论文标题
矢量场的烙印在太阳中微子通量上非标准耦合
Imprints of vector field non-standard couplings on solar neutrino flux
论文作者
论文摘要
关于深色能量量表和中微子质量的邻近性，可以在中微子风味转化率上获得对矢量场深色能量成分的探针特征的新见解。假定向量场通过筛选范式将矢量场与各种物质组成部分结合在一起。我们展示了振荡概率如何通过有限大小的物质密度（如Sun）（对于相关模型参数的不同值）进行不同的进化。考虑到现有的中微子风味转化数据，我们指出了这种非标准耦合如何影响中微子通量，并且还计算了太阳能电子中性旋转的总通量中的差异。
Regarding the proximity of dark energy scale and neutrino mass, one can get new insight into the probe signatures of vector field dark energy component on neutrino flavor conversion. A vector field is assumed to be conformally coupled to various matter components through a screening paradigm. We show how the oscillation probabilities evolve differently with a finite-size matter density like the Sun for different values of relevant model parameters. Considering existing neutrino flavor conversion data, we point out how this non-standard coupling affects neutrino fluxes and also we compute the discrepancy in the total flux of solar electron-neutrinos.
