Effects of Vainshtein screening on LSB galaxies and Milky Way

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

Abstract

We reproduced rotation curves by using the fifth force instead of dark matter halo. • In order to satisfy the observation, the fifth force at solar distance must be around half of the Newtonian force. • It is difficult to distinguish the effects of Galileon and DBIonic. • The character of screening inside an spherical object depends on density profile of the object.

Original languageEnglish
Title of host publicationProceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
PublisherKyoto University, Yukawa Institute for Theoretical Physics
Pages757-771
Number of pages15
ISBN (Electronic)9780000000002
Publication statusPublished - 2015
Event25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015 - Kyoto, Japan
Duration: 2015 Dec 72015 Dec 11

Publication series

NameProceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
Volume3

Conference

Conference25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
Country/TerritoryJapan
CityKyoto
Period15/12/715/12/11

ASJC Scopus subject areas

  • Atomic and Molecular Physics, and Optics

Fingerprint

Dive into the research topics of 'Effects of Vainshtein screening on LSB galaxies and Milky Way'. Together they form a unique fingerprint.

Cite this