スポンサーリンク
Research Institute for Theoretical Physics Hiroshima University | 論文
- 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
- Quantum Theory of Fields in an Expanding Space. I
- On a Canonical Treatment of the Einstein Equations in an Expanding Universe : Isotropic Coordinate Conditions
- Behavior of the Central Region of a Collapsing Star with Spherical Symmetry and Pressure Gradient
- Molecular Orientation in Vacuum-Deposited Poly(thiophene) Film Studied by Second-Harmonic Generation
- On an Extended Framework for the Description of Elementary Particles
- Parity Nonconserving Nuclear Force in the Process n+p → d+γ
- Enhancement of the |ΔS|=0 Weak Interactions
- Gas Flows and Gas Contents in Globular Clusters
- Infra-Red Asymptotic Form of the One-Fermion Green's Function in Two-Dimensional Quantum Chromodynamics
- Infrared Asymptotic Forms of the Gluon and Quark Propagators
- Infra-Red Asymptotic Form of the Gluon Propagator in Quantum Chromodynamics. II : Other Derivation
- Infra-Red Asymptotic Form of the Gluon Propagator in Four-Dimensional Quantum Chromodynamics
- The Many-Body-System-Like Structure of the Basic Particle
- Concepts of Space-Time in Physical Theories : Non-Spatio-Temporal Description and Universal Present
- Possible Cosmological Consequences of the Theory of Elementary Particles with Finite Degree of Freedom