Calabi–Yau manifold

A 2D slice of the 6D Calabi-Yau quintic manifold.

A Calabi–Yau manifold, also known as a Calabi–Yau space, is a special type of manifold that is described in certain branches of mathematics such as algebraic geometry. The Calabi–Yau manifold's properties, such as Ricci flatness, also yield applications in theoretical physics. Particularly in superstring theory, the extra dimensions of spacetime are sometimes conjectured to take the form of a 6-dimensional Calabi–Yau manifold, which led to the idea of mirror symmetry.

Calabi–Yau manifolds are complex manifolds that are generalizations of K3 surfaces in any number of complex dimensions (i.e. any even number of real dimensions). They were originally defined as compact Kähler manifolds with a vanishing first Chern class and a Ricci-flat metric, though many other similar but inequivalent definitions are sometimes used. They were named "Calabi–Yau spaces" by Candelas et al. (1985) after Eugenio Calabi (1954, 1957) who first conjectured that such surfaces might exist, and Shing-Tung Yau (1978) who proved the Calabi conjecture.

Definitions

The motivational definition given by Yau is of a compact Kähler manifold with a vanishing first Chern class, that is also Ricci flat.^[1] Calabi conjectured their existence and Yau proved the conjecture.

There are many other definitions of a Calabi–Yau manifold used by different authors, some inequivalent. This section summarizes some of the more common definitions and the relations between them.

A Calabi–Yau n-fold or Calabi–Yau manifold of (complex) dimension n is sometimes defined as a compact n-dimensional Kähler manifold M satisfying one of the following equivalent conditions:

• The canonical bundle of M is trivial.
• M has a holomorphic n-form that vanishes nowhere.
• The structure group of M can be reduced from U(n) to SU(n).
• M has a Kähler metric with global holonomy contained in SU(n).

These conditions imply that the first integral Chern class c₁(M) of M vanishes, but the converse is not true. The simplest examples where this happens are hyperelliptic surfaces, finite quotients of a complex torus of complex dimension 2, which have vanishing first integral Chern class but non-trivial canonical bundle.

For a compact n-dimensional Kähler manifold M the following conditions are equivalent to each other, but are weaker than the conditions above, and are sometimes used as the definition of a Calabi–Yau manifold:

• M has vanishing first real Chern class.
• M has a Kähler metric with vanishing Ricci curvature.
• M has a Kähler metric with local holonomy contained in SU(n).
• A positive power of the canonical bundle of M is trivial.
• M has a finite cover that has trivial canonical bundle.
• M has a finite cover that is a product of a torus and a simply connected manifold with trivial canonical bundle.

In particular if a compact Kähler manifold is simply connected then the weak definition above is equivalent to the stronger definition. Enriques surfaces give examples of complex manifolds that have Ricci-flat metrics, but their canonical bundles are not trivial so they are Calabi–Yau manifolds according to the second but not the first definition above. Their double covers are Calabi–Yau manifolds for both definitions (in fact K3 surfaces).

By far the hardest part of proving the equivalences between the various properties above is proving the existence of Ricci-flat metrics. This follows from Yau's proof of the Calabi conjecture, which implies that a compact Kähler manifold with a vanishing first real Chern class has a Kähler metric in the same class with vanishing Ricci curvature. (The class of a Kähler metric is the cohomology class of its associated 2-form.) Calabi showed such a metric is unique.

There are many other inequivalent definitions of Calabi–Yau manifolds that are sometimes used, which differ in the following ways (among others):

• The first Chern class may vanish as an integral class or as a real class.
• Most definitions assert that Calabi–Yau manifolds are compact, but some allow them to be non-compact. In the generalization to non-compact manifolds, the difference must vanish asymptotically. Here, is the Kähler form associated with the Kähler metric, (Gang Tian;Shing-Tung Yau 1990, 1991).
• Some definitions put restrictions on the fundamental group of a Calabi–Yau manifold, such as demanding that it be finite or trivial. Any Calabi–Yau manifold has a finite cover that is the product of a torus and a simply-connected Calabi–Yau manifold.
• Some definitions require that the holonomy be exactly equal to SU(n) rather than a subgroup of it, which implies that the Hodge numbers h^i,0 vanish for 0 < i < dim(M). Abelian surfaces have a Ricci flat metric with holonomy strictly smaller than SU(2) (in fact trivial) so are not Calabi–Yau manifolds according to such definitions.
• Most definitions assume that a Calabi–Yau manifold has a Riemannian metric, but some treat them as complex manifolds without a metric.
• Most definitions assume the manifold is non-singular, but some allow mild singularities. While the Chern class fails to be well-defined for singular Calabi–Yau's, the canonical bundle and canonical class may still be defined if all the singularities are Gorenstein, and so may be used to extend the definition of a smooth Calabi–Yau manifold to a possibly singular Calabi–Yau variety.

