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A Comment on Nadytko et al., “Amines in the Earth’s Atmosphere: A Density Functional Theory Study of the Thermochemistry of Pre-Nucleation Clusters”. Entropy 2011, 13, 554–569
Entropy 2011, 13(4), 924-935; doi:10.3390/e13040924

Holographic Dark Information Energy

Received: 11 February 2011 / Revised: 4 April 2011 / Accepted: 18 April 2011 / Published: 21 April 2011
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Abstract: Landauer’s principle and the Holographic principle are used to derive the holographic information energy contribution to the Universe. Information energy density has increased with star formation until sufficient to start accelerating the expansion of the universe. The resulting reduction in the rate of star formation due to the accelerated expansion may provide a feedback that limits the information energy density to a constant level. The characteristics of the universe’s holographic information energy then closely match those required to explain dark energy and also answer the cosmic coincidence problem. Furthermore the era of acceleration will be clearly limited in time.
Keywords: Landauer’s principle; holographic principle; dark energy; cosmology Landauer’s principle; holographic principle; dark energy; cosmology
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.

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MDPI and ACS Style

Gough, M.P. Holographic Dark Information Energy. Entropy 2011, 13, 924-935.

AMA Style

Gough MP. Holographic Dark Information Energy. Entropy. 2011; 13(4):924-935.

Chicago/Turabian Style

Gough, Michael Paul. 2011. "Holographic Dark Information Energy." Entropy 13, no. 4: 924-935.

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