Higher-Order Theories of Gravity  

In General > s.a. gravity; higher-order quantum gravity; phenomenology of higher-order gravity [including solutions]; spin-2 field theories.
* Idea: Theories of gravitation, first discussed by H Weyl in 1918 as alternatives to Einstein's theory, that include quadratic or higher order curvature terms in the action, e.g., R2, Rab Rab and Rabcd Rabcd (only two of these are independent – the integral of a combination of them gives the Euler number (M)).
* Motivation: One can alleviate the divergences in the quantum theory, and modify the predicted expansion history of the universe in cosmology.
* Action/Lagrangian: In 4D, the most general one with up to quadratic terms is

S = – ( Rab Rab R2 + R) dv ;

any other term can be absorbed into these using the Gauss-Bonnet theorem [true only in positive-definite case?]; The only one which gives second-order equations in d > 4 is the Lanczos Lagrangian; But S could have a different curvature dependence.
* Metric vs affine or Palatini forms: In general relativity, the purely affine picture and the two other formulations are dynamically equivalent, at least classically; This equivalence does not hold for theories of gravity with a non-linear dependence on the curvature.
* Ostrogradski theorem: The only potentially stable, local modification of general relativity is to make the Lagrangian an arbitrary function of the Ricci scalar.
* Bicknell theorem: A conformal relationship between fourth order gravity and scalar-tensor theory.
* Field equations: [@ Stelle PRD(77)]

Hab:= (–2) R;ab Rab;c;c – (–2) gab R + 2 Rmn Rambn +

– 2 R Rab gab ( Rmn RmnR2) + Rab  gab R = – Tab ,

where Hab satisfies Hab;b = 0 identically, as a consequence of the field equations.
@ Reviews: Cotsakis gq/97-MG8 [status]; Nojiri & Odintsov ht/06-ln [and dark energy]; Farhoudi GRG(06) [and trace anomaly relation]; Capozziello & Francaviglia a0706 [and phenomenology]; Schmidt IJGMP(07) [history and applications]; Sotiriou a0710-PhD; Sotiriou & Faraoni a0805-RMP.
@ General references: Stelle GRG(78); Brans CQG(88) [and metric redefinitions]; Essén IJTP(90); Allemandi & Francaviglia IJGMP(07) [variational].
@ Energy: Boulware et al PRL(83); Deser & Yang CQG(89); Borowiec et al GRG(94); Deser & Tekin PRL(02)ht, PRD(03)ht/02, PRD(07)gq; Fatibene et al IJGMP(06) [same solution in different theories]; Multamäki et al a0712 [energy-momentum complexes].
@ Noether symmetries: Sanyal et al GRG(05)ap/03; Modak et al GRG(05).
@ Metric vs Palatini (first- vs second-order): Shahid-Saless PRD(87) [R + R2 theory]; Olmo & Komp gq/04; Ezawa et al gq/03, NCB(04)gq [f(R) theories]; Deser CQG(06)gq, comment Kiriushcheva & Kuzmin CQG(07)gq/06 [obstacles with odd-derivative terms]; Sotiriou PLB(07) [instability in metric formulation]; Exirifard & Sheikh-Jabbari PLB(08)-a0705 [equivalence of formulations only for Lovelock gravity]; Poplawski a0706; Iglesias et al PRD(07)-a0708 [how (not) to Palatini]; Borunda et al a0804; Faraoni PLB(08)-a0806 [Palatini unphysical].
@ Cauchy / initial value problem: Teyssandier & Tourrenc JMP(83) [R + R2]; Jakubiec & Kijowski JMP(89) [well-posedness]; Lanahan-Tremblay & Faraoni CQG(07)-a0709 [well-posed for metric version].
@ Related topics: Eliezer NPB(89) [Regge calculus]; Ghoroku pr(90) [new variables]; Bartoli et al CQG(99)gq/98 [gauge fixing]; Woodard ap/06-in [choice of theory]; Carloni & Dunsby JPA(07)gq/06-in [dynamical systems approach]; Sotiriou gq/06-in [matter couplings]; > s.a. hamilton-jacobi theory, metric matching.

Examples of Theories > s.a. 2D gravity; 3D gravity; actions for gravity [curvature-saturated]; theories of gravity; torsion in physics.
* And general relativity: If we have a theory with Lagrangian

= |g|1/2 F(g, Ric(g)) + m(g, g, , g) ,

a redefinition of the metric (which need no longer be Lorentzian) gives a scalar-tensor theory with action

= |h|1/2 R(h) + m + +(h, h, ,h) ,  where  hab:= |det(/Rab)|–1/2 (/Rab) .

* f(R) theories: If L is a non-linear function of the curvature scalar, then the field equations are of fourth order in the metric; These equations were first discussed by H Weyl in 1918, as an alternative to Einstein's theory.
* R–1 theories: Motivated by the fact that they lead to cosmological acceleration; A 1/R action by itself is ruled out by constraints on scalar-tensor gravity, but could work as an extra contribution to the action.
@ And general relativity, scalar-tensor: Goenner in(87); Magnano et al GRG(87); Jakubiec & Kijowski PRD(88), JMP(89); Magnano & Sokolowski PRD(94)gq/93, Magnano gq/95-in; Sokolowski gq/95-in; Low GRG(95) [singularities]; Núñez & Solganik ht/04; Flanagan CQG(04)gq [equivalence]; Sotiriou CQG(06)gq; Bertolami & Páramos a0805 [and non-trivial matter coupling].
@ R2 theories: Folomeshkin CMP(71); Simon PRD(90) [non-locality]; Sanyal GRG(05)ht/04 [Hamiltonian]; Meng & Wang CQG(05) [R2 + R–1].
@ R–1 theories: Chiba PLB(03)ap [and scalar-tensor]; Cline ap/03-wd [as extra term].
@ Lanczos/Lovelock gravity: Lanczos JMP(69); Madore CQG(86) [action]; > s.a. thermodynamics.
@ Other theories: Havas GRG(77) [linearized]; Caprasse et al IJMPD(93) [cubic]; Hindawi et al PRD(96) [vacua and excitations]; Hurth et al PRD(97) [sugra]; Borowiec et al CQG(98)gq/96 [Rab Rab Lagrangians]; Meng & Wang PLB(04)ht/03 [ln R, Palatini]; Schmidt gq/06-in [4th-order]; Navarro & Van Acoleyen JCAP(06)gq/05 [MOND-like, and cosmology]; Gruzinov & Kleban CQG(07)ht/06 [causality constraints]; Baghram et al PRD(07)ap [f(R) = (R2R02)1/2]; Sotiriou PLB(08)-a0805, Sotiriou & Faraoni a0805 [with matter coupling to R]; Faraoni PLB-a0806 [f(R) and conformal rescaling].
@ Higher-dimensional: Ezawa et al CQG(99) [semiclassical stability]; Collins & Holdom JHEP(02) [4+1 with cosmological constant].
@ Action/Lagrangian: Nojiri & Odintsov PRD(00)ht/99 [surface terms].
@ Hamiltonian formulation: Szczyrba JMP(87); Ezawa et al CQG(99)gq/98; Querella gq/99-PhD; Ezawa et al CQG(06)gq/05.
@ From quantum gravity effective theory: Bojowald & Skirzewski IJGMP(07)ht/06-ln.
> Other: see brans-dicke; BRST; Conformal, Gauss-Bonnet, Lovelock Gravity; Metric-Affine; unified theories [fourth-order Weyl].


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