Presentation is loading. Please wait.

Presentation is loading. Please wait.

Gerard ’t Hooft Berlin November 1, 2007 Utrecht University of the.

Similar presentations


Presentation on theme: "Gerard ’t Hooft Berlin November 1, 2007 Utrecht University of the."— Presentation transcript:

1

2 Gerard ’t Hooft Berlin November 1, 2007 Utrecht University of the

3 How do we reconcile these with LOCALITY? paradox Black Holes require new axioms for the quantization of gravity Unitarity, Causality,... paradox Black Hole Quantum Coherence is realized in String/Membrane Theories ! -- at the expense of locality? -- How does Nature process information ?

4 The physical description of the difficulty...

5 horizon Here, gravitational interactions become strong !! brick wall

6 interaction horizon

7 b By taking back reaction into account, one can obtain a unitary scattering matrix

8 Gravitational effect from ingoing objects particles out in

9

10 Strategy: infinitesimal modification of in-state

11 a string theory amplitude !!nearly Repeat procedure:

12 The string world-sheet

13 Black Hole Formation & Evaporation by Closed Strings

14 Horizon Algebra

15 BLACK HOLE WHITE HOLE A black hole is a quantum superposition of white holes and vice versa !! The Difference between

16 very early very late in out S-matrix Ansatz: Qu. Gr. gives us a boundary condition here But, our algebra does not generate the area law. Can we be more precise? Transverse gravity? Now, let us look at the contributions from the Standard Model Scale

17 It all happens at the origin of Rindler Space

18 2-d surface

19 The Standard Model Contribution to the Horizon Algebra. I. The U (1) field

20

21 The role of the Standard Model’s scalar fields

22 Scalar field acts as quantum hair It generates a modification in the vector field equations:

23 are as their (Euclidean) quantum exp. values The average values of the scalar fields:

24 Questions: - What is the effect of Standard Model fermions ? - How do we handle non-Abelian vectors ? - What is the effect of the instanton angle  ? - What modifications of the algebra are generated by the transverse grav. force ? - Does this allow for a representation of the algebra with discrete states, as suggested by the entropy – area law?

25 A related question that we can answer: What is the effect of magnetic monopoles ? arg has a Dirac string - ambiguity 2  n N S

26

27 A non-Abelian gauge theory may now be treated in its Cartan subalgebra, where the diagonal components of electric and magnetic charges are well-defined.

28 Particles and horizons, the hybrid picture

29 We intend to obtain the complete algebra relating the in-operators to the out-operators from whatever Standard Model Lagrangian. Once the rules are clear, we should be able once again to add (transversal) gravity. The representation of our algebra should then respect the entropy / area law. The algebra should generate the details of quantum black hole dynamics. “The black Hole Horizon as a Dynamical System”, Int.J.Mod.Phys. D15 (2006) 1587 earlier version: gr-qc/0504120


Download ppt "Gerard ’t Hooft Berlin November 1, 2007 Utrecht University of the."

Similar presentations


Ads by Google