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... (+,-), non-singular – intrinsic time and R radial coordinate time are monotonic function of each other. (2) Black holes are elementary particles in superspce. (3) The boundary of the Rindler wedge corresponds to physical horizons and singularities of Black Holes. (4) Hamilton_Jacboi semi-classical l ...
... (+,-), non-singular – intrinsic time and R radial coordinate time are monotonic function of each other. (2) Black holes are elementary particles in superspce. (3) The boundary of the Rindler wedge corresponds to physical horizons and singularities of Black Holes. (4) Hamilton_Jacboi semi-classical l ...