An exact derivation of the Hawking effect in canonical formulation
arXiv:1707.03614 · doi:10.1103/PhysRevD.97.025016
Abstract
The Hawking effect is one of the most extensively studied topics in modern physics. Yet it remains relatively under-explored within the framework of canonical quantization. The key difficulty lies in the fact that the Hawking effect is principally understood using the relation between the ingoing modes which leave past null infinity and the outgoing modes which arrive at future null infinity. Naturally, these modes are described using advanced and retarded null coordinates instead of the usual Schwarzschild coordinates. However, null coordinates do not lead to a true Hamiltonian that describes the evolution of these modes. In order to overcome these hurdles in a canonical formulation, we introduce here a set of near-null coordinates which allows one to perform an exact Hamiltonian-based derivation of the Hawking effect. This derivation opens up an avenue to explore the Hawking effect using different canonical quantization methods such as polymer quantization.
arXiv comment11 pages, 3 figures, revtex4
References in corpus (27)
- Hawking Radiation as Tunneling
- Background Independent Quantum Gravity: A Status Report
- The Unruh effect and its applications
- Thermodynamical Aspects of Gravity: New insights
- Quantum gravity, shadow states, and quantum mechanics
- Essential and inessential features of Hawking radiation
- Black Hole Thermodynamics
- Quantum fields in curved spacetime
- Quantum Emission from Two-Dimensional Black Holes
- Complementarity of representations in quantum mechanics
- A Self-consistent Model of the Black Hole Evaporation
- Exercices de style: a homotopy theory for set theory, I
- Hawking radiation, Unruh radiation and the equivalence principle
- Do black holes radiate?
- Exact Hawking Radiation of Scalars, Fermions, and Bosons Using the Tunneling Method Without Back-Reaction
- The propagator in polymer quantum field theory
- Mass function and particle creation in Schwarzschild-de Sitter spacetime
- Black Holes: Eliminating Information or Illuminating New Physics?
- Hawking radiation of massive modes and undulations
- A quantum peek inside the black hole event horizon
- Quantum field theory in de Sitter and quasi-de Sitter spacetimes: Revisited
- Black hole kinematics: the "in"-vacuum energy density and flux for different observers
- Black holes and Hawking radiation in spacetime and its analogues
- Comment on Self-Consistent Model of Black Hole Formation and Evaporation
- Absence of Unruh effect in polymer quantization
- Hamiltonian analysis of the double null 2+2 decomposition of General Relativity expressed in terms of self-dual bivectors
- Transient response from Unruh-DeWitt detector along Rindler trajectory in polymer quantization
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- Quantum evolution of the Hawking state for black holes
- Schrödinger evolution of the Hawking state
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- Remarks on distinguishability of Schwarzschild spacetime and thermal Minkowski spacetime using Resonance Casimir-Polder interaction
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