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We compute the annihilation cross-section of two neutralinos at rest into two photons, which is of importance for the indirect detection of neutralino dark matter in the galactic halo through a quasi-monochromatic gamma-ray line. We include…

高能物理 - 唯象学 · 物理学 2008-11-26 Z. Bern , P. Gondolo , M. Perelstein

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 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

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

The lightest neutralino of R-parity conserving supersymmetric models serves as a compelling candidate to account for the presence of cold dark matter in the universe. In the minimal supergravity (mSUGRA) model, a relic density can be found…

高能物理 - 唯象学 · 物理学 2009-11-10 Howard Baer , Jorge O' Farrill

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

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 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 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

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 have computed the loop-induced processes of neutralino annihilation into two photons and, for the first time, into a photon and a Z boson in the framework of the NMSSM. The photons produced from these radiative modes are monochromatic…

高能物理 - 唯象学 · 物理学 2011-12-20 G. Chalons , A. Semenov

We consider extensions of the standard model based on open strings ending on D-branes, in which gauge bosons and their associated gauginos exist as strings attached to stacks of D-branes, and chiral matter exists as strings stretching…

高能物理 - 唯象学 · 物理学 2010-05-12 Luis A. Anchordoqui , Haim Goldberg , Dan Hooper , Danny Marfatia , Tomasz R. Taylor

The 1-loop computation of the processes $\tchi_i \tchi_j \to \gamma Z$ has been performed at an arbitrary c.m. energy for any pair of MSSM neutralinos. As an application suitable for Dark Matter (DM) searches, the neutralino-neutralino…

高能物理 - 唯象学 · 物理学 2009-11-11 Th. Diakonidis , G. J. Gounaris , J. Layssac , P. I. Porfyriadis , F. M. Renard

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

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

We consider the lightest supersymmetric particle (LSP), neutralino in minimal anomaly mediated supersymmetry breaking model (mAMSB) to be a possible candidate for weakly interacting massive particles (WIMP) or cold dark matter and…

高能物理 - 唯象学 · 物理学 2013-06-28 Kamakshya Prasad Modak , Debasish Majumdar

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

Under the hypothesis of a Dark Matter composed by supersymmetric particles like neutralinos, we investigate the possibility that their annihilation in the haloes of nearby galaxies could produce detectable fluxes of $\gamma$-photons.…

天体物理学 · 物理学 2009-11-10 Lidia Pieri , Enzo Branchini

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
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