Improvements to the Axion Dark Matter eXperiment High Resolution Axion Search

Details Improvements to the Axion Dark Matter eXperiment High Resolution Axion Search Improvements to the Axion Dark Matter eXperiment High Resolution Axion Search

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aps..aprd14003h&link_type=abstract

American Physical Society, APS April Meeting 2012, March 31-Apr 3, 2012, abstract #D14.003

Physics

Scientific paper

The Axion Dark Matter eXperiment (ADMX) High Resolution (HR) Channel searches for flows of non-thermalized halo axions, characterized by their very low velocity dispersion, via the inverse Primakoff Effect. A power spectrum would show such axion flows as a peak with spectral broadening of order Hz or lower. The HR Channel is sensitive to signals of this nature, having a spectral resolution as fine as 40 mHz. In this talk we present a means of analysis for the HR data which will improve upon ADMX's recently published results (resolution of 10.8 Hz) by performing several searches using a range of resolutions while still accounting for signal modulation due to terrestrial motion.

Affiliated with

Also associated with

No associations

Rating

Improvements to the Axion Dark Matter eXperiment High Resolution Axion Search does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Improvements to the Axion Dark Matter eXperiment High Resolution Axion Search, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Improvements to the Axion Dark Matter eXperiment High Resolution Axion Search will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1369779