Exotic Smooth 4-Manifolds and Gerbes as Geometry for QG
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Exotic Smooth 4-Manifolds and Gerbes as Geometry for QG
Exotic Smooth 4-Manifolds and Gerbes as Geometry for QG Jerzy Król University of Silesia Katowice, Poland 14 wrze±nia 2009 Matter to the Deepest USTRO 2009 Jerzy Król (US Katowice) Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 1 / 19 Motivations Classical gravity is described by GR: spacetime is a smooth manifold a pseudo-Riemannian metric g action for GR, in the absence of any other matter, is where (X , g ) R X with satisfying Einstein's eld equations. The S (X , g ) = X Rd volg R is the scalar curvature. The critical point for this action is just which describes both, gravity and geometry. Jerzy Król (US Katowice) Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 2 / 19 Motivations Classical gravity is described by GR: spacetime is a smooth manifold a pseudo-Riemannian metric g action for GR, in the absence of any other matter, is where (X , g ) R X with satisfying Einstein's eld equations. The S (X , g ) = X Rd volg R is the scalar curvature. The critical point for this action is just which describes both, gravity and geometry. What is geometry for quantum gravity? Jerzy Król (US Katowice) Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 2 / 19 Motivations Classical gravity is described by GR: spacetime is a smooth manifold a pseudo-Riemannian metric g action for GR, in the absence of any other matter, is where (X , g ) R X with satisfying Einstein's eld equations. The S (X , g ) = X Rd volg R is the scalar curvature. The critical point for this action is just which describes both, gravity and geometry. What is geometry for quantum gravity? ∗ Assume that QG, at least in some limit, is given by superstring theory. Jerzy Król (US Katowice) Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 2 / 19 Motivations Classical gravity is described by GR: spacetime is a smooth manifold a pseudo-Riemannian metric g action for GR, in the absence of any other matter, is where (X , g ) R X with satisfying Einstein's eld equations. The S (X , g ) = X Rd volg R is the scalar curvature. The critical point for this action is just which describes both, gravity and geometry. What is geometry for quantum gravity? ∗ Assume that QG, at least in some limit, is given by superstring theory. Then, spacetime as a smooth manifold at the fundamental level is meaningless. Jerzy Król (US Katowice) Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 2 / 19 Instead, we have string backgrounds. Jerzy Król (US Katowice) Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 3 / 19 Instead, we have string backgrounds. These backgrounds are described by 2-dim. CFT and Jerzy Król (US Katowice) Ustro«: Exotics, Gerbes and QG σ -models. 14 wrze±nia 2009 3 / 19 Instead, we have string backgrounds. These backgrounds are described by 2-dim. CFT and σ -models. They have the classical limit where geometry emerges: Jerzy Król (US Katowice) Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 3 / 19 Instead, we have string backgrounds. These backgrounds are described by 2-dim. CFT and σ -models. They have the classical limit where geometry emerges: Classical geometry from string theory are the triples (M , g , B ) where B (B-eld) is a local 2-form. Jerzy Król (US Katowice) Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 3 / 19 Conversely, given a classical string background (M , g , B ) one has the corresponding CFT and the string background. It is believed that every string background emerges in this way: UΣ ({γ1 , ..., γp }, {γp+1,...,γp+q }) = where γi are the boundary of all of the transportation along Jerzy Król (US Katowice) Σ R {φ:Σ→M } Σ's e iS (φ,B ) in the integral and from one set of γ 's Ustro«: Exotics, Gerbes and QG UΣ is the operator to the other. 14 wrze±nia 2009 4 / 19 B eld on M is the same as gerbe - the object from dierential geometry M. which is a generalization of bundles on (Abelian) Gerbes are classied by Jerzy Król (US Katowice) H 3 (M , Z). Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 5 / 19 This talk (based on the joint work with Torsten Asselmeyer-Maluga): Exotic smooth R4 's are related to gerbes and backgrounds of string theory. The geometry of QG refers to exotic 4-structures. Exotic R4 's are as fundamental for QG as the standard R4 for classical gravity: i. ii. Some eects of QG in spacetime can be locally cancelled by the suitable choice of exotic smooth structure on R4 . Exotic R4 's contain also quantum information of spacetime and gravity. The quantization of electric charge can be explained with exotic R4 instead of magnetic monopoles. Jerzy Król (US Katowice) Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 6 / 19 R4 : the early days 1 Exotic Smooth 2 Exotic 4-smoothness in (Q)Gravity and QFT Jerzy Król (US Katowice) Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 7 / 19 Exotic Smooth R4 : the early days Early Days of Exotic Smooth R4 Freedman (1982): there exists the smoothness of a topological R4 which is non-dieomorphic to the standard one (agreeing with the topological product of axes). Soon after Gompf showed that there are at least 3 such dierent smoothings. Next, Taubes proved, via physical Yang-Mills theories techniques of Donaldson, that there are innite smoothings of R4 . In any other dimension than Exotic R4 's continuum many such dierent four there exists only one such smooth Rn . are ordinary manifolds some of them have nite number of local coordinate patches (say 3,5...). The usual tools and techniques of dierential geometry and topology from higher and lower dimensions, fail in dimension 4. We do not have clear idea what the tools should be. Jerzy Król (US Katowice) Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 8 / 19 Exotic Smooth R4 : the early days 4 is the physical dimension and general relativity of Einstein can be formulated on any (exotic) smooth manifold. Brans (1994) conjectured and Asselmeyer (1996) and Sªadkowski (1999) proved, that exotic smooth R4 can act as sources for gravitational eld in 4-spacetime. continuum many dierent smooth R4 's, nobody can give even one example of exotic smooth function in any of the smooth structure. There exist innite This is a true limitation for physical applications and our mathematical understanding. Jerzy Król (US Katowice) Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 9 / 19 Exotic Smooth R4 : the early days What to do? It was proposed (JK, 2004) to use the tools of model theory and topoi. As the result the conjectures were formulated and analyzed: i. ii. The suitable choice of exotic smooth R4 can compensate some local eects (in spacetime) assigned to QG. Hence, exotic R4 's for QG are similarly fundamental as the standard R4 for classical gravity and (pseudo-)Riemannian 4-geometry. In the AdS/CFT correspondence the exotic 4-structures can cause the additional susy breaking (important for approaching the realistic QCD). Jerzy Król (US Katowice) Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 10 / 19 Exotic 4-smoothness in (Q)Gravity and QFT Exotic 4-smoothness in (Q)Gravity and QFT: exact results Still, the explicit calculations in local coordinate patches (and which are exotic smooth) were absent. Torsten Asselmeyer-Maluga, JK, hep-th/0904.1276: Take special S3 embedded in R4 and measure the relative changes of 4-smoothness on various structures on this S 3. The structures are: 3 1. Hoeiger co-dimension-1 foliations of S . 2. Z2 orbifolds of WZW model on S 3. 3. Generalized Hitchin's structures and 4. Groupoids U (1)-gerbes on S 3 . SU (2) × SU (2) ⇒ SU (2). Jerzy Król (US Katowice) Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 11 / 19 Exotic 4-smoothness in (Q)Gravity and QFT 1. Hoeiger co-dimension-1 foliations of S 3 , then: Dierent smooth R4 's correspond to dierent classes of Hoeiger foliations of S 3 , i.e. correspond to classes H 3 (S 3 , R). Jerzy Król (US Katowice) Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 12 / 19 Exotic 4-smoothness in (Q)Gravity and QFT 2. Given S 3 ' SU (2) we have WZW SU (2) models on this S 3 , then in the case 3 3 of H (S , Z)): Dierent smoothness of R4 correspond to the levels k of the Z2 orbifold of WZW model on SU(2). These appear as background solutions of some 5-branes congurations of sustring theory, hence QG. Jerzy Król (US Katowice) Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 13 / 19 Exotic 4-smoothness in (Q)Gravity and QFT 3. Abelian gerbes on H 3 (S 3 , Z) ' Z. S3 correspond to the integral cohomology classes Generalized Hitchin's structures on S3 can be dened, then: Dierent smoothness of R4 correspond to the deformed by U (1) gerbes generalized Hitchin's structures on S 3 . Again, the generalized complex structures and geometries of Hitchin play important role in ux compactication in string theory. Jerzy Król (US Katowice) Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 14 / 19 Exotic 4-smoothness in (Q)Gravity and QFT 4. A groupoid structure thus emerges: Dierent exotic smooth R4 's correspond to the deformed by S 1 -gerbes equivariant cohomologies of the groupoid SU (2) × SU (2) ⇒ SU (2), where SU (2) acts on itself by conjugations. These cohomologies are just the Verlinde algebras of SU (2) at the level k (Freed, Teleman, Hopkins, 2002). Jerzy Król (US Katowice) Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 15 / 19 Exotic 4-smoothness in (Q)Gravity and QFT Exotic smooth R4 's are surprisingly and deeply involved in the description of quantum gravity. Geometry of string theory is based rather on locally exotic than standard smooth 4-manifolds. Jerzy Król (US Katowice) Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 16 / 19 Exotic 4-smoothness in (Q)Gravity and QFT QFT The quantization of electric charge without magnetic monopoles: Some exotic R4 's in a region of 4-spacetime can act as the sources of the magnetic eld in this spacetime, hence give the condition for the quantization of electric charge. The theories with monopoles or monopolium give rise to the corrections of certain cross sections of processes like 4 the contributions from exotic R 's. e +e − or γγ . These can be seen as Some non-perturbative limits of a QCD-like YM theory can be reached when the theory is formulated on 4-manifolds which are locally exotic R4 . (monopoles are non-perturbative objects in eld theory and the dual, supersymmetric theory has monopoles as ground states (Witten, 2002)). Jerzy Król (US Katowice) Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 17 / 19 Exotic 4-smoothness in (Q)Gravity and QFT Meta-remarks (philosophical) Exotic R4 's should not be seen through their topological coordinate axes. Rather, these are non-reducible states of the axes. Due to this they contain also quantum information about spacetime, hence quantum gravity. Exotic 4-smoothness agrees rather with generalized topology than standard product topology. String theory favors geometry of manifolds with the presence of which is connected with exotic Jerzy Król (US Katowice) R4 B -eld, rather than standard one. Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 18 / 19 Exotic 4-smoothness in (Q)Gravity and QFT G. Segal, Topological structures in string theory, London, A359, 1389 (2001). Phil. Trans. Royal Soc. SU (2) models and exotic Comm. Math. Phys., hep-th/0904.1276. T.Asselmeyer-Maluga, J.Król, 2009, Gerbes, WZW smooth R4 , submitted to T. Asselmeyer, 1996, Generation of source terms in general relativity by dierential structures. Class. Quant. Grav., 14:749 758, 1996. J. Sªadkowski, 2001, Gravity on exotic Phys. D, 10, 311313 (2001). R4 with few symmetries, Int.J. Mod. J. Król, Exotic smoothness and non-commutative spaces. The model-theoretic approach. Found. of Physics, 34:843869, 2004. J. Król, 2005, Model theory and the AdS/CFT correspondence, hep-th/0506003. Jerzy Król (US Katowice) Ustro«: Exotics, Gerbes and QG 14 wrze±nia 2009 19 / 19