TY - GEN
T1 - Effects of Vainshtein screening on LSB galaxies and Milky Way
AU - Panpanich, Sirachak
N1 - Publisher Copyright:
© Proceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015. All rights reserved.
Copyright:
Copyright 2021 Elsevier B.V., All rights reserved.
PY - 2015
Y1 - 2015
N2 - 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.
AB - 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.
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M3 - Conference contribution
AN - SCOPUS:85092231339
T3 - Proceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
SP - 757
EP - 771
BT - Proceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
PB - Kyoto University, Yukawa Institute for Theoretical Physics
T2 - 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
Y2 - 7 December 2015 through 11 December 2015
ER -