The Impact of Helium Exposure on the PMTs of the SuperNEMO Experiment
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arXiv
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| Format: | Preprint |
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2025
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| author | SuperNEMO Collaboration Aguerre, X. Barabash, A. S. Basharina-Freshville, A. Bongrand, M. Bourgeois, Ch. Breton, D. Breier, R. Busto, J. Cerna, C. Ceschia, M. Chauveau, E. Chopra, A. Dawson, L. Duchesneau, D. Evans, J. J. Filosofov, D. Garrido, X. Girard-Carillo, C. Granjon, M. Hoballah, M. Hodák, R. Horner, G. Hussain, M. H. Islam, A. Jérémie, A. Jullian, S. Kaizer, J. Klimenko, A. Kochetov, O. Koňařík, F. Konovalov, S. I. Křižák, T. Kovalenko, S. Lahaie, A. Lang, K. Lemière, Y. Li, P. Maalmi, J. Macko, M. Mamedov, F. Marquet, C. Mauger, F. Mendl, A. Morgan, B. Nemchenok, I. Nomachi, M. Palušová, V. Patrick, C. Pavicic, T. Perrot, F. Petro, M. Piquemal, F. Povinec, P. Pratt, S. Proga, M. Quinn, W. S. Ramachers, Y. A. Riddle, C. L. Rukhadze, N. Saakyan, R. Salazar, R. Sedgbeer, J. Shitov, Yu. Simard, L. Šimkovic, F. Smolnikov, A. Söldner-Rembold, S. Štekl, I. Suhonen, J. Tedjditi, H. Thomas, J. Timkin, V. Tretyak, V. I. Tretyak, Vl. I. Turnbull, G. Umatov, V. I. Vereshchaka, Y. Waters, D. |
| author_facet | SuperNEMO Collaboration Aguerre, X. Barabash, A. S. Basharina-Freshville, A. Bongrand, M. Bourgeois, Ch. Breton, D. Breier, R. Busto, J. Cerna, C. Ceschia, M. Chauveau, E. Chopra, A. Dawson, L. Duchesneau, D. Evans, J. J. Filosofov, D. Garrido, X. Girard-Carillo, C. Granjon, M. Hoballah, M. Hodák, R. Horner, G. Hussain, M. H. Islam, A. Jérémie, A. Jullian, S. Kaizer, J. Klimenko, A. Kochetov, O. Koňařík, F. Konovalov, S. I. Křižák, T. Kovalenko, S. Lahaie, A. Lang, K. Lemière, Y. Li, P. Maalmi, J. Macko, M. Mamedov, F. Marquet, C. Mauger, F. Mendl, A. Morgan, B. Nemchenok, I. Nomachi, M. Palušová, V. Patrick, C. Pavicic, T. Perrot, F. Petro, M. Piquemal, F. Povinec, P. Pratt, S. Proga, M. Quinn, W. S. Ramachers, Y. A. Riddle, C. L. Rukhadze, N. Saakyan, R. Salazar, R. Sedgbeer, J. Shitov, Yu. Simard, L. Šimkovic, F. Smolnikov, A. Söldner-Rembold, S. Štekl, I. Suhonen, J. Tedjditi, H. Thomas, J. Timkin, V. Tretyak, V. I. Tretyak, Vl. I. Turnbull, G. Umatov, V. I. Vereshchaka, Y. Waters, D. |
| contents | The performance of Hamamatsu 8" photomultiplier tubes (PMTs) of the type used in the SuperNEMO neutrinoless double-beta decay experiment (R5912-MOD), is investigated as a function of exposure to helium (He) gas. Two PMTs were monitored for over a year, one exposed to varying concentrations of He, and the other kept in standard atmospheric conditions as a control. Both PMTs were exposed to light signals generated by a Bi-207 radioactive source that provided consistent large input PMT signals similar to those that are typical of the SuperNEMO experiment. The energy resolution of PMT signals corresponding to 1 MeV energy scale determined from the Bi-207 decay spectrum, shows a negligible degradation with He exposure; however the rate of after-pulsing shows a clear increase with He exposure, which is modelled and compared to diffusion theory. A method for reconstructing the partial pressure of He within the PMT and a method for determining the He breakdown point, are introduced. The implications for long-term SuperNEMO operations are briefly discussed. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2501_13755 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | The Impact of Helium Exposure on the PMTs of the SuperNEMO Experiment SuperNEMO Collaboration Aguerre, X. Barabash, A. S. Basharina-Freshville, A. Bongrand, M. Bourgeois, Ch. Breton, D. Breier, R. Busto, J. Cerna, C. Ceschia, M. Chauveau, E. Chopra, A. Dawson, L. Duchesneau, D. Evans, J. J. Filosofov, D. Garrido, X. Girard-Carillo, C. Granjon, M. Hoballah, M. Hodák, R. Horner, G. Hussain, M. H. Islam, A. Jérémie, A. Jullian, S. Kaizer, J. Klimenko, A. Kochetov, O. Koňařík, F. Konovalov, S. I. Křižák, T. Kovalenko, S. Lahaie, A. Lang, K. Lemière, Y. Li, P. Maalmi, J. Macko, M. Mamedov, F. Marquet, C. Mauger, F. Mendl, A. Morgan, B. Nemchenok, I. Nomachi, M. Palušová, V. Patrick, C. Pavicic, T. Perrot, F. Petro, M. Piquemal, F. Povinec, P. Pratt, S. Proga, M. Quinn, W. S. Ramachers, Y. A. Riddle, C. L. Rukhadze, N. Saakyan, R. Salazar, R. Sedgbeer, J. Shitov, Yu. Simard, L. Šimkovic, F. Smolnikov, A. Söldner-Rembold, S. Štekl, I. Suhonen, J. Tedjditi, H. Thomas, J. Timkin, V. Tretyak, V. I. Tretyak, Vl. I. Turnbull, G. Umatov, V. I. Vereshchaka, Y. Waters, D. Instrumentation and Detectors Nuclear Experiment The performance of Hamamatsu 8" photomultiplier tubes (PMTs) of the type used in the SuperNEMO neutrinoless double-beta decay experiment (R5912-MOD), is investigated as a function of exposure to helium (He) gas. Two PMTs were monitored for over a year, one exposed to varying concentrations of He, and the other kept in standard atmospheric conditions as a control. Both PMTs were exposed to light signals generated by a Bi-207 radioactive source that provided consistent large input PMT signals similar to those that are typical of the SuperNEMO experiment. The energy resolution of PMT signals corresponding to 1 MeV energy scale determined from the Bi-207 decay spectrum, shows a negligible degradation with He exposure; however the rate of after-pulsing shows a clear increase with He exposure, which is modelled and compared to diffusion theory. A method for reconstructing the partial pressure of He within the PMT and a method for determining the He breakdown point, are introduced. The implications for long-term SuperNEMO operations are briefly discussed. |
| title | The Impact of Helium Exposure on the PMTs of the SuperNEMO Experiment |
| topic | Instrumentation and Detectors Nuclear Experiment |
| url | https://arxiv.org/abs/2501.13755 |