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In this work, we investigate the possibility that the galaxy rotation curves can be explained in the framework of modified gravity models that introduce a Yukawa term in the gravitational potential.
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A. Stabile and S. Capozziello, Galaxy rotation curves in f(R,ϕ) gravity , Phys. Rev. D87
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2007
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C. Frigerio Martins and P. Salucci, Analysis of rotation curves in the framework of R n
2007
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2007
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M. Banados, Eddington-Born-Infeld action for dark matter and dark energy , Phys. Rev. D77
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2008
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2009
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D. C. Rodrigues, P. S. Letelier and I. L. Shapiro, Galaxy rotation curves from general relativity with renormalization group corrections , Journal of Cosmology and Astroparticle Physics 2010
2010
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2013
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2013
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2014
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2014
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2014
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2016
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C. Patrignani and Particle Data Group, Review of Particle Physics , Chinese Physics C 40
2016
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2016
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2017
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2017
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2018
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T. Damour and G. Esposito-Farese, Tensor-multi-scalar theories of gravitation , Classical and Quantum Gravity 9
2093
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