U.S.-Japan Joint Seminar: The Structure and Evolution of Neutron Stars/November 1990/Kyoto, Japan

美日联合研讨会：中子星的结构与演化/1990年11月/日本京都

• 批准号: 8915315
• 负责人: David Pines
• 金额: $ 1.75万
• 依托单位: University of Illinois at Urbana-Champaign
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 1990
• 资助国家: 美国
• 起止时间: 1990-09-01 至 1992-05-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=8915315&HistoricalAwards=false
• 关键词: U.S.; Japan; Joint; Seminar; Structure

This award will support the participation of six U.S. scientists in a U.S.-Japan joint seminar on the internal structure, dynamical behavior, formation, and evolution of neutron stars. Emphasis will be placed on theoretical work on these topics which is relevant to understanding X-ray, optical, and pulsar- timing observations, including the superfluidity and equation of state of hadron matter, the role of neutrinos and hot equations of state in neutron star formation and earliest evolution, theories relating to the recent supernova in our galaxy (SN1987A), and mechanisms of cooling and heating neutron stars. Participants in the meeting represent major U.S. and Japanese research groups concerned with the fundamental physics and astrophysics of neutron stars. Seminar co- organizers are Dr. David Pines, Department of Physics and Center for Advanced Study, University of Illinois at Urbana- Champaign, and Dr. Ryozo Tamagaki, Department of Physics, Kyoto University, Japan. The seminar will take place November 6-10, 1990, in Kyoto, under the auspices of the U.S.-Japan Cooperative Science Program. Since the discovery of pulsars and galactic X-ray sources, significant progress has been achieved in the field of neutron star physics. The discovery of Supernova 1987A in our galaxy stimulated much observational and theoretical work in this area, both in the U.S. and Japan. Though various meetings have been held to consider recent observational results, there has been much less opportunity for U.S. and Japanese neutron star theorists to meet and discuss their work relevant to understanding the observations. This seminar is intended to enhance significantly the interaction and exchange of knowledge among the currently most active experts of both countries in this field.

该奖项将支持六名美国科学家参与 在美国，日本内部结构联合研讨会， 中子星的动力学行为、形成和演化。 重点将放在这些主题的理论工作上 这与理解X射线、光学和脉冲星有关， 定时观测，包括超流性和方程 强子物质的状态，中微子和热的作用 中子星星形成和最早期的状态方程 进化论，与我们最近的超新星有关的理论， 星系（SN 1987 A），以及冷却和加热机制 中子星 与会者代表主要 美国和日本的研究团体关注的基本 中子星物理学和天体物理学。 研讨会共同- 组织者是物理系的大卫派恩斯博士， 伊利诺伊大学厄巴纳分校高级研究中心- 尚潘，和博士Ryozo Tamagaki，物理系， 日本京都大学。 研讨会将于11月举行。 1990年6月至10日，在美国的主持下，在京都举行-日本 合作科学计划。 自从发现了恒星和银河X射线源以来， 在中子领域取得了重大进展， 星星物理学。 超新星1987 A在银河系的发现 激发了许多观测和理论工作， 地区，无论是在美国和日本。 虽然各种会议 一直在考虑最近的观测结果， 美国和日本的机会要少得多， 中子星星理论家开会讨论他们的工作有关 来理解观察结果。 本次研讨会旨在 大大加强互动和交流， 目前最活跃的专家之间的知识， 国在这一领域。