Bekenstein Bound of Information Number N and its Relation to Cosmological Parameters in a Universe with and without Cosmological Constant
Ioannis Haranas, Ioannis Gkigkitzis

TL;DR
This paper explores the Bekenstein bound on information in the universe, deriving relations between cosmological parameters and information content, and finds that the universe's total information is approximately 10^122, regardless of the presence of a cosmological constant.
Contribution
The paper derives two bounds on the information number for universes with and without a cosmological constant and relates these bounds to cosmological parameters and total mass.
Findings
The information number N is approximately 10^122 for both universe types.
The total mass of the universe scales as the square root of N.
In self-gravitating systems, N relates to kinetic and thermal energies.
Abstract
Bekenstein has obtained is an upper limit on the entropy S, and from that, an information number bound N is deduced. In other words, this is the information contained within a given finite region of space that includes a finite amount of energy. Similarly, this can be thought as the maximum amount of information required to perfectly describe a given physical system down to its quantum level. If the energy and the region of space are finite then the number of information N required in describing the physical system is also finite. In this short letter two information number bounds are derived and compared for two types of universe. First, a universe without a cosmological constant lamda and second a universe with a cosmological constant lamda are investigated. This is achieved with the derivation of two different relations that connect the Hubble constant and cosmological constants to…
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