In General
* Idea: Non-singular,
complete solutions to the Euclideanized vacuum Einstein equation with or without
a cosmological constant, i.e., regular, real, Ricci-flat
or Einstein
Riemannian manifolds; Used to calculate tunneling probability amplitudes
in semiclassical quantum cosmology.
* Applications: Since
they represent local minima of the Euclideanized action, they are used in
the path integral approach to approximate amplitudes by perturbing
around them; Also used to deduce thermodynamic properties of black holes.
Special Solutions
@ Taub-Bolt: Mars & Simon JGP(99)gq/98 [uniqueness];
Fatibene et al AP(00)gq/99 [entropy];
Garfinkle & Mann CQG(00) [entropy]; Awad CQG(06)
[higher-dimensional].
@ Inflationary universes: Firouzjahi et al JHEP(04)ht [modified
Hartle-Hawking wave function in brane world].
@ Bianchi models: Barrow et al CQG(00)gq/99 [VI0 and
VII0];
Saffin PLB(99)gq [IX].
@ Black hole pair creation: Branoff & Brill gq/98-in;
Booth & Mann
PRL(98)gq,
NPB(99)gq/98 [charged,
rotating]; > s.a. quantum black holes.
@ Related topics: D'Auria & Regge NPB(82);
Nergiz & Saclioglu
PRD(96)ht/95 [and
foam]; Nutku PRL(96)
[and minimal surfaces]; Nutku et al CQG(97);
Hunter PRD(99)gq/98 [U(1)
symmetry, NUT
charge];
Nutku & Sheftel
gq/01 [axisymmetric, "heavenly"];
Demetrian PS(06)gq/04 [Coleman-de
Luccia, second-order]; Yang & Salizzoni PRL(06)ht/05 [from
non-commutative gauge theory instantons]; Etesi PLB(06)
[asymptotically flat, topology].
References > s.a. null infinity [BMS group]; unimodular
gravity.
@ General: Gibbons & Hawking PRD(77);
Hawking PLA(77),
in(79); Gibbons & Perry PRD(80);
Pope in(81); Rubakov & Tinyakov
PLB(88);
Mellor & Moss CQG(89);
Lorenz-Petzold
PTP(89);
't Hooft NPB(89); Ó Murchadha & Shanahan PRL(93);
Marathe & Martucci
NCB(98).
@ New variables: Samuel CQG(88);
Capovilla et al CQG(90);
Torre PLB(90);
Chang & Soo ht/92; Ishihara et al IJMPA(96)gq/95.
@ NP formalism: Goldblatt GRG(94); Aliev & Nutku gq/98 [hyper-Kähler
structure].
@ With matter / Kaluza-Klein: Copeland et al JHEP(00)ht [scalar];
Gray & Copeland
JHEP(01)gq [scalar
+ form in high-D].
@ In quantum cosmology: Bousso & Linde PRD(98)gq;
Garriga PRD(00)ht/98, ht/98;
Turok PLB(99)gq [stability
of Minkowski].
@ Singular instantons: Vilenkin PRD(98)ht;
Hashimoto PRD(01)
[action]; Kirklin et al PRD(01)
[made regular]; > s.a. inflation [from quantum
cosmology].
@ Entropy, topology: Liberati & Pollifrone PRD(97)ht.
@ And black hole radiation: Massar & Parentani PRL(97)gq.
@ Uniqueness results: Simon CQG(95)gq [Kerr
spacetime].
@ Perturbations: Torre PRD(90); Dunne & Wang PRD(06)
[bounce with scalar field].
@ Applications: Moss PLB(92);
Allen ap/99-in
[in cosm]; Xue ht/06 [and
the cosmological constant].
@ Related topics: Jibu & Yasue PLA(92)
[and Euclidean quantum mechanics]; Brill & Pirk in(93)gq/93 [pictures];
Bakas et al PLB(98)
[octonionic]; Ratcliffe & Tschantz
CQG(98)
[constant curvature], CQG(00)
[spin and complex structures], CQG(00)gq [growth
with V and Hartle-Hawking wave function].
> Related topics:
see quantum field theory in curved backgrounds [particle
creation].
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Send feedback and suggestions to bombelli at olemiss.edu – Modified
15 jul 2008