|  Spacetime Foam | 
In General
  > s.a. cell complex [froth]; equivalence principle [violations].
  * Idea: A version of quantum
    spacetime, modeled as a differentiable manifold with fluctuating small-scale
    topology; Introduced by Wheeler, could lead to consider particle phenomenology
    as a "chemistry of geometry"; To make this more precise, we must
    understand the quantum gravity vacuum and its fluctuations; Some versions of
    spacetime foam can be seen as a "sea of virtual black holes".
  * Conditions: It requires a
    cosmological constant (at least in Hawking's picture).
  @ General: Wheeler AP(57),
    62 pp 71-83;
    Hawking NPB(78),
    in(79);
    Crane & Smolin GRG(85),
    NPB(86);
    Friedman et al NPB(88) [and fermions];
    Kirillov & Turaev G&C(03)ht/01 [Coulomb & Newton V];
    Ng gq/04-MGX,
    LNP(05)gq/04 [and information];
    Frenkel a1011 ["spacetime foam formulas"];
    Ng a1102-proc.
  @ Phenomenological description:
    Amelino-Camelia gq/01.
Models
  > s.a. finsler geometry; kaluza-klein theory;
  spin foam; string phenomenology.
  * Strings and branes:
    The foamy structures are provided by lower-dimensional background brane
    defects in a D3-brane Universe, whose density is a free parameter to be
    constrained phenomenologically.
  @ Algebraic approach: Baez pr(84);
    Heller & Sasin IJTP(97) [classical model];
    Raptis & Zapatrin CQG(01)gq.
  @ Gas / superposition of wormholes: Preparata et al GRG(00)gq/98 [quantum gravity ground state];
    Garattini PLB(99)ht/98 [semiclassical wormholes],
    ZN(01)gq/00-proc,
    JOB(02)gq/01-proc,
    IJMPA(02)gq/01,
    IJTGN(02)gq [Reissner-Nordström wormholes];
    Cacciatori et al PLB(98)ht/97;
    Requardt a0910
      [non-local correlations and black-hole entropy, holography, entanglement].
  @ Strings and branes: Ellis et al PRD(01)ht/00 [interactions and GZK cutoff];
    Iqbal et al JHEP(08)ht/03 [topological strings];
    Hartnoll & Policastro ATMP(06)ht/04 [twistor string theory];
    Mavromatos AIP(09)-a0909,
    IJMPA(10)-a1010,
    JPCS(11)-a1010 [phenomenology];
    Mavromatos et al PLB(11) [and Finsler metrics];
    > s.a. phenomenology of cosmological perturbations [structure formation].
  @ Other models: Alberty PLB(89) [2D];
    Seriu PLB(93);
    Redmount & Suen PRD(93),
    PRD(94)gq/93;
    Nergiz & Saclioglu PRD(96)ht/95 [quasi-periodic Gibbons-Hawking metric];
    Zizzi IJTP(99) [and de Sitter space];
    Dzhunushaliev IJMPD(02)gq/00,
    gq/00-conf,
    FP(02)gq/01 [dielectric];
    Braden & Nekrasov CMP(04) [non-commutative instantons];
    Bernadotte & Klinkhamer PRD(07) [classical model with defects in Minkowski];
    Ng PLB(97)gq,
    Ent(08)-a0801,
    a1001-conf [holographic];
    Queiruga a1912 [non-metricity tensor];
    > s.a. quantum spacetime models;
      topology change; wormholes [gas].
Consequences
  > s.a. black-hole entropy; quantum-gravity
  phenomenology; gravitational thermodynamics.
  @ Gravity: Hawking PRD(96) [virtual black holes, black-hole evaporation];
    Garattini MPLA(98)gq,
    IJMPA(99)gq/98,
    ht/99-TX19 [black-hole pair production];
    Garattini NPPS(00)gq/99 [black-hole entropy, cosmological constant],
    IJMPD(02)gq/00 [cosmological constant];
    Dzhunushaliev IJMPD(02)gq/00,
      gq/00-conf [polarization by wormhole];
    Mäkelä & Peltola PRD(04)gq/03 [Schwarzschild horizon];
    Schulz FdP(18)-a1810 [cosmological constant, problem of time].
  @ Cosmology:
    Liu et al PRD(95) [entropy and flatness without inflation];
    Kirillov ap/07/MNRAS [dark energy, dark matter, etc];
    Arzano et al PLB(07) [holographic foam];
    Ng AIP(09)-a0808,
    a1910 [holographic foam and dark energy];
    > s.a. dark energy.
  @ Thermal properties: Garay PRL(98)gq,
    PRD(98)gq;
    Rosales gq/99 [electroweak coupling];
    Liu & Ma IJMP(00)gq/99;
    Agnese & La Camera NCB(01)gq/00 [black hole horizons];
    Garattini PLB(99)ht,
    Ent(00)gq,
    IJMPA(02)gq/01 [entropy].
  @ Field propagation, matter: Hawking PRD(96) [loss of coherence, Higgs particle, θQCD];
    Garay IJMPA(99)gq;
    Kirillov ht/00-proc [quantum field theory];
    Kirillov & Savelova a0806 [path integral and cutoff],
    a0808 [behavior of bosonic systems],
    G&C(08) [astrophysical effects];
    Mavromatos & Sarkar NJP(08) [model of flavour vacua];
    Kirillov et al PLB(08)-a0802 [cosmic-ray propagation];
    Sarkar FP(10) [neutral-kaon entanglement correlations];
    Savelova GRG(16)-a1405 [anisotropy in the vacuum speed of light, and dispersion];
    Oniga & Wang PRD(16)-a1603 [bosonic fields];
    > s.a. field theory phenomenology; matter
      phenomenology; photon phenomenology.
"When I hear that spacetime becomes a foam at the Planck scale, I don't reach for my gun. (I haven't any.)
  But I do wonder what that foam has to do with the macroscopic events that spacetime was constructed
  to represent and the macroscopic means we use to locate events.
  — N D Mermin
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