4.2 Article

Cosmogenic production as a background in searching for rare physics processes

Journal

ASTROPARTICLE PHYSICS
Volume 31, Issue 6, Pages 417-420

Publisher

ELSEVIER SCIENCE BV
DOI: 10.1016/j.astropartphys.2009.04.004

Keywords

Cosmogenic activation; Dark matter detection; Double-beta decay

Funding

  1. NSF [PHY-0758120]
  2. Office of Research at The University of South Dakota
  3. Laboratory Directed Research and Development at Los Alamos National Laboratory
  4. MOE of China [IRT0624]
  5. NFSC [10635020]
  6. Direct For Mathematical & Physical Scien
  7. Division Of Physics [758120] Funding Source: National Science Foundation

Ask authors/readers for more resources

We revisit calculations of the cosmogenic production rates for several long-lived isotopes that are potential sources of background in searching for rare physics processes such as the detection of dark matter and neutrinoless double-beta decay. Using updated cosmic-ray neutron flux measurements, we use TALYS 1.0 to investigate the cosmogenic activation of stable isotopes of several detector targets and find that the cosmogenic isotopes produced inside the target materials and cryostat can result in large backgrounds for dark matter searches and neutrinoless double-beta decay. We use previously published low-background HPGe data to constrain the production of H-3 on the surface and the upper limit is consistent with our calculation. We note that cosmogenic production of several isotopes in various targets can generate potential backgrounds for dark matter detection and neutrinoless double-beta decay with a massive detector, thus great care should be taken to limit and/or deal with the cosmogenic activation of the targets. Published by Elsevier B.V.

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