Characteristics and Evolution of Neutron Stars Just Born
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概要
- 論文の詳細を見る
The equation of state (EOS) of dense supernova matter is constructed by the finite-temperature Hartree-Fock approach with the effective two-nucleon interaction. On the basis of the EOS, characteristic features of neutron stars at the birth are demonstrated. The releasable energy and the extent of spin-up, as a result of the evolution to usual cold neutron stars, are also discussed.Hot neutron starspin-upreleasable energy
- 東北大学の論文
- 1991-01-31
著者
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Takatsuka Tatsuyuki
College Of Humanities And Social Sciences Iwate University
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Takatsuka Tatsuyuki
College Of Humaniteis And Social Sciences Iwate University
関連論文
- 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
- Proton Mixing in π^0-Condensed Phase of Neutron Star Matter : Nuclear Physics
- 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