Please use this identifier to cite or link to this item: https://dspace.iiti.ac.in/handle/123456789/11085
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dc.contributor.authorPradhan, Girija Sankaren_US
dc.contributor.authorSahoo, Raghunathen_US
dc.contributor.authorScaria, Ronalden_US
dc.date.accessioned2022-11-21T14:27:23Z-
dc.date.available2022-11-21T14:27:23Z-
dc.date.issued2022-
dc.identifier.citationScaria, R., Ahmad, S., Chakraborty, M., Chandra, A., Dugad, S. R., Gupta, S. K., . . . Zuberi, M. (2022). Investigation of K/ π ratio with Accelerator and Cosmic ray data. Paper presented at the Springer Proceedings in Physics, , 277 703-707. doi:10.1007/978-981-19-2354-8_127 Retrieved from www.scopus.comen_US
dc.identifier.isbn978-9811923531-
dc.identifier.issn0930-8989-
dc.identifier.otherEID(2-s2.0-85140751856)-
dc.identifier.urihttps://doi.org/10.1007/978-981-19-2354-8_127-
dc.identifier.urihttps://dspace.iiti.ac.in/handle/123456789/11085-
dc.description.abstractWe look at K/ π ratio as an indicator for strangeness enhancement and compare cosmic data with the collider data.We use CORSIKA to generate data on Extensive Air Showers (EAS) and compare the K/ π ratio with accelerator results.Experimentally observed cosmic K/ π values are also compared with results from hadronic and symmetric and asymmetric nucleus-nucleus collisions.Since Cosmic Rays (CRs) consist mostly of protons and the atmosphere is rich mainly in nitrogen and oxygen we expect more proton-nucleus type collisions to occur and such a scenario agrees well with the experimental values. © 2022, The Author(s), under exclusive license to Springer Nature Singapore Pte Ltd.en_US
dc.language.isoenen_US
dc.publisherSpringer Science and Business Media Deutschland GmbHen_US
dc.sourceSpringer Proceedings in Physicsen_US
dc.subjectCosmologyen_US
dc.subjectCosmicsen_US
dc.subjectExperimental valuesen_US
dc.subjectExtensive air showersen_US
dc.subjectHadronicsen_US
dc.subjectNucleus-nucleus collisionen_US
dc.subjectStrangeness enhancementen_US
dc.subjectSymmetricsen_US
dc.subjectCosmic raysen_US
dc.titleInvestigation of K/ π Ratio with Accelerator and Cosmic Ray Dataen_US
dc.typeConference Paperen_US
Appears in Collections:Department of Physics

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