On the potentiality of the ZnWO4 anisotropic detectors to measure the directionality of Dark Matter
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- 作者：F. Cappella (1)
R. Bernabei (2) (3)
P. Belli (3)
V. Caracciolo (4)
R. Cerulli (4)
F. A. Danevich (5)
A. d’Angelo (1) (6)
A. Di Marco (2) (3)
A. Incicchitti (6)
D. V. Poda (5)
V. I. Tretyak (5) - 刊名：The European Physical Journal C - Particles and Fields
- 出版年：2013
- 出版时间：January 2013
- 年：2013
- 卷：73
- 期：1
- 全文大小：914KB
- 参考文献：1. R. Bernabei et al., Riv. Nuovo Cimento 26(1), 1 (2003)
2. R. Bernabei et al., Eur. Phys. J. C 56, 333 (2008) f="http://dx.doi.org/10.1140/epjc/s10052-008-0662-y">CrossRef
3. R. Bernabei et al., Eur. Phys. J. C 67, 39 (2010) f="http://dx.doi.org/10.1140/epjc/s10052-010-1303-9">CrossRef
4. K.A. Drukier et al., Phys. Rev. D 33, 3495 (1986) f="http://dx.doi.org/10.1103/PhysRevD.33.3495">CrossRef
5. K. Freese et al., Phys. Rev. D 37, 3388 (1988) f="http://dx.doi.org/10.1103/PhysRevD.37.3388">CrossRef
6. R. Bernabei et al., Eur. Phys. J. C 18, 283 (2000) f="http://dx.doi.org/10.1007/s100520000540">CrossRef
7. R. Bernabei et al., Int. J. Mod. Phys. D 13, 2127 (2004) f="http://dx.doi.org/10.1142/S0218271804006619">CrossRef
8. K. Freese, M. Lisanti, C. Savage, f="http://arxiv.org/abs/arXiv:1209.3339v2">arXiv:1209.3339v2 [astro-ph.CO]
9. R. Cerulli, Direct detection of dark matter particles, in / Proceedings of Dark Force, LNF, Frascati, 2012. f="http://www.lnf.infn.it/conference/dark/">http://www.lnf.infn.it/conference/dark/
10. R. Bernabei, P. Belli, A. Incicchitti, D. Prosperi, f="http://arxiv.org/abs/arXiv:0806.0011v2">arXiv:0806.0011v2
11. J.I. Collar. f="http://arxiv.org/abs/arXiv:1204.3559">arXiv:1204.3559
12. J.I. Collar. f="http://arxiv.org/abs/arXiv:1106.0653">arXiv:1106.0653
13. J.I. Collar, f="http://arxiv.org/abs/arXiv:1103.3481">arXiv:1103.3481
14. J.I. Collar, f="http://arxiv.org/abs/arXiv:1010.5187">arXiv:1010.5187
15. C.E. Aalseth et al., Phys. Rev. Lett. 107, 141301 (2011) f="http://dx.doi.org/10.1103/PhysRevLett.107.141301">CrossRef
16. G. Angloher et al., Eur. Phys. J. C 72, 1971 (2012) f="http://dx.doi.org/10.1140/epjc/s10052-012-1971-8">CrossRef
17. R. Bernabei et al., Phys. Lett. B 389, 757 (1996)
18. R. Bernabei et al., Phys. Lett. B 424, 195 (1998) f="http://dx.doi.org/10.1016/S0370-2693(98)00172-5">CrossRef
19. R. Bernabei et al., Phys. Lett. B 450, 448 (1999) f="http://dx.doi.org/10.1016/S0370-2693(99)00091-X">CrossRef
20. P. Belli et al., Phys. Rev. D 61, 023512 (2000) f="http://dx.doi.org/10.1103/PhysRevD.61.023512">CrossRef
21. R. Bernabei et al., Phys. Lett. B 480, 23 (2000) f="http://dx.doi.org/10.1016/S0370-2693(00)00405-6">CrossRef
22. R. Bernabei et al., Phys. Lett. B 509, 197 (2001) f="http://dx.doi.org/10.1016/S0370-2693(01)00493-2">CrossRef
23. R. Bernabei et al., Eur. Phys. J. C 23, 61 (2002) f="http://dx.doi.org/10.1007/s100520100854">CrossRef
