The Redshift-Dependence of Radial Acceleration: Modified Gravity versus Particle Dark Matter
Autor: | Hossenfelder, Sabine, Mistele, Tobias |
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Rok vydání: | 2018 |
Předmět: | |
Druh dokumentu: | Working Paper |
DOI: | 10.1142/S0218271818470107 |
Popis: | Modified Newtonian Dynamics has one free parameter and requires an interpolation function to recover the normal Newtonian limit. We here show that this interpolation function is unnecessary in a recently proposed covariant completion of Erik Verlinde's emergent gravity, and that Verlinde's approach moreover fixes the function's one free parameter. The so-derived correlation between the observed acceleration (inferred from rotation curves) and the gravitational acceleration due to merely the baryonic matter fits well with data. We then argue that the redshift-dependence of galactic rotation curves could offer a way to tell apart different versions of modified gravity from particle dark matter. Comment: 7 pages, 4 figures |
Databáze: | arXiv |
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