Abstract
Core collapse supernovae are dominated by weakly interacting neutrinos. This provides a unique opportunity for macroscopic parity violation. We speculate that parity violation in a strong magnetic field can lead to an asymmetry in the explosion and a recoil of the newly formed neutron star. We estimate the size of this asymmetry from neutrino polarized-neutron elastic scattering, polarized electron capture and neutrino-nucleus elastic scattering in a (partially) polarized electron gas.
Original language | English |
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Pages (from-to) | 281-289 |
Number of pages | 9 |
Journal | Nuclear Physics A |
Volume | 640 |
Issue number | 2 |
DOIs | |
State | Published - 14 Sep 1998 |
Externally published | Yes |
Bibliographical note
Funding Information:This work was supported by the DOE under grant numbers DE-FG02-87ER40365,