Index 583emergent, 99, 109, 163, 178, 184, 230, 329, 559,566, 571foam, 434, 437foliation, 49, 54, 57, 69, 70, 75–78, 80, 81, 140,155, 195, 244, 253, 279, 332, 345–347, 414,418fractal, 124, 125fuzziness, 205, 434, 437, 439non-commutative, 301, 302, 431, 432, 437, 443,444, 466, 467, 469, 473, 476, 477, 484–487,489, 491, 500, 504, 510, 514, 529, 572, 574quantum, 5, 10, 88, 206, 262, 264, 284relational, 97, 151singularities, 249, 253, 403, 555, 566superpositions of, 5, 99, 104, 129, 148spin foam models, 8–10, 56, 129, 136, 137, 140, 141,147, 153, 156, 248, 254, 255, 265, 267–270,272, 275, 276, 279–288, 290, 300, 306, 308,310, 316, 317, 320–322, 324–326, 328, 329,364, 374, 379, 402, 403, 509, 549, 559, 566,570, 576–579spin foams, 56, 129, 136, 139–141, 147, 255, 265,267, 269, 270, 272, 275, 276, 279–287, 290,300, 306, 316, 317, 322, 329, 379, 403spin networks, 28, 139–141, 255, 259, 260, 263–267,269, 270, 278–282, 284, 285, 290, 293, 313,316, 317, 319, 325, 326, 332, 549, 550,552–554, 561–563, 566, 567, 579standard model, 3, 8, 13, 14, 17, 90, 116, 123, 146,162, 196, 231, 248, 400, 436, 451, 530, 532,534–536, 542, 543, 562, 567string field theory, 211–214, 216–226, 232string theory, 4, 6, 8–10, 15, 17, 22, 99, 129, 137, 150,169, 172–176, 178, 179, 181–184, 187, 188,190, 195, 199, 205, 207, 210–213, 217, 223,224, 226, 229–232, 236, 343, 344, 430, 431,435–437, 439, 528, 538, 572duality, 182, 195landscape, 22, 210, 211, 213, 218, 225, 226, 230non-perturbative, 9, 213, 216, 222perturbative, 9, 14, 211, 212, 215, 221strings, 8, 10, 84, 173, 174, 178, 181, 188, 210–213,215, 217, 220, 221, 223–225, 230, 232, 324supergravity, 171–174, 177, 180–182, 205, 206, 552,553, 572superspace, 64, 310, 311, 323, 327midi-, 47, 63mini-, 47, 63, 80supersymmetry, 170–173, 177, 181–183, 187–189,193, 199, 204–207, 211, 217, 220, 223, 231,232, 248, 435, 538, 539symmetryasymp<strong>to</strong>tic, 64, 178, 193conformal, 15, 173, 181, 183, 362CPT, 40, 434, 437–439, 481, 528diffeomorphism, 24, 178, 236, 245, 293, 295, 389,420, 512emergent, 24, 144, 539, 559, 560gauge, 13, 179, 180, 220, 263, 272, 276, 285, 291,293, 294, 312, 316, 320, 322, 370, 382, 389,530, 552, 558emergent, 178local, 96Lorentz, 153, 256, 270, 400, 402, 428, 433, 436,437, 440, 444, 445, 447, 500, 501, 529, 535,536, 538Poincaré, 158, 171, 304, 428, 433, 434, 436–438,440, 442, 500, 503, 510, 529tensor models, 320, 321timearrow, 198, 199background, 99, 103, 104, 106, 109, 144, 157cosmic, 126discrete, 16, 18, 109discretization, 194in his<strong>to</strong>ry formalism, 70, 72–74, 78multifingered, 140, 242ordering, 78pre-geometric, 144problem of, 6, 7, 46, 54, 80, 108–110, 148, 191,194, 242, 243, 273, 386, 393, 406in classical GR, 7in quantum gravity, 7, 14translations, 74, 172<strong>to</strong>pological defects, 18<strong>to</strong>pological field theory, 15, 18, 254, 267, 268, 275,286–288, 292, 310, 496, 552, 553, 555, 556,558, 577<strong>to</strong>pological gravity, 15, 324<strong>to</strong>pologychange, 155, 160, 178, 195, 230, 290, 310, 311,318, 323, 332, 343, 345, 374, 400, 417, 418sum over-, 317, 321, 324, 325, 343, 369,417–419<strong>to</strong>pos theory, 85, 87, 88, 91, 95, 97, 150cosmoi, 89twis<strong>to</strong>r theory, 65, 70unification, 123, 427, 548, 549, 561, 562, 567unitarity, 14, 20, 40, 125, 142, 207, 379, 387, 388,391, 419universality, 100, 101, 104, 373, 414, 417Wheeler–deWitt equation, 6Wick rotation, 39, 41, 347, 403Wilson loop, 174, 180, 259, 278, 357,552–554
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APPROACHES TO QUANTUM GRAVITYToward
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A Sandra
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viiiContents11 String theory, holog
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ContributorsJ. AmbjørnThe Niels Bo
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xiiList of contributorsD. OritiMax
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PrefaceQuantum Gravity is a dream,
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Prefacexviiare following in their s
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Prefacexixenormous amount of progre
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1Unfinished revolutionC. ROVELLIOne
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Unfinished revolution 5wit of empir
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Unfinished revolution 7In general r
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Unfinished revolution 9However, res
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Unfinished revolution 11References[
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2The fundamental nature of space an
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The fundamental nature of space and
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The fundamental nature of space and
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The fundamental nature of space and
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The fundamental nature of space and
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The fundamental nature of space and
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The fundamental nature of space and
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Does locality fail at intermediate
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Does locality fail at intermediate
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Does locality fail at intermediate
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Does locality fail at intermediate
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Does locality fail at intermediate
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∫Does locality fail at intermedia
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Does locality fail at intermediate
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Does locality fail at intermediate
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Does locality fail at intermediate
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Prolegomena to any future Quantum G
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Prolegomena to any future Quantum G
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Prolegomena to any future Quantum G
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Prolegomena to any future Quantum G
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Prolegomena to any future Quantum G
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Prolegomena to any future Quantum G
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Prolegomena to any future Quantum G
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Prolegomena to any future Quantum G
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Prolegomena to any future Quantum G
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Prolegomena to any future Quantum G
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Prolegomena to any future Quantum G
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Prolegomena to any future Quantum G
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Spacetime symmetries in histories c
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Spacetime symmetries in histories c
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Spacetime symmetries in histories c
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Spacetime symmetries in histories c
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Spacetime symmetries in histories c
