2006
DOI: 10.1016/j.nuclphysb.2006.07.009
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Comments on noncommutative gravity

Abstract: We study the possibility of obtaining noncommutative gravity dynamics from string theory in the Seiberg-Witten limit. We find that the resulting low-energy theory contains more interaction terms than those proposed in noncommutative deformations of gravity. The rôle of twisted diffeomorphisms in string theory is studied and it is found that they are not standard physical symmetries. It is argued that this might be the reason why twisted diffeomorphisms are not preserved by string theory in the low energy limit… Show more

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Cited by 110 publications
(156 citation statements)
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“…The electric (magnetic) charges there reduce the radius of otherwise S 2 and the effective radius can be expressed as h = r e ϕ(r) , where e ϕ(r) = e 2ϕ h − G N rr h 17) where the constant ϕ h is the value of ϕ at the event horizon r h . Then, the generic dS RN-like black hole geometry, to O(G N ) in the theory, is given by…”
Section: Spherically Symmetric Black Holesmentioning
confidence: 99%
“…The electric (magnetic) charges there reduce the radius of otherwise S 2 and the effective radius can be expressed as h = r e ϕ(r) , where e ϕ(r) = e 2ϕ h − G N rr h 17) where the constant ϕ h is the value of ϕ at the event horizon r h . Then, the generic dS RN-like black hole geometry, to O(G N ) in the theory, is given by…”
Section: Spherically Symmetric Black Holesmentioning
confidence: 99%
“…[1,2]). In this paper we would like to draw attention to interrelations between noncommutative quantum field theories and quantum groups [3].…”
mentioning
confidence: 99%
“…These solutions can thus be regarded as the first-order noncommutative contributions to full noncommutative Einstein-Maxwell pp-waves. To date, there are several extensions of noncommutative gravity [3,4,6,8], all of them sharing the property that corrections to the Einstein-Hilbert action start at order two in . Barring thus the eventuality that some specific symmetries might get lost through the coupling to a SW gauge field, our results do not depend on the particular model chosen for noncommutative gravity.…”
Section: Discussionmentioning
confidence: 99%
“…The first one is that Einstein gravity should remain applicable. This is justifiable since, as already mentioned, in more fundamental approaches [4,6] and in many deformation approaches [3,8] noncommutative corrections start at order two in . The second hypothesis is that noncommutative gravity modifications should already occur at order one in , since matter distributions from field theory classical actions receive contributions to this order.…”
Section: Introductionmentioning
confidence: 92%