THE CASE FOR A DIRECTIONAL DARK MATTER DETECTOR AND THE STATUS OF CURRENT EXPERIMENTAL EFFORTS-Reference-Cited by-同舟云学术

THE CASE FOR A DIRECTIONAL DARK MATTER DETECTOR AND THE STATUS OF CURRENT EXPERIMENTAL EFFORTS

Published:2010-01-10 Issue:01 Volume:25 Page:1-51
ISSN:0217-751X
Container-title:International Journal of Modern Physics A
language:en
Short-container-title:Int. J. Mod. Phys. A

Author:

AHLEN S.¹,AFSHORDI N.²³,BATTAT J. B. R.⁴,BILLARD J.⁵,BOZORGNIA N.⁶,BURGOS S.⁷,CALDWELL T.⁴⁸,CARMONA J. M.⁹¹⁰,CEBRIAN S.⁹¹⁰,COLAS P.¹¹,DAFNI T.⁹¹⁰,DAW E.¹²,DUJMIC D.⁴,DUSHKIN A.¹³,FEDUS W.⁴,FERRER E.¹¹,FINKBEINER D.¹⁴,FISHER P. H.⁴,FORBES J.⁷,FUSAYASU T.¹⁵,GALAN J.⁹¹⁰,GAMBLE T.¹²,GHAG C.¹⁶,GIOMATARIS I.¹¹,GOLD M.¹⁷,GOMEZ H.⁹¹⁰,GOMEZ M. E.¹⁸,GONDOLO P.¹⁹,GREEN A.²⁰,GRIGNON C.⁵,GUILLAUDIN O.⁵,HAGEMANN C.¹⁷,HATTORI K.²¹,HENDERSON S.⁴,HIGASHI N.²¹,IDA C.²¹,IGUAZ F. J.⁹¹⁰,INGLIS A.¹,IRASTORZA I. G.⁹¹⁰,IWAKI S.²¹,KABOTH A.⁴,KABUKI S.²¹,KADYK J.²²,KALLIVAYALIL N.⁴,KUBO H.²¹,KUROSAWA S.²¹,KUDRYAVTSEV V. A.¹²,LAMY T.⁵,LANZA R.⁴,LAWSON T. B.¹²,LEE A.⁴,LEE E. R.¹⁷,LIN T.¹⁴,LOOMBA D.¹⁷,LOPEZ J.⁴,LUZON G.⁹¹⁰,MANOBU T.²³,MARTOFF J.²⁴,MAYET F.⁵,McCLUSKEY B.¹²,MILLER E.¹⁷,MIUCHI K.²¹,MONROE J.⁴,MORGAN B.²⁵,MUNA D.²⁶,MURPHY A. St. J.¹⁶,NAKA T.²⁷,NAKAMURA K.²¹,NAKAMURA M.²⁷,NAKANO T.²⁷,NICKLIN G. G.¹²,NISHIMURA H.²¹,NIWA K.²⁷,PALING S. M.¹²,PARKER J.²¹,PETKOV A.⁷,PIPE M.¹²,PUSHKIN K.⁷,ROBINSON M.¹²,RODRIGUEZ A.⁹¹⁰,RODRIGUEZ-QUINTERO J.¹⁸,SAHIN T.⁴,SANDERSON R.⁴,SANGHI N.¹⁷,SANTOS D.⁵,SATO O.²⁷,SAWANO T.²¹,SCIOLLA G.⁴,SEKIYA H.²⁸,SLATYER T. R.¹⁴,SNOWDEN-IFFT D. P.⁷,SPOONER N. J. C.¹²,SUGIYAMA A.²⁹,TAKADA A.³⁰,TAKAHASHI M.²¹,TAKEDA A.²⁸,TANIMORI T.²¹,TANIUE K.²¹,TOMAS A.⁹¹⁰,TOMITA H.¹,TSUCHIYA K.²¹,TURK J.¹⁷,TZIAFERI E.¹²,UENO K.²¹,VAHSEN S.²²,VANDERSPEK R.⁴,VERGADOS J.³¹,VILLAR J. A.⁹¹⁰,WELLENSTEIN H.¹³,WOLFE I.⁴,YAMAMOTO R. K.⁴,YEGORYAN H.⁴

Affiliation:

1. Boston University, Boston, MA 02215, USA

2. Perimeter Institute for Theoretical Physics, Waterloo, ON N2L 2Y5, Canada

3. University of Waterloo, Waterloo, Ontario, N2L 3G1 Canada, Canada

4. Massachusetts Institute of Technology, Cambridge, MA 02139, USA

5. Laboratoire de Physique Subatomique et de Cosmologie, Université Joseph Fourier Grenoble 1, CNRS/IN2P3, Institut National Polytechnique de Grenoble, 53, rue de Martyrs, 38026 Grenoble, France

6. University of California Los Angeles, Los Angeles, CA 90095, USA

7. Occidental College, Los Angeles, CA 90041, USA

8. University of Pennsylvania, Philadelphia, PA 19104, USA

9. Laboratorio de Fisica Nuclear y Astroparticulas, Universidad de Zaragoza, 50009 Zaragoza, Spain

10. Laboratorio Subterráneo de Canfranc, Huesca, Spain

11. CEA Saclay, Cédex, France

12. University of Sheffield, Sheffield S3 7RH, UK

13. Brandeis University, Waltham, MA 02453, USA

14. Harvard University, Cambridge, MA, 02140, USA

15. Nagasaki Institute of Applied Science, Nagasaki, Japan

16. University of Edinburgh, Edinburgh, EH9 3JZ, UK

17. University of New Mexico, Albuquerque, NM, 87131, USA

18. Universidad de Huelva, Campus El Carmen, 21071 Huelva, Spain

19. University of Utah, Salt Lake City, UT 84112, USA

20. University of Nottingham, University Park, Nottingham, NG7 2RD, UK

21. Kyoto University Kitashirakawa-oiwakecho, Sakyo-ku, Kyoto, 606-8502, Japan

22. Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA

23. Institute of Particle and Nuclear Studies, KEK, Tsukuba, Japan

24. Temple University, Barton Hall, Philadelphia, PA 19122, USA

25. University of Warwick, Coventry, CV4 7AL, UK

26. New York University, New York, NY 10003, USA

27. Fundamental Particle Physics Laboratory, Nagoya University, Japan

28. Kamioka Observatory, ICRR, The University of Tokyo, Higashi-Mozumi, Kamioka cho, Hida 506-1205, Japan

29. Saga University, Saga, Japan

30. Scientific Balloon Laboratory, ISAS, JAXA, Yoshinodai 3-1-1, Sagamihara, Kanagawa, 229-8510, Japan

31. University of Ioannina, Ioannina, Gr 451 10, Greece

Abstract

We present the case for a dark matter detector with directional sensitivity. This document was developed at the 2009 CYGNUS workshop on directional dark matter detection, and contains contributions from theorists and experimental groups in the field. We describe the need for a dark matter detector with directional sensitivity; each directional dark matter experiment presents their project's status; and we close with a feasibility study for scaling up to a one ton directional detector, which would cost around $150M.

Publisher

World Scientific Pub Co Pte Lt

Subject

Astronomy and Astrophysics,Nuclear and High Energy Physics,Atomic and Molecular Physics, and Optics

Link

https://www.worldscientific.com/doi/pdf/10.1142/S0217751X10048172

Reference76 articles.

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