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| DOI | 10.1140/EPJC/S10052-024-13421-1 | ||||
| Año | 2024 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
In this study, we demonstrate the potential of the NA64 experiment at CERN SPS to search for New Physics processes involving e ->mu\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$e\rightarrow \mu $$\end{document} transitions after the collision of 100 GeV electrons with target nuclei. A new Dark Sector leptonic portal in which a scalar boson phi\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\varphi $$\end{document} could be produced in the lepton-flavor-changing bremsstrahlung-like reaction, eN ->mu N phi\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$eN\rightarrow \mu N\varphi $$\end{document}, is used as benchmark process. In this work, we develop a realistic Monte Carlo simulation of the NA64 experimental setup implementing the differential and total production cross-section computed at exact tree-level and applying the Weisz & auml;cker-Williams phase space approximation. Using this framework, we investigate the main background sources and calculate the expected sensitivity of the experiment. The results indicate that with minor setup optimization, NA64 can probe a large fraction of the available parameter space compatible with the muon g-2\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$g-2$$\end{document} anomaly and the Dark Matter relic predictions in the context of a new Dark Sector leptonic portal with 1011\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$10<^>{11}$$\end{document} EOT. This result paves the way to the exploration of lepton-flavour-changing transitions in NA64.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Ponten, A. | - |
UPPSALA UNIV - Suecia
Uppsala Universitet - Suecia |
| 2 | Sieber, H. | - |
ETH - Suiza
ETH Zurich - Suiza |
| 3 | Banto Oberhauser, B. | - |
ETH - Suiza
ETH Zurich - Suiza |
| 4 | Crivelli, P. | - |
ETH - Suiza
ETH Zurich - Suiza |
| 5 | Kirpichnikov, D. | - |
Russian Acad Sci - Rusia
Institute for Nuclear Research of the Russian Academy of Sciences - Rusia |
| 6 | Gninenko, S. N. | - |
Russian Acad Sci - Rusia
Universidad Nacional Andrés Bello - Chile Institute for Nuclear Research of the Russian Academy of Sciences - Rusia |
| 7 | Hösgen, M. | - |
UNIV BONN - Alemania
Universität Bonn - Alemania |
| 8 | Bueno, L. Molina | - |
UV - España
CSIC-UV - Instituto de Física Corpuscular (IFIC) - España |
| 9 | Mongillo, M. | - |
ETH - Suiza
ETH Zurich - Suiza |
| 10 | Zhevlakov, Alexey S. | Hombre |
JINR - Rusia
Matrosov Inst Syst Dynam & Control Theory SB RAS - Rusia Bogoliubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research - Rusia Matrosov Institute for System Dynamics and Control Theory of Siberian Branch of Russian Academy of Sciences - Rusia |
| Fuente |
|---|
| Ministerio de Ciencia e Innovación |
| SNSF |
| Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung |
| Agencia Estatal de Investigación |
| Eidgenossische Technische Hochschule Zurich |
| ETH |
| Ministerio de Ciencia e Innovacin |
| UE (Spain) |
| Agradecimiento |
|---|
| We acknowledge the members of the NA64 collaboration for fruitful discussions. In particular, we thank N. V. Krasnikov for his helpful suggestions and correspondence. The work of P. Crivelli, B. Banto Oberhauser, M. Mongillo, and H. Sieber is supported by the SNSF Grants No. 186158, and No. 197346 No. 216602, No. 219485 (Switzerland) and by ETH Grant No. 22-2 ETH-031. The work of L. Molina-Bueno is supported by SNSF Grant No. 186158 (Switzerland), RyC-030551-I, PID2021-123955NA-100 and CNS2022-135850 funded by MCIN/AEI/ 10.13039/501100011033/FEDER, UE (Spain). |
| We acknowledge the members of the NA64 collaboration for fruitful discussions. In particular, we thank N. V. Krasnikov for his helpful suggestions and correspondence. The work of P. Crivelli, B. Banto Oberhauser, M. Mongillo, and H. Sieber is supported by the SNSF Grants No. 186158, and No. 197346 No. 216602, No. 219485 (Switzerland) and by ETH Grant No. 22-2 ETH-031. The work of L. Molina-Bueno is supported by SNSF Grant No. 186158 (Switzerland), RyC-030551-I, PID2021-123955NA-100 and CNS2022-135850 funded by MCIN/AEI/ 10.13039/501100011033/FEDER, UE (Spain). |