Abstract:
Radio pulsars are rapidly spinning neutron stars with strong magnetic dipole fields. They slow-down by converting their rotational kinetic energy into radiation.
Although it is commonly accepted that they release magnetic dipole radiation there is wealth ofevidence for the existence of contributing processes.
I will discuss some of these processes:(i) the growth of magnetic fields, (2) increasing inclination angle between rotation and magnetic axis and (3) the presence of debris disks which couple to their magnetospheres.
Information about the speaker: //www.fizik.itu.edu.tr/eksiy
Speaker: K. Yavuz Ekşi (Istanbul Technical University)
May 14, 2014 Wednesday at 13:40-14:40 ,Sabancı University, SUNUM seminar room
May 14, 2014 Wednesday at 13:40-14:40 ,Sabancı University, SUNUM seminar room