A Search for Scalar Chameleons with ADMX

M. Hotz, Charles R. Martin,Richard F. Bradley,John Clarke, J. Hoskins, Darin Kinion, C. A. Hagmann,K. van Bibber, S.J. Asztalos,Pierre Sikivie,Gray Rybka, David B. Tanner, L.J. Rosenberg,Gianpaolo Carosi

Lawrence Berkeley National Laboratory（2010）

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摘要

Scalar fields with a “chameleon” property, in which the effective particle mass is a function of its local environment, are common to many theories beyond the standard model and could be responsible for dark energy. If these fields couple weakly to the photon, they could be detectable through the “afterglow” effect of photon-chameleon-photon transitions. The ADMX experiment was used in the first chameleon search with a microwave cavity to set a new limit on scalar chameleon

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