Stored light optimization and optical depth

ORAL

Abstract

Efficient storage of light in an atomic ensemble requires a large optical depth to contain an entire light pulse inside an atomic medium without incoherent absorption. In an idealized theoretical picture, very large optical depths should improve the efficiency of stored light. In practice, however, additional effects such as spin-exchange, radiation trapping, and non-linear processes can reduce the efficiency at large optical depths. Here we present an experimental study of stored light efficiency in Rb vapor as a function of optical depth, varying experimental parameters such as pulse duration and shape, storage time, retrieval field intensity, and cell and beam geometry.

Authors

  • Mason Klein

    Harvard-Smithsonian CfA, Harvard-Smithsonian Center for Astrophysics

  • Yanhong Xiao

    Harvard-Smithsonian CfA, Harvard-Smithsonian Center for Astrophysics and Harvard University, Harvard-Smithsonian Center for Astrophysics

  • Rita Kalra

    Harvard-Smithsonian CfA

  • Michael Hohensee

    Harvard-Smithsonian CfA

  • David F. Phillips

    Harvard-Smithsonian CfA, Harvard-Smithsonian Center for Astrophysics and Harvard University

  • Ronald L. Walsworth

    Harvard-Smithsonian CfA, Harvard-Smithsonian Center for Astrophysics and Harvard University, Harvard-Smithsonian Center for Astrophysics