Limits on spin-independent interactions of weakly interacting massive particles with nucleons from the two-tower run of the cryogenic dark matter search

Physical Review Letters

Volumn 96, Issue 1, 2006, Pages

  Akerib, D S ^b   Attisha, M J ^a   Bailey, C N ^b   Baudis, L ^k   Bauer, D A ^c   Brink, P L ^g   Brusov, P P ^b   Bunker, R ⁱ   Cabrera, B ^g   Caldwell, D O ⁱ   Chang, C L ^g   Cooley, J ^g   Crisler, M B ^c   Cushman, P ^f   Daal, M ^h   Dixon, R ^c   Dragowsky, M R ^b   Driscoll, D D ^b   Duong, L ^f   Ferril, R ⁱ   Filippini, J ^h   Gaitskell, R J ^a   Golwala, S R ^l   Grant, D R ^b   Hennings Yeomans, R ^b   Holmgren, D ^c   Huber, M E ^j   Kamat, S ^b   Leclercq, S ^k   Lu, A ^h   Mahapatra, R ⁱ   Mandic, V ^h   Meunier, P ^h   Mirabolfathi, N ^h   Nelson, H ⁱ   Nelson, R ⁱ   Ogburn, R W ^g   Perera, T A ^b   Pyle, M ^g   Ramberg, E ^c   Rau, W ^h   Reisetter, A ^f   Ross, R R ^d,h   Sadoulet, B ^d,h   Sander, J ⁱ   Savage, C ⁱ   Schnee, R W ^b   Seitz, D N ^h   Serfass, B ^h   Sundqvist, K M ^h   Thompson, J P F ^a   Wang, G ^b,l   Yellin, S ^g,i   Yoo, J ^c   Young, B A ^e   more..

^a BROWN UNIVERSITY   (United States)

^b CASE WESTERN RESERVE UNIVERSITY   (United States)

^c FERMI NATIONAL ACCELERATOR LABORATORY   (United States)

^d LAWRENCE BERKELEY NATIONAL LABORATORY   (United States)

^e SANTA CLARA UNIVERSITY   (United States)

^f University of Minnesota   (United States)

^g STANFORD UNIVERSITY   (United States)

^h UNIVERSITY OF CALIFORNIA   (United States)

ⁱ UNIVERSITY OF CALIFORNIA   (United States)

^j UNIVERSITY OF COLORADO   (United States)

^k University of Florida   (United States)

^l CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

more..

Author keywords

[No Author keywords available]

Indexed keywords

ASTROPHYSICS; CONSTRAINT THEORY; ELEMENTARY PARTICLES; QUANTUM THEORY; SIGNAL FILTERING AND PREDICTION;

CRYOGENIC DARK MATTER SEARCH (CDMS II); NUCLEON CROSS SECTION; RECOIL ENERGIES; WEAKLY INTERACTING MASSIVE PARTICLE (WIMP);

CRYOGENICS;

EID: 32644464259     PISSN: 00319007     EISSN: 10797114     Source Type: Journal    
DOI: 10.1103/PhysRevLett.96.011302     Document Type: Article

References (26)

1. D.N. Spergel (WMAP Collaboration), Astrophys. J. Suppl. Ser. 148, 175 (2003); APJSA2 0067-0049 10.1086/377226
2. M. Tegmark (SDSS Collaboration), Phys. Rev. D 69, 103501 (2004). PRVDAQ 0556-2821 10.1103/PhysRevD.69.103501
3. P. Salucci and A. Borriello, Lect. Notes Phys. 616, 66 (2003); LNPHA4 0075-8450
4. T. Broadhurst, Astrophys. J. 621, 53 (2005). ASJOAB 0004-637X 10.1086/426494
5. G. Steigman and M.S. Turner, Nucl. Phys. NUPBBO 0550-3213 B253, 375 (1985). 10.1016/0550-3213(85)90537-1
6. B.W. Lee and S. Weinberg, Phys. Rev. Lett. 39, 165 (1977); PRLTAO 0031-9007 10.1103/PhysRevLett.39.165
7. S. Weinberg, Phys. Rev. Lett. 48, 1303 (1982). PRLTAO 0031-9007 10.1103/PhysRevLett.48.1303
8. G. Jungman, M. Kamionkowski, and K. Griest, Phys. Rep. 267, 195 (1996); PRPLCM 0370-1573 10.1016/0370-1573(95)00058-5
9. G. Bertone, D. Hooper, and J. Silk, Phys. Rep. 405, 279 (2005). PRPLCM 0370-1573 10.1016/j.physrep.2004.08.031
10. D.S. Akerib (CDMS Collaboration), Phys. Rev. Lett. 93, 211301 (2004). PRLTAO 0031-9007 10.1103/PhysRevLett.93.211301
11. D.S. Akerib (CDMS Collaboration), Phys. Rev. D 72, 052009 (2005). PRVDAQ 0556-2821 10.1103/PhysRevD.72.052009
12. J.D. Lewin and P.F. Smith, Astropart. Phys. 6, 87 (1996). APHYEE 0927-6505 10.1016/S0927-6505(96)00047-3
13. A Majorana neutralino undergoes a scalar interaction of roughly equal strength for neutrons and protons; see K. Griest, Phys. Rev. D 38, 2357 (1988). PRVDAQ 0556-2821 10.1103/PhysRevD.38.2357
14. The SI scattering amplitude is generally sensitive to scalar, vector, and tensor interactions of a spin-1/2 WIMP; see A. Kurylov and M. Kamionkowski, Phys. Rev. D 69, 063503 (2004). PRVDAQ 0556-2821 10.1103/PhysRevD.69.063503
15. D.S. Akerib (CDMS Collaboration), Phys. Rev. D (to be published). PRVDAQ 0556-2821
16. K.D. Irwin, Rev. Sci. Instrum. RSINAK 0034-6748 66, 5322 (1995); 10.1063/1.1146105
17. T. Saab, AIP Conf. Proc. APCPCS 0094-243X 605, 497 (2002). 10.1063/1.1457694
18. T. Shutt, Phys. Rev. Lett. 69, 3425 (1992). PRLTAO 0031-9007 10.1103/PhysRevLett.69.3425
19. CDMS Collaboration (to be published); theses and notes at http://cdms.berkeley.edu/Dissertations.
20. R.M. Clarke, Appl. Phys. Lett. 76, 2958 (2000). APPLAB 0003-6951 10.1063/1.126529
21. A. Bottino, Phys. Rev. D 69, 037302 (2004). PRVDAQ 0556-2821 10.1103/PhysRevD.69.037302
22. J. Ellis, Phys. Rev. D 71, 095007 (2005). PRVDAQ 0556-2821 10.1103/PhysRevD.71.095007
23. We show the 90% allowed region from Fig. 2(a) of P. Gondolo and G. Gelmini, Phys. Rev. D 71, 123520 (2005). PRVDAQ 0556-2821 10.1103/PhysRevD.71. 123520
24. R. Bernabei, Phys. Lett. B 389, 757 (1996). PYLBAJ 0370-2693 10.1016/S0370-2693(96)01483-9
25. V. Sanglard (EDELWEISS Collaboration), Phys. Rev. D 71, 122002 (2005). PRVDAQ 0556-2821 10.1103/PhysRevD.71.122002
26. G.J. Alner (UK Dark Matter Collaboration), Astropart. Phys. 23, 444 (2005). APHYEE 0927-6505 10.1016/j.astropartphys.2005.02.004