A large number of particle detectors employ liquid argon as their target material owing to its high scintillation yield and its ability to drift ionization charge over large distances. Scintillation ...light from argon is peaked at 128 nm and a wavelength shifter is required for its efficient detection. In this work, we directly compare the light yield achieved in two identical liquid argon chambers, one of which is equipped with polyethylene naphthalate (PEN) and the other with tetraphenyl butadiene (TPB) wavelength shifter. Both chambers are lined with enhanced specular reflectors and instrumented with SiPMs with a coverage fraction of approximately 1%, which represents a geometry comparable to the future large scale detectors. We measured the light yield of the PEN chamber to be 39.4
±
0.4(stat)
±
1.9(syst)% of the yield of the TPB chamber. Using a Monte Carlo simulation this result is used to extract the wavelength shifting efficiency of PEN relative to TPB equal to 47.2
±
5.7%. This result paves the way for the use of easily available PEN foils as a wavelength shifter, which can substantially simplify the construction of future liquid argon detectors.
Celotno besedilo
Dostopno za:
DOBA, IZUM, KILJ, NUK, PILJ, PNG, SAZU, SIK, UILJ, UKNU, UL, UM, UPUK
Abstract
Detection of light signals is crucial to a wide range of
particle detectors. In particular, efficient detection of vacuum
ultraviolet (VUV) light will provide new opportunities for some
...novel detectors currently being developed, but is technically
challenging. In this article, we characterized the performance of
Hamamatsu VUV4 silicon photomultipliers (SiPMs) for detecting VUV
argon scintillation light without wavelength shifting. Using a
customized cryogenic amplifier design, we operated two models of
VUV4 SiPMs inside liquid argon and thoroughly examined their direct
sensitivities to liquid argon scintillation. In addition to
describing their cryogenic performance, we measured a photon
detection efficiency of 14.7
+1.1
-2.4
% and
17.2
+1.6
-3.0
% at 128 nm for these two VUV4 models for
operation at 4 V of overvoltage, with the main uncertainty arising
from the SiPM reflectivity for VUV light.
The solar neutrino experiment Borexino, which is located in the Gran Sasso underground laboratories, is in a unique position to study muon-induced backgrounds in an organic liquid scintillator. In ...this study, a large sample of cosmic muons is identified and tracked by a muon veto detector external to the liquid scintillator, and by the specific light patterns observed when muons cross the scintillator volume. The yield of muon-induced neutrons is found to be Y sub(n) = (3.10 + or - 0.11) times 10 super(-4) sub(n)/( mu times (g/cm super(2))). The distance prole between the parent muon track and the neutron capture point has the average value lambda = (81.5 + or - 2.7) cm. Additionally the yields of a number of cosmogenic radioisotopes are measured for super(12)N, super(12)B, super(8)He, super(9)C, super(9)Li, super(8)B, super(6)He, super(8)Li, super(11)Be, super(10)C and super(11)C. All results are compared with Monte Carlo simulation predictions using the Fluka and GEANT4 packages. General agreement between data and simulation is observed for the cosmogenic production yields with a few exceptions, the most prominent case being super(11)C yield for which both codes return about 50% lower values. The predicted mu -n distance prole and the neutron multiplicity distribution are found to be overall consistent with data.
Abstract
In this work we will document the design and the performances of a SiPM-based photo-detector with a surface area of 100 cm
2
conceived to operate as a replacement for PMTs. The signals from ...94 SiPMs are summed up to produce an aggregated output that exhibits in liquid nitrogen a dark count rate (DCR) lower than 100 cps over the entire surface, a signal to noise ratio better than 13, and a timing resolution better than 5.5 ns. The module feeds about 360 mW at 5 V with a dynamic range in excess of 500 photo-electrons on a 100 Ω differential line. The unit can also operate at room temperature, at the cost of an increase of DCR to 10
8
cps.
