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Distinguishing a core and a cusp within dark matter halos is complexified by the existence of mass-anisotropy degeneracy, where various combinations of velocity anisotropy ($\beta$) and inner density slope ($\gamma$) yield similar observational signa
Externí odkaz:
http://arxiv.org/abs/2404.12671
Publikováno v:
EPJ Web of Conferences, Vol 240, p 04002 (2020)
Local dark matter density, ρdm, is one of the crucial astrophysical inputs for the estimation of detection rates in dark matter direct search experi- ments. Knowing the value also helps us to investigate the shape of the Galactic dark halo, which is
Externí odkaz:
https://doaj.org/article/33f1e5d5e3db4d089c5d152620eaded1
Autor:
Soonthornthum, B., Malasan, H.L., Chey, C.O., Abu Kassim, H., Myint, K.S., Celebre, C., Diep, P.N., Yang, A., Wardana, M. Dafa, Wulandari, Hesti, Sulistiyowati, Khatami, Akbar H.
Publikováno v:
EPJ Web of Conferences; 8/21/2020, Vol. 240, p1-11, 11p