Consequences of large <math display='inline'><msub><mi>θ</mi><mn>13</mn></msub></math> for the turbulence signatures in supernova neutrinos [electronic resource]
Here, the transition probabilities for a single neutrino emitted from a point proto-neutron source after passage through a turbulent supernova density profile have been found to be random variates drawn from parent distributions whose properties depend upon the stage of the explosion, the neutrino e...
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| Online Access: |
Online Access (via OSTI) |
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| Format: | Government Document Electronic eBook |
| Language: | English |
| Published: |
Washington, D.C. : Oak Ridge, Tenn. :
United States. Department of Energy. Office of Nuclear Physics ; distributed by the Office of Scientific and Technical Information, U.S. Department of Energy,
2013.
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| Subjects: |
Internet
Online Access (via OSTI)Online
| Call Number: |
E 1.99:1325222
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| E 1.99:1325222 | Available |