论文部分内容阅读
Pulsars and Gravity
【机 构】
:
CSIRO Astronomy and Space Science Sydney Australia
【出 处】
:
2015 Pulsar and Gravitational- Wave School (脉冲星和引力波学派研讨会)
【发表日期】
:
2015年期
其他文献
What is the Bispectrum and Trispectrum In mathematics,in the area of statistical analysis,the bispectrum is a statistic used to search for nonlinear interaction
会议
The Unidentified Fermi sources The Large Area Telescope(LAT) aboard the Fermi satellite allows us to study the high-energy gamma-ray sky with unprecedented sens
会议
Outline Basic Observations(SMBMB) Hierarchical Models of Galaxy Formation Comic Evolution of MBHs BHB coalescence and Gravitational Waves星系的并合大质量黑洞的
会议
BACKGROUND It is difficult to localise the Gravitational wave(GW) source.However,localising the sources of GWs is vitally crucial to perform EM follow up and fu
会议
11,脉冲星到达时间的残差:As a weak gravitational wave passes through the solar system,the metric is given by ds2=-dt2+(1+A+)dx2+(1-A+)dy2+dz2+2Axdxdy.a pulsar of
会议
The overall work safety progress made in the past 10 years in the chemical process industry of China is briefly reviewed.Some weaknesses including abnormal
会议
PartⅠ 广义相对论的基本思想内容提要1弯曲时空的描述2弯曲时空中粒子运动3广义相对论的四大经验平直欧几里德空间笛卡尔坐标系:(x1,x2,x3)=(x,y,z),则空间线元为:ds2=(dx1)
会议
What was the idea? Search in known pulsars for more specific type:drifting subpulses of multiple drift rates.-observational:initial identification of switching
会议
Outline Test of GR in Solar System Introduction to Black Hole Astrophysics Probes of Strong Gravity in Black Hole Accretion System Strong Gravity strong or weak
会议