Modeling emission from the first explosions [electronic resource] : pitfalls and problems

Published: Washington, D.C. : United States. Dept. of Energy, 2010.
Oak Ridge, Tenn. : Distributed by the Office of Scientific and Technical Information, U.S. Dept. of Energy.
Additional Creators: Los Alamos National Laboratory, United States. Department of Energy, and United States. Department of Energy. Office of Scientific and Technical Information

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Summary

Observations of the explosions of the population III stars have the potential to teach us much about the formation and evolution of these zero metallicity objects. But to reach this potential, we must tie the observed emission to and explosion model. This requires accurate light-curve/spectral calculations. Here we discuss many of the pitfalls and problems involved in such calculations, presenting some preliminary results from radiation-hydrodynamics calculations.

Report Numbers

E 1.99:la-ur-10-03387
E 1.99: la-ur-10-3387
la-ur-10-3387
la-ur-10-03387

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Note

Published through SciTech Connect.
01/01/2010.
"la-ur-10-03387"
" la-ur-10-3387"
FT
Fryer, Christopher Lee; Whalen, Daniel J; Frey, Lucille H.

Funding Information

AC52-06NA25396

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