- Page 4 and 5: Quantum Field Theory and Gravity Co
- Page 6 and 7: Contents Preface ..................
- Page 8 and 9: Preface The present volume arose fr
- Page 10 and 11: Preface ix 6. (How) can we test qua
- Page 12 and 13: Preface xi Felix Finster, Andreas G
- Page 14 and 15: Preface xiii it is related to other
- Page 16 and 17: Quantum Gravity: Whence, Whither? C
- Page 18 and 19: Quantum Gravity: Whence, Whither? 3
- Page 20 and 21: Quantum Gravity: Whence, Whither? 5
- Page 22 and 23: Quantum Gravity: Whence, Whither? 7
- Page 24 and 25: Quantum Gravity: Whence, Whither? 9
- Page 26 and 27: Quantum Gravity: Whence, Whither? 1
- Page 30 and 31: Local Covariance and Background Ind
- Page 32 and 33: Local Covariance and Background Ind
- Page 34 and 35: Local Covariance and Background Ind
- Page 36 and 37: Local Covariance and Background Ind
- Page 38: Local Covariance and Background Ind
- Page 41 and 42: 26 B. Temple In [14] the authors in
- Page 43 and 44: 28 B. Temple Theorem 2.1. Assume p
- Page 45 and 46: 30 B. Temple conservation laws will
- Page 47 and 48: 32 B. Temple as to why small-scale
- Page 49 and 50: 34 B. Temple 5) How did you reach t
- Page 51 and 52: 36 B. Temple 9) How large would the
- Page 53 and 54: 38 B. Temple 13) If Dark Energy doe
- Page 55 and 56: 40 B. Temple [6] J. Glimm, P.D. Lax
- Page 57 and 58: 42 S. Gielen and D. Oriti In this c
- Page 59 and 60: 44 S. Gielen and D. Oriti multiplic
- Page 61 and 62: 46 S. Gielen and D. Oriti way that
- Page 63 and 64: 48 S. Gielen and D. Oriti ⃗p g on
- Page 65 and 66: 50 S. Gielen and D. Oriti Using the
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- Page 71 and 72: 56 S. Gielen and D. Oriti C 2 i 2 j
- Page 73 and 74: 58 S. Gielen and D. Oriti which one
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- Page 77 and 78: 62 S. Gielen and D. Oriti Reference
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64 S. Gielen and D. Oriti [42] Alej
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66 A. Döring and R. Soares Barbosa
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68 A. Döring and R. Soares Barbosa
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70 A. Döring and R. Soares Barbosa
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72 A. Döring and R. Soares Barbosa
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74 A. Döring and R. Soares Barbosa
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76 A. Döring and R. Soares Barbosa
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78 A. Döring and R. Soares Barbosa
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80 A. Döring and R. Soares Barbosa
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82 A. Döring and R. Soares Barbosa
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84 A. Döring and R. Soares Barbosa
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86 A. Döring and R. Soares Barbosa
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88 A. Döring and R. Soares Barbosa
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90 A. Döring and R. Soares Barbosa
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92 A. Döring and R. Soares Barbosa
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94 A. Döring and R. Soares Barbosa
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96 A. Döring and R. Soares Barbosa
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98 J. L. Flores, J. Herrera and M.
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100 J. L. Flores, J. Herrera and M.
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102 J. L. Flores, J. Herrera and M.
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104 J. L. Flores, J. Herrera and M.
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106 J. L. Flores, J. Herrera and M.
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108 J. L. Flores, J. Herrera and M.
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110 J. L. Flores, J. Herrera and M.
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112 J. L. Flores, J. Herrera and M.
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114 J. L. Flores, J. Herrera and M.
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116 J. L. Flores, J. Herrera and M.
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118 J. L. Flores, J. Herrera and M.