Examples

The most important fundamental fact is that any smooth algebraic variety embedded in a projective space is a Kähler manifold, because there is a natural Fubini–Study metric on a projective space which one can restrict to the algebraic variety. By definition, if ω is the Kähler metric on the algebraic variety X and the canonical bundle K_X is trivial, then X is Calabi–Yau. Moreover, there is unique Kähler metric ω on X such that [ω₀]=[ω]∈H²(X,R), a fact which was conjectured by Eugenio Calabi and proved by S. T. Yau (see Calabi conjecture).

In one complex dimension, the only compact examples are tori, which form a one-parameter family. The Ricci-flat metric on a torus is actually a flat metric, so that the holonomy is the trivial group SU(1). A one-dimensional Calabi–Yau manifold is a complex elliptic curve, and in particular, algebraic.

In two complex dimensions, the K3 surfaces furnish the only compact simply connected Calabi–Yau manifolds. Non simply-connected examples are given by abelian surfaces. Enriques surfaces and hyperelliptic surfaces have first Chern class that vanishes as an element of the real cohomology group, but not as an element of the integral cohomology group, so Yau's theorem about the existence of a Ricci-flat metric still applies to them but they are sometimes not considered to be Calabi–Yau manifolds. Abelian surfaces are sometimes excluded from the classification of being Calabi–Yau, as their holonomy (again the trivial group) is a proper subgroup of SU(2), instead of being isomorphic to SU(2).

In three complex dimensions, classification of the possible Calabi–Yau manifolds is an open problem, although Yau suspects that there is a finite number of families (albeit a much bigger number than his estimate from 20 years ago). In turn, it has also been conjectured by Miles Reid that the number of topological types of Calabi-Yau 3-folds is infinite, and that they can all be transformed continuously (through certain mild singularizations such as conifolds) one into another—much as Riemann surfaces can.^[2] One example of a three-dimensional Calabi–Yau manifold is a non-singular quintic threefold in CP⁴, which is the algebraic variety consisting of all of the zeros of a homogeneous quintic polynomial in the homogeneous coordinates of the CP⁴. Another example is a smooth model of the Barth–Nieto quintic. Some discrete quotients of the quintic by various Z₅ actions are also Calabi–Yau and have received a lot of attention in the literature. One of these is related to the original quintic by mirror symmetry.

For every positive integer n, the zero set of a non-singular homogeneous degree n+2 polynomial in the homogeneous coordinates of the complex projective space CPⁿ⁺¹ is a compact Calabi–Yau n-fold. The case n=1 describes an elliptic curve, while for n=2 one obtains a K3 surface.

All hyper-Kähler manifolds are Calabi–Yau.

Applications in superstring theory

Calabi–Yau manifolds are important in superstring theory. Essentially, Calabi–Yau manifolds are shapes that satisfy the requirement of space for the six "unseen" spatial dimensions of string theory, which may be smaller than our currently observable lengths as they have not yet been detected. A popular alternative known as large extra dimensions, which often occurs in braneworld models, is that the Calabi–Yau is large but we are confined to a small subset on which it intersects a D-brane.

In the most conventional superstring models, ten conjectural dimensions in string theory are supposed to come as four of which we are aware, carrying some kind of fibration with fiber dimension six. Compactification on Calabi–Yau n-folds are important because they leave some of the original supersymmetry unbroken. More precisely, in the absence of fluxes, compactification on a Calabi–Yau 3-fold (real dimension 6) leaves one quarter of the original supersymmetry unbroken if the holonomy is the full SU(3).

