Low surface brightness galaxy rotation curves in the low energy limit of Rn gravity: No need for dark matter?

Monthly Notices of the Royal Astronomical Society

Volumn 375, Issue 4, 2007, Pages 1423-1440

  Capozziello, S ^a   Cardone, V F ^b   Troisi, A ^a  

^a UNIVERSITY OF NAPLES FEDERICO II   (Italy)

^b UNIVERSITY OF SALERNO   (Italy)

Author keywords

Dark matter; Galaxies: kinematics and dynamics; Gravitation

Indexed keywords

CURVE FITTING; GALAXIES; LAGRANGE MULTIPLIERS; LUMINANCE; RELATIVITY; ROTATION; SUPERNOVAE;

DARK MATTER; DARK MATTER HALOS; GALAXIES: KINEMATICS AND DYNAMICS; GENERAL RELATIVITY; LAGRANGIAN; LOW-ENERGY LIMIT; POWER-LAW; ROTATION CURVES; SPIRAL GALAXIES; SURFACE BRIGHTNESS;

GRAVITATION;

EID: 33847336367     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.11401.x     Document Type: Article

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