ßäåðíà ô³çèêà òà åíåðãåòèêà
ISSN:
1818-331X (Print), 2074-0565 (Online) |
Home page | About |
DAMA/LIBRA results and perspectives of the second stage
R. Bernabei1, P. Belli1, F. Cappella2, V.Caracciolo3, R. Cerulli3, C. J. Dai4, A. d`Angelo2, A. Di Marco1, H. L. He4, A. Incicchitti2, X. H. Ma4, F. Montecchia1,5, X. D. Sheng4, R. G. Wang4, Z. P. Ye4,6
1Dipartimento di Fisica, Università di Roma "Tor Vergata"
and Istituto Nazionale di Fisica Nucleare, Sezione di Roma "Tor Vergata", Rome, Italy
2Dipartimento di Fisica, Università di Roma "La Sapienza"
and Istituto Nazionale di Fisica Nucleare, Sezione di Roma "La Sapienza", Rome, Italy
3Laboratorio Nazionali del Gran Sasso, Istituto Nazionale di Fisica Nucleare, Assergi (AQ), Italy
4Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, China
5Laboratorio Sperimentale Policentrico di Ingegneria Medica,
Università di Roma "Tor Vergata", Rome, Italy
6University of Jing Gangshan, Jiangxi, China
Abstract: The DAMA/LIBRA experiment is mainly dedicated to the investigation on DM particles in the Galactic halo by exploiting the model independent Dark Matter (DM) annual modulation signature. The present DAMA/LIBRA and the former DAMA/NaI (exposed masses: about 250 kg and about 100 kg of highly radiopure NaI(Tl), respectively) experiments have released so far a total exposure of 1.17 t · yr collected over 13 annual cycles; they provide a model independent evidence of the presence of DM particles in the galactic halo at 8.9 σ C.L. The data of another annual cycle in the same DAMA/LIBRA running conditions are at hand. After the substitution (at fall 2010) of all the photomultipliers (PMTs) with new ones, having higher quantum efficiency, DAMA/LIBRA has entered the phase 2; that substitution has allowed to lower the software energy threshold of the experiment in the present data taking. Future perspectives are mentioned.
Keywords: Dark Matter, annual modulation, NaI(Tl) scintillator.
References:1. Bernabei R. et al. Il Nuovo Cim. A 112 (1999) 545. https://doi.org/10.1007/BF03035868
2. Bernabei R. et al. Phys. Lett. B 389 (1996) 757; Phys. Lett. B 424 (1998) 195; Phys. Lett. B 450 (1999) 448; Phys. Rev. D 61 (2000) 023512; Phys. Lett. B 480 (2000) 23; Phys. Lett. B 509 (2001) 197; Eur. Phys. J. C 23 (2002) 61; Phys. Rev. D 66 (2002) 043503.
3. Bernabei R. et al. Eur. Phys. J. C 18 (2000) 283. https://doi.org/10.1007/s100520000540
4. Bernabei R. el al. La Rivista del Nuovo Cimento 26 (2003) 1. https://doi.org/10.1007/BF03548916
5. Bernabei R. et al. Int. J. Mod. Phys. D 13 (2004) 2127. https://doi.org/10.1142/S0218271804006619
6. Bernabei R. et al. Eur. Phys. J. C 47 (2006) 263. https://doi.org/10.1140/epjc/s2006-02559-9
7. Bernabei R. et al. Eur. Phys. J. C 53 (2008) 205. https://doi.org/10.1140/epjc/s10052-007-0479-0
8. Bernabei R. et al. Phys. Lett. B 408 (1997) 439; Belli P. et al. Phys. Lett. B 460 (1999) 236; Bernabei R. et al. Phys. Rev. Lett. 83 (1999) 4918; Belli P. et al. Phys. Rev. C 60 (1999) 065501; Bernabei R. et al. Il Nuovo Cimento A 112 (1999) 1541; Phys. Lett. B 515 (2001) 6; Cappella F. et al. Eur. Phys. J. C 14 (2002) 1; Bernabei R. et al. Eur. Phys. J. A 23 (2005) 7; Eur. Phys. J. A 24 (2005) 51; Astropart. Phys. 4 (1995) 45; The identification of Dark Matter (Singapore: World Sc. Pub., 1997) 574.
