Takatsuka Tatsuyuki | College Of Humaniteis And Social Sciences Iwate University

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著作論文

Chapter X Outlook
Chapter VIII Implications of Various Hadron Phases to Neutron Star Phenomena
Chapter VII Neutral Pion Condensation in Hot and Dense Nuclear Matter
Chapter V Toward Realistic Treatment of Neutral Pion-Condensed State
Chapter III Characteristic Aspects of Pion-Condensed Phases
Neutral Pion Condensation and Alternating Layer Spin Model Including Isobar Δ(1232) in Hot Symmetric Nuclear Matter
Single-Particle Potential of Isobar Δ(1232) in Nuclear Matter Based on Extended Effective Interaction
Pion Condensation and Alternating Layer Spin Model in Symmetric Nuclear Matter : Use of Extended Effective Nuclear Forces : Nuclear Physics
Postglitch Timing Behavior of Vela and Crab Pulsars in an Extended Starquake Model for Neutron Stars with Pion-Condensed Core : Nuclear Phusics
Phase Transition of Hot Neutron Matter to π^0-Condensed State : Astrophysics and Relativity
Proton ^1S_0-Dominant Superfluidity with Two-Dimensional Character under Well-Developed π^0 Condensation
Neutron ^3P_2-Dominant Superfluidity with Two-Dimensional Character under Well-Developed π^0 Condensation
Attenuation of ^3P_2-Superfluidity in Neutron Star Matter Due to Charged-Pion Condensation
Nuclear Matter at Finite Temperature : Dependence on Nuclear Incompressibility : Progress Letters
On the Effect of Non-Condensed Pions in Nuclear Medium
Characteristics and Evolution of Neutron Stars Just Born
Corequake Model of Pulsar Glitches for Neutron Stars with Pion-Condensed Core
Study on Neutron ^3P_2-Superfluidity with Two-Dimensional Character under π^0 Condensation in Neutron Star Matter
Hot Neutron Star with Pion Condensations and Characteristics of Neutrino Burst from SN1987A
A Note on Partial-Wave Contribution in [ALS]-Phase of Nuclear Medium
Pion-Condensed Neutron Star and Supernova 1987A
Density and Temperature of Compressed Nuclear Matter
Energy Gaps in Crust-Phase of Neutron Stars
Nucleon Superfluidity under Coexistent Condensation of Neutral and Charged Pions in Neutron Matter
Chapter II Superfluidity in Neutron Star Matter and Symmetric Nuclear Matter
Particular Properties of Dense Supernova Matter : Nuclear Physics
Properties of Hot Asymmetric Nuclear Matter : Nuclear Physics
Proton Abundance in Dense Supernova Matter
Effective Two-Nucleon Interaction in Asymmetric Nuclear Matter : Nuclear Physics
Neutral-Meson Condensation in Nuclear Medium from the Viewpoint of One-Boson-Exchange Model
Solidification and Pion Condensation in Nuclear Medium : Alternating-Layer-Spin Structure with One-Dimensional Localization Accompanying π^0 Condensate
Study on Characteristics of π^0-Condensate in Neutron Matter : Effective Nucleon Mass and Role of Non-Tensor Force
Effective Interaction Approach to Hot Nuclear Matter
Chapter IV Nucleon Superfluidity under Pion Condensation in Neutron Star Matter
Characteristic Features and Releasable Energy of Hot Neutron Stars

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