Publicación:
Resolving a challenging supersymmetric low-scale seesaw scenario at the ILC
Resolving a challenging supersymmetric low-scale seesaw scenario at the ILC
dc.contributor.author | Masias J. | es_PE |
dc.contributor.author | Cerna-Velazco N. | es_PE |
dc.contributor.author | Jones-Pérez J. | es_PE |
dc.contributor.author | Porod W. | es_PE |
dc.date.accessioned | 2024-05-30T23:13:38Z | |
dc.date.available | 2024-05-30T23:13:38Z | |
dc.date.issued | 2021 | |
dc.description.abstract | We investigate a scenario inspired by natural supersymmetry, where neutrino data is explained within a low-scale seesaw scenario. For this the minimal supersymmetric Standard Model is extended by adding light right-handed neutrinos and their superpartners, the R-sneutrinos. Moreover, we consider the lightest neutralinos to be Higgsino-like. We first update a previous analysis and assess to which extent does existing LHC data constrain the allowed slepton masses. Here we find scenarios where sleptons with masses as low as 175 GeV are consistent with existing data. However, we also show that the upcoming run will either discover or rule out sleptons with masses of 300 GeV, even for these challenging scenarios. We then take a scenario which is on the borderline of observability of the upcoming LHC run assuming a luminosity of 300 fb-1. We demonstrate that a prospective international e+e- linear collider with a center of mass energy of 1 TeV will be able to discover sleptons in scenarios which are difficult for the LHC. Moreover, we also show that a measurement of the spectrum will be possible within 1-3 percent accuracy. © 2021 authors. Published by the American Physical Society. Published by the American Physical Society under the terms of the "https://creativecommons.org/licenses/by/4.0/"Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. Funded by SCOAP3. | |
dc.description.sponsorship | The authors would like to thank Jenny List for discussing the mass measurement method. W. P. has been supported by DAAD, Project No. 57395885. N. C. V. was funded by Grant No. 236-2015-FONDECYT. J. J. P. and J. M. acknowledge funding by the Dirección de Gestión de la Investigación at PUCP, through Grant No. DGI-2019-3-0044. N. C. V., J. J. P., and J. M. have been also supported by the DAAD-CONCYTEC Project No. 131-2017-FONDECYT. | |
dc.identifier.doi | https://doi.org/10.1103/PhysRevD.103.115028 | |
dc.identifier.scopus | 2-s2.0-85108853538 | |
dc.identifier.uri | https://hdl.handle.net/20.500.12390/3048 | |
dc.language.iso | eng | |
dc.publisher | American Physical Society | |
dc.relation.ispartof | Physical Review D | |
dc.rights | info:eu-repo/semantics/openAccess | |
dc.rights.uri | https://creativecommons.org/licenses/by/4.0/ | |
dc.subject | Techniques | |
dc.subject | Physical Systems | es_PE |
dc.subject.ocde | https://purl.org/pe-repo/ocde/ford#1.01.02 | |
dc.title | Resolving a challenging supersymmetric low-scale seesaw scenario at the ILC | |
dc.type | info:eu-repo/semantics/article | |
dspace.entity.type | Publication | |
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