Neutron-Mirror Neutron conversion in Vacuum, Trap, Material and Neutron Star
B.O. Kerbikov
TL;DR
This paper explores neutron-mirror neutron transitions across various environments, from vacuum to neutron stars, using advanced quantum formalisms to understand potential swapping mechanisms and their implications.
Contribution
It introduces a comprehensive theoretical framework combining density matrix formalism, Lindblad and Bloch equations, and seesaw mechanism effects to analyze neutron-mirror neutron conversions.
Findings
Neutron-mirror neutron transitions are environment-dependent.
The formalism predicts possible observable effects in different settings.
Implications for neutron star physics and experimental detection methods.
Abstract
The possibility of neutron swapping between the ordinary and mirror sectors is today a subject of a great many theoretical and experimental studies. In this paper, we investigate the neutron-mirror neutron transitions in different environments from vacuum to neutron star. Our approach is based on the density matrix formalism, Lindblad and Bloch equations and the implication of the seesaw mechanism to the Hamiltonian diagonalization.
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