Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-24T00:50:08.407Z Has data issue: false hasContentIssue false

An f(R) gravitation for galactic environments

Published online by Cambridge University Press:  01 August 2006

Yousef Sobouti*
Affiliation:
Institute for Advanced Studies in Basic Sciences, P.O. Box 45195-1159, Zanjan, Iran email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We propose an action-based f(R) modification of Einstein's gravity which admits of a modified Schwarzschild-deSitter metric. In the weak field limit this amounts to adding a small logarithmic correction to the Newtonian potential. A test star moving in such a spacetime acquires a constant asymptotic speed at large distances. This speed turns out to be proportional to the fourth root of the mass of the central body in compliance with the Tully-Fisher relation. A variance of MOND's gravity emerges as an inevitable consequence of the proposed formalism.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007

References

Capozziello, S., Cardone, V. F., Carloni, S. & Troisi, A. 2003, astro-ph/0307018Google Scholar
Ferraris, M., Francaviglia, M. & Volvich, I. 1994, Class. Quantum Grav., 11, 1505CrossRefGoogle Scholar
Magnano, G. 1995, gr-qc/9511027Google Scholar
Milgrom, M. 1983, a, b, c, ApJ 271, 365, 371, 384CrossRefGoogle Scholar
Sanders, R. H. & Verheijen, M. A. W. 1998, astro-ph/9802240Google Scholar
Sanders, R. H. & McGough, S. S. 2002, astro-ph/0204521Google Scholar
Sobouti, Y. 2005, astro-ph/0503302Google Scholar