Changes for page Diego González Díaz
Last modified by Ricardo Julio Rodríguez Fernández on 2025/07/09 16:19
From version 3.1
edited by Ricardo Julio Rodríguez Fernández
on 2025/06/11 19:32
on 2025/06/11 19:32
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To version 4.1
edited by Ricardo Julio Rodríguez Fernández
on 2025/06/13 08:00
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... ... @@ -1,1 +1,1 @@ 1 - SergioBarreraCabodevila1 +High-pressure operation of optical time projection chambers for neutrino physics - Content
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... ... @@ -1,6 +1,10 @@ 1 1 === Speeding up the numerical solution of the Boltzmann Equation in Diffusion Approximation === 2 -==== Supervisor: SergioBarrera Cabodevila2 +==== Supervisor: Pablo Amedo Martínez 3 3 ==== 4 4 5 -The KineticTheoryframeworkisastate-of-the-art weak-couplingtoolto explore thethermalization in heavy-ioncollisions. The Boltzmann EquationinDiffusionApproximation(BEDA) is oneparticularimplementationofa kinetictheoryforwhichaGPU-basedcodehasbeenrecentlydeveloped.Thiscode has animportantissueof instabilitiesthat significantly decreasesits efficiency related to thenumerical integrationof thediffusionterms with thefinitevolume method.In thisstay,weproposethat thestudent modify this integrationwithaCrank-Nicolsonmethodthat doesnot sufferfromtheseinstabilities.Thestudentwillfamiliarizewiththe kinetic theoryframework, veryclosetothekinetic description instatistical mechanics, as well as novel computationaltoolssuch as GPUprogramming. It is strongly recommendedto have previousknowledgeof basic computationaltechniquestosolve partialdifferentialequations.Prior C++ knowledgeisalsoadvisable.5 +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. 6 6 7 +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). 8 + 9 +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. 10 +