Parity Violation

C. Horowitz
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引用次数: 8

Abstract

Core collapse supernovae are gigantic explosions of massive stars that radiate 99% of their energy in neutrinos. This provides a unique opportunity for large scale parity or charge conjugation violation. Parity violation in a strong magnetic field could lead to an asymmetry in the neutrino radiation and recoil of the newly formed neutron star. Charge conjugation violation in the neutrino-nucleon interaction reduces the ratio of neutrons to protons in the neutrino driven wind above the neutron star. This is a problem for r-process nucleosynthesis in this wind. On earth, parity violation is an excellent probe of neutrons because the weak charge of a neutron is much larger than that of a proton. The Parity Radius Experiment (PREX) at Jefferson Laboratory aims to precisely measure the neutron radius of Pb with parity violating elastic electron scattering. This has many implications for astrophysics, including the structure of neutron stars, and for atomic parity nonconservation experiments. PACS. 25.30.Bf , 11.30.Er, 26.60+c, and 97.60.Bw
宇称不守恒
核心坍缩超新星是大质量恒星的巨大爆炸,其99%的能量以中微子的形式辐射出来。这为大规模宇称或电荷共轭破坏提供了一个独特的机会。强磁场中的宇称破坏可能导致新形成的中子星的中微子辐射和反冲的不对称性。中子-核子相互作用中的电荷共轭破坏降低了中子星上方中微子驱动风中的中子与质子的比率。这是r-过程核合成的一个问题。在地球上,宇称破坏是一种很好的中子探测方法,因为中子的弱电荷比质子的弱电荷大得多。美国杰斐逊实验室的宇称半径实验(PREX)旨在利用宇称违反弹性电子散射精确测量Pb的中子半径。这对天体物理学有许多启示,包括中子星的结构,以及原子宇称非守恒实验。pac。25.30.男朋友,11点半。嗯,26.60+c和97.60 bw
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