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Violations of the Born rule in cool state-dependent horizons

Donald Marolf, Joseph Polchinski

TL;DR

This work analyzes state-dependent proposals for describing infalling observers at black hole horizons. It shows that making horizon observables nonlinear functions of the global state—enough to erase firewalls for typical states—inevitably induces large violations of the Born rule, with the dimensionality of near-horizon Hilbert spaces and energy-shift arguments driving the effect. A concrete, high-dimensional Hilbert-space construction demonstrates that almost all states in an excited sector map to internal excitations rather than vacuum, making the Born-rule departures, in principle, observable by infalling observers. The authors argue the result is general across state-dependent schemes, underscoring significant conflicts between such proposals and the standard framework of quantum mechanics, while acknowledging that resolving these tensions requires further, careful theoretical work, including how to yield definite interior predictions.

Abstract

The black hole information problem has motivated many proposals for new physics. One idea, known as state-dependence, is that quantum mechanics must be generalized to describe the physics of black holes, and that fixed linear operators do not provide the fundamental description of experiences for infalling observers. Instead, such experiences are to be described by operators with an extra dependence on the global quantum state. We show that any implementation of this idea strong enough to remove firewalls from generic states requires massive violations of the Born rule. We also demonstrate a sense in which such violations are visible to infalling observers involved in preparing the initial state of the black hole. We emphasize the generality of our results; no details of any specific proposal for state-dependence are required.

Violations of the Born rule in cool state-dependent horizons

TL;DR

This work analyzes state-dependent proposals for describing infalling observers at black hole horizons. It shows that making horizon observables nonlinear functions of the global state—enough to erase firewalls for typical states—inevitably induces large violations of the Born rule, with the dimensionality of near-horizon Hilbert spaces and energy-shift arguments driving the effect. A concrete, high-dimensional Hilbert-space construction demonstrates that almost all states in an excited sector map to internal excitations rather than vacuum, making the Born-rule departures, in principle, observable by infalling observers. The authors argue the result is general across state-dependent schemes, underscoring significant conflicts between such proposals and the standard framework of quantum mechanics, while acknowledging that resolving these tensions requires further, careful theoretical work, including how to yield definite interior predictions.

Abstract

The black hole information problem has motivated many proposals for new physics. One idea, known as state-dependence, is that quantum mechanics must be generalized to describe the physics of black holes, and that fixed linear operators do not provide the fundamental description of experiences for infalling observers. Instead, such experiences are to be described by operators with an extra dependence on the global quantum state. We show that any implementation of this idea strong enough to remove firewalls from generic states requires massive violations of the Born rule. We also demonstrate a sense in which such violations are visible to infalling observers involved in preparing the initial state of the black hole. We emphasize the generality of our results; no details of any specific proposal for state-dependence are required.

Paper Structure

This paper contains 7 sections, 24 equations, 1 figure.

Figures (1)

  • Figure 1: a) States with energy $E < E_0$. Atypical states, which are not in the infalling vacuum, are indicated by the small subregion. b) The image under a unitary $U$. States outside the subregion are excited. c) The states from (b) projected down to $E < E_+$. Rare states whose projection is not close to the identity are represented by the second hole. d) States with energy $E < E_+$, almost all of which are nearly parallel to excited states. The parametrically rare exceptions are those that project to the two subregions in (c), and those that are not close to the subspace in (c).