Fitting rotation curves of galaxies by de Rham-Gabadadze-Tolley massive gravity

Sirachak Panpanich, Piyabut Burikham

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

Since there is no direct constraint on C in the galactic scale, we can choose C to be very large to satisfy Lunar Laser Ranging experiments. For C = 1 − 1018 m, we find mg ∼ 10−21 − 10−30 eV.

Original languageEnglish
Title of host publicationProceedings of the 28th Workshop on General Relativity and Gravitation in Japan, JGRG 2018
PublisherRikkyo University
Pages327-341
Number of pages15
ISBN (Electronic)9780000000002
Publication statusPublished - 2018
Externally publishedYes
Event28th Workshop on General Relativity and Gravitation in Japan, JGRG 2018 - Tokyo, Japan
Duration: 2018 Nov 52018 Nov 9

Publication series

NameProceedings of the 28th Workshop on General Relativity and Gravitation in Japan, JGRG 2018
Volume1

Conference

Conference28th Workshop on General Relativity and Gravitation in Japan, JGRG 2018
CountryJapan
CityTokyo
Period18/11/518/11/9

ASJC Scopus subject areas

  • Atomic and Molecular Physics, and Optics

Fingerprint Dive into the research topics of 'Fitting rotation curves of galaxies by de Rham-Gabadadze-Tolley massive gravity'. Together they form a unique fingerprint.

Cite this