Blitzar

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In astronomy, blitzars are a hypothetical type of star, specifically pulsars that can rapidly collapse into black holes. Heino Falcke and Luciano Rezzolla[1] proposed these stars in 2013 as an explanation for fast radio bursts.[2]

Overview[edit]

These stars, if they exist, are thought to start from a neutron star with a mass that would cause it to collapse into a black hole if it were not rapidly spinning. Instead, the neutron star spins fast enough so that its centripetal force overcomes gravity. This makes the neutron star a typical but doomed pulsar whose strong magnetic field radiates energy away and slows its spin. Eventually the weakening centrifugal force is no longer able to stop the pulsar from its transformation into a black hole. At this moment, part of the pulsar's magnetic field outside the black hole is suddenly cut off from its vanished source. This magnetic energy is instantly transformed into a burst of wide spectrum radio energy.[3] As of January 20, 2015, seven [4] radio events detected so far might represent such possible collapses; they are projected to occur every 10 seconds within the observable universe.[3] Because the magnetic field had previously cleared the surrounding space of gas and dust, there is no nearby material that will fall into the new black hole. Thus there is no burst of X-rays or gamma rays that usually happens when other black holes form.[3]

If blitzars exist, they may offer a new way to observe details of black hole formation.[5]

References[edit]

  1. ^ "Afscheidsgroet van een stervende ster" (in Dutch). Radboud University Nijmegen. 4 July 2013. Retrieved 26 July 2015.[permanent dead link]
  2. ^ Heino Falcke; Luciano Rezzolla (2014). "Fast radio bursts: The last sign of supramassive neutron stars". Astronomy & Astrophysics. 562: A137. arXiv:1307.1409. Bibcode:2014A&A...562A.137F. doi:10.1051/0004-6361/201321996. S2CID 32284857.
  3. ^ a b c Thornton, D.; Stappers, B.; Bailes, M.; Barsdell, B.; Bates, S.; Bhat, N. D. R.; Burgay, M.; Burke-Spolaor, S.; Champion, D. J.; Coster, P.; d'Amico, N.; Jameson, A.; Johnston, S.; Keith, M.; Kramer, M.; Levin, L.; Milia, S.; Ng, C.; Possenti, A.; Van Straten, W. (5 July 2013). "A Population of Fast Radio Bursts at Cosmological Distances". Science. 341 (6141): 53–56. arXiv:1307.1628. Bibcode:2013Sci...341...53T. doi:10.1126/science.1236789. PMID 23828936. S2CID 206548502.. Summarized in Mysterious Radio Flashes May Be Farewell Greetings from Massive Stars Collapsing Into Black Holes and Cosmic Radio Bursts Point to Cataclysmic Origin
  4. ^ "Extremely short, sharp flash of radio waves from unknown source in the universe, caught as it was happening". 2015-01-19. Retrieved 2016-03-03.
  5. ^ Heino Falcke & Luciano Rezzolla. "Blitzars: Fast Radio Bursts from Supramassive Rotating Neutron Stars". Retrieved 8 July 2013.