Search for Halo Axions

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Description

A collaboration of MIT, LLNL, Univ. of Florida, FNAL, UC Berkeley and INR Moscow have built a large-scale RF cavity axion detector. The experiment has been taking production data since February of 1996 and is sensitive enough to detect plausible dark matter axions comprising a reasonable fraction of the mass in our galactic halo. After a brief introduction to axion physics, I discuss details of our instrumentation, our analysis methodology, our run plan and future goals of the experiments.

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13 p.

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Daw, E. J., & van Bibber, K. January 1, 1998.

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Description

A collaboration of MIT, LLNL, Univ. of Florida, FNAL, UC Berkeley and INR Moscow have built a large-scale RF cavity axion detector. The experiment has been taking production data since February of 1996 and is sensitive enough to detect plausible dark matter axions comprising a reasonable fraction of the mass in our galactic halo. After a brief introduction to axion physics, I discuss details of our instrumentation, our analysis methodology, our run plan and future goals of the experiments.

Physical Description

13 p.

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OSTI as DE98052209

Other: FDE: PDF; PL:

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  • International workshop on the identification of dark matter (IDM), Sheffield (United Kingdom), 8-11 Sep 1996

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  • Other: DE98052209
  • Report No.: UCRL-JC--129344
  • Report No.: CONF-9609179--
  • Grant Number: W-7405-ENG-48
  • Office of Scientific & Technical Information Report Number: 572564
  • Archival Resource Key: ark:/67531/metadc696905

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  • January 1, 1998

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  • Aug. 14, 2015, 8:43 a.m.

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  • April 10, 2017, 1:23 p.m.

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Daw, E. J., & van Bibber, K. Search for Halo Axions, article, January 1, 1998; California. (digital.library.unt.edu/ark:/67531/metadc696905/: accessed August 17, 2017), University of North Texas Libraries, Digital Library, digital.library.unt.edu; crediting UNT Libraries Government Documents Department.