Cosmophysics Seminar (Dr. T.Saito)

Abstract

Thanks to the successful operations of Fermi-LAT and MAGIC telescopes,
the emission mechanism of gamma-ray pulsars has been getting clearer
in the last 10 years. The number of detecter pulsars has increased
from less than 10 to more than 200, and those emission can be
basically explained as the Curvature radiation from the Outer Gap. On
the other hand, new problems have also been found. For example, very
high energy emission from the Crab pulsar could not be explained by
the Curvature radiation. In this seminar, I will talk about the basic
models of gamma-ray pulsar and observational and theoretical progress
in the last 10 years, together with the future prospect of CTA
observations.

• Conference
  Conference/Workshop23 Workshops hosted by KEK0
• Colloquium
  KEK Colloquium2 Theory Colloquium0 IMSS Colloquium0
• Seminar
  IPNS Seminar3 Physics Seminar9 Theory Seminar52 Detector Seminar0 IMSS Seminar2 ACC Seminar22 ACC-Physics Seminar0 PF Seminar0 放射光セミナー0 Open-Itセミナー0 技術セミナー0 低温工学センターセミナー0 測定器開発室セミナー3 Cosmophysics Seminar9 J-PARC素粒子原子核セミナー0 Joint Seminar2 CRC Seminar0
• 談話会・交流会
  物構研談話会1 技術交流会0 講義0 公聴会0 講習会0