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Article Dans Une Revue Computer Physics Communications Année : 2019

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

Résumé

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/ .

Dates et versions

hal-01833759 , version 1 (10-07-2018)

Identifiants

Citer

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