Superbunching in cathodoluminescence: a master equation approach
Tatsuro Yuge, Naoki Yamamoto, Takumi Sannomiya, Keiichirou Akiba

TL;DR
This paper introduces a master equation model for cathodoluminescence that explains superbunching phenomena by analyzing the second-order correlation function and the quantum state of emitted radiation.
Contribution
The paper develops a novel master equation approach to describe superbunching in cathodoluminescence, providing exact and approximate formulas for correlation functions.
Findings
The model accurately describes giant bunching in CL.
Superbunching arises from a mixture of excited photon and vacuum states.
Derived formulas for $g^{(2)}(0)$ and $g^{(2)}(\tau)$.
Abstract
We propose a theoretical model of a master equation for cathodoluminescence (CL). The master equation describes simultaneous excitation of multiple emitters by an incoming electron and radiative decay of individual emitters. We investigate the normalized second-order correlation function, , of this model. We derive the exact formula for the zero-time delay correlation, , and show that the model successfully describes giant bunching (superbunching) in the CL. We also derive an approximate form of , which is valid for small excitation rate. Furthermore, we discuss the state of the radiation field of the CL. We reveal that the superbunching results from a mixture of an excited photon state and the vacuum state and that this type of state is realized in the CL.
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Taxonomy
TopicsStrong Light-Matter Interactions · Atomic and Molecular Physics · Atmospheric Ozone and Climate
