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Luminosity decay


tex2html_wrap_inline3922   > 90% of energy in neutrinos

Luminosities dominated by
tex2html_wrap_inline3922   Fire ball initially
tex2html_wrap_inline3922   Radioactive decays at intermediate times
tex2html_wrap_inline3922   possibly pulsar powered at later times

Figure 27: The luminosity decay of supernovae.

Jon Bell
Thu Dec 19 15:15:11 GMT 1996