More generally, a flux-free compactification on an n-manifold with holonomy SU(n) leaves 2¹⁻ⁿ of the original supersymmetry unbroken, corresponding to 2⁶⁻ⁿ supercharges in a compactification of type II supergravity or 2⁵⁻ⁿ supercharges in a compactification of type I. When fluxes are included the supersymmetry condition instead implies that the compactification manifold be a generalized Calabi–Yau, a notion introduced by Hitchin (2003). These models are known as flux compactifications.

F-theory compactifications on various Calabi–Yau four-folds provide physicists with a method to find a large number of classical solution in the so-called string theory landscape.

Connected with each hole in the Calabi-Yau space is a group of low-energy string vibrational patterns. Since string theory states that our familiar elementary particles correspond to low-energy string vibrations, the presence of multiple holes causes the string patterns to fall into multiple groups, or families. Although the following statement has been simplified, it conveys the logic of the argument: if the Calabi-Yau has three holes, then three families of vibrational patterns and thus three families of particles will be observed experimentally.

Logically, since strings vibrate through all the dimensions, the shape of the curled-up ones will affect their vibrations and thus the properties of the elementary particles observed. For example, Andrew Strominger and Edward Witten have shown that the masses of particles depend on the manner of the intersection of the various holes in a Calabi-Yau. In other words, the positions of the holes relative to one another and to the substance of the Calabi-Yau space was found by Strominger and Witten to affect the masses of particles in a certain way. This, of course, is true of all particle properties.^[3]

See also

• G2 manifold
• Calabi–Yau algebra

References

Citations

1. ↑ Yau and Nadis (2010)
2. ↑ Reid, Miles (1987), "The Moduli Space of 3-Folds with K = 0 May Nevertheless be Irreducible", Math. Ann., 278, 329
3. ↑ "The Shape of Curled-Up Dimensions". Archived from the original on Sep 13, 2006. Retrieved 2006.  Check date values in: |access-date= (help)

Bibliography

• Besse, Arthur L. (1987), Einstein manifolds, Ergebnisse der Mathematik und ihrer Grenzgebiete (3), 10, Berlin, New York: Springer-Verlag, ISBN 978-3-540-15279-8, OCLC 13793300 
• Chan,Yat-Ming (2004)"Desingularization Of Calabi–Yau 3-Folds With A Conical Singularity"
• Calabi, Eugenio (1954), "The space of Kähler metrics", Proc. Internat. Congress Math. Amsterdam, 2, pp. 206–207 
• Calabi, Eugenio (1957), "On Kähler manifolds with vanishing canonical class", in Fox, Ralph H.; Spencer, D. C.; Tucker, A. W., Algebraic geometry and topology. A symposium in honor of S. Lefschetz, Princeton Mathematical Series, 12, Princeton University Press, pp. 78–89, MR 0085583 
• Greene, Brian "String Theory On Calabi–Yau Manifolds"
• Candelas, Philip; Horowitz, Gary; Strominger, Andrew; Witten, Edward (1985), "Vacuum configurations for superstrings", Nuclear Physics B, 258: 46–74, Bibcode:1985NuPhB.258...46C, doi:10.1016/0550-3213(85)90602-9 
• Gross, M.; Huybrechts, D.; Joyce, Dominic (2003), Calabi–Yau manifolds and related geometries, Universitext, Berlin, New York: Springer-Verlag, ISBN 978-3-540-44059-8, MR 1963559, OCLC 50695398 
• Hitchin, Nigel (2003), "Generalized Calabi–Yau manifolds", The Quarterly Journal of Mathematics, 54 (3): 281–308, arXiv:math.DG/0209099, doi:10.1093/qmath/hag025, MR 2013140 
• Hübsch, Tristan (1994), Calabi–Yau Manifolds: a Bestiary for Physicists, Singapore, New York: World Scientific, ISBN 981-02-1927-X, OCLC 34989218 
• Im, Mee Seong (2008) "Singularities-in-Calabi-Yau-varieties.pdf Singularities in Calabi–Yau varieties"
• Joyce, Dominic (2000), Compact Manifolds with Special Holonomy, Oxford University Press, ISBN 978-0-19-850601-0, OCLC 43864470 
• Tian, Gang; Yau, Shing-Tung (1990), "Complete Kähler manifolds with zero Ricci curvature, I", Amer. Math. Soc., 3 (3): 579–609, doi:10.2307/1990928, JSTOR 1990928 
• Tian, Gang; Yau, Shing-Tung (1991), "Complete Kähler manifolds with zero Ricci curvature, II", Invent. Math., 106 (1): 27–60, Bibcode:1991InMat.106...27T, doi:10.1007/BF01243902 
• Yau, Shing Tung (1978), "On the Ricci curvature of a compact Kähler manifold and the complex Monge-Ampère equation. I", Communications on Pure and Applied Mathematics, 31 (3): 339–411, doi:10.1002/cpa.3160310304, MR 480350 
• Yau, Shing-Tung (2009), "Surveys in differential geometry. Vol. XIII. Geometry, analysis, and algebraic geometry: forty years of the Journal of Differential Geometry", Scholarpedia, Surv. Differ. Geom., Somerville, Massachusetts: Int. Press, 4 (8): 277–318, Bibcode:2009SchpJ...4.6524Y, doi:10.4249/scholarpedia.6524, MR 2537089  |chapter= ignored (help)
• Yau, Shing-Tung and Nadis, Steve; The Shape of Inner Space, Basic Books, 2010.

