scholarly journals Notes on “Quantum Gravity” and Noncommutative Geometry

Author(s):  
J.M. Gracia-Bondía
2011 ◽  
Vol 28 (7) ◽  
pp. 075014 ◽  
Author(s):  
Johannes Aastrup ◽  
Jesper Møller Grimstrup ◽  
Mario Paschke

2005 ◽  
Vol 20 (17n18) ◽  
pp. 1315-1326 ◽  
Author(s):  
PIERRE MARTINETTI

We give a brief account of the description of the standard model in noncommutative geometry as well as the thermal time hypothesis, questioning their relevance for quantum gravity.


2011 ◽  
Vol 302 (3) ◽  
pp. 675-696 ◽  
Author(s):  
Johannes Aastrup ◽  
Jesper Møller Grimstrup ◽  
Mario Paschke ◽  
Ryszard Nest

2006 ◽  
Vol 21 (08) ◽  
pp. 639-647 ◽  
Author(s):  
CHONG-SUN CHU ◽  
OLAF LECHTENFELD

By considering a new form of dimensional reduction for noncommutative field theory, we show that the signature of spacetime may be changed. In particular, it is demonstrated that a temporal dimension can emerge from a purely Euclidean geometry. We suggest that this mechanism may hint at the origin of time in the fundamental theory of quantum gravity.


2009 ◽  
Vol 24 (15) ◽  
pp. 2792-2801 ◽  
Author(s):  
PIERRE MARTINETTI

We question the notion of line element in some quantum spaces that are expected to play a role in quantum gravity, namely noncommutative deformations of Minkowski spaces. We recall how the implementation of the Leibniz rule forbids to see some of the infinitesimal deformed Poincaré transformations as good candidates for Noether symmetries. Then we recall the more fundamental view on the line element proposed in noncommutative geometry, and re-interprete at this light some previous results on Connes' distance formula.


2019 ◽  
Vol 97 (5) ◽  
pp. 562-565
Author(s):  
Cuibai Luo ◽  
Chen Wu

Noncommutative geometry may be an alternative way to quantum gravity. We study the influence of the space–time noncommutative parameter on the Dirac quasi-normal modes in the noncommutative Schwarzschild black hole space–times. In comparison to the commutative Schwarzschild black hole, the numerical results show that the oscillation frequencies and magnitude of the imaginary part of the Dirac quasi-normal modes will increase. However, it is found that the influence of the space–time noncommutative parameter on the Dirac quasi-normal modes is tiny and negligible.


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