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Limits on a muon flux from Kaluza-Klein dark matter annihilations in the Sun from the IceCube 22-string detector

R Abbasi, Yasser Abdou, T Abu-Zayyad, J Adams, JA Aguilar, M Ahlers, K Andeen, J Auffenberg, X Bai, M Baker, et al. (2010) PHYSICAL REVIEW D. 81(5).
abstract
A search for muon neutrinos from Kaluza-Klein dark matter annihilations in the Sun has been performed with the 22-string configuration of the IceCube neutrino detector using data collected in 104.3 days of live time in 2007. No excess over the expected atmospheric background has been observed. Upper limits have been obtained on the annihilation rate of captured lightest Kaluza-Klein particle (LKP) WIMPs in the Sun and converted to limits on the LKP-proton cross sections for LKP masses in the range 250-3000 GeV. These results are the most stringent limits to date on LKP annihilation in the Sun.
Please use this url to cite or link to this publication:
author
organization
year
type
journalArticle (original)
publication status
published
subject
journal title
PHYSICAL REVIEW D
Phys. Rev. D
volume
81
issue
5
article number
057101
pages
6 pages
Web of Science type
Article
Web of Science id
000276194200102
JCR category
ASTRONOMY & ASTROPHYSICS
JCR impact factor
4.964 (2010)
JCR rank
7/54 (2010)
JCR quartile
1 (2010)
ISSN
1550-7998
DOI
10.1103/PhysRevD.81.057101
language
English
UGent publication?
yes
classification
A1
copyright statement
I have transferred the copyright for this publication to the publisher
id
1272044
handle
http://hdl.handle.net/1854/LU-1272044
date created
2011-06-22 09:18:49
date last changed
2016-12-21 15:41:55
@article{1272044,
  abstract     = {A search for muon neutrinos from Kaluza-Klein dark matter annihilations in the Sun has been performed with the 22-string configuration of the IceCube neutrino detector using data collected in 104.3 days of live time in 2007. No excess over the expected atmospheric background has been observed. Upper limits have been obtained on the annihilation rate of captured lightest Kaluza-Klein particle (LKP) WIMPs in the Sun and converted to limits on the LKP-proton cross sections for LKP masses in the range 250-3000 GeV. These results are the most stringent limits to date on LKP annihilation in the Sun.},
  articleno    = {057101},
  author       = {Abbasi, R and Abdou, Yasser and Abu-Zayyad, T and Adams, J and Aguilar, JA and Ahlers, M and Andeen, K and Auffenberg, J and Bai, X and Baker, M and Barwick, SW and Bay, R and Alba, JLB and Beattie, K and Beatty, JJ and Bechet, S and Becker, JK and Becker, KH and Benabderrahmane, ML and Berdermann, J and Berghaus, P and Berley, D and Bernardini, E and Bertrand, D and Besson, DZ and Bissok, M and Blaufuss, E and Boersma, DJ and Bohm, C and Bolmont, J and Botner, O and Bradley, L and Braun, J and Breder, D and Carson, Michael and Castermans, T and Chirkin, D and Christy, B and Clem, J and Cohen, S and Cowen, DF and D'Agostino, MV and Danninger, M and Day, CT and De Clercq, C and Demirors, L and Depaepe, O and Descamps, Freija and Desiati, P and De Vries-Uiterweerd, Garmt and DeYoung, T and Diaz-Velez, JC and Dreyer, J and Dumm, JP and Duvoort, MR and Edwards, WR and Ehrlich, R and Eisch, J and Ellsworth, RW and Engdegard, O and Euler, S and Evenson, PA and Fadiran, O and Fazely, AR and Feusels, Tom and Filimonov, K and Finley, C and Foerster, MM and Fox, BD and Franckowiak, A and Franke, R and Gaisser, TK and Gallagher, J and Ganugapati, R and Gerhardt, L and Gladstone, L and Goldschmidt, A and Goodman, JA and Gozzini, R and Grant, D and Griesel, T and Gross, A and Grullon, S and Gunasingha, RM and Gurtner, M and Ha, C and Hallgren, A and Halzen, F and Han, K and Hanson, K and Hasegawa, Y and Helbing, K and Herquet, P and Hickford, S and