. This channel can be quite important for the phenomenology of neutralino annihilation due to the well-known helicity…

高能物理 - 唯象学 · 物理学 2009-10-22 M. Drees , G. Jungman , M. Kamionkowski , M. Nojiri

For the first time, a full one-loop calculation of the process $\chi\chi\to 2\gamma$ is performed, where $\chi$ is the lightest neutralino in the minimal supersymmetric extension of the Standard Model. This process is of interest for dark…

高能物理 - 唯象学 · 物理学 2009-10-30 L. Bergstrom , P. Ullio

Assuming that the underlying model satisfies some general requirements such as renormalizability and CP conservation, we calculate the non-relativistic one-loop cross section for any self-conjugate dark matter particle annihilating into two…

高能物理 - 唯象学 · 物理学 2017-10-30 Camilo Garcia-Cely , Andres Rivera

We explore the prospects for indirect detection of neutralino dark matter in supersymmetric models with an extended Higgs sector (NMSSM). We compute, for the first time, one-loop amplitudes for NMSSM neutralino pair annihilation into two…

高能物理 - 唯象学 · 物理学 2008-11-26 Francesc Ferrer , Lawrence M. Krauss , Stefano Profumo

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 complete 1-loop computation of the processes $(\tchi^0_i \tchi^0_j \leftrightarrow\gamma\gamma, ~ gg)$, for any pair of the four MSSM neutralinos, has been performed for an arbitrary c.m energy. As a first application suitable for Dark…

高能物理 - 唯象学 · 物理学 2011-07-19 G. J. Gounaris , J. Layssac , P. I. Porfyriadis , F. M. Renard

We compute the pair annihilation cross section of light (spin-0) dark matter particles into two photons and discuss the detectability of the monochromatic line associated with these annihilations.

天体物理学 · 物理学 2008-11-26 C. Boehm , J. Orloff , P. Salati

We consider a model for neutralino dark matter candidates arising in anomaly-mediated supersymmetry breaking schemes, and examine its testability through the search for exotic cosmic rays produced by neutralino pair annihilations in the…

高能物理 - 唯象学 · 物理学 2010-02-03 Piero Ullio

We compute the pair annihilation cross section of light dark matter scalar particles into two photons, and discuss the detectability of the monochromatic line associated with these annihilations.

天体物理学 · 物理学 2008-05-09 Jean Orloff

The annihilations of neutralino dark matter (or other dark matter candidate) generate, among other Standard Model states, electrons and positrons. These particles emit synchrotron photons as a result of their interaction with the Galactic…

高能物理 - 唯象学 · 物理学 2008-11-26 Dan Hooper

We investigate the possibility to detect neutralino dark matter in a scenario in which the galactic dark halo is clumpy. We find that under customary assumptions on various astrophysical parameters, the antiproton and continuum gamma-ray…

天体物理学 · 物理学 2009-10-30 L. Bergstrom , J. Edsjo , P. Gondolo , P. Ullio

Recent advances in N-body simulations of cold dark matter halos point to a substantial density enhancement near the center. This means that, e.g., the $\gamma$ ray signals from neutralino dark matter annihilations would be significantly…

天体物理学 · 物理学 2010-11-30 L. Bergstrom , P. Ullio , J. Buckley

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

Motivated by recent claims of lines in the Fermi gamma-ray spectrum, we critically examine means of enhancing neutralino annihilation into neutral gauge bosons. The signal can be boosted while remaining consistent with continuum photon…

高能物理 - 唯象学 · 物理学 2015-06-12 Guillaume Chalons , Matthew J. Dolan , Christopher McCabe

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

Little Higgs models with T parity contain an attractive dark matter candidate, the heavy photon. We compute the cross section of the heavy photon annihilation into Z-photon pairs, which turns out to be substantially higher than the…

高能物理 - 唯象学 · 物理学 2008-11-26 Maxim Perelstein , Andrew Spray
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