2023/06/30 by Santos, Marcos V. dos, de Holanda, Pedro C., Neto, Pedro Dedin +1
#FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #High Energy Physics - Phenomenology (hep-ph) #High Energy Physics - Theory (hep-th)
paper · doi:10.48550/arxiv.2306.17591
Quantum decoherence effects in neutrinos, described by the open quantum systems formalism, serve as a gateway to explore potential new physics, including quantum gravity. Previous research extensively investigated these effects across various neutrino sources, imposing stringent constraints on the spontaneous loss of coherence. In this study, we demonstrate that even within the Supernovae environment, where neutrinos are released as incoherent states, quantum decoherence could influence the flavor equipartition of 3ν mixing. Additionally, we examine the potential energy dependence of quantum decoherence parameters (Γ= Γ0 (E/E0)n) with different power laws (n = 0, 2, 5/2). Our findings indicate that future-generation detectors (DUNE, Hyper-K, and JUNO) can significantly constrain quantum decoherence effects under different scenarios. For a Supernova located 10 kpc away from Earth, DUNE could potentially establish 3σ bounds of Γ≤ 6.2 × 10-14 eV in the normal mass hierarchy (NH) scenario, while Hyper-K could impose a 2σ limit of Γ≤ 3.6 × 10-14 eV for the inverted mass hierarchy (IH) scenario with n=0 - assuming no energy exchange between the neutrino subsystem and non-standard environment ([H,Vp] = 0). These limits become even more restrictive for a closer Supernova. When we relax the assumption of energy exchange ([H,Vp] ≠ 0), for a 10 kpc SN, DUNE can establish a 3σ limit of Γ8 ≤ 4.2 × 10-28 eV for NH, while Hyper-K could constrain Γ8 ≤ 1.3 × 10-27 eV for IH (n=0) with 2σ, representing the most stringent bounds reported to date. Furthermore, we examine the impact of neutrino loss during propagation for future Supernova detection.