USMEFT as a tool for discovery of universal new physics at high luminosity LHC
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| Main Authors: | , , , , |
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| Format: | Preprint |
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2026
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| _version_ | 1866914578924830720 |
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| author | Corbett, Tyler Desai, Jay Eboli, O. J. P. Gonzalez-Garcia, M. C. Martines, Matheus |
| author_facet | Corbett, Tyler Desai, Jay Eboli, O. J. P. Gonzalez-Garcia, M. C. Martines, Matheus |
| contents | We analyze the potential of the Universal SMEFT as a tool to study universal new physics in the neutral and charged Drell-Yan processes at the high-luminosity LHC. In order to do so, we generated pseudo-data containing the contributions of beyond the standard model vector bosons to the dilepton production. Our results show that fits with the minimal theoretical bias can be used not only to unveil the existence of new physics but also to accurately extract its properties. Moreover, the results are rather stable with respect to the order of truncation of the effective field theory. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2605_15262 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | USMEFT as a tool for discovery of universal new physics at high luminosity LHC Corbett, Tyler Desai, Jay Eboli, O. J. P. Gonzalez-Garcia, M. C. Martines, Matheus High Energy Physics - Phenomenology We analyze the potential of the Universal SMEFT as a tool to study universal new physics in the neutral and charged Drell-Yan processes at the high-luminosity LHC. In order to do so, we generated pseudo-data containing the contributions of beyond the standard model vector bosons to the dilepton production. Our results show that fits with the minimal theoretical bias can be used not only to unveil the existence of new physics but also to accurately extract its properties. Moreover, the results are rather stable with respect to the order of truncation of the effective field theory. |
| title | USMEFT as a tool for discovery of universal new physics at high luminosity LHC |
| topic | High Energy Physics - Phenomenology |
| url | https://arxiv.org/abs/2605.15262 |