TY - JOUR
T1 - Bianchi type I cosmology in N=2, D=5 supergravity
AU - Chen, Chiang Mei
AU - Harko, T.
AU - Mak, M. K.
PY - 2000/5/15
Y1 - 2000/5/15
N2 - The dynamics and evolution of Bianchi type I space-times are considered in the framework of the four-dimensional truncation of a reduced theory obtained from N=2, D=5 supergravity. The general solution of the gravitational field equations can be represented in an exact parametric form. All solutions have a singular behavior at the initial or final moment, except when the space-time geometry reduces to the isotropic flat case. Generically the obtained cosmological models describe an anisotropic, expanding or collapsing, singular universe with a noninflationary evolution for all times.
AB - The dynamics and evolution of Bianchi type I space-times are considered in the framework of the four-dimensional truncation of a reduced theory obtained from N=2, D=5 supergravity. The general solution of the gravitational field equations can be represented in an exact parametric form. All solutions have a singular behavior at the initial or final moment, except when the space-time geometry reduces to the isotropic flat case. Generically the obtained cosmological models describe an anisotropic, expanding or collapsing, singular universe with a noninflationary evolution for all times.
UR - http://www.scopus.com/inward/record.url?scp=17144411511&partnerID=8YFLogxK
U2 - 10.1103/PhysRevD.61.104017
DO - 10.1103/PhysRevD.61.104017
M3 - 期刊論文
AN - SCOPUS:17144411511
SN - 0556-2821
VL - 61
SP - 1
EP - 6
JO - Physical Review D - Particles, Fields, Gravitation and Cosmology
JF - Physical Review D - Particles, Fields, Gravitation and Cosmology
IS - 10
M1 - 104017
ER -