Authors: Yong Bao
We consider the relationship between energy density and its entropy density and the temperature of the Schwarzschild black hole (SBH) and holographic dark energy (HDE). On the basis of the literature [8], when the distance ε from the film to the horizon and the film thickness δ are constant, we obtain the energy density of the scalar field of SBH proportional to the square of the Hawking-Unruh temperature outside the event horizon. When ε and n are constant, their entropy density is proportional to the Hawking-Unruh temperature. On the basis of [16], we find the gravity energy density equation inside SBH; it is derived that the gravity energy density inside the SBH away from the event horizon is proportional to the square of effective temperature, whether the gravitational field of SBH is Coulomb-like or wavy-like; their entropy density is proportional to the effective temperature. Based on [20-22], we obtain a density of HDE proportional to the square of the Gibbons-Hawking temperature, which is proportional to the Gibbons-Hawking temperature. These equations are similar and have a relationship to each other. We suggest these relationships being interesting and important for SBH and HDE.
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[v1] 2014-09-23 03:25:37
[v2] 2014-10-21 01:24:37
[v3] 2015-01-08 19:06:37
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