On the Direct Detection of Dark Matter Annihilation
Abstract
We investigate the direct detection phenomenology of a class of dark matter (DM) models in which DM does not directly interact with nuclei, but rather, the products of its annihilation do. When these annihilation products are very light compared to the DM mass, the scattering in direct detection experiments is controlled by relativistic kinematics. This results in a distinctive recoil spectrum, a nonstandard and/or even absent annual modulation, and the ability to probe DM masses as low as a ~ 10 MeV. Here, we use current LUX data to show that experimental sensitivity to thermal relic annihilation cross sections has already been reached in a class of models. Moreover, the compatibility of dark matter direct detection experiments can be compared directly in E min space without making assumptions about DM astrophysics, mass, or scattering form factors. Lastly, when DM has direct couplings to nuclei, the limit from annihilation to relativistic particlesin the Sun can be stronger than that of conventional nonrelativistic direct detection by more than 3 orders of magnitude for masses in a 2–7 GeV window.
- Authors:
-
- Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
- Univ. of Southern Denmark, Odense (Denmark). CP3-Origins and the Danish Inst. for Advanced Study
- Publication Date:
- Research Org.:
- Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1454985
- Alternate Identifier(s):
- OSTI ID: 1184441
- Report Number(s):
- LA-UR-15-20058
Journal ID: ISSN 0031-9007; TRN: US1901183
- Grant/Contract Number:
- AC52-06NA25396
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review Letters
- Additional Journal Information:
- Journal Volume: 114; Journal Issue: 23; Journal ID: ISSN 0031-9007
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS
Citation Formats
Cherry, John Francis Jr., Frandsen, Mads T., and Shoemaker, Ian M. On the Direct Detection of Dark Matter Annihilation. United States: N. p., 2015.
Web. doi:10.1103/PhysRevLett.114.231303.
Cherry, John Francis Jr., Frandsen, Mads T., & Shoemaker, Ian M. On the Direct Detection of Dark Matter Annihilation. United States. https://doi.org/10.1103/PhysRevLett.114.231303
Cherry, John Francis Jr., Frandsen, Mads T., and Shoemaker, Ian M. Fri .
"On the Direct Detection of Dark Matter Annihilation". United States. https://doi.org/10.1103/PhysRevLett.114.231303. https://www.osti.gov/servlets/purl/1454985.
@article{osti_1454985,
title = {On the Direct Detection of Dark Matter Annihilation},
author = {Cherry, John Francis Jr. and Frandsen, Mads T. and Shoemaker, Ian M.},
abstractNote = {We investigate the direct detection phenomenology of a class of dark matter (DM) models in which DM does not directly interact with nuclei, but rather, the products of its annihilation do. When these annihilation products are very light compared to the DM mass, the scattering in direct detection experiments is controlled by relativistic kinematics. This results in a distinctive recoil spectrum, a nonstandard and/or even absent annual modulation, and the ability to probe DM masses as low as a ~ 10 MeV. Here, we use current LUX data to show that experimental sensitivity to thermal relic annihilation cross sections has already been reached in a class of models. Moreover, the compatibility of dark matter direct detection experiments can be compared directly in E min space without making assumptions about DM astrophysics, mass, or scattering form factors. Lastly, when DM has direct couplings to nuclei, the limit from annihilation to relativistic particlesin the Sun can be stronger than that of conventional nonrelativistic direct detection by more than 3 orders of magnitude for masses in a 2–7 GeV window.},
doi = {10.1103/PhysRevLett.114.231303},
journal = {Physical Review Letters},
number = 23,
volume = 114,
place = {United States},
year = {Fri Jun 12 00:00:00 EDT 2015},
month = {Fri Jun 12 00:00:00 EDT 2015}
}
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