Shock-Cloud Interaction in RX J1713.7−3946

Evidence for Cosmic-Ray Acceleration in the Young VHE γ-ray Supernova Remnant

Nonfiction, Science & Nature, Science, Physics, Nuclear Physics, Astrophysics & Space Science
Cover of the book Shock-Cloud Interaction in RX J1713.7−3946 by Hidetoshi Sano, Springer Japan
View on Amazon View on AbeBooks View on Kobo View on B.Depository View on eBay View on Walmart
Author: Hidetoshi Sano ISBN: 9784431556367
Publisher: Springer Japan Publication: November 14, 2016
Imprint: Springer Language: English
Author: Hidetoshi Sano
ISBN: 9784431556367
Publisher: Springer Japan
Publication: November 14, 2016
Imprint: Springer
Language: English

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.

View on Amazon View on AbeBooks View on Kobo View on B.Depository View on eBay View on Walmart

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.

More books from Springer Japan

Cover of the book ACL Injury and Its Treatment by Hidetoshi Sano
Cover of the book Mountain Hazards and Disaster Risk Reduction by Hidetoshi Sano
Cover of the book Beyond Global Capitalism by Hidetoshi Sano
Cover of the book Off-Pump Coronary Artery Bypass by Hidetoshi Sano
Cover of the book Esophageal Squamous Cell Carcinoma by Hidetoshi Sano
Cover of the book Molecular Pathology of Gastroenterological Cancer by Hidetoshi Sano
Cover of the book Nano/Micro Science and Technology in Biorheology by Hidetoshi Sano
Cover of the book Chronic Inflammation by Hidetoshi Sano
Cover of the book Urban Mining Systems by Hidetoshi Sano
Cover of the book Agent-Based Approaches in Economic and Social Complex Systems VIII by Hidetoshi Sano
Cover of the book Time Series Modeling for Analysis and Control by Hidetoshi Sano
Cover of the book Personalized Treatment of Breast Cancer by Hidetoshi Sano
Cover of the book Manufacturing and Service Enterprise with Risks II by Hidetoshi Sano
Cover of the book Basic Studies in Environmental Knowledge, Technology, Evaluation, and Strategy by Hidetoshi Sano
Cover of the book MRCP by Hidetoshi Sano
We use our own "cookies" and third party cookies to improve services and to see statistical information. By using this website, you agree to our Privacy Policy