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C"],"abstract":"Abstract<\/jats:title>$$\\varLambda $$<\/jats:tex-math>\n \u039b<\/mml:mi>\n <\/mml:math><\/jats:alternatives><\/jats:inline-formula>-Cold Dark Matter ($$\\varLambda $$<\/jats:tex-math>\n \u039b<\/mml:mi>\n <\/mml:math><\/jats:alternatives><\/jats:inline-formula>CDM) has been successful at explaining the large-scale structures in the universe but faces severe issues on smaller scales when compared to observations. Introducing self-interactions between dark matter particles claims to provide a solution to the small-scale issues in the $$\\varLambda $$<\/jats:tex-math>\n \u039b<\/mml:mi>\n <\/mml:math><\/jats:alternatives><\/jats:inline-formula>CDM simulations while being consistent with the observations at large scales. The existence of the energy region in which these self-interactions between dark matter particles come close to saturating the S-wave unitarity bound can result in the formation of dark matter bound states called darkonium. In this scenario, all the low energy scattering properties are determined by a single parameter, the inverse scattering length $$\\gamma $$<\/jats:tex-math>\n \u03b3<\/mml:mi>\n <\/mml:math><\/jats:alternatives><\/jats:inline-formula>. In this work, we set bounds on $$\\gamma $$<\/jats:tex-math>\n \u03b3<\/mml:mi>\n <\/mml:math><\/jats:alternatives><\/jats:inline-formula> by studying the impact of darkonium on the observations at direct detection experiments using data from CRESST-III and XENON1T. The exclusion limits on $$\\gamma $$<\/jats:tex-math>\n \u03b3<\/mml:mi>\n <\/mml:math><\/jats:alternatives><\/jats:inline-formula> are then subsequently converted to exclusion limits on the self-interaction cross-section and compared with the constraints from astrophysics and N-body simulations.<\/jats:p>","DOI":"10.1140\/epjc\/s10052-024-13472-4","type":"journal-article","created":{"date-parts":[[2024,11,18]],"date-time":"2024-11-18T13:11:38Z","timestamp":1731935498000},"update-policy":"https:\/\/doi.org\/10.1007\/springer_crossmark_policy","source":"Crossref","is-referenced-by-count":0,"title":["Constraints on self-interaction cross-sections of dark matter in universal bound states from direct detection"],"prefix":"10.1140","volume":"84","author":[{"given":"G.","family":"Angloher","sequence":"first","affiliation":[]},{"given":"S.","family":"Banik","sequence":"additional","affiliation":[]},{"given":"G.","family":"Benato","sequence":"additional","affiliation":[]},{"given":"A.","family":"Bento","sequence":"additional","affiliation":[]},{"given":"A.","family":"Bertolini","sequence":"additional","affiliation":[]},{"given":"R.","family":"Breier","sequence":"additional","affiliation":[]},{"given":"C.","family":"Bucci","sequence":"additional","affiliation":[]},{"given":"J.","family":"Burkhart","sequence":"additional","affiliation":[]},{"given":"E.","family":"Cipelli","sequence":"additional","affiliation":[]},{"given":"L.","family":"Canonica","sequence":"additional","affiliation":[]},{"given":"A.","family":"D\u2019Addabbo","sequence":"additional","affiliation":[]},{"given":"S.","family":"Di Lorenzo","sequence":"additional","affiliation":[]},{"given":"L.","family":"Einfalt","sequence":"additional","affiliation":[]},{"given":"A.","family":"Erb","sequence":"additional","affiliation":[]},{"given":"F. v.","family":"Feilitzsch","sequence":"additional","affiliation":[]},{"given":"S.","family":"Fichtinger","sequence":"additional","affiliation":[]},{"given":"D.","family":"Fuchs","sequence":"additional","affiliation":[]},{"given":"A.","family":"Garai","sequence":"additional","affiliation":[]},{"given":"V. 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