Pith. sign in

REVIEW 8 cited by

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2305.01150 v2 pith:HZ7UUDO3 submitted 2023-05-02 nucl-th astro-ph.HEhep-phquant-ph

Quantum information and quantum simulation of neutrino physics

classification nucl-th astro-ph.HEhep-phquant-ph
keywords flavorinteractionsneutrinosquantumenvironmentsevolutionneutrinocorrelations
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

In extreme astrophysical environments such as core-collapse supernovae and binary neutron star mergers, neutrinos play a major role in driving various dynamical and microphysical phenomena, such as baryonic matter outflows, the synthesis of heavy elements, and the supernova explosion mechanism itself. The interactions of neutrinos with matter in these environments are flavor-specific, which makes it of paramount importance to understand the flavor evolution of neutrinos. Flavor evolution in these environments can be a highly nontrivial problem thanks to a multitude of collective effects in flavor space, arising due to neutrino-neutrino ($\nu$-$\nu$) interactions in regions with high neutrino densities. A neutrino ensemble undergoing flavor oscillations under the influence of significant $\nu$-$\nu$ interactions is somewhat analogous to a system of coupled spins with long-range interactions among themselves and with an external field ('long-range' in momentum-space in the case of neutrinos). As a result, it becomes pertinent to consider whether these interactions can give rise to significant quantum correlations among the interacting neutrinos, and whether these correlations have any consequences for the flavor evolution of the ensemble. In particular, one may seek to utilize concepts and tools from quantum information science and quantum computing to deepen our understanding of these phenomena. In this article, we attempt to summarize recent work in this field. Furthermore, we also present some new results in a three-flavor setting, considering complex initial states.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 8 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Three-flavor supernova neutrino simulation using a hybrid quantum-classical algorithm with qutrits

    hep-ph 2026-05 unverdicted novelty 7.0

    A hybrid qutrit-based algorithm simulates supernova neutrino flavor evolution and matches exact classical integration up to moderate times.

  2. Tightening energy-based boson truncation bound using Monte Carlo-assisted methods

    hep-lat 2026-04 unverdicted novelty 7.0

    Monte Carlo-assisted tightening of the energy-based boson truncation bound substantially reduces volume dependence in (1+1)D scalar field theory and (2+1)D U(1) gauge theory.

  3. Tightening energy-based boson truncation bound using Monte Carlo-assisted methods

    hep-lat 2026-04 unverdicted novelty 7.0

    A Monte Carlo-assisted analytic method tightens energy-based bounds on boson truncation errors, substantially reducing the volume dependence of the required cutoff in scalar and gauge theories.

  4. Quantum resource redistribution drives spectral splits in dense neutrino gases

    quant-ph 2026-05 unverdicted novelty 6.0

    Tensor network simulations of two-flavor neutrinos link spectral splits to peaks in entanglement entropy and local minima in non-local magic, indicating resource redistribution drives the phenomenon.

  5. Collective neutrino oscillations: Many-body non-forward effects and non-classicality

    hep-ph 2026-06 unverdicted novelty 5.0

    In a neutrino-gas model, the many-body Hamiltonian yields different evolution timescales and asymptotics than the quantum kinetic approach with collisions, while quantum resources for the full case sit at the low end ...

  6. Neutrino helicity oscillations in astrophysical environments: a many-body approach

    hep-ph 2026-05 unverdicted novelty 5.0

    Many-body neutrino calculations in simple momentum-state configurations yield helicity conversion probabilities orders of magnitude above mean-field results due to momentum exchange.

  7. Tightening energy-based boson truncation bound using Monte Carlo-assisted methods

    hep-lat 2026-04 unverdicted novelty 5.0

    New analytic and Monte Carlo-assisted method tightens energy-based boson truncation bounds, reducing volume dependence in (1+1)D scalar and (2+1)D U(1) gauge theories.

  8. Quantum Simulation of Collective Neutrino Oscillations using Dicke States

    quant-ph 2026-04 unverdicted novelty 5.0

    New algorithms based on Dicke states enable qubit-efficient quantum simulations of collective neutrino oscillations with demonstrated performance on classical and quantum hardware.