Speaker
Prof.
Chung Yue Hui
(Chungnam National University)
Description
We have performed a statistical analysis to compare the populations of radio-quiet gamma-ray pulsars and non-recycled radio-loud gamma-ray pulsars. We found a number of physical properties of these two populations are different such as the magnetic field at the light cylinder, the gamma-ray to x-ray flux ratio, and their gamma-ray spectral curvature. Such differences can shed light on the acceleration mechanism in the pulsar magnetosphere.
Primary author
Prof.
Chung Yue Hui
(Chungnam National University)
Co-author
Prof.
Jumpei Takata
(Huazhong University of Science and Technology)
