Searcharxiv⌕ Search

arXiv subjects

Wladyslaw Trzaska

Publications and source records attributed to Wladyslaw Trzaska.

2 recordsLinked to original sources

IPbus extension for the ALFRED framework

We present a development of the ALFRED framework that includes support for the IPbus protocol, created for the Fast Interaction Trigger (FIT) detector in the ALICE experiment at CERN. This modification resolves the incompatibility between the current GBT-based slow-control protocols and the FIT electronics, which is based on the IPbus. A compatibility layer, named ALF IPbus, was created in C++ and integrated with DIM services, allowing for the transparent conversion of SWT frames into IPbus transactions. Benchmark tests indicated median execution times of less than 4.2 $μ$s per frame for sequences above 512 words, comfortably meeting the ALICE Detector Control System requirements. Long-term stability tests conducted in the FV0 detector achieved an uptime close to 100\% from the moment of implementation on the FIT-FV0 detector. This solution enables FIT operation without firmware changes, ensures smooth integration with SCADA systems, and provides a scalable pathway for future migration to GBT-based control. The approach is general and can be applied to other ALICE subdetectors and high-energy physics experiments requiring protocol bridging.

physics.ins-det↗

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↗