The interplay of self-interacting dark matter and baryons in shaping the halo evolution

© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. We use high-resolution hydrodynamical simulation to test the difference of halo properties in cold dark matter (CDM) and a self-interacting dark matter (SIDM) scenario with a constant cross-section...

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Detaylı Bibliyografya
Asıl Yazarlar: Despali, Giulia, Sparre, Martin, Vegetti, Simona, Vogelsberger, Mark, Zavala, Jesús, Marinacci, Federico
Materyal Türü: Makale
Dil:English
Baskı/Yayın Bilgisi: Oxford University Press (OUP) 2021
Online Erişim:https://hdl.handle.net/1721.1/135140

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