Tensor Spherical and Pseudo-Spherical Harmonics in Four-Dimensional Spaces

概要

論文の詳細を見る
Explicit expressions for tensor spherical harmonics on the 3 sphere in the four-dimensional Euclidean space are derived, and extended to derive those for pseudo-spherical harmonics. They are useful for the analyses of large-scale perturbations in the Friedmann universe models.
理論物理学刊行会の論文
1982-07-25

著者

関連論文

On the Dissipation of Primordial Turbulence in the Expanding Universe
Gravitational Lens Effect on the Cosmic Background Radiation Due to Nonlinear Inhomogeneities : Astrophysics and Relativity
On Anisotropic and Homogeneous Cosmological Models in the Renormalized Theory of Gravitation
Some Higher Dimensional Vacuum Solutions of Einstein Equations with a Cosmological Constant
Chapter III Formation of Proto-Galaxies in the Expanding Universe : Gravitational instability
On the Applicability of a Dust-like Model to a Collapsing or Anti-Collapsing Star at High Temperature
On the Problem of Gravitational Collapse
On the Gravitational Instability in an Expanding Universe : Reformulation of Lifshitz's Theory
A Simple and Well-Adjusted Exterior Metric for a Collapsing or Anti-Collapsing Star
On the Gravito-C-Field in an Empty Region with Spherical Symmetry
Gravitational Lens Effect on the Images of High Redshift Objects : Astrophysics and Relativity
Clustering of Galaxies and Clusters of Galaxies in a Decaying-Particle Cosmological Model with a Massive Decay Product : Astrophysics and Relativity
Partially Self-Similar Spacetimes and Fluid Motions
Scalar Perturbations at the Reheating Phase in a New Inflationary Universe : Astrophysics and Relativity
Primordial lrregularities in the Early Universe
Post-Newtonian Equations of Motion in an Expanding Universe
Decaying-Particle Universe Models with Nonzero Cosmological Constant and the Galactic Number Count Observation
Non-Linear Theory of Gravitational Instability in the Expanding Universe. II
Partially Self-Similar Solutions in General Relativity
Gravitational Collapse of a Rotating Star : Formulation I
Primordial Irregularities in an Early Universe with Vacuum Phase Transitions
Nonlinear Behavior of Nonspherical Perturbations of the Schwarzschild Metric
Non-Linear Theory of Gravitational Instability in the Expanding Universe. III
Galaxy Formation in the Neutrino Dominated Universe
Large-Scale Anisotropy of the Cosmic Background Radiation Due to Primordial Density and Gravitational-Wave Perturbations
Tensor Spherical and Pseudo-Spherical Harmonics in Four-Dimensional Spaces
On a Perfect-Fluid Sphere with Uniform Density
Non-Linear Theory of Gravitational Instability in the Expanding Universe
On the Removal of Initial Singularity in a Big-Bang Universe in Terms of a Renormalized Theory of Gravitation. II : Criteria for Obtaining a Physically Reasonable Model
Element Formation in a Chaotic Early Universe
On Inhomogeneous Cosmological Model Containing Space-Like and Time-Like Singularities Alternately
Formation of Gravitationally Bound Primordial Gas Clouds
On the Spectral Shift of Light Rays Emitted from a Pulsating Object
Formation of Gravitationally Bound Primordial Gas Clouds. II
Evolution of Irregularities in a Chaotic Early Universe
On the Non-Linear Behavior of Nonspherical Perturbations in Relativistic Gravitational Collapse
The Dipole anisotropy in the Decaying-Particle Universe Models with Nonzero Cosmological Constant
Theoretical Relations among Observable Quantities in an Anisotropic and Homogeneous Universe
An Oscillating Perfect-Fluid Sphere with Uniform Density
Reduction of Partially Self-Similar Space-Times to Self-Similar Ones in General Relativity

Tensor Spherical and Pseudo-Spherical Harmonics in Four-Dimensional Spaces

スポンサーリンク

概要

著者

関連論文

スポンサーリンク