|Approaches to Quantum Gravity|
In General > s.a. observables; phenomenology;
quantum cosmology; semiclassical general relativity;
* Main types: One may distinguish between (a) "conventional" approaches, which can be based on the quantization of a classical gravity theory (quantum geometrodynamics, loop quantum gravity, spin-foam models, Regge calculus and causal dynamic triangulations, group field theory) or on an extension of quantum field theory (string theory), and (b) other approaches, often discrete, sometimes combinatorial or based on condensed-matter physics ideas (causal sets, quantum graphity).
* "Conventional" approaches: The spacetime manifold remains, although one sometimes considers contributions from different ones; 1988, Most results have come just from quantum field theory in curved spacetime calculations; The next step is to include the back-reaction, necessary to achieve above goals and to understand things like dissipation of anisotropies.
* Rem: 2020, Some consider gauge-gravity duality our best hope for understanding quantum gravity.
@ General references: Mielczarek & Trześniewski GRG(18)-a1708 [links between approaches]; Latosh PPAN(20)-a2003 [issues with conservative approaches]; Jaksland Syn-a2005 [recovery of general relativity is not enough]; > s.a. quantum gravity [overviews].
> Related topics: see observable algebras; interpretations of quantum mechanics.
Perturbative Approaches > s.a. covariant quantum gravity;
renormalization; string theory.
* Idea: The fuzziness in the metric and causal relations is obtained by quantizing deviations from a background, reference metric, usually taken to be flat or (anti-)de Sitter, on a fixed manifold; Initially based on the Lorentz-covariant spin-2 field theory in 4D Minkowski (possibly including higher-derivative theories or supergravity, and/or using path integrals), and thus called "covariant quantum gravity"; It is the approach that has been most used in combination with other interactions, and later merged in part with superstrings/M-theory.
@ General references: Deser AdP(99)gq/99 [infinities, including supergravity]; Anselmi & Benini JHEP(07)-a0704 [higher-derivative corrections]; Bern et al PRD(08)-a0707 [unexpected cancellations]; Ward IJMPD(08), a2012-conf [resummed]; Akhoury et al PRD(11) [collinear and soft divergences]; Bellazzini et al PRD(16)-a1509 [constraints from unitarity and analyticity]; Anselmi JHEP(19)-a1909 [proof of perturbative unitarity]; Mitchell & Morris JHEP(20)-a2004 [continuum limit]; Kißler PLB(21)-a2007 [diagrammatic identities]; Pottel & Sibold a2012; > s.a. covariant quantum gravity [including infrared behavior]; friedmann equation [quantum corrections].
@ As an effective theory: Hossenfelder PLB(13)-a1208; Orland a2101 [SU(4) Yang-Mills field coupled to fermion and scalar fields].
@ Versions: Mandelstam AP(62), PR(68); Floreanini & Percacci PRD(92) [mean-field approach]; Ichinose & Ikeda IJMPA(99)ht/98; Bern LRR(02)gq [relationship with gauge theory]; Tsuneyama ht/04/PRD; Freidel & Starodubtsev ht/05 [topological field theory approach]; Brunetti & Fredenhagen gq/06-proc [background-independent]; Benedetti & Speziale JHEP(11)-a1105 [1st-order tetrad formalism and Immirzi parameter]; Vereshkov & Marochnik JModP(13)-a1108 [Heisenberg representation]; Brunetti et al CMP(16)-a1306 [as a locally covariant quantum field theory]; Upadhyay PLB(13)-a1305 [Batalin-Vilkovisky formalism], EPJC(14)-a1312 [gaugeon formalism]; Huang a1312 [in imaginary time]; Barvinsky et al PRD(18)-a1806, a2011 [Correlated Worldline theories]; Freidel & Shtanov a2006 [chiral].
@ With matter: Prinz AP(21)-a1812 [spinor electrodynamics].
@ Applications: Parentani NPB(97)gq/96 [radiative processes in quantum cosmology].
> s.a. canonical quantum gravity [including affine, lqg];
path-integral quantization; renormalization.
