Astrophysics > Instrumentation and Methods for Astrophysics
[Submitted on 27 Jan 2013 (v1), last revised 16 Apr 2013 (this version, v3)]
Title:Measurement of the proton light response of various LAB based scintillators and its implication for supernova neutrino detection via neutrino-proton scattering
View PDFAbstract:The proton light output function in electron-equivalent energy of various scintillators based on linear alkylbenzene (LAB) has been measured in the energy range from 1 MeV to 17.15 MeV for the first time. The measurement was performed at the Physikalisch-Technische Bundesanstalt (PTB) using a neutron beam with continuous energy distribution. The proton light output data is extracted from proton recoil spectra originating from neutron-proton scattering in the scintillator. The functional behavior of the proton light output is described succesfully by Birks' law with a Birks constant kB between (0.0094 +/- 0.0002) cm/MeV and (0.0098 +/- 0.0003) cm/MeV for the different LAB solutions. The constant C, parameterizing the quadratic term in the generalized Birks law, is consistent with zero for all investigated scintillators with an upper limit (95% CL) of about 10^{-7} cm^2/MeV^2. The resulting quenching factors are especially important for future planned supernova neutrino detection based on the elastic scattering of neutrinos on protons. The impact of proton quenching on the supernova event yield from neutrino-proton scattering is discussed.
Submission history
From: Belina von Krosigk [view email][v1] Sun, 27 Jan 2013 21:12:59 UTC (676 KB)
[v2] Tue, 29 Jan 2013 13:13:31 UTC (676 KB)
[v3] Tue, 16 Apr 2013 08:59:23 UTC (676 KB)
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