Wiki source code of High-pressure operation of optical time projection chambers for neutrino physics
Last modified by Ricardo Julio Rodríguez Fernández on 2025/06/13 08:11
Hide last authors
| author | version | line-number | content |
|---|---|---|---|
 |
2.1 | 1 | === Speeding up the numerical solution of the Boltzmann Equation in Diffusion Approximation === |
| |
6.1 | 2 | ==== Supervisor: Pablo Amedo Martínez ==== |
| 3 | ==== Supervisor: Diego Rodas Rodríguez | ||
| |
3.1 | 4 | ==== |
| |
2.1 | 5 | |
| |
4.1 | 6 | The recent technological demonstration of the ability to reconstruct minimum ionizing particles and time-tagging the interaction, simultaneously, by using ultra-fast optical cameras (2ns event rate) is transformational towards next-generation neutrino and rare event experiments. The ability to reconstruct the interaction at 2mm-sampling and 1ns-resolution, for the first time in gas phase, will allow to reconstruct the neutrino interaction to unprecedented precision in next-generation neutrino oscillation experiments, such as DUNE. |
| |
2.1 | 7 | |
| |
4.1 | 8 | We aim at an experimental campaign in July this year, designed to explore the pressure range above atmospheric (1-3bar) and establish the detector performance in those conditions, about half its way towards the envisaged conditions of our technological demonstrator (7bar). |
| 9 | |||
| 10 | Besides participating in the experimental campaign, working as part of a team, we expect the student to help processing the event images, and characterizing the detector performance in view of its final application as a neutrino detector. | ||
| 11 |