* Idea: (i) Canonical approach, including spin networks; (ii) Asymptotic quantization; (iii) Path integral quantization (Lorentzian or Euclidean), including spin foams; (iv) Numerical/discrete approaches auch as lattice gravity, Regge calculus, causal sets or dynamical triangulations; (v) Stochastic quantization.
@ References: Ambjørn et al PRP(12)-a1203 [CDT, asymptotic safety, lattice gravity]; Tavernelli a1801 [based on a geometrization of quantum mechanics]; Giddings FP(19)-a1803, a1805 [intrinsically quantum approach].
@ And topos theory: Flori PhD(09)-a0911, Dahlen a1111 [loop quantum gravity]; Döring a1306 [and neo-realist interpretation].
Discrete Approaches > s.a. causal sets;
discrete spacetime models [including quantum graphity];
lattice gravity and regge calculus.
@ References: Schmelzer gq/98 [condensed-matter type]; Holfter & Paschke JGP(03)ht/02 [and Dirac operator]; Gambini & Pullin in(09)gq/05; Hamma & Markopoulou NJP(11)-a1011 [condensed-matter-type spin models]; Gudder a1109-wd; Rivasseau AIP(12)-a1112, a1209-conf, FdP(14)-a1311, FdP(14)-a1406-proc, a1604-proc [tensor-track approach, including a sum over all topologies]; Oriti a1710-fs [spacetime as a quantum many-body system]; Majid CQG(19)-a1810 [on a square graph]; Eichhorn et al CQG(19)-a1811 [tensor models]; > s.a. quantum spacetime.
@ Information-based: Mandrin a1408, a1409, a1411 [from minimum information]; Chen a1412 [informationally-complete unification]; Cresswell a1909-PhD.
* At null infinity: It lies somewhere between the canonical approach and the covariant one; One avoids the 3+1 decomposition of the former and the linearization and use of a fixed background of the latter, and quantizes the radiation degrees of freedom (idea taken from QED), using the asymptotic properties of the gravitational field.
@ Null surfaces formulation: Frittelli et al PRD(97)gq/96; Domínguez & Tiglio PRD(99)gq [large effects].
@ At null infinity: Ashtekar PRL(81), JMP(81), in(81), 87.
@ At spatial infinity: Alexander & Bergmann FP(84) [electromagnetism], FP(86); Bergmann GRG(87), GRG(89).
Other Approaches > s.a. asymptotic safety;
effective theories; types
of approaches [including group field theory].
@ Other dimensions: Bjerrum-Bohr NPB(04)ht/03 [D → ∞]; Nieto a0704 [8D, background-independent Kaluza-Klein à la lqg]; Nieto RMF-a1003 [8D and (2+2) loop quantum gravity], IJGMP(12)-a1107 [in 2+2 dimensions]; Vaugon a1512 [pure geometry, of signature (–, –, +, ..., +)]; Deser GRG(16)-a1609 [1-loop divergences cannot all be removed in D > 4]; > s.a. 2D and 3D quantum gravity; regge calculus.
@ Using condensed matter ideas: Olmo & Rubiera-García IJMPD(15)-a1507 [point defects and dislocations described by non-metricity and torsion].
@ Based on paths: Bastianelli & Bonezzi a1304 [worldline approach]; Spaans 15 [based on paths]; > s.a. world function.
@ Analog models: Kiefer PLA(89) [analogy with brownian motion]; Baker a0810 [elastic-solid model]; Krein et al PRL(10)-a1006 [phonons in random fluids].
@ Categorical: Crane ht/93, gq/00; Isham ATMP(03)gq, ATMP(03)gq, ATMP(04)gq/03; Isham FP(05)qp/04-in; Baez qp/04; Raptis IJTP(06)gq/04-conf, IJTP(07) [and abstract differential geometry]; Crane gq/06-ch; Guo IJGMP(21)-a2008 [contextual extensions]; > s.a. categories in physics; quantum spacetime models; Topos Theory.
Based on modified gravity: see higher-order gravity; modified approaches [including linearized, deformed, pilot-wave, simplified models].
– journals – comments
– other sites – acknowledgements
send feedback and suggestions to bombelli at olemiss.edu – modified 23 may 2021