Abstract
- Received 3 December 2016
DOI:https://doi.org/10.1103/PhysRevD.95.029904
© 2017 American Physical Society
Erratum: First axion results from the XENON100 experiment [Phys. Rev. D 90, 062009 (2014)]
E. Aprile et al. (XENON100 Collaboration)
Phys. Rev. D 95, 029904 – Published 31 January 2017
Images
Figure 1
The XENON100 limit (90% C.L.) on ALP coupling to electrons as a function of the mass, under the assumption that ALPs constitute all the dark matter in our Galaxy (blue line). The expected sensitivity is shown by the green/yellow bands (). The other curves are constraints set by CoGeNT [1] (light brown dashed line), CDMS [2] (blue dashed line), and EDELWEISS-II [3] (brown dashed line). The indirect astrophysical bound from solar neutrinos [4] is represented as a continous light gray line. The benchmark Kim-Shifman-Vainshtein-Zakharov (KSVZ) model is represented by a black line [5, 6].
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