9. Belli P. et al. Astropart. Phys. 5 (1996) 217; Nuovo Cim. C 19 (1996) 537; Phys. Lett. B 387 (1996) 222; Phys. Lett. B 389 (1996) 783 err.; Bernabei R. et al. Phys. Lett. B 436 (1998) 379; Belli P. et al. Phys. Lett. B 465 (1999) 315; Phys. Rev. D 61 (2000) 117301; Bernabei R. et al. New J. of Phys. 2 (2000) 15.1; Phys. Lett. B 493 (2000) 12; Nucl. Instr. & Meth A 482 (2002) 728; Eur. Phys. J. direct C 11 (2001) 1; Phys. Lett. B 527 (2002)182; Phys. Lett. B 546 (2002) 23; Beyond the Desert 2003 (Berlin: Springer, 2003) 365; Eur. Phys. J. A 27 (2006) 35.
10. Bernabei R. et al. Astropart. Phys. 7 (1997) 73; Nuovo Cim. A 110 (1997) 189; Belli P. et al. Astropart. Phys. 10 (1999) 115; Nucl. Phys. B 563 (1999) 97; Bernabei R. et al. Nucl. Phys. A 705 (2002) 29; Belli P. et al. Nucl. Instr. & Meth. A 498 (2003) 352; Cerulli R. et al. Nucl. Instr. & Meth. A 525 (2004) 535; Bernabei R. et al. Nucl. Instr. & Meth. A 555 (2005) 270; Ukr. J. Phys. 51 (2006) 1037; Belli P. et al. Nucl. Phys. A 789 (2007)15; Phys. Rev. C 76 (2007) 064603; Phys. Lett. B 658 (2008) 193; Eur. Phys. J. A 36 (2008) 167; Nucl. Phys. A 826 (2009) 256; Nucl. Instr. & Meth. A 615 (2010) 301; Nucl. Instr. & Meth. A 626-627 (2011) 31; J. Phys. G: Nucl. Part. Phys. 38 (2011) 015103; Nucl. Inst. & Meth. A 670 (2012) 10. https://doi.org/10.1088/0954-3899/38/1/015103
11. Belli P. et al. Nucl. Instr. & Meth. A 572 (2007) 734; Nucl. Phys. A 806 (2008) 388; Nucl. Phys. A 824 (2009) 101; Proc. of the Int. Conf. "NPAE-2008" (Kyiv, 2009) 473; Eur. Phys. J. A 42 (2009) 171; Nucl. Phys. A 846 (2010) 143; Nucl. Phys. A 859 (2011) 126; Phys. Rev. C 83 (2011) 034603; Eur. Phys. J. A 47 (2011) 91; Phys. Lett. B 711 (2012) 41.
