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Tentative observations of cosmic-ray antihelium by the AMS-02 collaboration have re-energized the quest to use antinuclei to search for physics beyond the standard model. However, our transition to a data-driven era requires more accurate…

High Energy Astrophysical Phenomena · Physics 2024-04-23 Pedro De La Torre Luque , Martin Wolfgang Winkler , Tim Linden

AMS-02 has reached the sensitivity to probe canonical thermal WIMPs by their annihilation into antiprotons. Due to the high precision of the data, uncertainties in the astrophysical background have become the most limiting factor for…

High Energy Astrophysical Phenomena · Physics 2018-02-14 Annika Reinert , Martin Wolfgang Winkler

In the framework of the Inert Doublet Model, a very simple extension of the Standard Model, we study the production and propagation of antimatter in cosmic rays coming from annihilation of a scalar dark matter particle. We consider three…

High Energy Physics - Phenomenology · Physics 2009-05-06 Emmanuel Nezri , Michel H. G. Tytgat , Gilles Vertongen

We use the constraints on the diffusion parameters as obtained with stable nuclei to calculate the cosmic antiproton flux from annihilating relic neutralinos. We discuss the relevance of each characteristic parameter, describing our two…

Astrophysics · Physics 2007-05-23 Fiorenza Donato , Nicolao Fornengo , David Maurin , Pierre Salati , Richard Taillet

The interpretation of data from indirect detection experiments searching for dark matter annihilations requires computationally expensive simulations of cosmic-ray propagation. In this work we present a new method based on Recurrent Neural…

High Energy Astrophysical Phenomena · Physics 2021-12-21 Felix Kahlhoefer , Michael Korsmeier , Michael Krämer , Silvia Manconi , Kathrin Nippel

The leaky box model is now ruled out by measurements of a cosmic ray gradient throughout the galactic disk. It needs to be replaced by a more refined treatment which takes into account the diffusion of cosmic rays in the magnetic fields of…

Astrophysics · Physics 2009-10-28 P. Chardonnet , G. Mignola , P. Salati , R. Taillet

We calculate the antiproton flux due to relic neutralino annihilations, in a two-dimensional diffusion model compatible with stable and radioactive cosmic ray nuclei. We find that the uncertainty in the primary flux induced by the…

Astrophysics · Physics 2008-11-26 F. Donato , N. Fornengo , D. Maurin , P. Salati , R. Taillet

The General Antiparticle Spectrometer (GAPS) is designed to carry out indirect dark matter search by measuring low-energy cosmic-ray antiparticles. Below a few GeVs the flux of antiparticles produced by cosmic-ray collisions with the…

The indirect detection of particle dark matter (DM) is based on the search for anomalous components in cosmic rays (CRs) due to the annihilation of DM pairs in the galactic halo, on the top of the standard astrophysical production. These…

High Energy Astrophysical Phenomena · Physics 2010-03-23 P. Salati , F. Donato , N. Fornengo

Extra dimensions offer new ways to address long-standing problems in beyond the standard model particle physics. In some classes of extra-dimensional models, the lightest Kaluza-Klein particle is a viable dark matter candidate. In this…

[Abridged]. We take advantage of the galaxy-like 3D dark matter map extracted from the HORIZON Project results to calculate the positron and antiproton fluxes from dark matter annihilation, in a model-independent approach as well as for…

Astrophysics · Physics 2008-12-18 J. Lavalle , E. Nezri , F. -S. Ling , L. Athanassoula , R. Teyssier

The GAPS experiment is designed to carry out a sensitive dark matter search by measuring low-energy cosmic ray antideuterons and antiprotons. GAPS will provide a new avenue to access a wide range of dark matter models and masses that is…

The precise measurement of cosmic-ray antinuclei serves as an important means for identifying the nature of dark matter and other new astrophysical phenomena, and could be used with other cosmic-ray species to understand cosmic-ray…

The recent AMS-02 measurements of cosmic-ray (CR) deuteron fluxes suggest the presence of primary deuterons in quantities far exceeding predictions from Big Bang nucleosynthesis. This poses a significant challenge to modern astrophysics, as…

High Energy Astrophysical Phenomena · Physics 2025-06-25 Xing-Jian Lv , Xiao-Jun Bi , Kun Fang , Peng-Fei Yin , Meng-Jie Zhao

Antideuterons and antihelium nuclei in the cosmic-ray spectrum have long been considered a smoking gun signature of dark matter annihilation, making the tentative observation of several such events by AMS highly intriguing. Conventional…

High Energy Physics - Phenomenology · Physics 2026-03-16 Caleb Gemmell , Dan Hooper , Seth Koren , Fabrizio Vassallo

A new generation of upcoming space-based experiments will soon start to probe the spectrum of cosmic ray antiparticles with an unprecedented accuracy and, in particular, will open up a window to energies much higher than those accessible so…

Astrophysics · Physics 2008-11-26 Torsten Bringmann , Pierre Salati

The ANTARES neutrino telescope was completed in 2008 with the installation of its twelfth line. Its scientific scope is very broad, but the two main goals are the observation of astrophysical sources and the indirect detection of dark…

High Energy Astrophysical Phenomena · Physics 2015-06-04 J. D. Zornoza

In this work, we investigate dark matter (DM) detection in the context of weakly interacting massive particles (WIMPs). Upon annihilation, WIMPs generate cascades of secondary particles through various channels, many of which culminate in…

High Energy Astrophysical Phenomena · Physics 2026-03-24 Ignacio Martínez López , Rafael Alves Batista , Miguel A. Sánchez-Conde , Antonio Juan Rubio-Montero

The General Antiparticle Spectrometer (GAPS) is a novel approach for indirect dark matter searches that exploits cosmic antiparticles, especially antideuterons. The GAPS antideuteron measurement utilizes distinctive detection methods using…

High Energy Astrophysical Phenomena · Physics 2015-10-07 T. Aramaki , C. J. Hailey , S. E. Boggs , P. von Doetinchem , H. Fuke , S. I. Mognet , R. A. Ong , K. Perez , J. Zweerink

Antideuterons are a potential messenger for dark matter annihilation or decay in our own galaxy, with very low backgrounds expected from astrophysical processes. The standard coalescence model of antideuteron formation, while simple to…

High Energy Physics - Phenomenology · Physics 2015-08-14 L. A. Dal , A. R. Raklev