On the determination of the interaction time of GeV neutrinos in large argon gas TPCs
Next-generation megawatt-scale neutrino beams open the way to studying neutrino-nucleus scattering using gaseous targets for the first time. This represents an opportunity to improve the knowledge of neutrino cross sections in the energy region between hundreds of MeV and a few GeV, of interest for...
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Zusammenfassung: | Next-generation megawatt-scale neutrino beams open the way to studying
neutrino-nucleus scattering using gaseous targets for the first time. This
represents an opportunity to improve the knowledge of neutrino cross sections
in the energy region between hundreds of MeV and a few GeV, of interest for the
upcoming generation of long-baseline neutrino oscillation experiments. The
challenge is to accurately track and (especially) time the particles produced
in neutrino interactions in large and seamless volumes down to few-MeV
energies. We propose to accomplish this through an optically-read time
projection chamber (TPC) filled with high-pressure argon and equipped with both
tracking and timing functions. In this work, we present a detailed study of the
time-tagging capabilities of such a device, based on end-to-end optical
simulations that include the effect of photon propagation, photosensor
response, dark count rate and pulse reconstruction. We show that the neutrino
interaction time can be reconstructed from the primary scintillation signal
with a precision in the range of 1-2.5 ns ($\sigma$) for point-like deposits
with energies down to 5 MeV. A similar response is observed for
minimum-ionizing particle tracks extending over lengths of a few meters. A
discussion on previous limitations towards such a detection technology, and how
they can be realistically overcome in the near future thanks to recent
developments in the field, is presented. The performance demonstrated in our
analysis seems to be well within reach of next-generation neutrino-oscillation
experiments, through the instrumentation of the proposed TPC with conventional
reflective materials and a silicon photomultiplier array behind a transparent
cathode. |
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DOI: | 10.48550/arxiv.2401.09920 |