Please use this identifier to cite or link to this item: https://dspace.iiti.ac.in/handle/123456789/15187
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dc.contributor.authorScaria, Ronalden_US
dc.contributor.authorSingh, Captain R.en_US
dc.contributor.authorSahoo, Raghunathen_US
dc.date.accessioned2024-12-24T05:20:09Z-
dc.date.available2024-12-24T05:20:09Z-
dc.date.issued2024-
dc.identifier.citationScaria, R., Singh, C. R., Deb, S., & Sahoo, R. (2024). Muon Puzzle: Bridging the gap between cosmic ray and accelerator experiments. Proceedings of Science. Scopus. https://www.scopus.com/inward/record.uri?eid=2-s2.0-85212249561&partnerID=40&md5=5d5162980da0116c385d0abde1f3f604en_US
dc.identifier.issn1824-8039-
dc.identifier.otherEID(2-s2.0-85212249561)-
dc.identifier.urihttps://dspace.iiti.ac.in/handle/123456789/15187-
dc.description.abstractMultiple cosmic ray experiments have observed that the various high-energy physics models are unable to explain the muon multiplicities at very high primary energies. The models consistently predict lower numbers as compared to what is experimentally observed. This is termed as the “muon puzzle", as model tuning cannot resolve this issue. A possible solution proposed is the formation of quark-gluon plasma which invariantly produce more strange particles that decays into muons. We explore the electromagnetic to hadronic energy fraction in the final state particles and compare it with the strangeness production over different systems and energies used at the Large Hadron Collider using various models like EPOS LHC, SYBILL 2.3d, QGSJET II-04 and PYTHIA. The results will be presented with an outlook in view of the recently proposed OO and pO collisions at LHC. © Copyright owned by the author(s) under the terms of the Creative Commons.en_US
dc.language.isoenen_US
dc.publisherSissa Medialab Srlen_US
dc.sourceProceedings of Scienceen_US
dc.titleMuon Puzzle: Bridging the gap between cosmic ray and accelerator experimentsen_US
dc.typeConference Paperen_US
Appears in Collections:Department of Physics

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