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Consequences of statistical sense determination for WIMP directional detection
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Green, Anne M. and Morgan, Ben. (2008) Consequences of statistical sense determination for WIMP directional detection. Physical Review D (Particles, Fields, Gravitation and Cosmology), Vol.77 (No.2). ISSN 1550-7998
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Official URL: http://dx.doi.org/10.1103/PhysRevD.77.027303
Abstract
We study the consequences of limited recoil sense reconstruction on the number of events required to reject isotropy and detect a WIMP signal using a directional detector. For a constant probability of determining the sense correctly, 3-d readout and zero background, we find that as the probability is decreased from 1.0 to 0.75 the number of events required increases by a factor of a few. As the probability is decreased further the number of events increases sharply, and isotropy can be rejected more easily by discarding the sense information and using axial statistics. This however requires an order of magnitude more events than vectorial data with perfect sense determination. We also consider energy dependent probabilities of correctly measuring the sense. Our main finding is that correctly determining the sense of the abundant, but less anisotropic, low energy recoils is most important.
| Item Type: | Journal Article |
|---|---|
| Subjects: | Q Science > QB Astronomy Q Science > QC Physics |
| Divisions: | Faculty of Science > Physics |
| Library of Congress Subject Headings (LCSH): | Particles (Nuclear physics), Astrophysics, Nuclear counters, Particle tracks (Nuclear physics) |
| Journal or Publication Title: | Physical Review D (Particles, Fields, Gravitation and Cosmology) |
| Publisher: | American Physical Society |
| ISSN: | 1550-7998 |
| Date: | January 2008 |
| Volume: | Vol.77 |
| Number: | No.2 |
| Number of Pages: | 4 |
| Identification Number: | 10.1103/PhysRevD.77.027303 |
| Status: | Peer Reviewed |
| Publication Status: | Published |
| Access rights to Published version: | Restricted or Subscription Access |
| Funder: | Science and Technology Facilities Council (Great Britain) (STFC) |
| References: | [1] M.W. Goodman and E. Witten, Phys. Rev. D 31, 3059 (1985). [2] D. N. Spergel, Phys. Rev. D 37, 1353 (1988). [3] D. P. Snowden-Ifft, C. J. Martoff, and J. M. Burwell, Phys. Rev. D 61, 101301 (2000). [4] G. J. Alner et al., Nucl. Instrum. Methods Phys. Res., Sect. A 535, 644 (2004). [5] T. Tanimori et al., Phys. Lett. B 578, 241 (2004). [6] C. J. Martoff, electronic proceedings of SNIC06 Symposium, California, 3–6 July 2006. Available from: http://www-conf.slac.stanford.edu/snic/papers/0188.PDF. [7] C. J. Copi, J. Heo, and L. M. Krauss, Phys. Lett. B 461, 43 (1999); C. J. Copi and L. M. Krauss, Phys. Rev. D 63, 043507 (2001). [8] M. J. Lehner et al., Dark Matter in Astro and Particle Physics, Proceedings of the International Conference DARK2000, Heidelberg, Germany, 2000, edited by H.V. Klapdor-Kleingrothaus (Springer-Verlag, Berlin, 2001), p. 590. [9] B. Morgan, A. M. Green, and N. J. C. Spooner, Phys. Rev. D 71, 103507 (2005). [10] B. Morgan and A. M. Green, Phys. Rev. D 72, 123501 (2005). [11] C. J. Copi, L. M. Krauss, D. Simmons-Duffin, and S. R. Stroiney, Phys. Rev. D 75, 023514 (2007). [12] A. M. Green and B. Morgan, J. Cosmol. Astropart. Phys. 08 (2007) 022. [13] J. D. Vergados and A. Faessler, Phys. Rev. D 75, 055007 (2007). [14] This can be improved to a factor 30 if the reduced angles (with the direction of solar motion subtracted) are calculated and analyzed. [15] A. Hitachi, J. Phys.: Conf. Ser. 65, 012013 (2007). [16] J. F. Ziegler, J. P. Biersack, and U. Littmark, The Stopping and Range of Ions in Solids (Pergamon Press, New York, 1985), http://www.srim.org. [17] D. P. Snowden-Ifft, T. Ohnuki, E. S. Rykoff, and C. J. Martoff, Nucl. Instrum. Methods Phys. Res., Sect. A 498, 155 (2003). [18] Various talks at ‘‘Cygnus 2007: First Workshop on Direction Detection of Dark Matter,’’ available at http:// pppa.group.shef.ac.uk/cygnus2007/talks/. [19] D. Dujmic et al., arXiv:0708.2370. [20] G. Cowan, Statistical Data Analysis (OUP, New York, 1998). [21] B. Morgan, Ph.D. thesis, University of Sheffield (2004). [22] For 2-d readout the angular resolution will be a function of both the recoil energy and primary direction. [23] M. J. Carson et al., Nucl. Instrum. Methods Phys. Res., Sect. A 546, 509 (2005); Astropart. Phys. 21, 667 (2004). [24] Lord Rayleigh, Philos. Mag. 10, 73 (1880); Nature (London) 72, 318 (1905); Philos. Mag. 37, 321 (1918); G. M. Cordeiro and S. Ferrari, Biometrika 78, 573 (1991); K.V. Mardia and P. Jupp, Directional Statistics (Wiley, Chichester, 2002). |
| URI: | http://wrap.warwick.ac.uk/id/eprint/30608 |
Data sourced from Thomson Reuters' Web of Knowledge
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