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Geo- and reactor antineutrino sensitivity at THEIA

2022; Springer Science+Business Media; Volume: 82; Issue: 12 Linguagem: Inglês

10.1140/epjc/s10052-022-11106-1

1434-6052

S. Zsoldos, Z. Bagdasarian, G. D. Orebi Gann, Andrew Barna, Stephen T. Dye,

Dark Matter and Cosmic Phenomena

Abstract We present the sensitivity of the Theia experiment to low-energy geo- and reactor antineutrinos. For this study, we consider one of the possible proposed designs, a 17.8-ktonne fiducial volume Theia -25 detector filled with water-based liquid scintillator placed at Sanford Underground Research Facility (SURF). We demonstrate Theia ’s sensitivity to measure the geo- and reactor antineutrinos via inverse-beta decay interactions after one year of data taking with $$11.9 \times 10^{32}$$ 11.9 × 10 32 free target protons. Considering all uncertainties on input throughout the whole analysis chain, the expected number of geo- and reactor antineutrinos is $$220\,^{+30}_{-24}$$ 220 - 24 + 30 (stats+syst) and $$168\,^{+26}_{-24}$$ 168 - 24 + 26 (stat+sys), respectively, after one year of data taking. The corresponding expected fit precision of a sole experiment is evaluated at 8.7% and 10.1%, respectively. We also demonstrate the sensitivity towards fitting individual Th and U contributions, with best fit values of $$N_\text {Th}=40^{+26}_{-22}$$ N Th = 40 - 22 + 26 (stat+sys) and $$N_\text {U}=180^{+30}_{-24}$$ N U = 180 - 24 + 30 (stat+sys). Finally, from the fit results of individual Th and U contributions, we evaluate the mantle signal to be $$S_\text {mantle} = 9.3\,\pm [5.2,5.4]$$ S mantle = 9.3 ± [ 5.2 , 5.4 ] NIU (stat+sys). This was obtained assuming a full-range positive correlation ( $$\rho _c\in [0, 1]$$ ρ c ∈ [ 0 , 1 ] ) between Th and U, and the projected uncertainties on the crust contributions of 8.3% (Th) and 7.0% (U).