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Mayle, R.; Wilson, J.R.; Schramm, D.N.
Fermi National Accelerator Lab., Batavia, IL (USA)1986
Fermi National Accelerator Lab., Batavia, IL (USA)1986
AbstractAbstract
[en] Detailed calculations are made of the neutrino spectra emitted during gravitational collapse events (Type II supernovae). Those aspects of the neutrino signal which are relatively independent of the collapse model and those aspects which are sensitive to model details are discussed. The easier-to-detect high energy tail of the emitted neutrinos has been calculated using the Boltzmann equation which is compared with the result of the traditional multi-group flux limited diffusion calculations. 8 figs., 28 refs
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May 1986; 36 p; Available from NTIS, PC A03/MF A01 as DE86012304
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Numerical Data
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