Abstract

Pure states in quantum field theory can be represented by many-fingered block-time wave functions, which treat time on an equal footing with space and make the notions of “time evolution” and “state at a given time” fundamentally irrelevant. Instead of information destruction resulting from an attempt to use a “state at a given time” to describe semi-classical black-hole evaporation, the full many-fingered block-time wave function of the universe conserves information by describing the correlations of outgoing Hawking particles in the future with ingoing Hawking particles in the past.

Highlights

  • The semi-classical description of black-hole evaporation [1] predicts that the final state after the complete evaporation cannot be represented by a pure state [2]

  • We start with the observation that all these previous approaches share one common assumption: that the quantum state should be a function of time, or more generally, a functional of the spacelike hypersurface

  • One of the main messages of the theory of relativity is that time should be treated on an equal footing with space

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Summary

Introduction

The semi-classical description of black-hole evaporation [1] predicts that the final state after the complete evaporation cannot be represented by a pure state [2]. Many approaches to restore a pure-state description at late times have been attempted, but none of them seems to be completely satisfying (for reviews see, e.g., [4]) To overcome this problem, we start with the observation that all these previous approaches (with a notable exception in [5]) share one common assumption: that the quantum state (either pure or mixed) should be a function of time, or more generally, a functional of the spacelike hypersurface. We start with the observation that all these previous approaches (with a notable exception in [5]) share one common assumption: that the quantum state (either pure or mixed) should be a function of time, or more generally, a functional of the spacelike hypersurface Such an assumption is deeply rooted in our intuitive understanding of the concept of time, according to which universe evolves with time.

Treating time in QM on an equal footing with space
Implications on unitarity of Hawking evaporation
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