68 research outputs found
Antineutrino Geophysics with Liquid Scintillator Detectors
Detecting the antineutrinos emitted by the decay of radioactive elements in
the mantle and crust could provide a direct measurement of the total abundance
of uranium and thorium in the Earth. In calculating the antineutrino flux at
specific sites, the local geology of the crust and the background from the
world's nuclear power reactors are important considerations. Employing a global
crustal map, with type and thickness data, and using recent estimates of the
uranium and thorium distribution in the Earth, we calculate the antineutrino
event rate for two new neutrino detectors. We show that spectral features allow
terrestrial antineutrino events to be identified above reactor antineutrino
backgrounds and that the uranium and thorium contributions can be separately
determined.Comment: Published paper differs from original submitted preprint because
reviewers suggested updated continental crust U/Th abundances. Kamioka
geographical location error was in preprint, partially corrected in published
version. This version is the same as the published paper, with Kamioka fully
corrected. Because of recent interest in this topic, this version is being
made available, despite this work being 8 years ol
Scintillation efficiency measurement of Na recoils in NaI(Tl) below the DAMA/LIBRA energy threshold
The dark matter interpretation of the DAMA modulation signal depends on the
NaI(Tl) scintillation efficiency of nuclear recoils. Previous measurements for
Na recoils have large discrepancies, especially in the DAMA/LIBRA modulation
energy region. We report a quenching effect measurement of Na recoils in
NaI(Tl) from 3keV to 52keV, covering the whole
DAMA/LIBRA energy region for light WIMP interpretations. By using a low-energy,
pulsed neutron beam, a double time-of-flight technique, and pulse-shape
discrimination methods, we obtained the most accurate measurement of this kind
for NaI(Tl) to date. The results differ significantly from the DAMA reported
values at low energies, but fall between the other previous measurements. We
present the implications of the new quenching results for the dark matter
interpretation of the DAMA modulation signal
The SABRE project and the SABRE Proof-of-Principle
SABRE aims to directly measure the annual modulation of the dark matter interaction rate with NaI(Tl) crystals. A modulation compatible with the standard hypothesis, in which our Galaxy is immersed in a dark matter halo, has been measured by the DAMA experiment in the same target material. Other direct detection experiments, using different target materials, seem to exclude the interpretation of such modulation in the simplest scenario of WIMP-nucleon elastic scattering. The SABRE experiment aims to carry out an independent search with sufficient sensitivity to confirm or refute the DAMA claim. The goal of the SABRE experiment is to achieve the lowest background rate for a NaI(Tl) experiment (order of 0.1 cpd/kg/keV(ee) in the energy region of interest for dark matter). This challenging goal could be achievable by operating high-purity crystals inside a liquid scintillator veto for active background rejection. In addition, twin detectors will be located in the northern and southern hemispheres to identify possible contributions to the modulation from seasonal or site-related effects. The SABRE project includes an initial Proof-of-Principle phase at LNGS (Italy), to assess the radio-purity of the crystals and the efficiency of the liquid scintillator veto. This paper describes the general concept of SABRE and the expected sensitivity to WIMP annual modulation.The SABRE program is supported by funding from INFN (Italy), NSF (USA), and ARC (Australia Grants:
LE170100162, LE16010080, DP170101675, LP150100075). F. Froborg
has received funding from the European Union’s Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant
agreement No 703650. We acknowledge the generous hospitality and
constant support of the Laboratori Nazionali del Gran Sasso (Italy)
Characterization of SABRE crystal NaI-33 with direct underground counting
Ultra-pure NaI(Tl) crystals are the key element for a model-independent verification of the long standing DAMA result and a powerful means to search for the annual modulation signature of dark matter interactions. The SABRE collaboration has been developing cutting-edge techniques for the reduction of intrinsic backgrounds over several years. In this paper we report the first characterization of a 3.4 kg crystal, named NaI-33, performed in an underground passive shielding setup at LNGS. NaI-33 has a record low K contamination of 4.3 ± 0.2 ppb as determined by mass spectrometry. We measured a light yield of 11.1 ± 0.2 photoelectrons/keV and an energy resolution of 13.2% (FWHM/E) at 59.5 keV. We evaluated the activities of Ra and Th inside the crystal to be 5.9±0.6μBq/kg and 1.6±0.3μBq/kg, respectively, which would indicate a contamination from U and Th at part-per-trillion level. We measured an activity of 0.51 ± 0.02 mBq/kg due to Pb out of equilibrium and a α quenching factor of 0.63 ± 0.01 at 5304 keV. We illustrate the analyses techniques developed to reject electronic noise in the lower part of the energy spectrum. A cut-based strategy and a multivariate approach indicated a rate, attributed to the intrinsic radioactivity of the crystal, of ∼ 1 count/day/kg/keV in the [5–20] keV region.The SABRE program is supported by funding from INFN (Italy), NSF (US
Final results of Borexino Phase-I on low energy solar neutrino spectroscopy
Borexino has been running since May 2007 at the LNGS with the primary goal of
detecting solar neutrinos. The detector, a large, unsegmented liquid
scintillator calorimeter characterized by unprecedented low levels of intrinsic
radioactivity, is optimized for the study of the lower energy part of the
spectrum. During the Phase-I (2007-2010) Borexino first detected and then
precisely measured the flux of the 7Be solar neutrinos, ruled out any
significant day-night asymmetry of their interaction rate, made the first
direct observation of the pep neutrinos, and set the tightest upper limit on
the flux of CNO neutrinos. In this paper we discuss the signal signature and
provide a comprehensive description of the backgrounds, quantify their event
rates, describe the methods for their identification, selection or subtraction,
and describe data analysis. Key features are an extensive in situ calibration
program using radioactive sources, the detailed modeling of the detector
response, the ability to define an innermost fiducial volume with extremely low
background via software cuts, and the excellent pulse-shape discrimination
capability of the scintillator that allows particle identification. We report a
measurement of the annual modulation of the 7 Be neutrino interaction rate. The
period, the amplitude, and the phase of the observed modulation are consistent
with the solar origin of these events, and the absence of their annual
modulation is rejected with higher than 99% C.L. The physics implications of
phase-I results in the context of the neutrino oscillation physics and solar
models are presented
- …