Research output: Contribution to journal › Article › peer-review
Dark matter from non-relativistic embedding gravity. / Paston, S. A.
In: Modern Physics Letters A, Vol. 36, No. 15, 2150101, 20.05.2021.Research output: Contribution to journal › Article › peer-review
}
TY - JOUR
T1 - Dark matter from non-relativistic embedding gravity
AU - Paston, S. A.
N1 - Publisher Copyright: © 2021 World Scientific Publishing Company. Copyright: Copyright 2021 Elsevier B.V., All rights reserved.
PY - 2021/5/20
Y1 - 2021/5/20
N2 - We study the possibility to explain the mystery of the dark matter (DM) through the transition from General Relativity to embedding gravity. This modification of gravity, which was proposed by Regge and Teitelboim, is based on a simple string-inspired geometrical principle: our spacetime is considered here as a four-dimensional surface in a flat bulk. We show that among the solutions of embedding gravity, there is a class of solutions equivalent to solutions of GR with an additional contribution of non-relativistic embedding matter, which can serve as cold DM. We prove the stability of such type of solutions and obtain an explicit form of the equations of motion of embedding matter in the non-relativistic limit. According to them, embedding matter turns out to have a certain self-interaction, which could be useful in the context of solving the core-cusp problem that appears in the CDM model.
AB - We study the possibility to explain the mystery of the dark matter (DM) through the transition from General Relativity to embedding gravity. This modification of gravity, which was proposed by Regge and Teitelboim, is based on a simple string-inspired geometrical principle: our spacetime is considered here as a four-dimensional surface in a flat bulk. We show that among the solutions of embedding gravity, there is a class of solutions equivalent to solutions of GR with an additional contribution of non-relativistic embedding matter, which can serve as cold DM. We prove the stability of such type of solutions and obtain an explicit form of the equations of motion of embedding matter in the non-relativistic limit. According to them, embedding matter turns out to have a certain self-interaction, which could be useful in the context of solving the core-cusp problem that appears in the CDM model.
KW - core-cusp problem
KW - Dark matter
KW - embedding gravity
KW - embedding theory
KW - isometric embedding
KW - modified gravity
KW - Regge-Teitelboim gravity
KW - self-interacting dark matter
KW - SEARCHES
KW - SCALE
KW - MODEL
KW - MIMETIC GRAVITY
UR - http://www.scopus.com/inward/record.url?scp=85106443662&partnerID=8YFLogxK
U2 - 10.1142/S0217732321501017
DO - 10.1142/S0217732321501017
M3 - Article
AN - SCOPUS:85106443662
VL - 36
JO - Modern Physics Letters A
JF - Modern Physics Letters A
SN - 0217-7323
IS - 15
M1 - 2150101
ER -
ID: 77299183