Search for dark matter annihilation in the Sun using the full ANTARES dataset

Weakly Interacting Massive Particles (WIMPs) are among the most popular candidates for particle dark matter. In certain scenarios, WIMPs could be gravitationally captured into massive celestial objects and then annihilate into Standard Model particles, possibly leading to the emission of neutrinos. The ANTARES neutrino telescope, located in the Mediterranean Sea, is sensitive to neutrinos with energies ranging from a few tens of GeV to the TeV scale, making it well suited to search for the annihilation of WIMPs with masses below a few TeV/c$^2$. One of the closest potential astrophysical sources of neutrinos from WIMP annihilations is the Sun. In this work, a search for high-energy neutrinos originating from the Sun, using the full dataset recorded by ANTARES from 2007 to 2022 was conducted. The analysis yielded no significant evidence for a neutrino excess over the expected background, and upper limits on the WIMP-proton interaction cross section have been obtained, for both spin-dependent and spin-independent processes. These limits are valid for dark matter masses ranging from 35 GeV/c$^2$ to 10 TeV/c$^2$ for the annihilation benchmark channels WIMP$+$WIMP $\longrightarrow$ $b\bar{b},τ^+τ^-, W^+W^-$, assuming a 100$\%$ branching ratio for each of these channels. These results improve on those previously obtained by the ANTARES Collaboration by a factor of two-three and are consistent with those reported by other experiments in direct and indirect searches for dark matter.

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Authors

A. Albert; S. Alves; M. André; M. Ardid; S. Ardid; J. -J. Aubert; J. Aublin; B. Baret; S. Basa; Y. Becherini; B. Belhorma; F. Benfenati; V. Bertin; S. Biagi; J. Boumaaza; M. Bouta; M. C. Bouwhuis; H. Brânzaş; R. Bruijn; J. Brunner; J. Busto; B. Caiffi; D. Calvo; S. Campion; A. Capone; L. Caramete; F. Carenini; J. Carr; V. Carretero; T. Cartraud; S. Celli; M. Chabab; T. Chiarusi; M. Circella; J. A. B. Coelho; A. Coleiro; R. Coniglione; P. Coyle; A. Creusot; A. F. Díaz; B. De Martino; C. Distefano; I. Di Palma; C. Donzaud; D. Dornic; D. Drouhin; T. Eberl; A. Eddymaoui; T. van Eeden; D. van Eijk; S. El Hedri; A. Enzenhöfer; P. Fermani; G. Ferrara; F. Filippini; L. A. Fusco; S. Gagliardini; J. García-Méndez; C. Gatius Oliver; P. Gay; N. Geißelbrecht; H. Glotin; R. Gozzini; R. Gracia Ruiz; K. Graf; C. Guidi; L. Haegel; H. van Haren; A. J. Heijboer; Y. Hello; L. Hennig; J. J. Hernández-Rey; J. Hößl; F. Huang; G. Illuminati; B. Jisse-Jung; M. de Jong; P. de Jong; M. Kadler; O. Kalekin; U. Katz; A. Kouchner; I. Kreykenbohm; V. Kulikovskiy; R. Lahmann; M. Lamoureux; A. Lazo; D. Lefèvre; E. Leonora; G. Levi; S. Le Stum; S. Loucatos; J. Manczak; M. Marcelin; A. Margiotta; A. Marinelli; P. Migliozzi; A. Moussa; R. Muller; S. Navas; E. Nezri; B. Ó Fearraigh; E. Oukacha; A. M. Păun; G. E. Păvălaş; S. Peña-Martínez; M. Perrin-Terrin; P. Piattelli; C. Poirè; T. Pradier; N. Randazzo; D. Real; G. Riccobene; A. Romanov; A. Sánchez Losa; A. Saina; F. Salesa Greus; D. F. E. Samtleben; M. Sanguineti; P. Sapienza; F. Schüssler; J. Seneca; M. Spurio; Th. Stolarczyk; M. Taiuti; Y. Tayalati; B. Vallage; G. Vannoye; V. Van Elewyck; S. Viola; D. Vivolo; J. Wilms; S. Zavatarelli; A. Zegarelli; J. D. Zornoza; J. Zúñiga

Published

Sep 29, 2026

Paper type

preprint

Source

Arxiv