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| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Prasad, Suraj | en_US |
| dc.contributor.author | Mallick, Neelkamal | en_US |
| dc.contributor.author | Sahoo, Raghunath | en_US |
| dc.date.accessioned | 2026-09-21T12:20:42Z | - |
| dc.date.available | 2026-09-21T12:20:42Z | - |
| dc.date.issued | 2026 | - |
| dc.identifier.citation | Prasad, S., Mallick, N., Sahoo, R., & Barnaföldi, G. G. (2026). Exploring the effects of α-clustered structure of 16O nuclei in anisotropic flow fluctuations in 16O-16O collisions at the LHC within a CGC+Hydro framework. Journal of Subatomic Particles and Cosmology, 5. https://doi.org/10.1016/j.jspc.2026.100290 | en_US |
| dc.identifier.issn | 3050-4805 | - |
| dc.identifier.other | EID(2-s2.0-105048807579) | - |
| dc.identifier.uri | https://dx.doi.org/10.1016/j.jspc.2026.100290 | - |
| dc.identifier.uri | https://dspace.iiti.ac.in/handle/123456789/19221 | - |
| dc.description.abstract | In this paper, we explore the effects of the presence of clustered nuclear structure of 16O in the final state elliptic flow fluctuations through 16O-16O collisions at (Formula presented) TeV within a hybrid model, IPGlasma+MUSIC+iSS+ UrQMD. We compare the results of elliptic flow fluctuations using α-clustered nuclear structure to the Woods-Saxon nuclear profile having no clustered structure. We observe a significant difference in the elliptic flow fluctuations, which arise due to the consideration of a clustered nuclear structure of 16O. © 2026 Elsevier Ltd. All rights are reserved, including those for text and data mining, AI training, and similar technologies. | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | Elsevier B.V. | en_US |
| dc.source | Journal of Subatomic Particles and Cosmology | en_US |
| dc.title | Exploring the effects of α-clustered structure of 16O nuclei in anisotropic flow fluctuations in 16O-16O collisions at the LHC within a CGC+Hydro framework | en_US |
| dc.type | Journal Article | en_US |
| Appears in Collections: | Department of Physics | |
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