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We calculate the cross section for s-wave neutralino annihilation to three-body final states below the W^+ W^- and t-bar t thresholds. Such three-body channels may dominate the annihilation cross section if the neutralino mass is not too…

High Energy Physics - Phenomenology · Physics 2009-10-31 Xuelei Chen , Marc Kamionkowski

The Indirect Detection of neutralino Dark Matter is most promising through annihilation channels producing a hard energy spectrum for the detected particles, such as the neutralino annihilation into $Zh$. A cancellation however makes this…

High Energy Physics - Phenomenology · Physics 2009-01-07 Benjamin Labonne , Emmanuel Nezri , Jean Orloff

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…

High Energy Physics - Phenomenology · Physics 2009-10-22 M. Drees , G. Jungman , M. Kamionkowski , M. Nojiri

We discuss a robust and fairly model-independent upper bound on the possible neutrino flux produced by neutralino annihilation in the center of our galaxy, and show that its detection with present or future neutrino telescopes is highly…

Astrophysics · Physics 2007-05-23 J. Orloff

We present exact analytic cross sections for all neutralino-neutralino coannihilations into two-body tree level final states. These expressions allow the calculation of important contributions to the neutralino relic abundance over large…

High Energy Physics - Phenomenology · Physics 2014-11-17 A. Birkedal-Hansen , E. Jeong

We consider dark matter annihilation into Standard Model particles and show that the least detectable final states, namely neutrinos, define an upper bound on the total cross section. Calculating the cosmic diffuse neutrino signal, and…

Astrophysics · Physics 2008-11-26 John F. Beacom , Nicole F. Bell , Gregory D. Mack

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,…

High Energy Physics - Phenomenology · Physics 2010-11-30 P. Ullio , L. Bergstrom

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…

Astrophysics · Physics 2008-11-26 E. A. Baltz , C. Briot , P. Salati , R. Taillet , J. Silk

We present the first exact and most general neutralino-neutralino annihilation cross sections in the presence of flavor violation. The existing set of calculations in literature do not include flavour violation. These calculations are…

High Energy Physics - Phenomenology · Physics 2015-01-05 V. Suryanarayana Mummidi

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…

High Energy Physics - Phenomenology · Physics 2008-11-26 Z. Bern , P. Gondolo , M. Perelstein

This article provides a concise review of selected topics in the many-body physics of low density nuclear systems. The discussion includes the condensation of alpha particles in supernova envelopes, formation of three-body bound states and…

Nuclear Theory · Physics 2017-08-23 Armen Sedrakian , John W. Clark

The cosmological significance of the neutralino sector is studied for a class of models in which electroweak symmetry breaking is seeded by a gauge singlet. Extensive use is made of the renormalisation group equations to significantly…

High Energy Physics - Phenomenology · Physics 2011-02-16 S. A. Abel , S. Sarkar , I. B. Whittingham

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…

Astrophysics · Physics 2010-11-30 L. Bergstrom , P. Ullio , J. Buckley

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…

High Energy Physics - Phenomenology · Physics 2016-09-01 Gerard Jungman , Marc Kamionkowski

We investigate the prospects for distinguishing dark matter annihilation channels using the neutrino flux from gravitationally captured dark matter particles annihilating inside the sun. We show that, even with experimental error in energy…

High Energy Physics - Phenomenology · Physics 2013-05-30 Rouzbeh Allahverdi , Katherine Richardson

The annihilation rate of dark matter particles plays a crucial role in dark matter studies, for it determines their relic density and their indirect detection signal. In this paper, we show that this annihilation rate can receive large…

High Energy Physics - Phenomenology · Physics 2010-11-30 Carlos E. Yaguna

Neutralino dark matter, and in particular different aspects of its detection at neutrino telescopes, has been studied within the Minimal Supersymmetric extension of the Standard Model, the MSSM. The relic density of neutralinos has been…

High Energy Physics - Phenomenology · Physics 2007-05-23 J. Edsjo

A sub-component of dark matter with a short collision length compared to a planetary size leads to efficient accumulation of dark matter in astrophysical bodies. We analyze possible neutrino signals from the annihilation of such dark matter…

High Energy Physics - Phenomenology · Physics 2024-01-15 Maxim Pospelov , Anupam Ray

A long-standing problem to account for the electron-positron annihilation in positron Hydrogen scattering above the Positronium formation threshold has been resolved by the use of the three-body Faddeev formalism. The multichannel…

Atomic Physics · Physics 2007-05-23 S. L. Yakovlev , C-. Y. Hu

Once supersymmetric neutralinos $\tilde{\chi}^0$ are produced copiously at $e^+e^-$ linear colliders, their characteristics can be measured with high precision. In particular, the fundamental parameters in the gaugino/higgsino sector of the…

High Energy Physics - Phenomenology · Physics 2009-11-11 S. Y. Choi , M. Drees , J. Song
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