Unleashing the full power of LHCb to probe stealth new physics

dc.contributor.affiliationUniversidade de Santiago de Compostela. Instituto Galego de Física de Altas Enerxías (IGFAE)
dc.contributor.authorBorsato, Martino
dc.contributor.authorCid Vidal, Xabier
dc.contributor.authorZupan, Jure
dc.date.accessioned2026-01-21T12:22:23Z
dc.date.available2026-01-21T12:22:23Z
dc.date.issued2022-02-16
dc.description.abstractIn this paper, we describe the potential of the LHCb experiment to detect Stealth physics. This refers to dynamics beyond the Standard Model that would elude searches that focus on energetic objects or precision measurements of known processes. Stealth signatures include long-lived particles and light resonances that are produced very rarely or together with overwhelming backgrounds. We will discuss why LHCb is equipped to discover this kind of physics at the Large Hadron Collider and provide examples of well-motivated theoretical models that can be probed with great detail at the experiment.
dc.description.peerreviewedSI
dc.description.sponsorshipWe thank the participants in the “Stealth Physics at LHCb” workshop, held in Santiago de Compostela in February 2020 [336], for many fruitful discussions and for triggering many ideas that were developed here. We also thank the LHC Long-Lived Particle community, and the LPCC LHC Long-lived Particle and Dark Matter working groups for fostering and nurturing the interest in the ideas here discussed. We kindly acknowledge Vladimir Gligorov, Stephen Farry and Niels Tuning for kindly reading and providing comments to this document. The work of XCV is supported by MINECO (Spain) through the Ramon y Cajal program RYC-2016-20073 and by XuntaGAL under the ED431F 2018/01 project. ACV thanks the support of the Spanish Research Agency through the program “The Standard Model to the limits: BSM searches with LHCb” with reference PRE2018-083399. This project has also been supported by the Europen Union ESF program. JZ is supported by the Generalitat Valenciana (Spain) through the plan GenT program (CIDEGENT/2019/068). GA acknowledges support by a McGill Trottier Chair Astrophysics Postdoctoral Fellowship, and by the Natural Sciences and Engineering Research Council, Canada. The work of ME is supported by a Fellowship of the Alexander von Humboldt Foundation. JK has received funding from the Slovenian Research Agency (research core funding No. P1-0035). LH acknowledges the support from the ERC Consolidator Grant SELDOM G. A. 771642. MR acknowledges support by Fundaçao para a Ciencia e a Tecnologia (FCT) under the grant PD/BD/142773/2018 and the project CERN/FIS-PAR/0024/2019, as well as by LIP (FCT,COMPETE2020-Portugal2020, FEDER, POCI-01-0145-FEDER-007334). MSR and EP certify that this study was financed in part by the Coordenaçao de Aperfeiçoamento de Pessoal de Nivel Superior – Brasil (CAPES) – Finance Code 001, CNPq and FAPERJ. YS is supported by grants from NSF-BSF, ISF and the Azrieli foundation and is a Taub fellow (supported by the Taub Family Foundation). YT is supported by the NSF grant PHY2014165. The research of SW is supported by the German Research Foundation (DFG) under grant no. 396021762–TRR 257. The work of IGFAE members authoring this paper has received financial support from XuntaGAL (Centro singular de investigacion de Galicia accreditation 2019-2022), by European Union ERDF and ESF, by the “María de Maeztu” Units of Excellence program MDM-2016-0692 and the Spanish Research State Agency.
dc.identifier.citationM Borsato et al 2022 Rep. Prog. Phys. 85 024201
dc.identifier.doi10.1088/1361-6633/ac4649
dc.identifier.essn1361-6633
dc.identifier.issn0034-4885
dc.identifier.urihttps://hdl.handle.net/10347/45312
dc.issue.number024201
dc.journal.titleReports on Progress in Physics
dc.language.isoeng
dc.publisherIOP Publishing
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internationalen
dc.rights.accessRightsopen access
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/
dc.titleUnleashing the full power of LHCb to probe stealth new physics
dc.typejournal article
dc.type.hasVersionAM
dc.volume.number85
dspace.entity.typePublication
relation.isAuthorOfPublication75692f9e-5811-44e8-9d4f-957b88d7f397
relation.isAuthorOfPublication.latestForDiscovery75692f9e-5811-44e8-9d4f-957b88d7f397

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