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Noncommutative Inspired Black Holes in Extra Dimensions

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arxiv hep-ph/0606051 v2 pith:ZJCECQ4S submitted 2006-06-05 hep-ph gr-qchep-th

classification hep-phgr-qchep-th
keywords blackdimensionsextraholenoncommutativescaleapproachenergy
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

In a recent string theory motivated paper, Nicolini, Smailagic and Spallucci (NSS) presented an interesting model for a noncommutative inspired, Schwarzschild-like black hole solution in 4-dimensions. The essential effect of having noncommutative co-ordinates in this approach is to smear out matter distributions on a scale associated with the turn-on of noncommutativity which was taken to be near the 4-d Planck mass. In particular, NSS took this smearing to be essentially Gaussian. This energy scale is sufficiently large that in 4-d such effects may remain invisible indefinitely. Extra dimensional models which attempt to address the gauge hierarchy problem, however, allow for the possibility that the effective fundamental scale may not be far from $\sim$ 1 TeV, an energy regime that will soon be probed by experiments at both the LHC and ILC. In this paper we generalize the NSS model to the case where flat, toroidally compactified extra dimensions are accessible at the Terascale and examine the resulting modifications in black hole properties due to the existence of noncommutativity. We show that while many of the noncommutativity-induced black hole features found in 4-d by NSS persist, in some cases there can be significant modifications due the presence of extra dimensions. We also demonstrate that the essential features of this approach are not particularly sensitive to the Gaussian nature of the smearing employed by NSS.

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Cited by 1 Pith paper

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  1. On the consistency of non-commutative geometry inspired Reissner-Nordstr\"{o}m black hole solution

    gr-qc 2025-07 conditional novelty 6.0 of 10

    The smeared-charge Reissner-Nordström metric used in noncommutative black hole papers is not a full solution of Einstein's equations unless the electromagnetic stress tensor is modified by hand.

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