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Spacetime symmetries in histories c
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Spacetime symmetries in histories c
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Spacetime symmetries in histories c
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Categorical geometry and the mathem
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Categorical geometry and the mathem
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Categorical geometry and the mathem
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Categorical geometry and the mathem
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Categorical geometry and the mathem
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Categorical geometry and the mathem
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Categorical geometry and the mathem
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7Emergent relativityO. DREYER7.1 In
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A(a)Emergent relativity 101(b)(c)B(
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Emergent relativity 103It is here t
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Emergent relativity 105spacetime co
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Emergent relativity 107φABFig. 7.4
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Emergent relativity 109If, on the o
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8Asymptotic safetyR. PERCACCI8.1 In
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Asymptotic safety 113field and the
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Asymptotic safety 115For example, t
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Asymptotic safety 117If we choose k
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Asymptotic safety 119complex fields
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Asymptotic safety 1212G ~ ~1.510.5-
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Asymptotic safety 123larger, and it
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Asymptotic safety 125Dimensional an
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Asymptotic safety 127References[1]
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9New directions in background indep
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New directions in background indepe
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New directions in background indepe
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New directions in background indepe
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New directions in background indepe
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New directions in background indepe
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New directions in background indepe
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New directions in background indepe
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New directions in background indepe
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New directions in background indepe
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New directions in background indepe
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Questions and answers 151Quantum Gr
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Questions and answers 153was that t
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Questions and answers 155causality
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Questions and answers 157to hold),
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Questions and answers 159of how gra
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Questions and answers 161the action
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Questions and answers 163allow us t
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Questions and answers 165- A-F.Mark
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10Gauge/gravity dualityG. HOROWITZ
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Gauge/gravity duality 171strong and
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Gauge/gravity duality 173decomposed
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Gauge/gravity duality 175Here l s i
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Gauge/gravity duality 177There is a
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Gauge/gravity duality 179these are
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Gauge/gravity duality 181leading to
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Gauge/gravity duality 183states to
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Gauge/gravity duality 185[6] N. Ber
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11String theory, holography and Qua
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String theory, holography and Quant
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String theory, holography and Quant
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String theory, holography and Quant
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String theory, holography and Quant
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String theory, holography and Quant
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String theory, holography and Quant
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String theory, holography and Quant
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String theory, holography and Quant
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String theory, holography and Quant
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String theory, holography and Quant
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String theory, holography and Quant
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String field theory 211no tools to
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String field theory 213made an insi
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(d) Cyclicity: ∫ ⋆= (−1) G G
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String field theory 217however, the
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String field theory 21912.2.3 Outst
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String field theory 221a review) gi
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String field theory 223similar comp
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String field theory 225this; the ph
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String field theory 227[11] T. G. E
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Questions and answers• Q - D. Ori
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Questions and answers 231condition
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Part IIILoop quantum gravity and sp
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236 T. Thiemann(anti)commute. We se
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238 T. ThiemannNotice that in gener
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240 T. Thiemannspectrum of all the
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242 T. Thiemannorder to avoid anoma
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244 T. ThiemannWe consider spacetim
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246 T. ThiemannHence both gauge gro
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248 T. Thiemannthat Ĉ(N) cannot be
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250 T. Thiemann[8] R. Brunetti, K.
