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Нова модель просторового розподілу густини в гало ферміонної темної матерії

We formulate a new model of density distribution for halos made of warm dark matter (WDM) particles. The model is described by a single microphysical parameter – the mass (or, equivalently, the maximal value of the initial phase-space density distribution) of dark matter particles. Given the WDM par...

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Bibliographic Details
Date:2018
Main Authors: Rudakovskyi, A. V., Savchenko, D. O.
Format: Article
Language:English
Published: Publishing house "Academperiodika" 2018
Online Access:https://ujp.bitp.kiev.ua/index.php/ujp/article/view/2018156
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Journal Title:Ukrainian Journal of Physics

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Ukrainian Journal of Physics

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