{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2026,4,19]],"date-time":"2026-04-19T05:36:34Z","timestamp":1776576994832,"version":"3.51.2"},"reference-count":70,"publisher":"MDPI AG","issue":"11","license":[{"start":{"date-parts":[[2018,11,13]],"date-time":"2018-11-13T00:00:00Z","timestamp":1542067200000},"content-version":"vor","delay-in-days":0,"URL":"https:\/\/creativecommons.org\/licenses\/by\/4.0\/"}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Symmetry"],"abstract":"<jats:p>The cosmic expansion phenomenon is being studied through the interaction of newly proposed dark energy models (Tsallis, R\u00e9nyi and Sharma-Mittal holographic dark energy (HDE) models) with cold dark matter in the framework of loop quantum cosmology. We investigate different cosmic implications such as equation of state parameter, squared sound speed and cosmological plane (\u03c9 d    -    \u03c9  d  \u2032    ,     \u03c9 d     and     \u03c9 d \u2032     represent the equation of state (EoS) parameter and its evolution, respectively). It is found that EoS parameter exhibits quintom like behavior of the universe for all three models of HDE. The squared speed of sound represents the stable behavior of R\u00e9nyi HDE and Sharma-Mittal HDE at the latter epoch while unstable behavior for Tsallis HDE. Moreover,     \u03c9 d    -    \u03c9  d  \u2032     plane lies in the thawing region for all three HDE models.<\/jats:p>","DOI":"10.3390\/sym10110635","type":"journal-article","created":{"date-parts":[[2018,11,14]],"date-time":"2018-11-14T10:58:22Z","timestamp":1542193102000},"page":"635","update-policy":"https:\/\/doi.org\/10.3390\/mdpi_crossmark_policy","source":"Crossref","is-referenced-by-count":61,"title":["Tsallis, R\u00e9nyi and Sharma-Mittal Holographic Dark Energy Models in Loop Quantum Cosmology"],"prefix":"10.3390","volume":"10","author":[{"ORCID":"https:\/\/orcid.org\/0000-0001-5249-803X","authenticated-orcid":false,"given":"Abdul","family":"Jawad","sequence":"first","affiliation":[{"name":"Department of Mathematics, COMSATS University Islamabad, Lahore Campus, Lahore-54000, Pakistan"}]},{"given":"Kazuharu","family":"Bamba","sequence":"additional","affiliation":[{"name":"Division of Human Support System, Faculty of Symbiotic Systems Science, Fukushima University, Fukushima 960-1296, Japan"}]},{"given":"Muhammad","family":"Younas","sequence":"additional","affiliation":[{"name":"Department of Mathematics, COMSATS University Islamabad, Lahore Campus, Lahore-54000, Pakistan"}]},{"given":"Saba","family":"Qummer","sequence":"additional","affiliation":[{"name":"Department of Mathematics, COMSATS University Islamabad, Lahore Campus, Lahore-54000, Pakistan"}]},{"given":"Shamaila","family":"Rani","sequence":"additional","affiliation":[{"name":"Department of Mathematics, COMSATS University Islamabad, Lahore Campus, Lahore-54000, Pakistan"}]}],"member":"1968","published-online":{"date-parts":[[2018,11,13]]},"reference":[{"key":"ref_1","doi-asserted-by":"crossref","first-page":"1009","DOI":"10.1086\/300499","article-title":"Observational evidence from supernovae for an accelerating Universe and a cosmological constant","volume":"116","author":"Riess","year":"1998","journal-title":"Astron. 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