NowJorge Pullin at Louisiana State University and Rodolfo Gambini at the University of the Republic in Montevideo Uruguay, have applied LQG on a much smaller scale--to an individual black hole--in the hope of removing that singularity too. To simplify things, the pair applied the equations of LQG to a model of a spherically symmetrical, non-rotating "Schwarzschild" black hole. In this new model, the gravitational field still increases as one nears the black hole's core.
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