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J.Va'vra: A New Possible Way to Explain DAMA Results
The cross-section prediction for the DAMA experiment was
compared to limits obtained by Tevatron and LHC experiments
ATLAS and CMS. Although there are still several unknowns in
our assumptions, there seems to be a large discrepancy. This
weakens the argument of this paper somewhat, but since the
WIMP was not yet discovered, it may be interesting to pursue
these thoughts further.
4. Acknowledgements
I would like to thanks Profs. L. Ronaldi and E.V. Kolb for pro-
viding several references, which allowed me to enter the up-to-
date status of the collider WIMP searches. I would like also to
thank Prof. E. Nappi for showing interest in the idea, sharing it
with Prof. C. Broggini, and asking very good questions about
early version of the paper.
References
R.Bernabei et al., Dark Matter investigation by DAMA at Gran Sasso,
arXiv:1308.5109, 2013.
K.A.Kudin et al., Effect of C03 and OH impurities on thermal growing condi-
tions of large size NaI(Tl) crystals and their quality, Functional Materials
18, No.2 (2011).
G. Knoll, Radiation detection and measurement, Wiley, ISBN: 978-0-470-
13148-0, 4th edition, 2010, page 240.
R.Catena and P.Ullio, The local Dark Matter phase-space density and impact on
WIMP direct detection, arXiv:1111.3556v1, 15 Nov., 2011.
M.Beltran et al., Maverick dark matter at colliders, arXiv:1002.4137v2, 2010.
ATLAS collaboration, Search for dark matter candidates and large extra di-
mensions in events with a jet and missing transverse momentum with the
ATLAS detector, arXiv:1002.4137v2, 2013.
CMS collaboration, Search for new physics in monojet events in pp collisions at
8 TeV, CMS PAS EXO-12-048, 2013.3
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Va'vra, J. A New Way to Explain DAMA Results, article, January 7, 2014; United States. (https://digital.library.unt.edu/ark:/67531/metadc868459/m1/3/: accessed April 25, 2024), University of North Texas Libraries, UNT Digital Library, https://digital.library.unt.edu; crediting UNT Libraries Government Documents Department.