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Radiación de Hawking (Spanish Wikipedia)

Analysis of information sources in references of the Wikipedia article "Radiación de Hawking" in Spanish language version.

refsWebsite
Global rank Spanish rank
2harvard.edu
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2doi.org
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2wikipedia.org
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1cerncourier.com
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1timesonline.co.uk
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1web.archive.org
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1arxiv.org
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1nih.gov
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arxiv.org

cerncourier.com

doi.org

dx.doi.org

  • See page 596: table 1 and the "black hole decay" section and previous sentence on that page in Frautschi, Steven (1982). «Entropy in an Expanding Universe». Science 217 (4560): 593-599. Bibcode:1982Sci...217..593F. PMID 17817517. doi:10.1126/science.217.4560.593. «Since we have assumed a maximum scale of gravitational binding – for instance, superclusters of galaxies – black hole formation eventually comes to an end in our model, with masses of up to 1014 ... the timescale for black holes to radiate away all their energy ranges from to 1064 years for black holes of one solar mass ...» 
  • Page, Don N. (1976). «Particle emission rates from a black hole: Massless particles from an uncharged, nonrotating hole». Physical Review D 13 (2): 198-206. Bibcode:1976PhRvD..13..198P. doi:10.1103/PhysRevD.13.198.  See in particular equation (27).

harvard.edu

adsabs.harvard.edu

  • See page 596: table 1 and the "black hole decay" section and previous sentence on that page in Frautschi, Steven (1982). «Entropy in an Expanding Universe». Science 217 (4560): 593-599. Bibcode:1982Sci...217..593F. PMID 17817517. doi:10.1126/science.217.4560.593. «Since we have assumed a maximum scale of gravitational binding – for instance, superclusters of galaxies – black hole formation eventually comes to an end in our model, with masses of up to 1014 ... the timescale for black holes to radiate away all their energy ranges from to 1064 years for black holes of one solar mass ...» 
  • Page, Don N. (1976). «Particle emission rates from a black hole: Massless particles from an uncharged, nonrotating hole». Physical Review D 13 (2): 198-206. Bibcode:1976PhRvD..13..198P. doi:10.1103/PhysRevD.13.198.  See in particular equation (27).

nih.gov

ncbi.nlm.nih.gov

  • See page 596: table 1 and the "black hole decay" section and previous sentence on that page in Frautschi, Steven (1982). «Entropy in an Expanding Universe». Science 217 (4560): 593-599. Bibcode:1982Sci...217..593F. PMID 17817517. doi:10.1126/science.217.4560.593. «Since we have assumed a maximum scale of gravitational binding – for instance, superclusters of galaxies – black hole formation eventually comes to an end in our model, with masses of up to 1014 ... the timescale for black holes to radiate away all their energy ranges from to 1064 years for black holes of one solar mass ...» 

timesonline.co.uk

web.archive.org

wikipedia.org

es.wikipedia.org

  • «Agujero negro» |url= incorrecta con autorreferencia (ayuda). Wikipedia, la enciclopedia libre. 22 de octubre de 2019. Consultado el 11 de noviembre de 2019. 

en.wikipedia.org