CLUMPY v3: γ-ray and ν signals from dark matter at all scales

Hütten, Moritz; Combet, Céline; Maurin, David

doi:10.1016/j.cpc.2018.10.001

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CLUMPY v3: γ-ray and ν signals from dark matter at all scales

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Hütten, Moritz
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Combet, Céline
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Maurin, David
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

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Citation

Hütten, M., Combet, C., & Maurin, D. (2019). CLUMPY v3: γ-ray and ν signals from dark matter at all scales. Computer Physics Communications, 235, 336. doi:10.1016/j.cpc.2018.10.001.

Cite as: https://hdl.handle.net/21.11116/0000-0005-D6E5-7

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 ∆. 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/. Program