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In this second part of our series of two papers, where spacetime is modelled by a graph, where Planck size quantum black holes lie on the vertices, we consider the thermodynamics of spacetime.
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S. W. Hawking, Commun. Math. Phys. 43
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R. M. Wald, General Relativity
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J. Mäkelä (First paper)
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P. K. Townsend, gr-qc/9707012
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J. Mäkelä and A. Peltola, gr-qc/0612078. (Accepted for publication in Int. J. Mod. Phys. D)
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The role of the cosmological constant in the present observations of dark energy has been discussed, for example, by R. Bean, S. Carroll and M. Trodden, astro-ph/0510059
Cited in the paper.
See, for instance, V. Husain and R. B. Mann, arXiv:0812.0399
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W. G. Unruh, Phys. Rev. D14
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T. Jacobson, Phys. Rev. Lett. 75
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For similar ideas, see T. Padmanabhan, Class. Quant. Grav. 21
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