24. P. Belli et al., Phys. Rev. D 66, 043503 (2002) f="http://dx.doi.org/10.1103/PhysRevD.66.043503">CrossRef
25. R. Bernabei et al., Int. J. Mod. Phys. A 21, 1445 (2006) f="http://dx.doi.org/10.1142/S0217751X06030874">CrossRef
26. R. Bernabei et al., Eur. Phys. J. C 47, 263 (2006) f="http://dx.doi.org/10.1140/epjc/s2006-02559-9">CrossRef
27. R. Bernabei et al., Int. J. Mod. Phys. A 22, 3155 (2007) f="http://dx.doi.org/10.1142/S0217751X07037093">CrossRef
28. R. Bernabei et al., Eur. Phys. J. C 53, 205 (2008) f="http://dx.doi.org/10.1140/epjc/s10052-007-0479-0">CrossRef
29. R. Bernabei et al., Phys. Rev. D 77, 023506 (2008) f="http://dx.doi.org/10.1103/PhysRevD.77.023506">CrossRef
30. R. Bernabei et al., Mod. Phys. Lett. A 23, 2125 (2008) f="http://dx.doi.org/10.1142/S0217732308027473">CrossRef
31. A. Bottino et al., Phys. Rev. D 81, 107302 (2010) f="http://dx.doi.org/10.1103/PhysRevD.81.107302">CrossRef
32. N. Fornengo et al., Phys. Rev. D 83, 15001 (2011) f="http://dx.doi.org/10.1103/PhysRevD.83.015001">CrossRef
33. A.L. Fitzpatrick et al., Phys. Rev. D 81, 115005 (2010) f="http://dx.doi.org/10.1103/PhysRevD.81.115005">CrossRef
34. D. Hooper et al., Phys. Rev. D 82, 123509 (2010) f="http://dx.doi.org/10.1103/PhysRevD.82.123509">CrossRef
35. D.G. Cerdeno, O. Seto, J. Cosmol. Astropart. Phys. 0908, 032 (2009) f="http://dx.doi.org/10.1088/1475-7516/2009/08/032">CrossRef
36. D.G. Cerdeno, C. Munoz, O. Seto, Phys. Rev. D 79, 023510 (2009) f="http://dx.doi.org/10.1103/PhysRevD.79.023510">CrossRef
37. D.G. Cerdeno et al., J. Cosmol. Astropart. Phys. 0706, 008 (2007) f="http://dx.doi.org/10.1088/1475-7516/2007/06/008">CrossRef
38. J.F. Gunion et?al., f="http://arxiv.org/abs/arXiv:1009.2555">arXiv:1009.2555
39. A.V. Belikov et al., Phys. Lett. B 705, 82 (2011) f="http://dx.doi.org/10.1016/j.physletb.2011.09.081">CrossRef
40. C. Arina, F. Fornengo, J. High Energy Phys. 11, 029 (2007) f="http://dx.doi.org/10.1088/1126-6708/2007/11/029">CrossRef
41. G. Belanger et al., J. High Energy Phys. 1107, 083 (2011) f="http://dx.doi.org/10.1007/JHEP07(2011)083">CrossRef
42. S. Chang et al., Phys. Rev. D 79, 043513 (2009) f="http://dx.doi.org/10.1103/PhysRevD.79.043513">CrossRef
43. S. Chang et al., Phys. Rev. Lett. 106, 011301 (2011) f="http://dx.doi.org/10.1103/PhysRevLett.106.011301">CrossRef
44. R. Foot, Phys. Rev. D 81, 087302 (2010) f="http://dx.doi.org/10.1103/PhysRevD.81.087302">CrossRef
45. R. Foot, Phys. Lett. B 703, 7 (2011) f="http://dx.doi.org/10.1016/j.physletb.2011.07.044">CrossRef
46. R. Foot, Phys. Rev. D 82, 095001 (2010) f="http://dx.doi.org/10.1103/PhysRevD.82.095001">CrossRef
47. Y. Mambrini, J. Cosmol. Astropart. Phys. 1107, 009 (2011) f="http://dx.doi.org/10.1088/1475-7516/2011/07/009">CrossRef
48. Y. Mambrini, J. Cosmol. Astropart. Phys. 1009, 022 (2010) f="http://dx.doi.org/10.1088/1475-7516/2010/09/022">CrossRef