A new system to assign accurate timestamps to events recorded by experiments running underground has been designed, installed and tested at INFN Gran Sasso National Laboratory, Italy. This facility ...is based on a Master unit installed on surface and receiving time information from a GPS receiver, and Slave units placed underground which get data packet from the Master via optical fiber and assign the timestamps. The system is able to provide a time accuracy of 15 ns (1σ) and precise reference frequencies to the experiments. It is now part of the infrastructure of the Laboratory for all the experimental activities which need accurate timestamps.
The Recoil Directionality (ReD) Experiment Sanfilippo, S; Agnes, P; Albergo, S ...
Journal of physics. Conference series,
11/2022, Letnik:
2374, Številka:
1
Journal Article
Recenzirano
Odprti dostop
Directional sensitivity to nuclear recoils would provide a smoking gun for a possible discovery of dark matter in the form of WIMPs (Weakly Interacting Massive Particles). A hint of directional ...dependence of the response of a dual-phase argon Time Projection Chamber (TPC) was found in the SCENE experiment. Given the potential importance of such a capability in the framework of dark matter searches, a new dedicated experiment, ReD (Recoil Directionality), was designed by the Global Argon Dark Matter Collaboration, in order to scrutinize this hint. Prior to the irradiation with a neutron beam, the ReD TPC underwent a long campaign of characterization and optimization: some selected results are presented in this contribution.
Abstract
The scintillation time response of liquid argon has a key
role in the discrimination of electronic backgrounds in dark matter
search experiments. However, its extraordinary rejection power ...can
be affected by various detector effects such as the delayed light
emission of TetraPhenyl Butadiene, the most commonly used wavelength
shifter, and the electric drift field applied in Time Projection
Chambers. In this work, we characterized the TetraPhenyl Butadiene
delayed response and the dependence of the pulse shape
discrimination on the electric field, exploiting the data acquired
with the ARIS, a small-scale single-phase liquid argon detector
exposed to monochromatic neutron and gamma sources at the ALTO
facility of IJC Lab in Orsay.
SiPM-based readouts are becoming the standard for light detection in particle detectors given their superior resolution and ease of use with respect to vacuum tube photo-multipliers. However, the ...contributions of noise detection such as the dark rate, cross-talk, and after-pulsing (AP) may significantly impact their performance. In this work, we present the development of highly reflective single-phase argon chambers capable of displaying light yields up to 32 photo-electrons per keV, with approximately 12 being primary photo-electrons generated by the argon scintillation, while the rest are accounted by optical cross-talk. Furthermore, the presence of compound processes results in a generalized Fano factor larger than 2 already at an over-voltage of 5 V. Finally, we present a parametrization of the optical cross-talk for the FBK NUV-HD-Cryo SiPMs at 87 K that can be extended to future detectors with tailored optical simulations.
Borexino was the first experiment to detect solar neutrinos in real-time in the sub- MeV region. In order to achieve high precision in the determination of neutrino rates, the detector design ...includes an internal and an external calibration system. This paper describes both calibration systems and the calibration campaigns that were carried out in the period between 2008 and 2011. We discuss some of the results and show that the calibration procedures preserved the radiopurity of the scintillator. The calibrations provided a detailed understanding of the detector response and led to a significant reduction of the systematic uncertainties in the Borexino measurements.
We report the measurement of the time of flight of ∼17 GeV ν(μ) on the CNGS baseline (732 km) with the Large Volume Detector (LVD) at the Gran Sasso Laboratory. The CERN-SPS accelerator has been ...operated from May 10th to May 24th 2012, with a tightly bunched-beam structure to allow the velocity of neutrinos to be accurately measured on an event-by-event basis. LVD has detected 48 neutrino events, associated with the beam, with a high absolute time accuracy. These events allow us to establish the following limit on the difference between the neutrino speed and the light velocity: -3.8 × 10(-6) < (v(ν)-c)/c < 3.1 × 10(-6) (at 99% C.L.). This value is an order of magnitude lower than previous direct measurements.
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