学术文献库

We argue that the reflection of relic neutrinos from the surface of the Earth results in a significant local $ν-\barν$ asymmetry, far exceeding the expected primordial lepton asymmetry. The net fractional electron neutrino number $\frac{n_{ν_e}-n_{\barν_e}}{n_{ν_e}}$ is up to $\mathcal{O}(10^5) \sqrt{\frac{m_ν}{0.1~\text{eV}}}$ larger than that implied by the baryon asymmetry. This enhancement is due to the weak 4-Fermi repulsion of the $ν_e$ from ordinary matter which slows down the $ν_e$ near the Earth's surface, and to the resulting evanescent neutrino wave that penetrates below the surface. This repulsion thus creates a net $ν_e$ overdensity in a shell $\sim 7~\text{meters} \sqrt{\frac{0.1~\text{eV}}{m_ν}}$ thick around the Earth's surface. Similarly the repulsion between $\barν_μ$ or $\barν_τ$ and ordinary matter creates an overdensity of $\barν_{μ, τ}$ of similar size. These local enhancements increase the size of $\mathcal{O}(G_F)$ torques of the $CνB$ on spin-polarized matter by a factor of order $10^5$. In addition, they create a gradient of the net neutrino density which naturally provides a way out of the forty-year-old ``no-go'' theorems on the vanishing of $\mathcal{O}(G_F)$ forces. The torque resulting from such a gradient force can be $10^8$ times larger than that of earlier proposals. Although the size of these effects is still far from current reach, they may point to new directions for $CνB$ detection.