2020
DOI: 10.48550/arxiv.2006.06291
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The cosmological constant of emergent spacetime in the Newtonian approximation

J. C. Castro-Palacio,
P. Fernandez de Cordoba,
J. M. Isidro

Abstract: We present a simple quantum-mechanical estimate of the cosmological constant of a Newtonian Universe. We first mimic the dynamics of a Newtonian spacetime by means of a nonrelativistic quantum mechanics for the matter contents of the Universe (baryonic and dark) within a fixed (i.e., nondynamical) Euclidean spacetime. Then we identify an operator that plays, on the matter states, a role analogous to that played by the cosmological constant. Finally we prove that there exists a quantum state for the matter fiel… Show more

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Cited by 4 publications
(19 citation statements)
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References 15 publications
(27 reference statements)
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“…In this article we present a toy model of Newtonian Universe in positively curved space, in which a certain repulsive force plays a role analogous to that played by the cosmological constant Λ in general relativity. This follows previous work by the same authors [7], where we have computed the cosmological constant of flat, Newtonian space. In the present paper we extend this previous analysis to the case of positive (but constant) scalar curvature, still within the limit of weak gravity.…”
Section: Introductionsupporting
confidence: 67%
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“…In this article we present a toy model of Newtonian Universe in positively curved space, in which a certain repulsive force plays a role analogous to that played by the cosmological constant Λ in general relativity. This follows previous work by the same authors [7], where we have computed the cosmological constant of flat, Newtonian space. In the present paper we extend this previous analysis to the case of positive (but constant) scalar curvature, still within the limit of weak gravity.…”
Section: Introductionsupporting
confidence: 67%
“…In this section we verify that the results obtained in S 3 correctly reduce to their counterparts in R 3 [5,7,9] as one lets R 0 → ∞.…”
Section: The Flat-space Limitsupporting
confidence: 60%
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