Skip to main content
Book cover

Revealing the Most Energetic Light from Pulsars and Their Nebulae

  • Book
  • © 2019

Overview

  • Nominated as an outstanding Ph.D. thesis by the Complutense University of Madrid, Spain
  • Offers a comprehensive introduction to VHE emissions from pulsars, together with a detailed compilation of VHE observations of the Crab Pulsar and novel scientific results
  • Provides the most complete picture of VHE emissions from the Crab Pulsar to date

Part of the book series: Springer Theses (Springer Theses)

  • 2686 Accesses

This is a preview of subscription content, log in via an institution to check access.

Access this book

eBook USD 84.99
Price excludes VAT (USA)
  • Available as EPUB and PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book USD 109.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info
Hardcover Book USD 109.99
Price excludes VAT (USA)
  • Durable hardcover edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Other ways to access

Licence this eBook for your library

Institutional subscriptions

Table of contents (9 chapters)

  1. The Very-High-Energy Sky and the MAGIC Telescopes

  2. Search for TeV Emission from the Crab and Other Pulsars

  3. Looking for a Pulsar Wind Nebula in the Outer Part of Our Galaxy

Keywords

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. 



Authors and Affiliations

  • Faculty of Physics, Complutense University of Madrid, Madrid, Spain

    David Carreto Fidalgo

Bibliographic Information

Publish with us