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252 T. Thiemann[48] M. Bojowald, H.
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254 E. LivineSU(2) gauge theory. Th
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256 E. Livinespace; η IJ is the fl
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258 E. LivineHowever, in contrast t
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260 E. Livine(i) Either we work wit
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262 E. LivineAt the end of the day,
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264 E. Livineprojector at the end v
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266 E. Livinefor a surface S inters
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268 E. LivineThis constraint is sat
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270 E. Livinewe do not need the sec
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15The spin foam representation of l
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274 A. Perezin classical general re
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276 A. Perezwhere M = ×R (for an
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278 A. Perezthe Levi-Civita tensor.
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280 A. PerezkTr[ k (W p )] ✄jP=
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282 A. Perezjjjkjkmkmjjjjmkmkmkmkkj
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284 A. PerezHere we studied the int
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286 A. PerezA spin foam representat
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288 A. Perezmaster-constraint progr
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16Three-dimensional spin foam Quant
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292 L. Freidel16.3 The Ponzano-Regg
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294 L. Freidelunder usual gauge tra
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296 L. Freidelis now constrained to
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298 L. Freidel16.4.1 Mathematical s
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300 L. FreidelTherefore, at first o
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302 L. FreidelThe inverse group Fou
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304 L. FreidelFrom this identity, i
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306 L. Freidelchoice of statistics.
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308 L. FreidelA deeper study of the
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17The group field theory approach t
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312 D. Oritisimplicial complex, or
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314 D. Oritiare not all simultaneou
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316 D. Oritidiagrams correspond to
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318 D. Oritiis the simple fact that
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320 D. Oritibetter, by a single mat
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322 D. Oritior SO(3, 1)) [8; 9; 10]
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324 D. Oritiwhere: g i ∈ G, s i
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326 D. Oritiobservables in GFTs are
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328 D. Oritiresearch. On the other
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330 D. Oritiof the possibility of a
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Questions and answers• Q - L. Cra
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334 Questions and answersI partly d
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336 Questions and answersspectrum i
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Part IVDiscrete Quantum Gravity
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342 J. Ambjørn, J. Jurkiewicz and
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344 J. Ambjørn, J. Jurkiewicz and
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346 J. Ambjørn, J. Jurkiewicz and
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348 J. Ambjørn, J. Jurkiewicz and
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350 J. Ambjørn, J. Jurkiewicz and
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352 J. Ambjørn, J. Jurkiewicz and
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354 J. Ambjørn, J. Jurkiewicz and
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356 J. Ambjørn, J. Jurkiewicz and
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358 J. Ambjørn, J. Jurkiewicz and
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19Quantum Regge calculusR. WILLIAMS
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362 R. Williamsonly in flat space a
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364 R. Williamswhere V is the volum
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366 R. Williamsequations of motion.
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368 R. WilliamsDropping the 1/d cor
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370 R. WilliamsAt a typical interio
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372 R. Williamsabout which it makes
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374 R. Williamsdealt with include t
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376 R. Williams[27] H. W. Hamber, P
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20Consistent discretizations as a r
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380 R. Gambini and J. PullinThe mod
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382 R. Gambini and J. Pullinphase s
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384 R. Gambini and J. Pullin21q 20-
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386 R. Gambini and J. Pullinof the
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388 R. Gambini and J. Pullinaccepts
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390 R. Gambini and J. Pullinisomorp
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392 R. Gambini and J. Pullin[3] C.
