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Typical density profile for warm dark matter haloes

✍ Scribed by Jordi Viñas; Eduard Salvador-Solé; Alberto Manrique

Book ID
114842866
Publisher
John Wiley and Sons
Year
2012
Tongue
English
Weight
300 KB
Volume
424
Category
Article
ISSN
1745-3925

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We present density profiles, that are solutions of the spherical Jeans equation, derived under the following two 3 2a assumptions: (i) the coarse grained phase-density follows a power-law of radius, r /s ~r , and (ii) the velocity anisotropy 2 parameter is given by the relation b (r) 5 b 1 2b (r /r