Entropy 2013, 15(3), 1135-1151; doi:10.3390/e15031135

Holographic Dark Information Energy: Predicted Dark Energy Measurement

Received: 17 January 2013; in revised form: 11 March 2013 / Accepted: 19 March 2013 / Published: 22 March 2013
This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Abstract: 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 < 1, the HDIE model results in smaller Hubble parameter values at higher redshifts, z > 1, reaching a maximum difference of 2.6 ± 0.5% around z ~ 1.7. The next generation of dark energy measurements, both those scheduled to be made in space (ESA’s Euclid and NASA’s 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.
Keywords: Landauer’s principle; Holographic principle; dark energy experiments; dark energy theory; cosmological constant experiments
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MDPI and ACS Style

Gough, M.P. Holographic Dark Information Energy: Predicted Dark Energy Measurement. Entropy 2013, 15, 1135-1151.

AMA Style

Gough MP. Holographic Dark Information Energy: Predicted Dark Energy Measurement. Entropy. 2013; 15(3):1135-1151.

Chicago/Turabian Style

Gough, Michael P. 2013. "Holographic Dark Information Energy: Predicted Dark Energy Measurement." Entropy 15, no. 3: 1135-1151.

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