Pramana | |
Relativistic theory of inverse beta-decay of polarized neutron in strong magnetic field | |
A Studenikin11  S Shinkevich1  | |
[1] Department of Theoretical Physics, Moscow State University, 119992, Moscow, Russia$$ | |
关键词: Inverse beta-decay; strong magnetic fields; neutron stars.; | |
DOI : | |
学科分类:物理(综合) | |
来源: Indian Academy of Sciences | |
【 摘 要 】
The relativistic theory of the inverse beta-decay of polarized neutron, ð‘£ð‘’ + 𑛠→ ð‘ + ð‘’-, in strong magnetic field is developed. For the proton wave function we use the exact solution of the Dirac equation in the magnetic filed that enables us to account exactly for effects of the proton momentum quantization in the magnetic field and also for the proton recoil motion. The effect of nucleons anomalous magnetic moments in strong magnetic fields is also discussed. We examine the cross-section for different energies and directions of propagation of the initial neutrino accounting for neutron polarization. It is shown that in the super-strong magnetic field the totally polarized neutron matter is transparent for neutrinos propagating antiparallel to the direction of polarization. The developed relativistic approach can be used for calculations of cross-sections of the other URCA processes in strong magnetic fields.
【 授权许可】
Unknown
【 预 览 】
Files | Size | Format | View |
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RO201912040496908ZK.pdf | 831KB | download |