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Falling into a black hole

Samir D. Mathur

Abstract

String theory tells us that quantum gravity has a dual description as a field theory (without gravity). We use the field theory dual to ask what happens to an object as it falls into the simplest black hole: the 2-charge extremal hole. In the field theory description the wavefunction of a particle is spread over a large number of `loops', and the particle has a well-defined position in space only if it has the same `position' on each loop. For the infalling particle we find one definition of `same position' on each loop, but there is a different definition for outgoing particles and no canonical definition in general in the horizon region. Thus the meaning of `position' becomes ill-defined inside the horizon.

Falling into a black hole

Abstract

String theory tells us that quantum gravity has a dual description as a field theory (without gravity). We use the field theory dual to ask what happens to an object as it falls into the simplest black hole: the 2-charge extremal hole. In the field theory description the wavefunction of a particle is spread over a large number of `loops', and the particle has a well-defined position in space only if it has the same `position' on each loop. For the infalling particle we find one definition of `same position' on each loop, but there is a different definition for outgoing particles and no canonical definition in general in the horizon region. Thus the meaning of `position' becomes ill-defined inside the horizon.

Paper Structure

This paper contains 13 equations, 5 figures.

Figures (5)

  • Figure 1: Field theory states
  • Figure 2: Gravity solutions for different microstates
  • Figure 3: Evolution in the classical state 1(a), 2(a).
  • Figure 4: The state $\Psi_{in}$; the excitations have moved the same distance on each loop
  • Figure 5: The state $\Psi_{out}$