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.
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Authors
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Mason Klein
Harvard-Smithsonian CfA, Harvard-Smithsonian Center for Astrophysics
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Yanhong Xiao
Harvard-Smithsonian CfA, Harvard-Smithsonian Center for Astrophysics and Harvard University, Harvard-Smithsonian Center for Astrophysics
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Rita Kalra
Harvard-Smithsonian CfA
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Michael Hohensee
Harvard-Smithsonian CfA
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David F. Phillips
Harvard-Smithsonian CfA, Harvard-Smithsonian Center for Astrophysics and Harvard University
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Ronald L. Walsworth
Harvard-Smithsonian CfA, Harvard-Smithsonian Center for Astrophysics and Harvard University, Harvard-Smithsonian Center for Astrophysics