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The possibility that a neutron can be transformed to a hidden sector particle remains intriguingly open. Proposed theoretical models conjecture that the hidden sector can be represented by a mirror sector, and the neutron n can oscillate…

高能物理 - 唯象学 · 物理学 2021-11-04 Yuri Kamyshkov , James Ternullo , Louis Varriano , Zurab Berezhiani

The neutron to mirror neutron transitions in neutron stars would possibly result in significant effects. In this work we show that collisional decoherence entails exponential relaxation in lieu of oscillations. Decoherence is a great many…

高能物理 - 唯象学 · 物理学 2026-03-13 B. O. Kerbikov

We discuss the possibility of the transition magnetic moments (TMM) between the neutron n and mirror neutron n', its hypothetical sterile twin from parallel particle "mirror" sector. The neutron can be spontaneously converted into mirror…

核理论 · 物理学 2019-09-09 Zurab Berezhiani , Riccardo Biondi , Yuri Kamyshkov , Louis Varriano

Mirror Dark Matter (MDM) has been considered as an elegant framework for a particle theory of Dark Matter (DM). It is supposed that there exists a dark sector which is mirror of the ordinary matter. Some MDM models allow particle…

高能天体物理现象 · 物理学 2020-11-26 Itzhak Goldman

The oscillation of neutrons $n$ into mirror neutrons $n'$, their mass degenerate partners from dark mirror sector, can have interesting implications for neutron stars: an ordinary neutron star could gradually transform into a mixed star…

高能天体物理现象 · 物理学 2021-12-08 Zurab Berezhiani , Riccardo Biondi , Massimo Mannarelli , Francesco Tonelli

The theory of mirror matter predicts a hidden sector made up of a copy of the Standard Model particles and interactions but with opposite parity. If mirror matter interacts with ordinary matter, there could be experimentally accessible…

The mass loss in putative neutron star to mixed neutron - mirror neutron star transition implies a significant change of orbital period. The precise constancy of the latter can restrict scenarios recently suggested where neutron to mirror…

高能物理 - 唯象学 · 物理学 2020-11-26 Itzhak Goldman , Rabindra N. Mohapatra , Shmuel Nussinov

The oscillation of the neutron $n$ into mirror neutron $n'$, its partner from dark mirror sector, can gradually transform an ordinary neutron star into a mixed star consisting in part of mirror dark matter. The implications of the reverse…

高能天体物理现象 · 物理学 2021-06-22 Zurab Berezhiani

The purpose of this paper is to demonstrate that if the transformation of a neutron to a mirror neutron exists with an oscillation time of the order of ten seconds, it can be detected in a rather simple disappearance and/or regeneration…

高能物理 - 实验 · 物理学 2017-09-06 Zurab Berezhiani , Matthew Frost , Yuri Kamyshkov , Ben Rybolt , Louis Varriano

We report a novel neutron interferometry scheme aimed at probing the potential existence of mirror neutrons, which have been proposed as viable dark matter candidates. Our theoretical analysis demonstrates that if mirror neutrons exist,…

高能物理 - 唯象学 · 物理学 2025-03-05 Antonio Capolupo , Gabriele Pisacane , Aniello Quaranta , Francesco Romeo

The discrepancy between the neutron lifetimes measured in the beam and trap experiments can be explained via the neutron $n$ conversion into mirror neutron $n'$, its dark partner from parallel mirror sector, provided that $n$ and $n'$ have…

高能物理 - 唯象学 · 物理学 2019-06-26 Zurab Berezhiani

Mirror matter is considered as a candidate for dark matter. In connection with this an experimental search for neutron - mirror neutron (nn') transitions has been carried out using storage of ultracold neutrons in a trap with different…

We propose a novel neutron interferometry setup to explore the potential existence of mirror neutrons, a candidate for dark matter. Our work demonstrates that if mirror neutrons exist, neutrons will acquire an observable geometric phase due…

高能物理 - 唯象学 · 物理学 2024-06-12 Antonio Capolupo , Gabriele Pisacane , Aniello Quaranta , Francesco Romeo

We inspect the possibility that neutron star interiors are a mixture of ordinary matter and mirror dark matter. This is a scenario that can be naturally envisaged according to well studied accretion mechanisms, including the Bondi-Hoyle…

高能天体物理现象 · 物理学 2020-11-06 Raul Ciancarella , Francesco Pannarale , Andrea Addazi , Antonino Marciano

The mirror twin Higgs model is a candidate for (strongly-interacting) complex dark matter, which mirrors SM interactions with heavier quark masses. A consequence of this model are mirror neutron stars -- exotic stars made entirely of mirror…

高能天体物理现象 · 物理学 2023-07-05 Maurício Hippert , Emily Dillingham , Hung Tan , David Curtin , Jacquelyn Noronha-Hostler , Nicolás Yunes

An unexplained $>4\,\sigma$ discrepancy persists between "beam" and "bottle" measurements of the neutron lifetime. A new model proposed that conversions of neutrons $n$ into mirror neutrons $n'$, part of a dark mirror sector, can increase…

We discuss the phenomenological implications of the neutron (n) oscillation into the mirror neutron (n'), a hypothetical particle exactly degenerate in mass with the neutron but sterile to normal matter. We show that the present…

高能物理 - 唯象学 · 物理学 2015-06-25 Zurab Berezhiani , Luis Bento

Present experiments do not exclude that the neutron transforms into some invisible degenerate twin, so called mirror neutron, with an appreciable probability. These transitions are actively studied by monitoring neutron losses in ultra-cold…

高能物理 - 唯象学 · 物理学 2015-06-04 Z. Berezhiani , F. Nesti

An analysis is made of the role played by the gas environment in neutron-mirror-neutron and neutron-antineutron oscillations. In the first process the interaction with the ambient medium induces a refraction energy shift which plays the…

高能物理 - 唯象学 · 物理学 2015-12-11 B. O. Kerbikov , M. S. Lukashov , Y. A. Kamyshkov , L. J. Varriano

We study the conversion of neutron matter into strange matter as a detonation wave. The detonation is assumed to originate from a central region in a spherically symmetric background of neutrons with a varying radial density distribution.…

天体物理学 · 物理学 2011-07-19 I. Tokareva , A. Nusser , V. Gurovich , V. Folomeev
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