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Some Mathematical Aspects of the Ha
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Hawking Effect for Rotating Black H
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Hawking Effect for Rotating Black H
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Hawking Effect for Rotating Black H
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Hawking Effect for Rotating Black H
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Hawking Effect for Rotating Black H
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Hawking Effect for Rotating Black H
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Hawking Effect for Rotating Black H
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Observables in the General Boundary
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Observables in the General Boundary
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Observables in the General Boundary
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Observables in the General Boundary
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4. Quantization Observables in the
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Observables in the General Boundary
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Observables in the General Boundary
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Observables in the General Boundary
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Observables in the General Boundary
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Observables in the General Boundary
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Causal Fermion Systems: A Quantum S
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Causal Fermion Systems 159 We have
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Causal Fermion Systems 161 1.2.1. F
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Causal Fermion Systems 163 The spac
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Causal Fermion Systems 165 property
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Causal Fermion Systems 167 1.3. An
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2. Spontaneous structure formation
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Causal Fermion Systems 171 We next
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Causal Fermion Systems 173 3.2. A t
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Causal Fermion Systems 175 In order
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Causal Fermion Systems 177 Figure 1
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Causal Fermion Systems 179 allow τ
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References Causal Fermion Systems 1
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CCR- versus CAR-Quantization on Cur
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CCR- versus CAR-Quantization on Cur
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CCR- versus CAR-Quantization on Cur
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CCR- versus CAR-Quantization on Cur
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CCR- versus CAR-Quantization on Cur
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CCR- versus CAR-Quantization on Cur
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CCR- versus CAR-Quantization on Cur
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CCR- versus CAR-Quantization on Cur
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CCR- versus CAR-Quantization on Cur
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CCR- versus CAR-Quantization on Cur
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CCR- versus CAR-Quantization on Cur
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CCR- versus CAR-Quantization on Cur
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On the Notion of ‘the Same Physic
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The Same Physics in All Spacetimes
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The Same Physics in All Spacetimes
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The Same Physics in All Spacetimes
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The Same Physics in All Spacetimes
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The Same Physics in All Spacetimes
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The Same Physics in All Spacetimes
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The Same Physics in All Spacetimes
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The Same Physics in All Spacetimes
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The Same Physics in All Spacetimes
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The Same Physics in All Spacetimes
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230 R. Verch The basic idea of loca
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232 R. Verch The conditions LCSE-1.
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234 R. Verch for the just defined s
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236 R. Verch quantum fields in curv
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238 R. Verch (i) Let D be a subset
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240 R. Verch Figure 1. Sketch of te
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242 R. Verch Structure of the set o
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244 R. Verch are referred to as sym
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246 R. Verch (δ) Finally we mentio
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248 R. Verch such that ω β(x) (ϑ
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250 R. Verch a state with respect t
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252 R. Verch if such solutions coul
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254 R. Verch properties of quantum
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256 R. Verch [35] A. Strohmaier, R.
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258 J. Barbour theory. My aim in th
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260 J. Barbour relative to each oth
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262 J. Barbour Figure 2. In Newtoni
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264 J. Barbour Five more data are n
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266 J. Barbour signal is generated
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268 J. Barbour a b a b c Figure 4.
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270 J. Barbour Figure 5. The action
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272 J. Barbour Figure 6. The distin
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274 J. Barbour be expressed through
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276 J. Barbour In this connection,
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278 J. Barbour they leave all lengt
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280 J. Barbour Slicings of spacetim
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282 J. Barbour definition, structur
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284 J. Barbour would indicate a spu
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286 J. Barbour whole idea: general
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288 J. Barbour other variables. It
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290 J. Barbour geometrodynamics is
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292 J. Barbour a straight line at a
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294 J. Barbour occur in dynamics. E
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296 J. Barbour [7] J Barbour. The D
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On the Motion of Point Defects in R
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On the Motion of Point Defects in R
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On the Motion of Point Defects in R
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On the Motion of Point Defects in R
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On the Motion of Point Defects in R
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On the Motion of Point Defects in R
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On the Motion of Point Defects in R
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On the Motion of Point Defects in R
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On the Motion of Point Defects in R
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On the Motion of Point Defects in R
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On the Motion of Point Defects in R
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On the Motion of Point Defects in R
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On the Motion of Point Defects in R
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On the Motion of Point Defects in R
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On the Motion of Point Defects in R
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On the Motion of Point Defects in R
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On the Motion of Point Defects in R
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On the Motion of Point Defects in R
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On the Motion of Point Defects in R
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338 S. Hollands asymptotically flat
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340 S. Hollands In the case where
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342 S. Hollands The black hole hori
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344 S. Hollands [18] Hollands, S.,
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346 D. Giulini well either fail to
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348 D. Giulini taken along differen
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350 D. Giulini M2. The trajectories
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352 D. Giulini as that of test part
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354 D. Giulini one, since the energ
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356 D. Giulini acceleration is just
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358 D. Giulini The time evolution o
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360 D. Giulini with ĥ := h/f, so t
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362 D. Giulini transferring momentu
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364 D. Giulini The calculation of (
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366 D. Giulini in which the left-ha
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368 D. Giulini 6. Conclusion I conc
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370 D. Giulini [26] Pippa Storey an
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372 Index Bose-Einstein condensate,
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374 Index entropy flux density, 242
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376 Index loop order (of diagram),
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378 Index gravitational, 2 Reeh-Sch
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380 Index UV, see ultraviolet vacuu