CLUMPY v3: $\gamma$-ray and $\nu$ signals from dark matter at all scales

Abstract : We present the third release of the CLUMPY code for calculating γ -ray and ν signals from annihilations or decays in dark matter structures. This version includes the mean extragalactic signal with several pre-defined options and keywords related to cosmological parameters, mass functions for the dark matter structures, and γ -ray absorption up to high redshift. For more flexibility and consistency, dark matter halo masses and concentrations are now defined with respect to a user-defined overdensity Δ . We have also made changes for the user’s benefit: distribution and versioning of the code via git , less dependencies and a simplified installation, better handling of options in run command lines, consistent naming of parameters, and a new Sphinx documentation at http://lpsc.in2p3.fr/clumpy/ .
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https://hal.archives-ouvertes.fr/hal-01833759
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Submitted on : Tuesday, July 10, 2018 - 1:06:28 AM
Last modification on : Thursday, October 17, 2019 - 5:09:15 AM

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Moritz Hütten, Céline Combet, David Maurin. CLUMPY v3: $\gamma$-ray and $\nu$ signals from dark matter at all scales. Comput.Phys.Commun., 2019, 235, pp.336-345. ⟨10.1016/j.cpc.2018.10.001⟩. ⟨hal-01833759⟩

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