Collective scattering of massive stars in higher order gravity
| Contribuinte(s) |
Universidade Estadual Paulista (UNESP) |
|---|---|
| Data(s) |
27/05/2014
27/05/2014
15/01/1997
|
| Resumo |
In the weak field approximation of higher order gravity theory a gravitational potential is described by a Newtonian plus a Yukawa-like term. This new term is used to explain some aspects of galactic dynamics, without considering dark matter. Its presence modifies the scattering probability of a massive intruder star and relaxation time of the stellar system. |
| Formato |
733-738 |
| Identificador |
http://dx.doi.org/10.1103/PhysRevD.55.733 Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 55, n. 2, p. 733-738, 1997. 0556-2821 http://hdl.handle.net/11449/65025 10.1103/PhysRevD.55.733 WOS:A1997WF29600031 2-s2.0-0011085755 2-s2.0-0011085755.pdf |
| Idioma(s) |
eng |
| Relação |
Physical Review D: Particles, Fields, Gravitation and Cosmology |
| Direitos |
closedAccess |
| Tipo |
info:eu-repo/semantics/article |
