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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