Tensile Strength and the Mining of Black Holes
arXiv:1207.3342 · doi:10.1103/PhysRevLett.111.211301
Abstract
There are a number of important thought experiments that involve raising and lowering boxes full of radiation in the vicinity of black hole horizons. This paper looks at the limitations placed on these thought experiments by the null energy condition, which imposes a fundamental bound on the tensile-strength-to-weight ratio of the materials involved, makes it impossible to build a box near the horizon that is wider than a single wavelength of the Hawking quanta and puts a severe constraint on the operation of 'space elevators' near black holes. In particular, it is shown that proposals for mining black holes by lowering boxes near the horizon, collecting some Hawking radiation and dragging it out to infinity cannot proceed nearly as rapidly as has previously been claimed and that as a consequence of this limitation the boxes and all the moving parts are superfluous and black holes can be destroyed equally rapidly by threading the horizon with strings.
arXiv comment23 pages
References in corpus (15)
- Black Holes: Complementarity or Firewalls?
- Black Holes Radiate Mainly on the Brane
- String Theory and the Principle of Black Hole Complementarity
- Brownian motion in AdS/CFT
- Black Hole Evaporation along Macroscopic Strings
- Light-sheets and Bekenstein's bound
- Non-Archimedean character of quantum buoyancy and the generalized second law of thermodynamics
- Propagation of perturbations along strings
- The bound on viscosity and the generalized second law of thermodynamics
- Stability of strings binding heavy-quark mesons
- Mining Energy from a Black Hole by Strings
- Perfect mirrors and the self-accelerating box paradox
- Thorny Spheres and Black Holes with Strings
- Aspects of open strings in Rindler Space
- The Catenary Revisited: From Newtonian Strings to Superstrings
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- Jerusalem Lectures on Black Holes and Quantum Information
- Complementarity Is Not Enough
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- Nonviolent information transfer from black holes: a field theory parameterization
- Event Horizon Telescope Observations as Probes for Quantum Structure of Astrophysical Black Holes
- Nonviolent unitarization: basic postulates to soft quantum structure of black holes
- Violations of the Born rule in cool state-dependent horizons
- Firewalls From Double Purity
- Spacetime and Universal Soft Modes --- Black Holes and Beyond
- Effective field theory models for nonviolent information transfer from black holes
- An Uneventful Horizon in Two Dimensions
- The Black Hole Interior in Quantum Gravity
- The Smeared Null Energy Condition
- Reanalyzing an Evaporating Black Hole
- Statistical physics of black holes as quantum-mechanical systems
- Energy and Information Near Black Hole Horizons
- Firewalls and flat mirrors: An alternative to the AMPS experiment which evades the Harlow-Hayden obstacle
- Black Hole and de Sitter Microstructures from a Semiclassical Perspective
- Cold Black Holes in the Harlow-Hayden Approach to Firewalls
- Black Holes, Entropies, and Semiclassical Spacetime in Quantum Gravity
- Why Firewalls Need Not Exist
- Dynamical obstruction to perpetual motion from Lorentz-violating black holes
- Relativeness in Quantum Gravity: Limitations and Frame Dependence of Semiclassical Descriptions
- Complementarity + Back-reaction is enough
- Extracting Hawking Radiation Near the Horizon of AdS Black Holes
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