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NASA NTRS ยท 19750016367

Difference equation for superradiance

Abstract

The evolution of a completely excited system of N two-level atoms, distributed over a large region and interacting with all modes of radiation field, is studied. The distinction between r-conserving (RC) and r-nonconserving (RNC) processes is emphasized. Considering the number of photons emitted as the discrete independent variable, the evolution is described by a partial difference equation. Numerical solution of this equation shows the transition from RNC dominance at the beginning to RC dominance later. This is also a transition from incoherent to coherent emission of radiation.

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BibTeXRIS

Lee, C. T.. 1974-01-01. Difference equation for superradiance. https://ntrs.nasa.gov/citations/19750016367

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