Extra force in f(R) modified theories of gravity
By O. Bertolami, C. Boehmer, Tiberiu Harko, Francisco S. N. Lobo. 2007
666 citations recorded by the source corpus.
The equation of motion for massive particles in f(R) modified theories of gravity is derived. By considering an explicit coupling between an arbitrary function of the scalar curvature, R, and the Lagrangian density of matter, it is shown that an extra force arises. This extra force is orthogonal to the four-velocity and the corresponding acceleration law is obtained in the weak-field limit. Connections with MOND and with the Pioneer anomaly are further discussed.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/b75506cc692de1be1c4a93ae7ec530314790bb09
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
- Salvatore Capozziello
- Tiberiu Harko
- Francisco S. N. Lobo
- Emmanuel N. Saridakis
- M. De Laurentis
- Valerio Faraoni
- G. Olmo
- Sergei D. Odintsov
In Nuclear and High Energy Physics
- Tiberiu Harko
- Salvatore Capozziello
- Francisco S. N. Lobo
- M. De Laurentis
- Valerio Faraoni
- Emmanuel N. Saridakis
- G. Olmo
- T. Sotiriou
Citations in the corpus
- Hybrid Metric-Palatini Gravity (2015, background): “Other extensions of the f(R) framework modify the coupling of matter to gravity by defining an action which depends linearly [39] or nonlinearly upon the matter Lagrangian [40–47], or its trace [48–50].”
- Generalized Curvature-Matter Couplings in Modified Gravity (2014, methodology): “In the Newtonian limit, the extra-acceleration generated by the curvature-matter coupling can be expressed in a similar form [9].”
- Evolution of cosmological perturbations in Bose–Einstein condensate dark matter (2011, background): “…theoretical models to explain the galactic rotation curves have also been elaborated recently (Milgrom 1983; Mannheim 1993; Bekenstein 2004; Mak & Harko 2004; Brownstein & Moffat 2006; Harko & Cheng 2006; Bertolami et al. 2007; Boehmer & Harko 2007; Boehmer et al. 2008a,b; Capozziello et al. 2009).”