Table of Contents
Fetching ...

CP violations in neutrino oscillations modulated by singular and non-singular gravities

Ze-Wen Li, Shu-Jun Rong, Ya-Ru Wang

Abstract

Flavor oscillations in curved space-time provide a novel channel to explore the unknown parameters of neutrinos. In this work, the gravity-modulated CP violations (CPVs) in neutrino oscillations were investigated under the Reissner-Nordstrom, Hayward, and Simpson-Visser metric. The interplay among the CPV, the properties of neutrinos, and the space-time is illustrated with analytical and numerical methods. The morphologies of the flavor-oscillation curves show that the information on the mass-ordering, the absolute mass, and the gravitational parameters could be encoded into the amplitudes and periods of the CPVs. Hence, the characteristic of the space-time background may be identified through its modulation effects on the CPV, such as amplification, damping on the amplitudes.

CP violations in neutrino oscillations modulated by singular and non-singular gravities

Abstract

Flavor oscillations in curved space-time provide a novel channel to explore the unknown parameters of neutrinos. In this work, the gravity-modulated CP violations (CPVs) in neutrino oscillations were investigated under the Reissner-Nordstrom, Hayward, and Simpson-Visser metric. The interplay among the CPV, the properties of neutrinos, and the space-time is illustrated with analytical and numerical methods. The morphologies of the flavor-oscillation curves show that the information on the mass-ordering, the absolute mass, and the gravitational parameters could be encoded into the amplitudes and periods of the CPVs. Hence, the characteristic of the space-time background may be identified through its modulation effects on the CPV, such as amplification, damping on the amplitudes.
Paper Structure (16 sections, 58 equations, 11 figures)

This paper contains 16 sections, 58 equations, 11 figures.

Figures (11)

  • Figure 1: Schematic neutrino propagation impacted by gravitational lensing. $S$ is the source, $D$ is the detector. $b$ is the impact factor, $\delta$ is the deflection angle and $\gamma$ marks the misalignment of the coordinates $(x,y)$ and $(x',y')$. For the original construction of the plot, see Swami:2020qdi and the adapted versions see Chakrabarty:2021bprAlloqulov:2024snsShi:2024flw.
  • Figure 2: CP violation including the lensing effects of RN metric under weak-field, with $m_{l}=0$.
  • Figure 3: CP violation including the lensing effects of RN metric under strong-field, with $m_{l}=0$.
  • Figure 4: CP violation including the lensing effects of HA metric under weak-field, with $m_{l}=0$.
  • Figure 5: CP violation including the lensing effects of HA metric under strong-field, with $m_{l}=0$.
  • ...and 6 more figures