49. Y. Bai, P.J. Fox, J. High Energy Phys. 0911, 052 (2009) f="http://dx.doi.org/10.1088/1126-6708/2009/11/052">CrossRef
50. J. Alwall et al., Phys. Rev. D 81, 114027 (2010) f="http://dx.doi.org/10.1103/PhysRevD.81.114027">CrossRef
51. M.Yu. Khlopov et al., Int. J. Mod. Phys. D 19, 1385 (2010) f="http://dx.doi.org/10.1142/S0218271810017962">CrossRef
52. S. Andreas et al., Phys. Rev. D 82, 043522 (2010) f="http://dx.doi.org/10.1103/PhysRevD.82.043522">CrossRef
53. M.S. Boucenna, S. Profumo, Phys. Rev. D 84, 055011 (2011) f="http://dx.doi.org/10.1103/PhysRevD.84.055011">CrossRef
54. P.W. Graham et al., Phys. Rev. D 82, 063512 (2010) f="http://dx.doi.org/10.1103/PhysRevD.82.063512">CrossRef
55. B. Batell, M. Pospelov, A. Ritz, Phys. Rev. D 79, 115019 (2009) f="http://dx.doi.org/10.1103/PhysRevD.79.115019">CrossRef
56. E. Del Nobile et al., Phys. Rev. D 84, 027301 (2011) f="http://dx.doi.org/10.1103/PhysRevD.84.027301">CrossRef
57. J. Kopp et al., J. Cosmol. Astropart. Phys. 1002, 014 (2010) f="http://dx.doi.org/10.1088/1475-7516/2010/02/014">CrossRef
58. V. Barger et al., Phys. Rev. D 82, 035019 (2010) f="http://dx.doi.org/10.1103/PhysRevD.82.035019">CrossRef
59. S. Chang et al., J. Cosmol. Astropart. Phys. 1008, 018 (2010) f="http://dx.doi.org/10.1088/1475-7516/2010/08/018">CrossRef
60. J.L. Feng et al., Phys. Lett. B 703, 124 (2011) f="http://dx.doi.org/10.1016/j.physletb.2011.07.083">CrossRef
61. M.T. Frandsen et al., Phys. Rev. D 84, 041301 (2011) f="http://dx.doi.org/10.1103/PhysRevD.84.041301">CrossRef
62. Y.G. Kim, S. Shin, J. High Energy Phys. 0905, 036 (2009) f="http://dx.doi.org/10.1088/1126-6708/2009/05/036">CrossRef
63. S. Shin, in / PoS IDM2010 (2011), p. 094
64. M.R. Buckley, Phys. Lett. B 703, 343 (2011) f="http://dx.doi.org/10.1016/j.physletb.2011.08.014">CrossRef
65. N. Fornengo et al., Phys. Rev. D 84, 115002 (2011) f="http://dx.doi.org/10.1103/PhysRevD.84.115002">CrossRef
66. P. Gondolo et al., Phys. Rev. D 85, 035022 (2012) f="http://dx.doi.org/10.1103/PhysRevD.85.035022">CrossRef
67. E. Kuflik et al., Phys. Rev. D 81, 111701 (2010) f="http://dx.doi.org/10.1103/PhysRevD.81.111701">CrossRef
68. C. Arina et al., J. Cosmol. Astropart. Phys. 1109, 022 (2011) f="http://dx.doi.org/10.1088/1475-7516/2011/09/022">CrossRef
69. M.R. Buckley et al., Phys. Lett. B 702, 216 (2011) f="http://dx.doi.org/10.1016/j.physletb.2011.06.090">CrossRef
70. A. Bottino et?al., f="http://arxiv.org/abs/arXiv:1112.5666">arXiv:1112.5666
71. P. Belli et al., Phys. Rev. D 84, 055014 (2011) f="http://dx.doi.org/10.1103/PhysRevD.84.055014">CrossRef
72. A. Bottino et al., Phys. Rev. D 85, 095013 (2012) f="http://dx.doi.org/10.1103/PhysRevD.85.095013">CrossRef
73. D.N. Spergel, Phys. Rev. D 37, 1353 (1988) f="http://dx.doi.org/10.1103/PhysRevD.37.1353">CrossRef
