Solar neutrino detection in liquid xenon detectors via charged-current scattering to excited states
Haselschwardt, S., Lenardo, B., Pirinen, P., & Suhonen, J. (2020). Solar neutrino detection in liquid xenon detectors via charged-current scattering to excited states. Physical Review D, 102(7), Article 072009. https://doi.org/10.1103/physrevd.102.072009
Published in
Physical Review DDate
2020Copyright
© Authors,, 2020
We investigate the prospects for real-time detection of solar neutrinos via the charged-current neutrino-nucleus scattering process in liquid xenon time projection chambers. We use a nuclear shell model, benchmarked with experimental data, to calculate the cross sections for populating specific excited states of the cesium nuclei produced by neutrino capture on 131Xe and 136Xe. The shell model is further used to compute the decay schemes of the low-lying 1+ excited states of 136Cs, for which there is sparse experimental data. We explore the possibility of tagging the characteristic deexcitation γ rays/conversion electrons using two techniques: spatial separation of their energy deposits using event topology and their time separation using delayed coincidence. The efficiencies in each case are evaluated within a range of realistic detector parameters. We find that the topological signatures are likely to be dominated by radon backgrounds, but that a delayed-coincidence signature from long-lived states predicted in 136Cs may enable background-free detection of CNO neutrino interactions in next-generation experiments with smaller uncertainty than current measurements. We also estimate the sensitivity as a function of exposure for detecting the solar-temperature-induced line shift in 7Be neutrino emission, which may provide a new test of solar models.
...
![showless](/themes/JYX2//images/showless.png)
![showmore](/themes/JYX2//images/showmore.png)
Publisher
American Physical Society (APS)ISSN Search the Publication Forum
2470-0010Keywords
Publication in research information system
https://converis.jyu.fi/converis/portal/detail/Publication/43480791
Metadata
Show full item recordCollections
Related funder(s)
Research Council of FinlandFunding program(s)
Academy Project, AoFAdditional information about funding
This work was supported by the U.S. Department of Energy Office of Science under Contract No. DE-AC02-05CH11231 and by DOE-NP Grant No. DE-SC0017970. B. L. acknowledges the support of a Karl Van Bibber fellowship from Stanford University. This work has been partially supported by the Academy of Finland under Project No. 318043.License
Related items
Showing items with similar title or keywords.
-
Theoretical predictions of wimp-nucleus and neutrino-nucleus scattering in context of dark matter direct detection
Pirinen, Pekka (University of Jyväskylä, 2018)The nature of dark matter is at present an open question. Assuming the main component of dark matter consists of weakly interacting massive particles (WIMPs), directly detecting such particle via a scattering process ... -
Calculated solar-neutrino capture rate for a radiochemical 205Tl-based solar-neutrino detector
Kostensalo, Joel; Suhonen, Jouni; Zuber, K. (American Physical Society, 2020)Radiochemical experiments for low-energy solar-neutrino detection have been making headlines by exploiting the isotopes 37Cl and 71Ga. Such a very low-threshold measurement of this type can also be performed using 205Tl, ... -
Neutral-current supernova-neutrino cross sections for 204,206,208Pb calculated by Skyrme quasiparticle random-phase approximation
Almosly, Wafa; Carlsson, B. G.; Suhonen, Jouni; Ydrefors, E. (American Physical Society, 2019)The present work constitutes a detailed study of neutral-current (NC) supernova-neutrino scattering off the stable even-even lead isotopes 204,206,208Pb. This is a continuation of our previous work [Almosly et al., Phys. ... -
Charged-current neutrino-nucleus scattering off Xe isotopes
Pirinen, Pekka; Suhonen, Jouni; Ydrefors, E. (American Physical Society, 2019)Xenon detectors are used in the search for dark matter and neutrinoless double-beta decay ( 0 ν β β ) . As the next-generation detectors reach masses in the ton scale, neutrinos from astrophysical sources are soon ... -
Charged-current neutrino-nucleus scattering off 127I and 133Cs
Hellgren, Matti; Suhonen, Jouni (American Physical Society (APS), 2024)Calculations of (anti)neutrino-nucleus scattering cross sections are vital since experimental results for these cross sections for terrestrial-based (anti)neutrino sources in the low-to-intermediate energy ranges are ...