Hamiltonian Approach to 2D Dilaton-Gravities and Invariant Adm Mass
arXiv:hep-th/9301119 · doi:10.1103/PhysRevD.47.5408
Abstract
The formula existing in the literature for the ADM mass of 2D dilaton gravity is incomplete. For example, in the case of an infalling matter shockwave this formula fails to give a time-independent mass, unless a very special coordinate system is chosen. We carefully carry out the canonical formulation of 2D dilaton gravity theories (classical, CGHS and RST). As in 4D general relativity one must add a boundary term to the bulk Hamiltonian to obtain a well-defined variational problem. This boundary term coincides with the numerical value of the Hamiltonian and gives the correct mass which obviously is time-independent.
revised, 12 pages, PUPT-1379; we added a reference and corrected some minor typos
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- Classical and quantum geometrodynamics of 2d vacuum dilatonic black holes
- Unitary Theory of Evaporating 2D Black Holes
- Predictability and Semiclassical Approximation at the onset of Black Hole formation
- Hamiltonian thermodynamics of two-dimensional vacuum dilatonic black holes
- Two Dimensional Quantum Dilaton Gravity and the Positivity of Energy
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- The No-Hair Conjecture in 2D Dilaton Supergravity
- Baby universes and energy (non-)conservation in (1+1)-dimensional dilaton gravity
- Canonical Structure of 2D Black Holes
- Two non-commutative parameters and regular cosmological phase transition in the semi-classical dilaton cosmology
- Black Hole Physics from Two Dimensional Dilaton Gravity based on Coset Model
- Quantum-Corrected Bondi Mass for 2D Hawking Radiation