Hill, GC and Hoffman, KD and Homeier, A and Hoshina, K and Hubert, D and Huelsnitz, W and Hulss, JP and Hulth, PO and Hultqvist, K and Hussain, S and Imlay, RL and Inaba, M and Ishihara, A and Jacobsen, J and Japaridze, GS and Johansson, H and Joseph, JM and Kampert, KH and Kappes, A and Karg, T and Karle, A and Kelley, JL and Kemming, N and Kenny, P and Kiryluk, J and Kislat, F and Klein, SR and Knops, S and Kohnen, G and Kolanoski, H and Kopke, L and Koskinen, DJ and Kowalski, M and Kowarik, T and Krasberg, M and Krings, T and Kroll, G and Kuehn, K and Kuwabara, T and Labare, M and Lafebre, S and Laihem, K and Landsman, H and Lauer, R and Lehmann, R and Lennarz, D and Lucke, A and Lundberg, J and Lunemann, J and Madsen, J and Majumdar, P and Maruyama, R and Mase, K and Matis, HS and McParland, CP and Meagher, K and Merck, M and Meszaros, P and Meures, T and Middell, E and Milke, N and Miyamoto, H and Montaruli, T and Morse, R and Movit, SM and Nahnhauer, R and Nam, JW and Niessen, P and Nygren, DR and Odrowski, S and Olivas, A and Olivo, M and Ono, M and Panknin, S and Patton, S and Paul, L and Heros, CPDL and Petrovic, J and Piegsa, A and Pieloth, D and Pohl, AC and Porrata, R and Potthoff, N and Price, PB and Prikockis, M and Przybylski, GT and Rawlins, K and Redl, P and Resconi, E and Rhode, W and Ribordy, M and Rizzo, A and Rodrigues, JP and Roth, P and Rothmaier, F and Rott, C and Roucelle, C and Rutledge, D and Ruzybayev, B and Ryckbosch, Dirk and Sander, HG and Sarkar, S and Schatto, K and Schlenstedt, S and Schmidt, T and Schneider, D and Schukraft, A and Schulz, O and Schunck, M and Seckel, D and Semburg, B and Seo, SH and Sestayo, Y and Seunarine, S and Silvestri, A and Slipak, A and Spiczak, GM and Spiering, C and Stamatikos, M and Stanev, T and Stephens, G and Stezelberger, T and Stokstad, RG and Stoufer, MC and Stoyanov, S and Strahler, EA and Straszheim, T and Sulanke, KH and Sullivan, GW and Swillens, Q and Taboada, I and Tamburro, A and Tarasova, O and Tepe, A and Ter-Antonyan, S and Terranova, C and Tilav, S and Toale, PA and Tooker, J and Tosi, D and Turcan, D and van Eijndhoven, N and Vandenbroucke, J and Van Overloop, Arne and van Santen, J and Voigt, B and Walck, C and Waldenmaier, T and Wallraff, M and Walter, M and Wendt, C and Westerhoff, S and Whitehorn, N and Wiebe, K and Wiebusch, CH and Wiedemann, A and Wikstrom, G and Williams, DR and Wischnewski, R and Wissing, H and Woschnagg, K and Xu, C and Xu, XW and Yodh, G and Yoshida, S},
  issn         = {1550-7998},
  journal      = {PHYSICAL REVIEW D},
  language     = {eng},
  number       = {5},
  pages        = {6},
  title        = {Limits on a muon flux from Kaluza-Klein dark matter annihilations in the Sun from the IceCube 22-string detector},
  url          = {http://dx.doi.org/10.1103/PhysRevD.81.057101},
  volume       = {81},
  year         = {2010},
}

Chicago
Abbasi, R, Yasser Abdou, T Abu-Zayyad, J Adams, JA Aguilar, M Ahlers, K Andeen, et al. 2010. “Limits on a Muon Flux from Kaluza-Klein Dark Matter Annihilations in the Sun from the IceCube 22-string Detector.” Physical Review D 81 (5).
APA
Abbasi, R., Abdou, Y., Abu-Zayyad, T., Adams, J., Aguilar, J., Ahlers, M., Andeen, K., et al. (2010). Limits on a muon flux from Kaluza-Klein dark matter annihilations in the Sun from the IceCube 22-string detector. PHYSICAL REVIEW D, 81(5).
Vancouver
1.
Abbasi R, Abdou Y, Abu-Zayyad T, Adams J, Aguilar J, Ahlers M, et al. Limits on a muon flux from Kaluza-Klein dark matter annihilations in the Sun from the IceCube 22-string detector. PHYSICAL REVIEW D. 2010;81(5).
MLA
Abbasi, R, Yasser Abdou, T Abu-Zayyad, et al. “Limits on a Muon Flux from Kaluza-Klein Dark Matter Annihilations in the Sun from the IceCube 22-string Detector.” PHYSICAL REVIEW D 81.5 (2010): n. pag. Print.