74. M.J. Lehner et?al., f="http://arxiv.org/abs/astro-ph/9905074">astro-ph/9905074
75. G.J. Alner et al., Nucl. Instrum. Methods A 555, 173 (2005) f="http://dx.doi.org/10.1016/j.nima.2005.09.011">CrossRef
76. P. Belli et al., Nuovo Cimento C 15, 475 (1992)
77. R. Bernabei et al., Eur. Phys. J. C 28, 203 (2003) f="http://dx.doi.org/10.1140/epjc/s2003-01190-8">CrossRef
78. N.J.C. Spooner et al., in / International Workshop IDM (World Scientific, Singapore, 1997), p.?481
79. Y. Shimizu, M. Minowa, H. Sekiya, Y. Inoue, Nucl. Instrum. Methods A 496, 347 (2003) f="http://dx.doi.org/10.1016/S0168-9002(02)01661-3">CrossRef
80. P. Belli et al., Nucl. Instrum. Methods A 626-27, 31 (2011) f="http://dx.doi.org/10.1016/j.nima.2010.10.027">CrossRef
81. P. Belli et al., J.?Phys. G 38, 115107 (2011) f="http://dx.doi.org/10.1088/0954-3899/38/11/115107">CrossRef
82. J.B. Birks, / The Theory and Practice of Scintillation Counting (Pergamon, London, 1964)
83. P.H. Heckmann, Z. Phys. 157, 10 (1959)
84. P.H. Heckmann et al., Z.?Phys. 162, 84 (1961)
85. W.F. Kienzle, A. Flammersfeld, Z.?Phys. 165, 1 (1961)
86. K. Tsukada, S. Kikuchi, Nucl. Instrum. Methods 17, 286 (1962) f="http://dx.doi.org/10.1016/0029-554X(62)90007-1">CrossRef
87. K. Tsukada et al., Nucl. Instrum. Methods 37, 69 (1965) f="http://dx.doi.org/10.1016/0029-554X(65)90339-3">CrossRef
88. F.J. Kratochwill, Z.?Phys. 234, 74 (1970)
89. F.D. Brooks, D.T. Jones, Nucl. Instrum. Methods 121, 69 (1974) f="http://dx.doi.org/10.1016/0029-554X(74)90141-4">CrossRef
90. V.I. Tretyak, Astropart. Phys. 33, 40 (2010) f="http://dx.doi.org/10.1016/j.astropartphys.2009.11.002">CrossRef
91. E. Gatti, F. De Martini, in / Nuclear Electronics, vol.?2 (IAEA, Vienna, 1962), p.?265
92. F.A. Kroger, in / Some Aspects of the Luminescence in Solids (Elsevier, Amsterdam, 1948), p.?109
93. B.C. Grabmaier, IEEE Trans. Nucl. Sci. NS-31, 372 (1984) f="http://dx.doi.org/10.1109/TNS.1984.4333280">CrossRef
94. Y.C. Zhu et al., Nucl. Instrum. Methods A 244, 579 (1986) f="http://dx.doi.org/10.1016/0168-9002(86)91089-2">CrossRef
95. F.A. Danevich et al., Prib. Tekh. Eksp. 5, 80 (1989) [Instrum. Exp. Tech. 32, 1059 (1989)]
96. L.L. Nagornaya et al., IEEE Trans. Nucl. Sci. 55, 1469 (2008) f="http://dx.doi.org/10.1109/TNS.2007.910974">CrossRef
97. L.L. Nagornaya et al., IEEE Trans. Nucl. Sci. 56, 994 (2009) f="http://dx.doi.org/10.1109/TNS.2009.2016342">CrossRef
98. E.N. Galashov et al., Funct. Mater. 16, 63 (2009)
99. F.A. Danevich et al., Nucl. Instrum. Methods A 544, 553 (2005) f="http://dx.doi.org/10.1016/j.nima.2005.01.303">CrossRef
100. P. Belli et al., Phys. Lett. B 658, 193 (2008) f="http://dx.doi.org/10.1016/j.physletb.2007.10.075">CrossRef
101. P. Belli et al., Nucl. Phys. A 826, 256 (2009) f="http://dx.doi.org/10.1016/j.nuclphysa.2009.05.139">CrossRef
