universe
Article
Gravitational Effects on Neutrino Decoherence in the
Lense–Thirring Metric
Giuseppe Gaetano Luciano
1,2,
*
,†
and Massimo Blasone
1,2,
*
,†
Citation: Luciano, G.G.; Blasone, M.
Gravitational Effects on Neutrino
Decoherence in the Lense–Thirring
Metric. Universe 2021, 7, 417. https://
doi.org/10.3390/universe7110417
Academic Editor: Tina Kahniashvili
Received: 27 September 2021
Accepted: 29 October 2021
Published: 1 November 2021
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1
Dipartimento di Fisica, Università di Salerno, 84084 Fisciano, SA, Italy
2
Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Gruppo Collegato di Salerno,
84084 Fisciano, SA, Italy
* Correspondence: gluciano@sa.infn.it (G.G.L.); blasone@sa.infn.it (M.B.)
† These authors contributed equally to this work.
Abstract: We analyze the effects of gravity on neutrino wave packet decoherence. As a specific
example, we consider the gravitational field of a spinning spherical body described by the Lense–
Thirring metric. By working in the weak-field limit and employing Gaussian wave packets, we show
that the characteristic coherence length of neutrino oscillation processes is nontrivially affected, with
the corrections being dependent on the mass and angular velocity of the gravity source. Possible
experimental implications are finally discussed.
Keywords: neutrino oscillations; decoherence; gravity; Lense–Thirring metric; wave packets
1. Introduction
Neutrinos are among the elementary particles in the Standard Model (SM) of funda-
mental interactions. In spite of this, their essential nature has not yet been fully revealed,
and has become even more puzzling after Pontecorvo’s pioneering idea of neutrino mass
and mixing [1–3] and the subsequent discovery of flavor oscillations [4–7]. Further studies
in Quantum Field Theory (QFT) have highlighted the shortcomings of the standard quan-
tum mechanical (QM) predictions by pointing out the unitary inequivalence between the
Fock spaces for definite flavor fields and definite mass fields [8–10]. Phenomenological
implications of this inequivalence have been investigated in a variety of contexts, ranging
from vacuum effects [11–15] to particle decays [16–19] and apparent violations of the weak
equivalence principle [20].
Neutrino mixing and oscillations are typically analyzed in the plane wave approxi-
mation. However, a more realistic treatment that accounts for neutrinos being localized
particles should involve the use of wave packets (WPs), which introduce decoherence
among the mass eigenstates. The first WP approach was developed in [21], showing the
existence of a coherence length beyond which the interference between massive neu-
trinos becomes negligible. This effect arises from the different group velocities of the
different mass states, which leads WPs to spread over macroscopic sizes and separate
during the propagation. Wave packet models of neutrino oscillations were later developed
within the framework of QM [22–24] and QFT [25–28], both in vacuum and matter [29–31]
(see [32] for a review). In particular, in dense environments, decoherence through WP
separation was shown to depend on the model chosen for the adiabaticity violation of WP
evolution [30,31].
All of the above investigations were performed in flat spacetime. The effects of gravity
on neutrino decoherence were addressed in [33] by considering a static and spherically
symmetric field described by the Schwarzschild metric. By adopting the density matrix for-
malism [31] with Gaussian WPs and exploiting previous achievements of [34–36], neutrino
decoherence was quantified by a coherence coordinate distance and a proper time. As a
result, it was shown that these quantities are nontrivially modified with respect to the flat
Universe 2021, 7, 417. https://doi.org/10.3390/universe7110417 https://www.mdpi.com/journal/universe