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394 J. Hensonall the other subjects
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396 J. HensonzyxFig. 21.1. A causal
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398 J. Hensonthis way, no discreten
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400 J. Hensonout various sprinkling
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402 J. Hensoncommutes with rotation
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404 J. Hensonblack hole entropy (or
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406 J. Henson“Kleitman-Rothschild
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408 J. Hensonhistories suggest any
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410 J. Hensonthe type normally used
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412 J. Henson[17] R. D. Sorkin (199
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Questions and answers• Q - J. Hen
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416 Questions and answersthat the l
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418 Questions and answers2. The abo
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420 Questions and answersnot unimpo
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422 Questions and answers- A - R. G
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Part VEffective models and Quantum
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428 G. Amelino-CameliaFor this phen
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430 G. Amelino-Cameliacorrection to
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432 G. Amelino-Cameliato the fact t
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434 G. Amelino-Camelia22.2.2 Planck
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436 G. Amelino-Cameliaformalism in
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438 G. Amelino-Camelia22.3 On the s
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440 G. Amelino-Camelia22.4 Aside on
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442 G. Amelino-CameliaA theory will
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444 G. Amelino-Cameliawe might be c
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446 G. Amelino-CameliaFor the dispe
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448 G. Amelino-CameliaReferences[1]
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23Quantum Gravity and precision tes
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452 C. Burgesswith the following sc
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454 C. BurgessFor this reason it is
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456 C. Burgess) E ( m) P( ( 1 2L EA
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458 C. Burgessthe low-energy experi
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460 C. Burgesscouplings contribute.
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462 C. BurgessNon-relativistic sour
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464 C. Burgesscontribute at any giv
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24Algebraic approach to Quantum Gra
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468 S. Majidhas been called a ‘Pl
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470 S. Majidα → u −1 αu + u
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472 S. Majidcoordinates the coprodu
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474 S. MajidPositionMomentumGravity
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476 S. Majidquantum group acts cova
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478 S. Majidwhere we introduce p 0
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480 S. Majidλ p 0 2θ < 01.51A0.50
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482 S. Majidto complete the structu
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484 S. MajidC[SO 3,1 ]◮⊳U(R 3 >
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486 S. Majid24.5 Physical interpret
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488 S. Majidimage. This brings with
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490 S. Majiddirection, even though
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492 S. Majid[4] S. Majid and L. Fre
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494 J. Kowalski-GlikmanNow DSR post
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496 J. Kowalski-Glikmanas it is bel
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498 J. Kowalski-Glikmanformer reduc
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500 J. Kowalski-Glikmanalgebra beco
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502 J. Kowalski-GlikmanRelativistic
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504 J. Kowalski-GlikmanLeibniz rule
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506 J. Kowalski-Glikman(Quantum) Gr
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508 J. Kowalski-Glikman[8] L. Freid
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510 F. GirelliThe new Lagrangian ˜
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512 F. GirelliThe discussion can be
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514 F. GirelliThe first key questio
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516 F. GirelliBy doing a sequence o
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518 F. GirelliM P as a maximum mass
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520 F. Girellithe Legendre transfor
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522 F. Girelliwhere λ i are Lagran
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524 F. GirelliWe can define differe
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526 F. Girelligroups, but also push
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27Lorentz invariance violation and
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530 J. Collins, A. Perez and D. Sud
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532 J. Collins, A. Perez and D. Sud
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534 J. Collins, A. Perez and D. Sud
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536 J. Collins, A. Perez and D. Sud
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538 J. Collins, A. Perez and D. Sud
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540 J. Collins, A. Perez and D. Sud
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542 J. Collins, A. Perez and D. Sud
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544 J. Collins, A. Perez and D. Sud
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546 J. Collins, A. Perez and D. Sud
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28Generic predictions of quantum th
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550 L. Smolin28.2 Assumptions of ba
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552 L. SmolinGeneral Relativity is
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554 L. SmolinStarting with the acti
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556 L. Smolintheory should dominate
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- Page 1178: 568 L. SmolinJ. Magueijo, S. Majid,
- Page 1182: 570 L. Smolin[54] L. Freidel, E. R.
- Page 1186: 572 Questions and answerssay much a
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- Page 1194: 576 Questions and answersconsider a
- Page 1198: 578 Questions and answersAs a resul
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