Conveners
Poster advertisment
- Diane Markoff
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Matteo del Gallo Roccagiovine (Sapienza University of Rome)22/03/2023, 16:00Poster
By combining a BGO scintillator crystal, and a Kinetic Inductance Detector light readout, we can take advantage of the BGO's high density, high Z, high radiopurity, high light-yield at cryogenic temperatures and relatively fast timing, and combine it with a KID's fast response time, ease of readout, natural multiplexing and sub-0.1keV resolution, to obtain a fast sensor that is well suited to...
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James Browning, Ryan Bouabid22/03/2023, 16:03Poster
The COHERENT High Purity Germanium detector array (ge-mini) is a dedicated low background CE$\nu$NS experiment deployed at the Spallation Neutron Source (SNS) at Oak Ridge National Lab. The SNS delivers a pulsed source of neutrinos which provides an excellent suppression of steady state backgrounds as well as unique challenges in data acquisition. In this poster we will report on the...
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Jules COLAS22/03/2023, 16:06Poster
In precision CEvNS experiments like RICOCHET at Laue Langevin Institute reactor, the recoil energy is encoded in the amplitudes of pulses. In such experiments, detectors like the CRYOCUBE use multi-channel cryogenic solid-state detectors which is a promising technology to achieve low threshold gamma/neutron discrimination by measuring the ionization yield against heat energy. The CEvNS...
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Nicolas MARTINI (IP2I)22/03/2023, 16:09Poster
The RICOCHET reactor neutrinos observatory is planned to be installed at Laue Langevin Institute (ILL) starting in mid-2022. The scientific goal of the RICOCHET international collaboration is to perform a low-energy and percentage-precision CEvNS measurement. To that end, RICOCHET will host two cryogenic detector arrays : the CRYOCUBE (Ge target) and the Q-ARRAY (Zn target).
The CryoCube...
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Nityasa Mishra22/03/2023, 16:12Poster
Direct dark matter detectors can be sensitive to detection of solar neutrinos through the CEvNS process at low thresholds. We analyse the possibility of detecting radiative correction to the tree level cross-sections at the dark matter detectors. Utilizing neutrino flavour oscillation of solar neutrinos as a source of flavour dependent flux, we explore the likelihood of detecting radiative...
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Bo Johnson (Indiana University)22/03/2023, 16:15Poster
Coherent elastic neutrino-nucleus scattering (CEvNS) was detected on liquid argon (LAr) using the CENNS-10 detector at Oak Ridge National Laboratory in 2021. Ongoing research is focused on developing a ton-scale LAr detector that can measure CEvNS with greater precision, including sensitivity to charge-current neutrino interactions and an increased detection rate twenty times greater than that...
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Adryanna Major (Duke University)22/03/2023, 16:18Poster
The COHERENT collaboration operates a multi-target suite of low-threshold neutrino detectors at the Spallation Neutron Source (SNS) at Oak Ridge National Laboratory. These detectors are uniquely equipped to observe the dominant low-energy (E$_\nu \sim$ 10s of MeV) interaction of coherent elastic neutrino-nucleus scattering (CE$\nu$NS). The only experimental trace is a nuclear recoil of mere...
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Dmitrii Rudik (MEPhI)22/03/2023, 16:21Poster
RED-100 is a two phase emission LXe detector exposed at Kalinin NPP to study coherent elastic neutrino nucleus scattering (CEvNS) in a flux of reactor antineutrinos. Several campaigns were carried out to study external background at the detector location under the reactor core. During RED-100 data taking, continuous monitoring was organized in order to check the external background flux...
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Keyu Ding (University of South Dakota)22/03/2023, 16:24Poster
Inorganic scintillating detectors are widely used in the detection of dark matter and neutrinos due to their relatively high light yields and easy light readout with PMTs at room temperature. Our prototype, pure CsI coupled with SiPMs at cryogenic temperature, can achieve a much higher light yield. The high light yield illustrates the great potential of this novel combination for neutrino and...
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Emma van Nieuwenhuizen22/03/2023, 16:27Poster
Ge-mini is a germanium detector subsystem, part of the COHERENT experiment at the Spallation Neutron Source at Oak Ridge National Lab. As a CEvNS experiment, Ge-mini is sensitive to backgrounds from varying sources, mitigated by multiple layers of shielding including High Density Polyethylene (HDPE), copper, and approximately 6 US tons of lead. Since Ge-mini is located at a depth of ~ 8...
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James Runge22/03/2023, 16:30Poster
Accurate calculations of B(GT) are essential for predicting rates in low energy neutrino scattering experiments. However, past experiments have shown discrepancies between theoretical calculations and experimental measurements of B(GT) in some isotopes. This poster presents the current state of B(GT) measurements for isotopes relevant to neutrino scattering, including both charged-current and...
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Aitor Bracho22/03/2023, 16:33Poster
The reactor antineutrino anomaly features a spectral bump in the 5-7 MeV range. Previous analyses have suggested that current models can be improved upon through use of the summation method for spectral calculation. However, this method suffers from compounding uncertainties from fission product yield data in nuclear databases. Moreover, nineteen and twenty fission products have been...
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JaeJin Choi (Seoul national university)22/03/2023, 16:36Poster
NEON (Neutrino Elastic-scattering Observation with NaI) aims an observation of the coherent elastic neutrino-nucleus scattering (CEvNS) using reactor anti-electron neutrino with NaI(Tl) crystal detectors at Hanbit nuclear power plant in Yeonggwang, South Korea. For the observation of the CEvNS with the NEON detector, we need to achieve 0.2 keV energy corresponding to five photoelectrons...
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