Anatomy of Eddington-like inversion methods in the context of dark matter searches

DOI10.1088/1475-7516/2018/09/040OpenAlexW3098632126WikidataQ129245026 ScholiaQ129245026MaRDI QIDQ5023439

Martin Stref, Julien Lavalle, Thomas Lacroix

Publication date: 21 January 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1805.02403

zbMATH Keywords

dark matter theorygalaxy dynamicssemi-analytic modeling

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (3)

Predicting the dark matter velocity distribution in galactic structures: tests against hydrodynamic cosmological simulations ⋮ The velocity-dependent J-factor of the Milky Way halo: does what happens in the galactic bulge stay in the galactic bulge? ⋮ Towards a more rigorous treatment of uncertainties on the velocity distribution of dark matter particles for capture in stars

Cites Work

• Unnamed Item
• Studies in the Equilibrium of Globular Clusters (II)
• A Study of the Equilibrium of Globular Clusters

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