The DAMA/LIBRA apparatus

By R. Bernabei, P. Belli, A. Bussolotti, F. Cappella, R. Cerulli, C. Dai, A. D'angelo, H. L. He, A. Incicchitti, H. Kuang and 13 more. 2008

355 citations recorded by the source corpus.

The similar or equal to 250 kg highly radiopure NaI(Tl) DAMA/LIBRA apparatus, running at the Gran Sasso National Laboratory (LNGS) of the INFN, is described. (C) 2008 Elsevier B.V. All rights reserved.

Subfields: Atomic and Molecular Physics, and Optics, Nuclear and High Energy Physics, Radiation

View Paper: https://www.semanticscholar.org/paper/e819c5cb621a621994de285332a74a8999d6ed1e

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In Atomic and Molecular Physics, and Optics

1. L. Rauch
2. T. Undagoitia
3. P. Madau
4. B. Moore
5. Marcel Zemp
6. J. Diemand
7. Joachim Stadel
8. Michael Kuhlen

In Nuclear and High Energy Physics

1. Michael Kuhlen
2. P. Madau
3. M. Lisanti
4. J. Diemand
5. T. Schwetz
6. L. Strigari
7. B. Moore
8. James S. Bullock

In Radiation

1. T. Schwetz

Citations in the corpus

• First model independent results from DAMA/LIBRA-phase2 (2018, background): “Calibrations with X-rays/γ sources are periodically performed down to the keV energy region in the same running condition [20,36].”
• WIMP dark matter candidates and searches—current status and future prospects (2017, methodology): “ the plot correspond to the favored regions for DM interpretations of anomalies reported in the literature by the CDMS-Si [176] (blue), CoGeNT [170] (grey) CRESST-II [180] (light blue) and DAMA/LIBRA [154] (light green) collaborations. The shaded area below the solid orange line on the bottom of the”
• Colloquium: Annual modulation of dark matter (2013, background): “…(Aalseth et al., 2011a, 2011b, 2013), COUPP (Behnke et al., 2012), CRESST (Angloher et al., 2012), DAMA/NaI (Bernabei et al., 2003), DAMA/LIBRA (Bernabei et al., 2008, 2010), DEAP/CLEAN (Kos, 2010), DM-Ice (Cherwinka et al., 2012), DRIFT (Alner et al., 2005; Daw et al., 2012), EDELWEISS…”
• Dark matter direct-detection experiments (2015, background): “ated in coincidence with the crystals to reduce further the background. The DAMA experiment at the LNGS underground laboratoryxis searching for dark matter using ultra low-radioactive NaI(Tl) crystals[271]. A combined dataset of DAMA and its successor DAMA/LIBRA have collected 1.33ton y exposure sho”
• Dark matter direct detection with non-Maxwellian velocity structure (2009, methodology): “We employ energy smearing at DAMA by assuming that the smearing reported for the one of 25 targets of DAMA/LIBRA [72] is characteristic of all of them.”
• Spin-independent elastic WIMP scattering and the DAMA annual modulation signal (2008, methodology): “For example, figure 26 of [39] shows that the efficiency for DAMA single-hit events starts to deviate from 1 below about 8 keVee, just in the signal region.”