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arxiv: astro-ph/0211238 · v1 · submitted 2002-11-12 · 🌌 astro-ph

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DarkSUSY - A numerical package for supersymmetric dark matter calculations

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classification 🌌 astro-ph
keywords supersymmetricdetectiondarkdarksusylightestmatterneutralinocalculations
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The question of the nature of dark matter in the Universe remains one of the most outstanding unsolved problems in basic science. One of the best motivated particle physics candidates is the lightest supersymmetric particle, assumed to be the lightest neutralino. We here describe DarkSUSY, an advanced numerical FORTRAN package for supersymmetric dark matter calculations. With DarkSUSY one can: (i) compute masses and compositions of various supersymmetric particles; (ii) compute the relic density of the lightest neutralino, using accurate methods which include the effects of resonances, pair production thresholds and coannihilations; (iii) check accelerator bounds to identify allowed supersymmetric models; and (iv) obtain neutralino detection rates for a variety of detection methods, including direct detection and indirect detection through antiprotons, gamma-rays and positrons from the Galactic halo or neutrinos from the center of the Earth or the Sun.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. A New Timing Signature of Black Hole Spin: Time-Delay Asymmetry in Kerr Accretion Flows

    astro-ph.HE 2026-05 unverdicted novelty 7.0

    A mirror-paired asymmetry in photon arrival times from opposite sides of the projected spin axis provides a direct general-relativistic timing signature of black hole spin.

  2. A New Timing Signature of Black Hole Spin: Time-Delay Asymmetry in Kerr Accretion Flows

    astro-ph.HE 2026-05 unverdicted novelty 6.0

    A mirror-paired time-delay asymmetry At vanishes for non-spinning black holes but is nonzero and increases with spin for Kerr black holes, depending on inclination and emission radius.