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Causality Problem in a Holographic Dark Energy Model

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arxiv 1208.3729 v1 pith:KAI6J6HF submitted 2012-08-18 gr-qc astro-ph.COhep-th

Causality Problem in a Holographic Dark Energy Model

classification gr-qc astro-ph.COhep-th
keywords problemcausalitycirculardarkenergyequationeventfuture
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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In the model of holographic dark energy, there is a notorious problem of circular reasoning between the introduction of future event horizon and the accelerating expansion of the universe. We examine the problem after dividing into two parts, the causality problem of the equation of motion and the circular logic on the use of the future event horizon. We specify and isolate the root of the problem from causal equation of motion as a boundary condition, which can be determined from the initial data of the universe. We show that there is no violation of causality if it is defined appropriately and the circular logic problem can be reduced to an initial value problem.

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    For generalized-entropy holographic dark energy with a future-event-horizon cutoff, the phantom-divide crossing on the kinematic branch is unique, quintessence-to-phantom, and fixes the local entropy-scaling dimension...