Fermionic warm dark matter produces galaxy cores in the observed scales because of quantum mechanics

New Astronomy

Volumn 22, Issue , 2013, Pages 39-50

  Destri, C ^a   De Vega, H J ^b,c   Sanchez, N G ^c  

^a UNIVERSITY OF MILANO BICOCCA   (Italy)

^b LPTHE   (France)

^c OBSERVATOIRE DE PARIS   (France)

Author keywords

Cosmology: dark matter; Galaxies: halos; Galaxies: kinematics and dynamics

Indexed keywords

EID: 84873653312     PISSN: 13841076     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.newast.2012.12.003     Document Type: Article

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