102. I. Bavykina et al., IEEE Trans. Nucl. Sci. 55, 1449 (2008) f="http://dx.doi.org/10.1109/TNS.2008.922809">CrossRef
103. F.A. Danevich et al., Phys. Rev. C 67, 014310 (2003) f="http://dx.doi.org/10.1103/PhysRevC.67.014310">CrossRef
104. R. Bernabei et al., J.?Instrum. 7, P03009 (2012) f="http://dx.doi.org/10.1088/1748-0221/7/03/P03009">CrossRef
105. I. Holl et al., IEEE Trans. Nucl. Sci. NS-35, 105 (1988) f="http://dx.doi.org/10.1109/23.12684">CrossRef
106. H. Kraus et al., Nucl. Instrum. Methods A 600, 594 (2009) f="http://dx.doi.org/10.1016/j.nima.2008.12.142">CrossRef
107. R. Bernabey et al., Metallofiz. Noveishie Tekhnol. 30, 477 (2008)
108. P. Belli et al., Nucl. Instrum. Methods A 615, 301 (2010) f="http://dx.doi.org/10.1016/j.nima.2010.01.081">CrossRef
109. G.P. Kovtun et al., Funct. Mater. 18, 121 (2011)
110. D.V. Poda et?al., CdWO4 crystal scintillators from enriched isotopes for double beta decay experiments. in / Rad. Meas. as a Proc. of LUMDETR-2012 Conference (in press)
111. A.S. Barabash et al., J. Instrum. 06, P08011 (2011) f="http://dx.doi.org/10.1088/1748-0221/6/08/P08011">CrossRef
112. R. Bernabei et al., Nucl. Instrum. Methods A 592, 297 (2008) f="http://dx.doi.org/10.1016/j.nima.2008.04.082">CrossRef
113. P. Belli et al., Phys. Rev. D 84, 055014 (2011) f="http://dx.doi.org/10.1103/PhysRevD.84.055014">CrossRef
114. R. Bernabei et al., Eur. Phys. J. C 53, 205 (2008) f="http://dx.doi.org/10.1140/epjc/s10052-007-0479-0">CrossRef - 作者单位：F. Cappella (1)
R. Bernabei (2) (3)
P. Belli (3)
V. Caracciolo (4)
R. Cerulli (4)
F. A. Danevich (5)
A. d’Angelo (1) (6)
A. Di Marco (2) (3)
A. Incicchitti (6)
D. V. Poda (5)
V. I. Tretyak (5)
1. Dip. di Fisica, Università di Roma “La Sapienza- 00185, Rome, Italy
2. Dip. di Fisica, Università di Roma “Tor Vergata- 00133, Rome, Italy
3. Sez. Roma “Tor Vergata- INFN, 00133, Rome, Italy
4. Laboratori Nazionali del Gran Sasso, INFN, 67100, Assergi, Italy
5. Institute for Nuclear Research, MSP, 03680, Kyiv, Ukraine
6. Sez. Roma, INFN, 00185, Rome, Italy - ISSN：1434-6052
文摘
In the anisotropic scintillators the light output and the pulse shape for heavy particles (p, α, nuclear recoils) depend on the direction with respect to the crystal axes; the response to γ/β radiation is isotropic instead. This feature offers the possibility to study the directionality approach, which is applicable in the particular case of those Dark Matter candidate particles inducing just nuclear recoils. Among the anisotropic scintillators, the ZnWO4 has unique features, which make it an excellent candidate for this type of research, and there is still plenty of room for the improvement of its performances. In this paper the possibility of a low background pioneer experiment (named ADAMO—Anisotropic detectors for DArk Matter Observation) to exploit deep underground the directionality approach by using anisotropic ZnWO4 scintillators is discussed.