Published June 24, 2014
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Xenophobic Dark Matter
Abstract
We describe models in which dark matter is xenophobic, with significantly reduced signal strength in direct detection experiments using xenon as a target material. Such models alleviate tension between xenon-based constraints and possible signal at other direct detection experiments, and in particular regions of interest at CoGeNT and CDMS are largely below XENON100 bounds in the purely xenophobic limit. We also show the constraints from upcoming LUX results and orthogonal searches using Fermi-LAT results from line searches in dwarf spheroidals and monojet searches at CMS.
Additional Information
© 2014 AIP Publishing LLC. Published: 24 June 2014. We are grateful to the Center for Theoretical Underground Physics and Related Areas (CETUP* 2013) in South Dakota for its support and hospitality. We are grateful to J. Feng, J. Kumar, D. Marfatia, and L. Strigari for collaboration. DS is supported in part by U.S. Department of Energy grant DE–FG02–92ER40701 and by the Gordon and Betty Moore Foundation through Grant No. 776 to the Caltech Moore Center for Theoretical Cosmology and Physics.Attached Files
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Additional details
- Eprint ID
- 46864
- Resolver ID
- CaltechAUTHORS:20140707-080005855
- Department of Energy (DOE)
- DE-FG02-92ER40701
- Gordon and Betty Moore Foundation
- 776
- Created
-
2014-07-07Created from EPrint's datestamp field
- Updated
-
2021-11-10Created from EPrint's last_modified field
- Caltech groups
- Caltech Theory, Moore Center for Theoretical Cosmology and Physics
- Series Name
- AIP conference proceedings
- Series Volume or Issue Number
- 1604