{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2026,3,1]],"date-time":"2026-03-01T19:30:22Z","timestamp":1772393422647,"version":"3.50.1"},"reference-count":64,"publisher":"MDPI AG","issue":"4","license":[{"start":{"date-parts":[[2019,4,8]],"date-time":"2019-04-08T00:00:00Z","timestamp":1554681600000},"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>In this paper, we reconstruct various solutions for the accelerated universe in the Einstein-Aether theory of gravity. For this purpose, we obtain the effective density and pressure for Einstein-Aether theory. We reconstruct the Einstein-Aether models by comparing its energy density with various newly proposed holographic dark energy models such as Tsallis, R\u00e9nyi and Sharma-Mittal. For this reconstruction, we use two forms of the scale factor, power-law and exponential forms. The cosmological analysis of the underlying scenario has been done by exploring different cosmological parameters. This includes equation of state parameter, squared speed of sound and evolutionary equation of state parameter via graphical representation. We obtain some favorable results for some values of model parameters<\/jats:p>","DOI":"10.3390\/sym11040509","type":"journal-article","created":{"date-parts":[[2019,4,8]],"date-time":"2019-04-08T11:54:52Z","timestamp":1554724492000},"page":"509","update-policy":"https:\/\/doi.org\/10.3390\/mdpi_crossmark_policy","source":"Crossref","is-referenced-by-count":22,"title":["Cosmological Consequences of New Dark Energy Models in Einstein-Aether Gravity"],"prefix":"10.3390","volume":"11","author":[{"given":"Shamaila","family":"Rani","sequence":"first","affiliation":[{"name":"Department of Mathematics, COMSATS University Islamabad, Lahore-Campus, Lahore 54000, Pakistan"}]},{"ORCID":"https:\/\/orcid.org\/0000-0001-5249-803X","authenticated-orcid":false,"given":"Abdul","family":"Jawad","sequence":"additional","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":"Irfan Ullah","family":"Malik","sequence":"additional","affiliation":[{"name":"Allied School, Ali Campus, Muhafiz Town Canal Road, Lahore 54000, Pakistan"}]}],"member":"1968","published-online":{"date-parts":[[2019,4,8]]},"reference":[{"key":"ref_1","doi-asserted-by":"crossref","first-page":"330","DOI":"10.1088\/0067-0049\/180\/2\/330","article-title":"Five-year Wilkinson Microwave Anisotropy probe Observations: Cosmological Interpretation","volume":"180","author":"Komatsu","year":"2009","journal-title":"Astrophys. 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