Table of contents
About this book
This book reports on the extraordinary observation of TeV gamma rays from the Crab Pulsar, the most energetic light ever detected from this type of object. It presents detailed information on the painstaking analysis of the unprecedentedly large dataset from the MAGIC telescopes, and comprehensively discusses the implications of pulsed TeV gamma rays for state-of-the-art pulsar emission models. Using these results, the book subsequently explores new testing methodologies for Lorentz Invariance Violation, in terms of a wavelength-dependent speed of light. The book also covers an updated search for Very-High-Energy (VHE), >100 GeV, emissions from millisecond pulsars using the Large Area Telescope on board the Fermi satellite, as well as a study on the promising Pulsar Wind Nebula candidate PSR J0631.
The observation of VHE gamma rays is essential to studying the non-thermal sources of radiation in our Universe. Rotating neutron stars, also known as pulsars, are an extreme source class known to emit VHE gamma rays. However, to date only two pulsars have been detected with emissions above 100 GeV, and our understanding of their emission mechanism is still lacking.
Crab Pulsar TeV Emission MAGIC Telescopes VHE Gamma Rays from Pulsars Pulsar Wind Nebula TeV Emission Lorentz Invariance Violation Crab Pulsar VHE Gamma Rays from Millisecond Pulsars Fermi-LAT Observations of MSPs
- DOI https://doi.org/10.1007/978-3-030-24194-0
- Copyright Information Springer Nature Switzerland AG 2019
- Publisher Name Springer, Cham
- eBook Packages Physics and Astronomy
- Print ISBN 978-3-030-24193-3
- Online ISBN 978-3-030-24194-0
- Series Print ISSN 2190-5053
- Series Online ISSN 2190-5061
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