Spherically symmetric systems of fields and black holes. III. Positivity of energy and of a new type Euclidean action
Journal Article
·
· Phys. Rev. D; (United States)
Within the scope of the two-dimensional model of gravity which was defined and studied in the two preceding papers, we investigate the three famous positivity problems of general relativity: (1) energy, (2) Euclidean action, and (3) divergence identities. We show that the energy can be split in a unique way into a black-hole mass and a field energy. If there are no fields in the model which could discharge the hole, then the field energy itself is non-negative and has a zero minimum for the vacuum value of the fields. In the opposite case, the greatest lower bound for the total energy is the irreducible mass of the hole. We define a new type of Euclidean action for gravity theories, which is different from the action used currently in Euclidean quantum gravity. The new Euclidean action is obtained by a true analytical continuation of a reduced Lorentzian action so that the relation between the Euclidean and Lorentzian regimes is well defined. We prove that the new Euclidean action is positive definite without any additional ''complexification.'' We show that the possibility of gravitational collapse leads to an unusual, saturation-curve-like form, of the Hamiltonian and of the new Euclidean action.
- Research Organization:
- Institute for Theoretical Physics, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland
- OSTI ID:
- 6409473
- Journal Information:
- Phys. Rev. D; (United States), Journal Name: Phys. Rev. D; (United States) Vol. 30:6; ISSN PRVDA
- Country of Publication:
- United States
- Language:
- English
Similar Records
Black-hole thermodynamics and the Euclidean Einstein action
Black-hole uniqueness theorems in Euclidean quantum gravity
Journal Article
·
Mon Apr 14 23:00:00 EST 1986
· Phys. Rev. D; (United States)
·
OSTI ID:6060672
Black-hole uniqueness theorems in Euclidean quantum gravity
Journal Article
·
Wed Oct 15 00:00:00 EDT 1980
· Phys. Rev., D; (United States)
·
OSTI ID:5003895
Related Subjects
640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar
Radio & X-Ray Sources
657003 -- Theoretical & Mathematical Physics-- Relativity & Gravitation
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
BLACK HOLES
EINSTEIN FIELD EQUATIONS
EQUATIONS
EUCLIDEAN SPACE
FIELD EQUATIONS
FIELD THEORIES
GENERAL RELATIVITY THEORY
GRAVITATIONAL COLLAPSE
GRAVITATIONAL FIELDS
HAMILTONIANS
MATHEMATICAL OPERATORS
MATHEMATICAL SPACE
METRICS
QUANTUM FIELD THEORY
QUANTUM GRAVITY
QUANTUM OPERATORS
RIEMANN SPACE
SPACE
SPACE-TIME
SYMMETRY
Radio & X-Ray Sources
657003 -- Theoretical & Mathematical Physics-- Relativity & Gravitation
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
BLACK HOLES
EINSTEIN FIELD EQUATIONS
EQUATIONS
EUCLIDEAN SPACE
FIELD EQUATIONS
FIELD THEORIES
GENERAL RELATIVITY THEORY
GRAVITATIONAL COLLAPSE
GRAVITATIONAL FIELDS
HAMILTONIANS
MATHEMATICAL OPERATORS
MATHEMATICAL SPACE
METRICS
QUANTUM FIELD THEORY
QUANTUM GRAVITY
QUANTUM OPERATORS
RIEMANN SPACE
SPACE
SPACE-TIME
SYMMETRY