TY - BOOK AU - Sano,Hidetoshi ED - SpringerLink (Online service) TI - Shock-Cloud Interaction in RX J1713.7−3946: Evidence for Cosmic-Ray Acceleration in the Young VHE γ-ray Supernova Remnant T2 - Springer Theses, Recognizing Outstanding Ph.D. Research, SN - 9784431556367 AV - QB460-466 U1 - 523.01 23 PY - 2017/// CY - Tokyo PB - Springer Japan, Imprint: Springer KW - Astrophysics KW - Particle acceleration KW - Astrophysics and Astroparticles KW - Particle Acceleration and Detection, Beam Physics N1 - Introduction -- Non-Thermal X-ray Enhancement around Dense Gas Clumps -- Evidence for the Acceleration of Cosmic Ray Protons -- Evidence for Efficient Acceleration of Cosmic Rays -- Summary and Future Prospects; Available to subscribing member institutions only. Доступно лише організаціям членам підписки N2 - This book presents a study of the young supernova remnant RX J1713.7-3946 in order to reveal the origin of cosmic rays in our galaxy. The study focuses on the X-ray and gamma radiation from the cosmic ray electrons and protons in the supernova remnant as well as the emission from the surrounding interstellar gas measured by the NANTEN2 4-m radio telescope at Nagoya University. The gamma rays show a good spatial correspondence with the interstellar gas, which for the first time provides strong evidence of the acceleration of cosmic ray protons. Additionally, the author determines that an interaction between the supernova shockwaves and interstellar gas, referred to as “shock-cloud interaction,” promotes the efficient acceleration of cosmic ray electrons in the supernova remnant. The book reveals that the interstellar gas plays an essential role in producing the high-energy radiation and cosmic rays, offering vital new insights into the origin and behavior of galactic cosmic rays UR - https://doi.org/10.1007/978-4-431-55636-7 ER -