|  Types of Field Theories | 
In General > s.a. field theory;
  types of quantum field theories [including algebra-valued].
  * Idea: Models have been studied,
    of fields and interactions which do not have a known realization in nature;
    These may be easier to study and can give insight into the structure of more
    realistic theories.
  * Massless: Many field theory
    results obtained for massless particles do not coincide with the limit of
    the corresponding results for massive particles as m → 0; But
    the differences are due to things like mode counting, since massless particles
    can only have two helicity states, which is not true for any m ≠ 0;
    In cases where spin is not relevant (e.g., scalar particles) one does not expect
    the limit to be singular.
  @ Free fields and interactions: Lev JPA(99)qp/98;
    Singh & Dadhich MPLA(01)gq [field theories from equations of motion];
    > s.a. interactions.
  > Important types: see electromagnetism;
    gauge theory (and solutions); general
    relativity and gravitation.
  > Types of solutions: see BIon;
    Compacton; particle models; soliton
    [for non-linear theories]; waves [for linear theories].
  > Related concepts: see boundaries in field theory;
    generalized quantum field theories [finite-temperature]; symmetries.
 Specific Types
  > s.a. hamiltonian systems; strings;
  supersymmetric; topological field theories;
  tachyons; types of quantum field theories.
  * Main types: Local theories
    (the dynamical variables are local fields, tensorial, spinorial or other),
    non-local theories.
  * Ultralocal: A field theory
    is ultralocal if each space point is dynamically decoupled; For example,
    the strong-coupling limit of general relativity.
  * Exceptional field theory:
    A theory in an extended spacetime that makes supergravity fully covariant
    under the U-duality groups of M-theory;
    > s.a. Extended.
  @ In curved spacetime: Fabbri IJTP(11)-a0907 [causality and equivalence consistency constraints].
  @ Generally covariant: Bergmann PR(49) [field equations, conservation laws];
    Husain CQG(92) [2+1 model without Hamiltonian constraint];
    Henneaux et al NPB(92) [gauge invariance];
    Hoppe & Ratiu CQG(97)ht/96 [Hamiltonian reduction];
    Pons CQG(03) [diffeomorphisms and phase space],
    et al PRD(97)gq/96 [gauge];
    in Brunetti & Fredenhagen LNP(09)-a0901;
    > s.a. Covariance; diffeomorphisms;
      higher-spin theories; observables;
      statistical mechanics.
  @ Connections: Husain CQG(99)ht [diffeomorphism-invariant SU(N)];
    > s.a. connection form of general relativity; gauge theory.
  @ Bivectors: Einstein & Bargmann AM(44),
    Einstein AM(44); 
    > s.a. BF theory.
  @ Antisymmetric, forms:
    Caicedo et al ht/97 [geometry];
    Quevedo & Trugenberger NPB(97);
    Barbero & Villaseñor PRD(02) [4D 2-forms, kinetic terms];
    Arias et al PRD(03)ht/02 [path integral];
    Guendelman et al ht/04-proc [volume element as dynamical field];
    Contreras et al PRD(10)-a1005 [duality transformations];
    Aydemir et al JPCS(10)-a1009,
    PRD(11) [4-form];
    > s.a. brst approach; canonical
      formulation of gravity [covariant]; forms.
  @ Fermions:
    Robinson et al JMP(09) [symplectic];
    Skvortsov & Zinoviev NPB(11) [frame-like action];
    Rejzner RVMP(11)-a1101 [functional approach];
    Leclerc a1211 [symmetric Poisson bracket];
    Espin a1502-proc [non-hermitian second-order Lagrangian];
    Palumbo EPL(16)-a1502 [based on spinor-topological field theory, and emergent Dirac theory];
    > s.a. spinors.
  @ Non-linear field equations: Adam & Santamaria JHEP(16)-a1609 [solutions, by order reduction];
    > s.a. Bogomolny Equation;
      sigma-model; soliton.
  @ Non-linear field space:
    Mielczarek & Trześniewski PLB(16)-a1601;
    Mielczarek a1612 [scalar field theory, and spin].
  @ Exceptional field theory:  Hohm  & Samtleben PRD(14)-a1406
      [for E\(_{8(8)}^~\), on (3+248)-D generalized spacetime];
    Rudolph FdP(15)-a1512-proc [solutions];
    Berman a1903-proc [Kaluza-Klein approach].
  @ Discrete:  de Souza ht/01;
    Vankerschaver JMP(07)mp/06 [Euler-Poincaré reduction];
    > s.a. Discretization.
  @ Fields on generalized backgrounds: Calcagni JHEP(12)-a1107 [multi-fractional spacetime];
    > s.a. cell complex; fractals in physics.
  @ Partially massless fields: Hinterbichler & Joyce JHEP(16)-a1608,
    Brust & Hinterbichler JHEP(17)-a1610,
    JHEP(17)-a1610 [higher spin].
  @ Various dimensionalities: Fletcher et al a1709 [features of gravity and relativistic field theory in 2D];
    > s.a. higher-dimensional gravity.
  @ Other types: Lerner & Clarke CMP(77) [massless free fields];
    Guerra PRP(81) [stochastic];
    Huang IJMPA(06)ht/04 [daor fields];
    Akhmeteli IJQI(11)qp/05 [charged real fields and quantum mechanics];
    Konopka MPLA(08) [with Lorentz-invariant energy scale];
    Bender & Klevansky PRL(10)-a1002
      [Lagrangian describing similar particles with different masses];
    Atiyah & Moore a1009
      [based on "shifted differential equations", Dirac and Einstein-Maxwell fields];
    Ben Geloun JMP(12) [classical group field theories];
    Jaffe et al CMP(14)-a1201 [complex, and quantum field theory];
    Curtright NPB(19)-a1907 [4D massive dual fields].
  @ Generalized: Balachandran et al IJMPA(01)ht/00 [fuzzy];
    Jadczyk AACA(09)-a0711 ["kairons", wavicles with initial data on timelike worldlines];
    Kleinert 08 [multivalued];
    Gorantla et al a2007 [non-standard theories related to fractons].
  > According to spin value:
    see scalar fields (including klein-gordon fields);
    low-spin fields [including vector theories]; spin-2 fields;
    high and arbitrary spin.
  > Other: see Auxiliary Field;
    anomalies [relative field theories]; Conformal,
    Double, non-commutative,
    non-local field theories [including bilocal]; approaches
    to quantum gravity [group field theory]; Effective Field Theory;
    fluids; higher-derivative theories; lattice
    field theory; Sine-Gordon; Stealth Fields.
Integrable Field Theories > s.a. integrable system
  / Ernst Equation; QCD; self-dual gauge fields;
  Sine-Gordon Equation; wave equations[solvable].
  * KP equation: (Kadomtsov-Petviashvili)
    The equation (4 ut −
    12 u ux −
    uxxx)x
    = 3 uyy; A completely integrable system.
  * Other examples: 2D
    field theories obtained from 4D ones using isometry groups (> see
    solutions of general relativity with symmetries
    and generating methods).
  @ General references: Alvarez et al NPB(98) [new approach, any dimension];
    Andrianov et al JPA(99)si/98 [and supersymmetric quantum mechanics];
    Lorente in(00)qp/04,
    JCAM(03)mp/04 [on the lattice];
    Papachristou a0803 [symmetry and integrability];
    Ferreira et al AIP(13)-a1307 [quasi-integrable theories].
  @ KP: Dickey LMP(99) [modified];
    Tu LMP(99) [q-deformed];
    Kisisel mp/01,
    mp/01 [discretized, Hamiltonian];
    Akhmetshin et al ht/02 [solutions].
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