Tobias Heinz | Searcharxiv

arXiv2025

A novel method for measuring the attenuation length and the group velocity of transparent liquids in a variable length cavity

The transparency of liquid scintillators or water is an important parameter for many detectors in particle and astroparticle physics. In this work, the Cavity Enhanced Long Light Path Attenuation Length Screening (CELLPALS) method for the determination of the attenuation length is presented for the first time. The method is based on an experimental setup similar to a Fabry-Pérot interferometer but adding up multiple-reflected intensities of a modulated light source. CELLPALS was developed to measure the attenuation length of highly transparent liquids (> 10 m) with significantly lower uncertainties than with UV-Vis spectroscopy, which is a standard method for determining the attenuation length. In addition to the attenuation length, the group velocity of light in the sample can also be derived from the free spectral range of the cavity, which is not provided by any conventional method for determining the attenuation length. In this work, the CELLPALS method, its achievable precision and an experimental setup to demonstrate its feasibility are discussed. The attenuation lengths and group velocities of several transparent liquids were measured at wavelengths between 420 nm and 435 nm. In addition, the attenuation length and group velocity of linear alkylbenzene (LAB) samples after different purification stages and a purified LAB-based liquid scintillator were measured at a wavelength of 425 nm. The results confirmed the potential of CELLPALS to determine the attenuation length with an uncertainty of ~ 2 %. The group velocity of light in the sample can be determined with an uncertainty of ~ 0.03 %.

physics.ins-det↗

arXiv2022

Potential for a precision measurement of solar $pp$ neutrinos in the Serappis Experiment

The Serappis (SEarch for RAre PP-neutrinos In Scintillator) project aims at a precision measurement of the flux of solar $pp$ neutrinos on the few-percent level. Such a measurement will be a relevant contribution to the study of solar neutrino oscillation parameters and a sensitive test of the solar luminosity constraint. The concept of Serappis relies on a small organic liquid scintillator detector ($\sim$20 m$^3$) with excellent energy resolution ($\sim$2.5 % at 1 MeV), low internal background and sufficient shielding from surrounding radioactivity. This can be achieved by a minor upgrade of the OSIRIS facility at the site of the JUNO neutrino experiment in southern China. To go substantially beyond current accuracy levels for the $pp$ flux, an organic scintillator with ultra-low $^{14}$C levels (below $10^{-18}$) is required. The existing OSIRIS detector and JUNO infrastructure will be instrumental in identifying suitable scintillator materials, offering a unique chance for a low-budget high-precision measurement of a fundamental property of our Sun that will be otherwise hard to access.

physics.ins-det↗