Jump to content
 







Main menu
   


Navigation  



Main page
Contents
Current events
Random article
About Wikipedia
Contact us
Donate
 




Contribute  



Help
Learn to edit
Community portal
Recent changes
Upload file
 








Search  

































Create account

Log in
 









Create account
 Log in
 




Pages for logged out editors learn more  



Contributions
Talk
 



















Contents

   



(Top)
 


1 Overview  





2 References  














Blitzar






العربية
Français

Polski
Русский
Українська
 

Edit links
 









Article
Talk
 

















Read
Edit
View history
 








Tools
   


Actions  



Read
Edit
View history
 




General  



What links here
Related changes
Upload file
Special pages
Permanent link
Page information
Cite this page
Get shortened URL
Download QR code
Wikidata item
 




Print/export  



Download as PDF
Printable version
 
















Appearance
   

 






From Wikipedia, the free encyclopedia
 


Inastronomy, blitzars are a hypothetical type of neutron star, specifically pulsars that can rapidly collapse into black holes if their spinning slows down. 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 centrifugal 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 halt the pulsar from collapsing into a black hole. At that 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.[5] As of January 2015, seven[6] radio events detected so far might represent such possible collapses; they are projected to occur every 10 seconds within the observable universe.[5] 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-raysorgamma rays that usually happens when other black holes form.[5]

If blitzars exist, they may offer a new way to observe details of black hole formation.[7]

References[edit]

  1. ^ "Afscheidsgroet van een stervende ster" (Press release) (in Dutch). Nijmegen, NL: Radboud University. 4 July 2013. Retrieved 26 July 2015.[permanent dead link]
  • ^ 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.
  • ^ "Mysterious radio flashes may be farewell greetings from massive stars collapsing into black holes". ScienceDaily (Press release). July 2013.
  • ^ "Cosmic radio bursts point to cataclysmic origin". ScienceDaily (Press release). July 2013.
  • ^ a b c Thornton, D.; Stappers, B.; Bailes, M.; Barsdell, B.; Bates, S.; Bhat, N.D.R.; et al. (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.
    For a popular summary see[3][4]
  • ^ "Extremely short, sharp flash of radio waves from unknown source in the universe, caught as it was happening". ScienceDaily (Press release). 19 January 2015. Retrieved 3 March 2016.
  • ^ Falcke, Heino; Rezzolla, Luciano. "Blitzars: Fast radio bursts from supramassive rotating neutron stars". Astronomy. Nijmegen, NL: Radboud University. Retrieved 8 July 2013.

  • Retrieved from "https://en.wikipedia.org/w/index.php?title=Blitzar&oldid=1213461443"

    Categories: 
    Hypothetical stars
    Neutron stars
    Black holes
    Hidden categories: 
    CS1 Dutch-language sources (nl)
    All articles with dead external links
    Articles with dead external links from July 2020
    Articles with permanently dead external links
    Use dmy dates from May 2022
    Articles with short description
    Short description is different from Wikidata
     



    This page was last edited on 13 March 2024, at 06:13 (UTC).

    Text is available under the Creative Commons Attribution-ShareAlike License 4.0; additional terms may apply. By using this site, you agree to the Terms of Use and Privacy Policy. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc., a non-profit organization.



    Privacy policy

    About Wikipedia

    Disclaimers

    Contact Wikipedia

    Code of Conduct

    Developers

    Statistics

    Cookie statement

    Mobile view



    Wikimedia Foundation
    Powered by MediaWiki