Derivation of MOND from Hossenfelder-Verlinde gravity

被引:1
|
作者
Yoon, Youngsub [1 ,2 ,3 ]
机构
[1] Chungnam Natl Univ, Dept Phys, Daejeon 34134, South Korea
[2] Chungnam Natl Univ, Inst Quantum Syst IQS, Daejeon 34134, South Korea
[3] Inst Basic Sci IBS, Ctr Theoret Phys Universe, Particle Theory & Cosmol Grp, Daejeon 34126, South Korea
基金
新加坡国家研究基金会;
关键词
modified Newtonian dynamics; Hossenfelder-Verlinde gravity; dark matter; NEWTONIAN DYNAMICS;
D O I
10.1088/1361-6382/acf8aa
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Verlinde proposed emergent gravity, which naturally explains the Tully-Fisher relation, an empirical relation in galaxy rotation curves. Inspired by this theory, Hossenfelder constructed a covariant formulation of Verlinde's emergent gravity. In this work, we show that the equation of motion gains an extra acceleration in addition to the usual geodesic equation, according to Hossenfelder's theory. Moreover, we show that the extra acceleration is precisely the square root of the Newtonian gravitational acceleration if the mass of the imposter field is negligible, thus completing the proof that Hossenfelder's theory reduces to modified Newtonian dynamics (MOND) and determining which version of MOND it reduces to. We also obtain the value of L in Hossenfelder-Verlinde gravity theory, which is a constant, contrary to what Hossenfelder claimed. Finally, we suggest how the Newtonian limit that suitably describes our observations in Solar System is recovered in Hossenfelder's theory, by considering the mass of the imposter field.
引用
收藏
页数:12
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