PNNL

Abstract

The eV axion is a well-motivated extension to the standard model. The Axion Dark Matter 27 eXperiment (ADMX) collaboration seeks to discover this particle by looking for the resonant con28 version of dark-matter axions to microwave photons in a strong magnetic eld. In this paper we 29 report results from an ADMX pathnder experiment, the ADMX \Sidecar", which is designed to 30 pave the way for future, higher mass, searches. The Sidecar experiment excludes masses in three 31 widely spaced frequency ranges (4202-4249 MHz, 5086-5799 MHz and 7173-7203 MHz), correspond32 ing to masses favored by some cosmic string simulations. In addition, Sidecar demonstrates the 33 successful use of piezoelectric actuators for both cavity tuning and antenna coupling. Finally, this publication is the rst to report data taken on both the TM010 and TM020 modes.