中子寿命和中子和氢的暗衰变

Q2 Physics and Astronomy
Z. Berezhiani
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引用次数: 27

摘要

中子,除了它的$\beta$ -衰变$n\to p e\bar\nu_e$,可能有一个新的衰变通道$n\to n' X$变成镜像中子$n'$,它来自平行暗扇区的近质量简并双胞胎,以及一个无质量玻色子$X$,它可以是普通光子和镜像光子,或者一些更奇特的粒子。这种看不见的衰变可以缓解中子寿命在束流和阱实验中测量的张力。我讨论了这种情况的一些现象学和天体物理学后果,这取决于镜像中子的质量范围$n'$。也就是说,在$m_{n'} m_p + m_e$的情况下,衰变$n'\to pe\bar \nu_e$是允许的,$n'$可以代表一个不稳定的暗物质成分,它的寿命相当长,超过了宇宙的年龄。然而,这种衰变会产生大量的漫射伽马背景。然而,暗衰变对寿命之谜的解释与测量中子衰变$\beta$ -不对称性的最后实验结果存在矛盾。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Neutron lifetime and dark decay of the neutron and hydrogen
The neutron, besides its $\beta$-decay $n\to p e\bar\nu_e$, might have a new decay channel $n\to n' X$ into mirror neutron $n'$, its nearly mass degenerate twin from parallel dark sector, and a massless boson $X$ which can be ordinary and mirror photons or some more exotic particle. Such an invisible decay could alleviate the tension between the neutron lifetimes measured in the beam and trap experiments. I discuss some phenomenological and astrophysical consequences of this scenario, which depends on the mass range of mirror neutron $n'$. Namely, the case $m_{n'} m_p + m_e$, then the decay $n'\to pe\bar \nu_e$ is allowed and $n'$ can represent an unstable dark matter component with rather large lifetime exceeding the age of the Universe. Nevertheless, this decay would produce substantial diffuse gamma background. The dark decay explanation of the lifetime puzzle, however, has a tension with the last experimental results measuring $\beta$-asymmetry in the neutron decay.
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来源期刊
Letters in High Energy Physics
Letters in High Energy Physics Physics and Astronomy-Nuclear and High Energy Physics
CiteScore
1.20
自引率
0.00%
发文量
4
审稿时长
12 weeks
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