{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2025,10,12]],"date-time":"2025-10-12T04:30:24Z","timestamp":1760243424608,"version":"build-2065373602"},"reference-count":70,"publisher":"MDPI AG","issue":"3","license":[{"start":{"date-parts":[[2013,3,22]],"date-time":"2013-03-22T00:00:00Z","timestamp":1363910400000},"content-version":"vor","delay-in-days":0,"URL":"https:\/\/creativecommons.org\/licenses\/by\/3.0\/"}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Entropy"],"abstract":"<jats:p>Several models have been proposed to explain the dark energy that is causing universe expansion to accelerate. Here the acceleration predicted by the Holographic Dark Information Energy (HDIE) model is compared to the acceleration that would be produced by a cosmological constant. While identical to a cosmological constant at low redshifts, z &lt; 1, the HDIE model results in smaller Hubble parameter values at higher redshifts, z &gt; 1, reaching a maximum difference of 2.6 \u00b1 0.5% around z ~ 1.7. The next generation of dark energy measurements, both those scheduled to be made in space (ESA\u2019s Euclid and NASA\u2019s WFIRST missions) and those to be made on the ground (BigBOSS, LSST and Dark Energy Survey), should be capable of determining whether such a difference exists or not. In addition a computer simulation thought experiment is used to show that the algorithmic entropy of the universe always increases because the extra states produced by the accelerating expansion compensate for the loss of entropy from star formation.<\/jats:p>","DOI":"10.3390\/e15031135","type":"journal-article","created":{"date-parts":[[2013,3,22]],"date-time":"2013-03-22T12:44:31Z","timestamp":1363956271000},"page":"1135-1151","update-policy":"https:\/\/doi.org\/10.3390\/mdpi_crossmark_policy","source":"Crossref","is-referenced-by-count":5,"title":["Holographic Dark Information Energy: Predicted Dark  Energy Measurement"],"prefix":"10.3390","volume":"15","author":[{"given":"Michael","family":"Gough","sequence":"first","affiliation":[{"name":"Department of Engineering and Design, University of Sussex, Brighton, BN1 9QT, UK,"}]}],"member":"1968","published-online":{"date-parts":[[2013,3,22]]},"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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