The gamma-ray energy output from a supernova explosion

Details The gamma-ray energy output from a supernova explosion The gamma-ray energy output from a supernova explosion

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988chjss...8...47d&link_type=abstract

(Chinese Journal of Space Science, vol. 8, Jan. 1988, p. 47-52) Chinese Physics (ISSN 0273-429X), vol. 8, Oct.-Dec. 1988, p. 965

Astronomy and Astrophysics

Astronomy

Carbon 14, Energy Sources, Gamma Ray Astronomy, Supernovae, Upper Atmosphere, Electromagnetic Radiation, Planetary Evolution, Radio Waves, Solar System

Scientific paper

Using a two-box model, the dependence of C-14 concentration in the atmosphere on the C-14 production rate, the inventories and residence time of carbon in the atmosphere and ocean are deduced. Then a formula for calculating the increment of number of C-14 nuclei in the atmosphere after a supernova explosion according to tree ring C-14 data and a formula for estimating the gamma-ray energy output emitted from the explosion are successively given.

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