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Testing Yukawa-like potentials from f(R)-gravity in elliptical galaxies
Astrophysical Journal (2012)
  • N. R. Napolitano
  • S. Capozziello
  • Aaron J. Romanowsky, San Jose State University
  • M. Capaccioli
  • C. Tortora

We present the first analysis of extended stellar kinematics of elliptical galaxies where a Yukawa-like correction to the Newtonian gravitational potential derived from f(R)-gravity is considered as an alternative to dark matter. In this framework, we model long-slit data and planetary nebula data out to 7 R eff of three galaxies with either decreasing or flat dispersion profiles. We use the corrected Newtonian potential in a dispersion-kurtosis Jeans analysis to account for the mass-anisotropy degeneracy. We find that these modified potentials are able to fit nicely all three elliptical galaxies and the anisotropy distribution is consistent with that estimated if a dark halo is considered. The parameter which measures the "strength" of the Yukawa-like correction is, on average, smaller than the one found previously in spiral galaxies and correlates both with the scale length of the Yukawa-like term and the orbital anisotropy.

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Copyright © 2012 Institute of Physics. The published version of the article can be found online at:
Citation Information
N. R. Napolitano, S. Capozziello, Aaron J. Romanowsky, M. Capaccioli, et al.. "Testing Yukawa-like potentials from f(R)-gravity in elliptical galaxies" Astrophysical Journal Vol. 748 Iss. L24 (2012)
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