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1
PHYSREVD.88.045020
PHYSREVD.88.045020
http://dx.doi.org/10.1103/PHYSREVD.88.045020
Does the finite size of the proto-neutron star preclude supernova neutrino flavor scintillation due to turbulence?
P356
Q57426076-3FFDABC4-7CFE-47CA-83F7-5EF203E8A2B1
P356
PHYSREVD.88.045020
http://dx.doi.org/10.1103/PHYSREVD.88.045020