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In this code we implemented the density profile of dark matter halos in galaxy clusters and its logarithmic slope for different models existent in the literature, to be specific the Hernquist, NFW and Einasto profiles. For these models, we've also implemented the surface mass density, average surface mass density and excess surface mass density.

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victorportog/galaxyclusters_profiles

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README.md
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profiles.ipynb
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profiles_monography.ipynb
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galaxyclusters_profiles

Here you can find two jupyter notebook scripts:

  • profiles.ipynb was developed during a year for the scientific initiation program 2019/2020 of the University of Brasília (UnB). It composes the work "Perfis de densidade de matéria de aglomerados de galáxias" (translation: Galaxy Cluster Matter Density Profiles).

  • profiles_monography.ipynb is a modified version of profiles.ipynb with a few more features. It is a part of my undergraduate course final monography titled "Lenteamento Gravitacional Fraco e Perfis de Densidade de Matéria de Aglomerados de Galáxias" (translation: Galaxy Cluster Weak Gravitational Lensing and Matter Density Profiles).

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In this code we implemented the density profile of dark matter halos in galaxy clusters and its logarithmic slope for different models existent in the literature, to be specific the Hernquist, NFW and Einasto profiles. For these models, we've also implemented the surface mass density, average surface mass density and excess surface mass density.

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