Design, Status and Physics Potential of JUNO

Steiger, Hans Jakob

doi:10.22323/1.405.0086

Cited by 2 publications

(2 citation statements)

References 12 publications

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“…The effects of the cutoff in the coherence length would be evident in the low energy spectrum, since, in the absence of the CS effect, for sufficiently low energy smaller than E thr ν it would be possible to observe the neutrino oscillation suppression caused by the presence of the SGWB. Also, the latter effect would be possible to observe: considering for example the JUNO experiment, the energy is ∼ 3% MeV/E [119,186] so that the neutrino search is more sensitive towards the higher end of the spectrum, within the threshold E ν ∼ 50 MeV.…”

Section: Jcap01(2023)011mentioning

confidence: 99%

Gravitational waves and neutrino oscillations in Chern-Simons axion gravity

Lambiase

Mastrototaro

Visinelli

2023

J. Cosmol. Astropart. Phys.

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We investigate the modifications in the neutrino flavor oscillations under the influence of a stochastic gravitational wave background (SGWB), in a scenario in which General Relativity is modified by an additional Chern-Simons (CS) term. Assuming that the dark matter halo is in the form of axions, the CS coupling modifies the pattern of the neutrino flavor oscillations at Earth up to a total suppression in some frequency range. At the same time, the SGWB in the halo could stimulate the axion decay into gravitons over a narrow frequency range, leading to a potentially detectable resonance peak in the enhanced SGWB strain. A consistent picture would require these features to potentially show up in neutrino detection from supernovae, gravitational wave detectors, and experiments aimed at the search for axions in the Milky Way halo.

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Section: Jcap01(2023)011mentioning

confidence: 99%

Gravitational waves and neutrino oscillations in Chern-Simons axion gravity

Lambiase

Mastrototaro

Visinelli

2023

J. Cosmol. Astropart. Phys.

View full text Add to dashboard Cite

show abstract

“…The effects of the cutoff in the coherence length would be evident in the low energy spectrum, since, in the absent of the CS effect, for a sufficiently low energy smaller than E thr ν it would be possible to observe the neutrino oscillation suppression caused by the presence of the SGWB. Also, the latter effect would be possible to observe: considering for example the JUNO experiment, the energy resolution is ∼ 3% MeV/E [111,164] so that the neutrino search is more sensitive towards the higher end of the spectrum, within the threshold E ν ∼ 50 MeV.…”

Section: B Effects On Neutrino Oscillationsmentioning

confidence: 99%