Spectrum of a radio pulse from an exploding black hole

Details Spectrum of a radio pulse from an exploding black hole Spectrum of a radio pulse from an exploding black hole

Nov 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mnras.181..489b&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 181, Nov. 1977, p. 489-498.

Astronomy and Astrophysics

Astronomy

13

Black Holes (Astronomy), Explosions, Interstellar Magnetic Fields, Radio Spectra, Stellar Radiation, Electron-Positron Pairs, Positrons, Pulsed Radiation, Stellar Models

Scientific paper

Black holes of mass below approximately 10 to the 11th power kg may be able to radiate all of their rest mass in an essentially instantaneous explosion by the Hawking process provided that the number of available modes increases sufficiently rapidly with temperature. Rees has pointed out that should this happen, electron-positron pairs may form a significant fraction of the explosion products and that if the hole is surrounded by a typical interstellar magnetic field, the kinetic energy of the pairs may be efficiently transformed into radio waves. In this paper the spectrum of the observed radiation is calculated and conditions necessary for this to be detectable are further discussed.

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