Please use this identifier to cite or link to this item: http://hdl.handle.net/11452/28314
Title: Secondary avalanches in gas mixtures
Authors: Veenhof, Robert J.
Uludağ Üniversitesi/Fen-Edebiyat Fakültesi/Fizik Anabilim Dalı.
0000-0003-3940-7222
Şahin, Özkan
Tapan, İlhan
AAH-6445-2021
I-9715-2017
36053592700
8905787000
Keywords: Instruments & instrumentation
Nuclear science & technology
Physics
Excited states
Gas gain
Photon feedback
Proportional-counters
Excited states
Excited atoms
Gases
Atoms
Gas mixtures
Inert gases
Ionization
Photons
Gas gain
Exponential increase
Feedback parameters
Noble gas atoms
Photon emissions
Quencher concentration
Secondary avalanche
Issue Date: 1-Aug-2013
Publisher: Elsevier
Citation: Şahin, Ö. vd. (2013). "Secondary avalanches in gas mixtures". Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 718, 432-433.
Abstract: Avalanche development in gas-based detectors relies not only on direct ionisation but also on excitation of noble gas atoms. Some quencher molecules can be ionised when they collide with excited atoms, a process on which we reported earlier In Alternatively, excited atoms can decay by photon emission. If these photons are insufficiently absorbed by the quencher, yet capable of ionising, then they may escape from the avalanche region and start secondary avalanches. This process, called photon feedback, leads to an over-exponential increase of the gas gain which limits the working range. In this paper, we derive photon feedback parameters from published gain measurements for several gas mixtures and fit these parameters in a model which describes their dependence on the quencher concentration and the pressure.
Description: Bu çalışma, 20-26 Mayıs 2012 tarihleri arasında İtalya’da düzenlenen 12. Pisa Meeting on Advanced Detectors’da bildiri olarak sunulmuştur.
URI: https://doi.org/10.1016/j.nima.2012.08.067
http://hdl.handle.net/11452/28314
ISSN: 0168-9002
1872-9576
Appears in Collections:Scopus
Web of Science

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