SEMICLASSICAL GRAVITY IN 1+1 DIMENSIONS

被引：97

作者：

MANN, RB ^{[1
]}

MORSINK, SM ^{[1
]}

SIKKEMA, AE ^{[1
]}

STEELE, TG ^{[1
]}

机构：

[1] UNIV WESTERN ONTARIO,DEPT PHYS,LONDON N6A 2E2,ONTARIO,CANADA

来源：

PHYSICAL REVIEW D | 1991年 / 43卷 / 12期

关键词：

D O I：

10.1103/PhysRevD.43.3948

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Relativistic wave equations are solved exactly in the classical space-time background of a two-dimensional gravitational theory. In the simplest nontrivial geometry without horizons, the solutions are necessarily bound states and the constraints on the energy eigenvalues are determined. Aspects of quantum field theory in the background of the (1 + 1)-dimensional black hole are also examined.

引用

页码：3948 / 3957

页数：10

共 37 条

[1]

Abramowitz M.., 1972, HDB MATH FUNCTIONS

[2]

[Anonymous], 1996, TABLES INTEGRALS SER

[3] 3-DIMENSIONAL CLASSICAL SPACETIMES [J].

BARROW, JD ;

BURD, AB ;

LANCASTER, D .

CLASSICAL AND QUANTUM GRAVITY, 1986, 3 (04) :551-567

[4]

Birrell N. D., 1982, Quantum fields in curved space

[5] QUANTUM FIELD-THEORY IN SCHWARZSCHILD AND RINDLER SPACES [J].

BOULWARE, DG .

PHYSICAL REVIEW D, 1975, 11 (06) :1404-1423

[6] SPIN-1/2 QUANTUM FIELD-THEORY IN SCHWARZSCHILD SPACE [J].

BOULWARE, DG .

PHYSICAL REVIEW D, 1975, 12 (02) :350-367

[7] BLACK-HOLES IN 2 SPACETIME DIMENSIONS [J].

BROWN, JD ;

HENNEAUX, M ;

TEITELBOIM, C .

PHYSICAL REVIEW D, 1986, 33 (02) :319-323

[8] TRACE ANOMALIES AND HAWKING EFFECT [J].

CHRISTENSEN, SM ;

FULLING, SA .

PHYSICAL REVIEW D, 1977, 15 (08) :2088-2104

[9] THERMODYNAMICS OF BLACK-HOLES [J].

DAVIES, PCW .

REPORTS ON PROGRESS IN PHYSICS, 1978, 41 (08) :1313-1355

[10] QUANTUM-MECHANICS IN CURVED SPACE [J].

DONOGHUE, JF ;

HOLSTEIN, BR .

AMERICAN JOURNAL OF PHYSICS, 1986, 54 (09) :827-831

← 1 2 3 4 →