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Title: PPPC 4 DMν: a Poor Particle Physicist Cookbook for Neutrinos from Dark Matter annihilations in the Sun

We provide ingredients and recipes for computing neutrino signals of TeV-scale Dark Matter (DM) annihilations in the Sun. For each annihilation channel and DM mass we present the energy spectra of neutrinos at production, including: state-of-the-art energy losses of primary particles in solar matter, secondary neutrinos, electroweak radiation. We then present the spectra after propagation to the Earth, including (vacuum and matter) flavor oscillations and interactions in solar matter. We also provide a numerical computation of the capture rate of DM particles in the Sun. These results are available in numerical form http://www.marcocirelli.net/PPPC4DMID.html.
Authors:
 [1] ;  [2] ;  [3] ;  [4] ; ;  [3] ;  [3] ;  [5]
  1. Scuola Normale Superiore and INFN, Piazza dei Cavalieri 7, Pisa, 56126 (Italy)
  2. Institut de Physique Théorique, CNRS URA 2306 & CEA-Saclay, Gif-sur-Yvette, 91191 (France)
  3. National Institute of Chemical Physics and Biophysics, Ravala 10, Tallinn (Estonia)
  4. (Finland)
  5. (Italy)
Publication Date:
OSTI Identifier:
22454495
Resource Type:
Journal Article
Resource Relation:
Journal Name: Journal of Cosmology and Astroparticle Physics; Journal Volume: 2014; Journal Issue: 03; Other Information: PUBLISHER-ID: JCAP03(2014)053; OAI: oai:repo.scoap3.org:1787; Article funded by SCOAP3. Content from this work may be used under the terms of the Creative Commons Attribution 3.0 License. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.; Country of input: International Atomic Energy Agency (IAEA)
Sponsoring Org:
SCOAP3, CERN, Geneva (Switzerland)
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; 79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; ANNIHILATION; CALCULATION METHODS; ENERGY LOSSES; ENERGY SPECTRA; FLAVOR MODEL; MASS; NEUTRINOS; NONLUMINOUS MATTER; OSCILLATIONS; SIGNALS; SUN; TEV RANGE; WEINBERG-SALAM GAUGE MODEL