12. Bernabei R. et al. Nucl. Instr. & Meth. A 592 (2008) 297.
13. Bernabei R. et al. Eur. Phys. J. C 56 (2008) 333. https://doi.org/10.1140/epjc/s10052-008-0662-y
14. Bernabei R. et al. Eur. Phys. J. C 67 (2010) 39. https://doi.org/10.1140/epjc/s10052-010-1303-9
15. Bernabei R. et al. Eur. Phys. J. C 62 (2009) 327. https://doi.org/10.1140/epjc/s10052-009-1068-1
16. Bernabei R. et al. Eur. Phys. J. C 72 (2012) 1920.
17. Bernabei R. et al. Eur. Phys. J. C 72 (2012) 2064. https://doi.org/10.1140/epjc/s10052-012-2064-4
18. Bernabei R. et al. Phys. Rev. D 77 (2008) 023506.
19. Bernabei R. et al. Mod. Phys. Lett. A 23 (2008) 2125. https://doi.org/10.1142/S0217732308027473
20. Bernabei R. et al. Int. J. Mod. Phys. A 21 (2006) 1445. https://doi.org/10.1142/S0217751X06030874
21. Bernabei R. et al. Int. J. Mod. Phys. A 22 (2007) 3155. https://doi.org/10.1142/S0217751X07037093
22. Smith D., Weiner N. Phys. Rev. D 64 (2001) 043502; https://doi.org/10.1103/PhysRevD.64.043502
Tucker-Smith D., Weiner N. Phys. Rev. D 72 (2005) 063509. https://doi.org/10.1103/PhysRevD.72.06350923. Freese K. et al. Phys. Rev. D 71 (2005) 043516; https://doi.org/10.1103/PhysRevD.71.043516
Phys. Rev. Lett. 92 (2004) 111301. https://doi.org/10.1103/PhysRevLett.92.11130124. Ling F. S., Sikivie P., Wick S. Phys. Rev. D 70 (2004) 123503. https://doi.org/10.1103/PhysRevD.70.123503
25. Bernabei R. et al. AIP Conf. Proceed 1223 (2010) 50 [arXiv:0912.0660]; J. Phys.: Conf. Ser. 203 (2010) 012040 [arXiv:0912.4200]; (http://taup2009.lngs.infn.it/slides/jul3/nozzoli.pdf), talk given by F. Nozzoli; Can. J. Phys. 89 (2011) 141; SIF Atti Conf. 103 (2011) [arXiv:1007.0595]; Physics Procedia 37 (2012) 1095.
26. Bottino A. et al. Phys. Rev. D 81 (2010) 107302; Fornengo N. et al. D 83 (Phys. Rev) 015001; Fitzpatrick A. L. et al. Phys. Rev. D 81 (2010) 115005; Hooper D. et al. Phys. Rev. D 82 (2010) 123509; Belikov A. V. et al. Phys. Lett. B 705 (2011) 82; Kuflik E. et al. Phys. Rev. D 81 (2010) 111701; Chang S. et al. Phys. Rev. D 79 (2009) 043513; Chang S. et al. Phys. Rev. Lett. 106 (2011) 011301; Foot R. Phys. Rev. D 81 (2010) 087302; Bai Y., Fox P. J. JHEP 0911 (2009) 052; Alwall J. et al. Phys. Rev. D 81 (2010) 114027; Khlopov M. Yu. et al. arXiv:1003.1144; Andreas S. et al. Phys. Rev. D 82 (2010) 043522; Kopp J. et al. JCAP 1002 (2010) 014; Barger V. et al. Phys. Rev. D 82 (2010) 035019; Feng J. L. et al. Phys. Lett. B 703 (2011) 124.
27. Belli P. et al. Phys. Rev. D 84 (2011) 055014. https://doi.org/10.1103/PhysRevD.84.055014
28. Bottino A. et al. Phys. Rev. D 85 (2012) 095013. https://doi.org/10.1103/PhysRevD.85.095013
29. Aalseth C. E. et al. Phys. Rev. Lett. 106 (2011) 131301; Aalseth C. E. et al. Phys. Rev. Lett. 107 (2011) 141301.
30. Angloher G. et al. arXiv:1109.0702.
31. Ahmed Z. et al. Science 327 (2010) 1619. https://doi.org/10.1126/science.1186112
32. Armengaud E. et al. Phys. Lett. B 702 (2011) 329.
33. Aprile E. et al. Phys. Rev. Lett. 105 (2010) 131302.
34. Bernabei R. et al. "Liquid Noble gases for Dark Matter searches: a synoptic survey", Exorma Ed., Roma, ISBN 978-88-95688-12-1, 2009, pp. 1-53 [arXiv:0806.0011v2].
35. Collar J. I., McKinsey D. N. arXiv:1005.0838; arXiv:1005.3723; Collar J. I. arXiv:1006.2031; arXiv:1010.5187; arXiv:1103.3481; arXiv:1106.0653; arXiv:1106.3559.
36. Hudson R. Found. Phys. 39 (2009) 174. https://doi.org/10.1007/s10701-009-9271-3
37. Bernabei R. et al. Journal of Instrumentation 7 (2012) P03009. https://doi.org/10.1088/1748-0221/7/03/P03009