搜索结果: 1-6 共查到“理论物理学 cosmological models”相关记录6条 . 查询时间(0.062 秒)
Oscillations toward the singularity of LRS Bianchi type IX cosmological models with Vlasov matter
Oscillations singularity of LRS Bianchi type IX cosmological models Vlasov matter
2010/12/20
We analyze the dynamics of a class of cosmological solutions of the Einstein-Vlasov equa-
tions. These equations describe an ensemble of collisionless particles (which represent galaxies or clusters ...
Cosmological Models with Fractional Derivatives and Fractional Action Functional
Fractional Derivative and Integral Cosmology
2010/12/20
Cosmological models of a scalar field with dynamical equations containing fractional derivatives or derived from the Einstein-Hilbert action of fractional order, are constructed. A number of exact sol...
Cosmological Constant and Stability of the Cosmological Models
cosmology cosmological models general relativity
2007/8/15
2002Vol.37No.6pp.667-670DOI:
Cosmological Constant and Stability of the Cosmological Models
WANG Yong-Jiu and TANG Zhi-Ming
Institute of Physics, Hunan Normal University...
Bianchi-Type II String Cosmological Models with Bulk Viscosity
string cosmological
model Bianchi-type II space-time bulk viscosity
2007/8/15
2004Vol.41No.5pp.726-728DOI:
Bianchi-Type II String Cosmological Models with Bulk Viscosity
WANG Xing-Xiang
Department of Physics, Anhui Normal University, Wuhu 241000, ...
Five Dimensional Anisotropic Homogeneous Cosmological Models in Second Self Creation Theory of Gravitation
Five dimensions self creation theory anisotropic spacetime
2010/4/9
Five dimensional homogeneous anisotropic cosmological models in Barber's second self creation theory are constructed when the gravitational field is generated by a perfect fluid. Under the power law d...
Chaos in Closed Isotropic Cosmological Models with Steep Scalar Field Potential
Closed Isotropic Cosmological Steep Scalar Field Potential
2010/4/15
The dynamics of closed scalar field FRW cosmological models is studied for several types of exponentially and more than exponentially steep potentials. The parameters of scalar field potentials which ...