Abstract

We discuss a possible link between the deformation parameter Theta ^{mu nu } arising in the framework of noncommutative geometry and the parameter beta of the generalized uncertainty principle (GUP). We compute the shift of the Hawking temperature induced by the Theta ^{mu nu }-deformed Schwarzschild geometry, and then we relate it to one obtained by GUP. Results suggest a granular structure of specetime at the Planck scales. The current bounds on beta allow to constraint the noncommutative parameter Theta ^{mu nu }.

Highlights

  • The possibility to describe spacetime in noncommutive frameworks was noted long time ago [1], and its interest renewed recently owing to the discovery of SeibergWitten map [2], which relates noncommutative to commutative gauge theories

  • By comparing the temperature (3.11) with the generalized uncertainty principle (GUP)-deformed Hawking temperature given by Eq (2.3), one obtains β

  • In this paper we have derived an upper bound on the deformation parameter Υ of the noncommutative geometry, by relating Υ to the coefficients β of GUP

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Summary

Introduction

The possibility to describe spacetime in noncommutive frameworks was noted long time ago [1], and its interest renewed recently owing to the discovery of SeibergWitten map [2], which relates noncommutative to commutative gauge theories. The general idea is to define the fields over phase space by replacing the ordinary product of fields with the GronewaldMoyal product and map (via the Seiberg-Witten) this theory in the equivalent commutative theory with expansion of the fields in terms of the noncommutative parameter This approach has been extensively used to study many gauge theories [22,23,24,25,26,27,28] (see [29,30,31,32]), and since gravity can be considered as a gauge theory, the commutative equivalent approach appears to be a promising formulation2 [33,48,62,63,64,65,66,67,68,69,70,71,72].

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GUP and Hawking temperature
Temperature from a μν-Schwarzschild metric
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Temperature shift from the deformed Schwarzschild metric
Conclusions
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