Quantum Gravity

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INTERNATIONAL SERIESOFMONOGRAPHS ON PHYSICSSERIES EDITORSJ. BIRMAN CITY UNIVERSITY OF NEW YORKS. F. EDWARDS UNIVERSITY OF CAMBRIDGER. FRIEND UNIVERSITY OF CAMBRIDGEM. REES UNIVERSITY OF CAMBRIDGED. SHERRINGTON UNIVERSITY OF OXFORDG. VENEZIANO CERN, GENEVA
Page 4: International Series of Monographs
Page 8: 3Great Clarendon Street, Oxford OX2
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Page 16: viiiPrefaceIt is clear that my book
Page 20: xCONTENTS4.2.2 Hamiltonian form of
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Page 28: 2 WHY QUANTUM GRAVITY?fundamental f
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14 WHY QUANTUM GRAVITY?1.1.5 Quantu
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16 WHY QUANTUM GRAVITY?In this sens
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18 WHY QUANTUM GRAVITY?Writing agai
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20 WHY QUANTUM GRAVITY?If one makes
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22 WHY QUANTUM GRAVITY?It is shown
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24 WHY QUANTUM GRAVITY?is assumed t
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26 COVARIANT APPROACHES TO QUANTUM
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74 PARAMETRIZED AND RELATIONAL SYST
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4HAMILTONIAN FORMULATION OF GENERAL
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100 HAMILTONIAN FORMULATION OF GENE
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THE 3+1 DECOMPOSITION OF GENERAL RE
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CANONICAL GRAVITY WITH CONNECTIONS
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5QUANTUM GEOMETRODYNAMICS5.1 The pr
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THE PROGRAMME OF CANONICAL QUANTIZA
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THE PROBLEM OF TIME 137parameter (a
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THE PROBLEM OF TIME 139One can deri
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THE PROBLEM OF TIME 141The main pro
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THE PROBLEM OF TIME 143∫ ∏〈Ψ
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THE GEOMETRODYNAMICAL WAVE FUNCTION
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THE SEMICLASSICAL APPROXIMATION 165
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6QUANTUM GRAVITY WITH CONNECTIONS A
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CONNECTION AND LOOP VARIABLES 183h
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CONNECTION AND LOOP VARIABLES 185«
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CONNECTION AND LOOP VARIABLES 187
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QUANTIZATION OF AREA 189S and S ′
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∫Ê i [S]U[A, α] =−8πβiQUANT
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QUANTIZATION OF AREA 193(and higher
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QUANTUM HAMILTONIAN CONSTRAINT 195i
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Furthermore, one can show thatQUANT
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7QUANTIZATION OF BLACK HOLES7.1 Bla
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BLACK-HOLE THERMODYNAMICS AND HAWKI
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CANONICAL QUANTIZATION OF THE SCHWA
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BLACK-HOLE SPECTROSCOPY AND ENTROPY
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BLACK-HOLE SPECTROSCOPY AND ENTROPY
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QUANTUM THEORY OF COLLAPSING DUST S
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THE LEMAîTRE-TOLMAN-BONDI MODEL 22
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THE INFORMATION-LOSS PROBLEM 237bla
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PRIMORDIAL BLACK HOLES 239time of m
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PRIMORDIAL BLACK HOLES 241Table 7.2
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8QUANTUM COSMOLOGY8.1 Minisuperspac
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MINISUPERSPACE MODELS 245The usual
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MINISUPERSPACE MODELS 247Integratin
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MINISUPERSPACE MODELS 249term which
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MINISUPERSPACE MODELS 251boundary c
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MINISUPERSPACE MODELS 253( )∂2Ĥ
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MINISUPERSPACE MODELS 255Ψ=A(a, φ
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MINISUPERSPACE MODELS 257flat (for
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INTRODUCTION OF INHOMOGENEITIES 259
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INTRODUCTION OF INHOMOGENEITIES 261
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BOUNDARY CONDITIONS 263as artificia
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BOUNDARY CONDITIONS 265decided by a
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BOUNDARY CONDITIONS 267a’’00000
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BOUNDARY CONDITIONS 269does ‘outg
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BOUNDARY CONDITIONS 271Information
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LOOP QUANTUM COSMOLOGY 273construct
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LOOP QUANTUM COSMOLOGY 275obeying
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LOOP QUANTUM COSMOLOGY 277(V µ+5δ
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9STRING THEORY9.1 General introduct
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GENERAL INTRODUCTION 281The quantit
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GENERAL INTRODUCTION 283as the usua
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QUANTUM-GRAVITATIONAL ASPECTS 285ma
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QUANTUM-GRAVITATIONAL ASPECTS 287·
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QUANTUM-GRAVITATIONAL ASPECTS 289S
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QUANTUM-GRAVITATIONAL ASPECTS 291ac
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QUANTUM-GRAVITATIONAL ASPECTS 293an
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QUANTUM-GRAVITATIONAL ASPECTS 295cf
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QUANTUM-GRAVITATIONAL ASPECTS 297Wh
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QUANTUM-GRAVITATIONAL ASPECTS 299th
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QUANTUM-GRAVITATIONAL ASPECTS 301Th
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QUANTUM-GRAVITATIONAL ASPECTS 303th
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QUANTUM-GRAVITATIONAL ASPECTS 305´
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10QUANTUM GRAVITY AND THE INTERPRET
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DECOHERENCE AND THE QUANTUM UNIVERS
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ARROW OF TIME 319Kiefer et al. (199
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ARROW OF TIME 321to understand the
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ARROW OF TIME 323these variables (
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OUTLOOK 325observable universe were
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REFERENCESAchúcarro, A. and Townse
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REFERENCES 329Barceló, C., Liberat
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REFERENCES 331(ed. D. Howard and J.
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REFERENCES 333to quantum (ed. J. Eh
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REFERENCES 335New York.DeWitt, B. S
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REFERENCES 337Fredenhagen, K. and H
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REFERENCES 339quantum conchology).
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REFERENCES 341Hogan, C. J. (2002).
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REFERENCES 343Kiefer, C. (2001a). P
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REFERENCES 345Lämmerzahl, C. (1998
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REFERENCES 347Misner, C. W. (1957).
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REFERENCES 349Penrose, R. (1996). O
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REFERENCES 351Singh, T. P. (2005).
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REFERENCES 353Uzan, J.-P. (2003). T
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REFERENCES 355Zeh, H. D. (1986). Em
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INDEXabsolute elements, 73accelerat
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INDEX 359Hawking temperature, 14, 2
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INDEX 361in minisuperspace, 249Wick
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