1、 06 年南京引力波天文学暑期学校课程表上 午 (am)下 午 (pm)8:00 -9:4010:00-11:4014:30-16:1016:30-17:207月 24日/星期一报到(Registration)高能天体物理讨论会(Workshop on High Energy Astrophysics)7月 25日/星期二高能天体物理讨论会(Workshop on High Energy Astrophysics)7月 26日(星期三)恒星演化与核合成(彭秋和)广义相对论(须重明)高能天体物理(1)(戴子高)广义相对论(须重明)7月 27日(星期四)恒星演化与核合成(彭秋和)广义相对论(须重明
2、)高能天体物理(1)(戴子高)广义相对论(须重明)7月 28日(星期五)恒星演化与核合成(彭秋和)广义相对论(须重明)高能天体物理(2)(李向东)广义相对论(须重明)7月 29日(星期六)高能天体物理(3)(徐仁新)广义相对论(须重明)相对论天体物理(袁业飞)7月 30日/星期日休 息(Rest day)7月 31日(星期一)相对论天体物理(袁业飞)广义相对论(须重明)宇宙学(景益鹏)广义相对论(张鹏杰)8月 1日(星期二)拍照宇宙学(张鹏杰)考试(examination)Overview of GW Science(M. Diaz)Weak GWs in Flat Space(W. Ande
3、rson)GW Discussion8月 2日(星期三)Weak field Generation of GWs(W. Anderson)What is the gravitational wave research community?(M. Diaz)Discussion(USA)LectureEarth-Based Gravitational Wave detectors (interferometers and bars)(M. Diaz)Discussion(USA)8月 3日(星期四)LIGO Data Analysis(W. Anderson)Discussion(USA)LIG
4、O Data Analysis(W. Anderson)The LISA Mission(M. Benacquista)Discussion(USA)8月 4日(星期五)The LISA Mission(M. Benacquista)Radio Pulsars: an overview(G. Hobbs)Discussion(USA)Current Limits on theories of gravity using radio pulsars(G. Hobbs)Gravitational Wave Detection Using Pulsar Timing (Part I)(F. Jene
5、t)Discussion(USA)8月 5日/星期六8月 6日/星期日休 息(Rest day)8月 7日(星期一)Gravitational Wave Detection Using Pulsar Timing (Part II)(F. Jenet)Pulsar Timing and Gravitational Wave Detection Experiments(G. Hobbs)Discussion(USA)The Big-Bang Observatory(M. Diaz)Gravitational wave detection using CMB polarization(F. Jen
6、et)Discussion(USA)8月 8日(星期二)Particle Orbits, particle perturbation theory, EMRIs(R. Price)Particle Orbits, particle perturbation theory, EMRIs(R. Price)Discussion(USA)Particle Orbits, particle perturbation theory, EMRIs(R. Price)BH and NS perturbations, QN ringing, Relativistic NS(R. Price)Discussio
7、n(USA)8月 9日(星期三)BH and NS perturbations, QN ringing, Relativistic NS(R. Price)Astrophysical Phenomenology of Binary-Star GW sources(M. Benacquista)Discussion(USA)Astrophysical Phenomenology of Binary-Star GW sources(M. Benacquista)Dynamical processes in dense stellar environments(M. Benacquista)Disc
8、ussion(USA)8月 10日(星期四)Dynamical processes in dense stellar environments(M. Benacquista)Cosmology and Gravitational Waves(F. Jenet)Discussion(USA)Numerical Rel and equal mass inspiral(R. Price)Summary with emphasis on remaining problems(M. Diaz)Discussion(USA)8月 11日(星期五)Discussion(USA)Discussion(USA)
9、相对论天体物理讨论会(Workshop on relativistic Astronomy)8月 12日(星期六)相对论天体物理讨论会(Workshop on relativistic Astronomy)会议以及上课地点：知行楼一楼报告厅引力波天文学讲座内容 (每一讲 2小时)PART I: INTRODUCTION-Overview of Gravitational Wave Science (1) (MD)Weak Gravitational Waves in Flat Space-time (1) (WA)Generation of Gravitational waves (Weak
10、Field) (1) (WA)PART II: DETECTING AND UNDERSTANDING GWs-What is the gravitational wave research community? (1) (MD)Earth-Based Gravitational Wave detectors (interfers and bars) (2) (MD)LIGO Data Analysis (3) (WA)The LISA mission (2) (MB)Radio pulsars: an overview (1) (GH)Current limits on theories o
11、f gravity using radio pulsars (1) (GH)Gravitational wave detection using pulsar timing (2) (FJ)Pulsar timing and Gravitational wave detection experiments (1) (GH)The Big-Bang Observatory (1) (MD)GW detection using CMB polarization (1) (FJ)PART III: GENERATION OF GWs-Particle orbits, particle perturb
12、ation theory, EMRIs. (3) (RP)BH and NS perturbations, QN ringing, Relativistic NS (2) (RP)Astrophysical Phenomenology of Binary-Star GW sources (2) (MB)Dynamical processes in dense stellar environments (2) (MB)PART IV: BRIDGES TO OTHER AREAS OF RELATIVITY-Cosmology and Gravitational Waves (1) (FJ)Numerical Rel and equal mass inspiral (1) (RP)PART V: SUMMARY-Summary with emphasis on remaining problems (1) (MD)- 1 -
