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Discovery of a radiation component from the Vela pulsar reaching 20 teraelectronvolts

  • The H.E.S.S. Collaboration et al.
  • Dublin Institute for Advanced Studies
  • Max-Planck-Institut für Kernphysik
  • Yerevan State University
  • Universität Heidelberg
  • Landessternwarte Heidelberg
  • University of Amsterdam
  • Department of Physics
  • University of Namibia
  • Centre for Space Research
  • North-West University
  • c/o DESY
  • School of Physics
  • University of the Witwatersrand, Johannesburg
  • Astroparticule and Cosmol APC
  • Department of Physics and Electrical Engineering
  • Linnaeus University, Växjö
  • Institut für Physik
  • Humboldt-Universität zu Berlin
  • University of Tübingen
  • LUTH - Laboratoire de l'Univers et de ses Theories
  • Sorbonne Université
  • CNRS
  • Université Savoie Mont Blanc
  • Université Paris-Saclay
  • Friedrich-Alexander University (FAU) Erlangen-Nürnberg and Universitätsklinikum Erlangen
  • University of Warsaw
  • Institute for Nuclear Physics
  • University of Oxford
  • University of Potsdam
  • Aix-Marseille Université
  • University of Adelaide
  • Ip Paris
  • Laboratoire Univers et Particules de Montpellier

Research output: Contribution to journalArticlepeer-review

29 Citations (Scopus)

Abstract

Gamma-ray observations have established energetic isolated pulsars as outstanding particle accelerators and antimatter factories. However, many questions are still open regarding the acceleration and radiation processes involved, as well as the locations where they occur. The radiation spectra of all gamma-ray pulsars observed to date show strong cutoffs or a break above energies of a few gigaelectronvolts. Using the High Energy Stereoscopic System’s Cherenkov telescopes, we discovered a radiation component from the Vela pulsar which emerges beyond this generic cutoff and extends up to energies of at least 20 teraelectronvolts. This is an order of magnitude larger than in the case of the Crab pulsar, the only other pulsar detected in the teraelectronvolt energy range. Our results challenge the state-of-the-art models for the high-energy emission of pulsars. Furthermore, they pave the way for investigating other pulsars through their multiteraelectronvolt emission, thereby imposing additional constraints on the acceleration and emission processes in their extreme energy limit.

Original languageEnglish
Pages (from-to)1341-1350
Number of pages10
JournalNature Astronomy
Volume7
Issue number11
DOIs
Publication statusPublished - 1 Nov 2023

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