Analysis of the Yukawa gravitational potential in f(R) gravity. I. Semiclassical periastron advance

Ivan De Martino, Ruth Lazkoz, and Mariafelicia De Laurentis
Phys. Rev. D 97, 104067 – Published 31 May 2018

Abstract

The concordance cosmological model has been successfully tested over the last decades. Despite its successes, the fundamental nature of dark matter and dark energy is still unknown. Modifications of the gravitational action have been proposed as an alternative to these dark components. The straightforward modification of gravity is to generalize the action to a function, f(R), of the scalar curvature. Thus one is able to describe the emergence and the evolution of the large scale structure without any additional (unknown) dark component. In the weak field limit of the f(R)-gravity, a modified Newtonian gravitational potential arises. This gravitational potential accounts for an extra force, generally called fifth force, that produces a precession of the orbital motion even in the classic mechanical approach. We have shown that the orbits in the modified potential can be written as Keplerian orbits under some conditions on the strength and scale length of this extra force. Nevertheless, we have also shown that this extra term gives rise to the precession of the orbit. Thus, comparing our prediction with the measurements of the precession of some planetary motions, we have found that the strength of the fifth force must be in the range [2.706.70]×109 with the characteristic scale length to fix to the fiducial values of 5000AU.

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  • Received 24 October 2017

DOI:https://doi.org/10.1103/PhysRevD.97.104067

© 2018 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Ivan De Martino* and Ruth Lazkoz

  • Department of Theoretical Physics and History of Science, University of the Basque Country UPV/EHU, Faculty of Science and Technology, Barrio Sarriena s/n, 48940 Leioa, Spain

Mariafelicia De Laurentis

  • Institute for Theoretical Physics, Goethe University, Max-von-Laue-Str. 1, 60438 Frankfurt, Germany and Dipartimento di Fisica “E. Pancini”, Universitá di Napoli “Federico II”, Complesso Universitario di Monte S. Angelo, Edificio G, Via Cinthia, I-80126, Napoli, Italy and Laboratory of Theoretical Cosmology, Tomsk State University of Control Systems and Radioelectronics (TUSUR), 634050 Tomsk, Russia

  • *ivan.demartino@ehu.eus
  • ruth.lazkoz@ehu.eus
  • laurentis@th.physik.uni-frankfurt.de

See Also

Analysis of the Yukawa gravitational potential in f(R) gravity. II. Relativistic periastron advance

Mariafelicia De Laurentis, Ivan De Martino, and Ruth Lazkoz
Phys. Rev. D 97, 104068 (2018)

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Vol. 97, Iss. 10 — 15 May 2018

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