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The Directional Dark Matter Detector (D3)

Published online by Cambridge University Press:  15 February 2012

S.E. Vahsen
Affiliation:
University of Hawaii, 2505 Correa Road, Honolulu, HI 96822, USA
H. Feng
Affiliation:
University of Hawaii, 2505 Correa Road, Honolulu, HI 96822, USA
M. Garcia-Sciveres
Affiliation:
Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, CA 94720, USA
I. Jaegle
Affiliation:
University of Hawaii, 2505 Correa Road, Honolulu, HI 96822, USA
J. Kadyk
Affiliation:
Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, CA 94720, USA
Y. Nguyen
Affiliation:
Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, CA 94720, USA
M. Rosen
Affiliation:
University of Hawaii, 2505 Correa Road, Honolulu, HI 96822, USA
S. Ross
Affiliation:
University of Hawaii, 2505 Correa Road, Honolulu, HI 96822, USA
T. Thorpe
Affiliation:
University of Hawaii, 2505 Correa Road, Honolulu, HI 96822, USA
J. Yamaoka
Affiliation:
University of Hawaii, 2505 Correa Road, Honolulu, HI 96822, USA
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Abstract

Gas-filled Time Projection Chambers (TPCs) with Gas Electron Multipliers (GEMs) and pixels appear suitable for direction-sensitive WIMP dark matter searches. We present the background and motivation for our work on this technology, past and ongoing prototype work, and a development path towards an affordable, 1-m3-scale directional dark matter detector, D3. Such a detector may be particularly suitable for low-mass WIMP searches, and perhaps sufficiently sensitive to clearly determine whether the signals seen by DAMA, CoGeNT, and CRESST-II are due to low-mass WIMPs or background.

Type
Research Article
Copyright
© EAS, EDP Sciences 2012

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References

Aad, G., et al., 2008, JINST, 3, P07007 CrossRef
Aalseth, C.E., et al., 2011 [CoGeNT Collaboration], Phys. Rev. Lett., 106, 131301 CrossRef
Ahlen, S., et al., 2010, Int. J. Mod. Phys. A, 25, 1-51 CrossRef
Ahmed, Z., et al., 2010 [The CDMS-II Collaboration], Science, 327, 1619-1621
Angloher, G., et al., 2011 [arXiv:1109.0702]
Aprile, E., et al., 2011 [XENON100 Collaboration] [arXiv:1104.2549]
Bernabei, R., et al., 2008 [DAMA Collaboration], Eur. Phys. J. C, 56, 333-355 CrossRef
Burgos, S., Daw, E., Forbes, J., et al., 2009, JINST, 4, P04014 CrossRef
For a possible mechanism, see Feng, J.L., Kumar, J., Marfatia, D., & Sanford, D., 2011, Phys. Lett. B, 703, 124-127 CrossRef
Hinshaw, G., et al., 2009, Astrophys. J. Suppl., 180, 225-245 CrossRef
Jaegle, I., et al., 2012, EAS Publications Series, 53, 111 CrossRef
Kim, T., Freytsis, M., Button-Shafer, J., et al., 2008, Nucl. Instrum. Meth. A, 589, 173-184 CrossRef
Lehner, M.J., Buckland, K.N., & Masek, G.E., 1997, Astropart. Phys., 8, 43-50 CrossRef
Miuchi, K., Nishimura, H., Hattori, K., et al., 2010, Phys. Lett. B, 686, 11-17 CrossRef
Miyamoto, J., Shipsey, I., Martoff, C.J., et al., 2004, Nucl. Instrum. Meth. A, 526, 409-412 CrossRef
Moulin, E., Mayet, F., & Santos, D., 2005, Phys. Lett. B, 614, 143-154 CrossRef
Muna, D., 2007 [DRIFT Dark Matter Collaboration], Nucl. Phys. Proc. Suppl., 173, 172-175 CrossRef
Ralston, J.P., 2010 [arXiv:1006.5255]
Sauli, F., 1997, Nucl. Instrum. Meth. A, 386, 531-534 CrossRef
Sciolla, G., et al., 2008, PoS IDM2008, 002
See, e.g., Censier, B., 2012, EAS Publications Series, 53, 59 CrossRef
Spergel, D.N., 1988, Phys. Rev. D, 37, 1353 CrossRef