Effects of Vainshtein screening on LSB galaxies and Milky Way

Sirachak Panpanich*

*この研究の対応する著者

研究成果: Conference contribution

抄録

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.

本文言語English
ホスト出版物のタイトルProceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
出版社Kyoto University, Yukawa Institute for Theoretical Physics
ページ757-771
ページ数15
ISBN(電子版)9780000000002
出版ステータスPublished - 2015
イベント25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015 - Kyoto, Japan
継続期間: 2015 12 72015 12 11

出版物シリーズ

名前Proceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
3

Conference

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

ASJC Scopus subject areas

  • 原子分子物理学および光学

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