Scintillators for particle physics in the frame of TWISMA European project

28 січ. 2026 р., 15:00
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Доповідач

Oleg Sidletskiy (ISMA)

Опис

The collaboration between ISMA and CERN began in the early 1990s when ISMA (then part of the Institute for Single Crystals), played a pioneering role in the development of lead tungstate (PbWO4), a scintillator implemented in detectors at the Large Hadron Collider (LHC). Works by L. Nagornaya and co-authors demonstrated the feasibility of achieving an extremely fast scintillation response and growing highly uniform large PbWO4 crystals with a high radiation tolerance [1].

The works continued with the INTELUM European project (2015-2019), which focused on the fabrication technology of garnet scintillation fibers for high-granularity calorimeters. Ce-doped Y3Al5O12 (YAG:Ce) and Lu3Al5O12 (LuAG:Ce) fibers with 1-2 mm cross-section and lengths of up to 55 cm were produced using the micro-pulling-down method in collaboration with the Institute of Light and Matter (ILM). The luminescence attenuation length in LuAG:Ce fibers reached 1 m, meeting transparency requirements [2]. Meanwhile, it was realized that although the micro-pulling-down technology could provide ready-to-use fiber-shaped crystals without post-growth mechanical treatment, the growth of bulk crystals and cutting them into fibers proved to be a more reliable approach for producing many thousands of fibers required for large-scale experiments at colliders.

The Horizon Europe TWISMA project (2023-2025) involving ISMA, CERN, and ILM was focused on bulk crystals produced by the Czochralski method. It addressed rare earth garnets such as YAG:Ce and Gd3(Al,Ga)5O12:Ce (GAGG:Ce) with accelerated luminescence rise/decay times and enhanced time resolution. LHCb detectors at the high-luminosity LHC must provide no pileup of signals at the frequency of particle collision of 25 ns, hence scintillators with a decay time of <15 ns and an approximate light yield over 15000 phot/MeV are required. Various codoping schemes of garnet crystals were verified to achieve a balance between a faster decay and reasonable light yield. Another focus of TWISMA was crystals for dual-readout detectors for simultaneous registration of scintillation and Cherenkov light at future colliders. Bi4Si3O12 (BSO) and Bi4(Ge1-xSix)3O12 have been proposed [3] as monolithic crystals capable of registering both scintillation light emitted in the visible band and providing a wide transparency window in the UV at >290 nm for Cherenkov light registration. Tests of calorimeter prototypes based on BSO and garnet scintillators are underway in CERN.

[1] L.L. Nagornaya, V.D. Ryzhikov, 1.A.Tupitsina, Proc. of 1994 IEEE Nuclear Science Symposium (1994), 156-158.

[2] V. Kononets, K. Lebbou, O. Sidletskiy, Yu. Zorenko, M. Lucchini, K. Pauwels, and E. Auffray, M. Korzhik and A. Gektin (eds.), Engineering of Scintillation Materials and Radiation Technologies, Springer Proceedings in Physics 200 (2017), pp. 114-128

[3] R. Cala’, N. Kratochwil, L. Martinazzoli, M.T. Lucchini, S. Gundacker, E. Galenin, I. Gerasymov, O. Sidletskiy, M. Nikl, E. Auffray, NIM. A 1032 (2022) 166527.

Authors

Boris Grynyov (National Academy of Sciences of Ukraine (UA)) Boris Grynyov (Kharkov State University (KSU)) Etiennette Auffray Hillemanns (CERN) Oleg Sidletskiy (National Academy of Sciences of Ukraine (UA)) Д-р. Oleg Sidletskiy (Institute for scintillation Materials NAS of Ukraine) Oleg Sidletskiy (ISMA) kheirreddine. Lebbou

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