By B.J. West
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The vacuum state of quantum gravity contains large virtual masses. 24, pp. 1899-1909 Modanese, G. & Junker T. (2008). Conditions for stimulated emission in anomalous gravity-superconductors interactions. N. K. s), 245-269, Nova Publishers, Hauppauge, USA Modanese, G. (2011) Quantum Gravity Evaluation of Stimulated Graviton Emission in Superconductors. In: Gravity-Superconductors Interaction: Theory and Experiment, G. A. s), Ch. O. W. (1974). 10, p. 2345 Niedermaier M. & Reuter M. (2006). 9, p. 5 Novello, M.
32] dubbed “S–duality", is generalized in Section 5 to our topological supergravity model. In Section 6 and in an Outlook, we consider the still speculative applicability of this model to the * Permanent address: Departamento de Física, Facultad de Ciencias, Universidad del Zulia, Venezuela 38 2 Quantum Gravity Will-be-set-by-IN-TECH ϑα Γα Tα Rαβ Σα ταβ ηα objects vector vector vector bivector vector bivector vector components n2 n2 n2 (n − 1)/2 n2 (n − 1)2 /4 n2 n2 (n − 1)/2 n2 p-forms 1 1 2 2 n−1 n−1 n−1 n=4 16 16 24 36 16 24 16 3 9 9 9 9 9 9 9 2 1 1 2 1 4 2 4 Table 1.
If we expand the Feynman propagator in four-momentum space, we can see which energies and momenta are exchanged. One first finds T /2 T /2 1 e ipr iE( t1 t2 ) dt1 dt2 dE d 3 p 2 2 T T E p i T /2 T /2 U (r ) Gm1m2 lim (43) Changing variables to (t1+t2), (t1-t2) we find that the integral in (t1+t2) cancels the factor 1/T. e. s (43) and (44) we use natural units h/2=c=1). Finally we have 22 Quantum Gravity U ( r ) Gm1m2 d 3 p sin p ' 2Gm1m2 eipr dp ' p' r 0 p2 (44) with p ' p r .