External links

Wikimedia Commons has media related to Calabi-Yau variety.

• Calabi–Yau Homepage is an interactive reference which describes many examples and classes of Calabi–Yau manifolds and also the physical theories in which they appear.
• Spinning Calabi–Yau Space video.
• Calabi–Yau Space by Andrew J. Hanson with additional contributions by Jeff Bryant, Wolfram Demonstrations Project.
• Weisstein, Eric W. "Calabi–Yau Space". MathWorld. 

• Yau, S. T., Calabi–Yau manifold, Scholarpedia  (similar to (Yau 2009))

String theory
Background	Strings History of string theory First superstring revolution Second superstring revolution String theory landscape
Theory	Nambu–Goto action Polyakov action Bosonic string theory Superstring theory Type I string Type II string Type IIA string theory Type IIB string theory Heterotic string N=2 superstring F-theory String field theory Matrix string theory Nonlinear sigma model Tachyon condensation RNS formalism
Concepts	String duality T-duality S-duality U-duality Montonen–Olive duality Mysterious duality Particles and fields Graviton Dilaton Tachyon Ramond–Ramond field Kalb–Ramond field Magnetic monopole Branes D-brane S-brane Black brane Black holes Black string Brane cosmology Quiver diagram Hanany–Witten transition
Conformal field theory	Virasoro algebra Mirror symmetry Conformal anomaly Conformal algebra Superconformal algebra Vertex operator algebra Loop algebra Kac–Moody algebra Wess–Zumino–Witten model
Gauge theory	Anomalies Instantons Chern–Simons form Bogomol'nyi–Prasad–Sommerfield bound Exceptional Lie groups (G2, F4, E6, E7, E8) ADE classification Dirac string P-form electrodynamics
Geometry	Kaluza–Klein theory Compactification Why 10 dimensions? Kähler manifold Ricci-flat manifold Calabi–Yau manifold Hyperkähler manifold K3 surface G2 manifold Spin(7) manifold Generalized complex manifold Orbifold Conifold Orientifold Moduli space Hořava–Witten domain wall K-theory (physics) Twisted K-theory
Supersymmetry	Supergravity Superspace Lie superalgebra Lie supergroup
Holography	Holographic principle AdS/CFT correspondence
M-theory	Matrix theory Introduction to M-theory
String theorists	Nima Arkani-Hamed Michael Francis Atiyah Tom Banks David Berenstein Gerald Cleaver Robbert Dijkgraaf Jacques Distler Michael Douglas Michael Duff Sergio Ferrara Willy Fischler Daniel Friedan Rajesh Gopakumar Michael Green Brian Greene David Gross Steven Gubser Sergei Gukov Jeffrey Harvey Petr Hořava Gary Gibbons Michio Kaku Renata Kallosh Theodor Kaluza Anton Kapustin Igor Klebanov Oskar Klein Hong Liu Juan Maldacena Donald Marolf Emil Martinecm Shiraz Minwalla Gregory Moore Lubos Motl Sunil Mukhi Robert Myers Asad Naqvi K. S. Narain Horatiu Nastase Nikita Nekrasov André Neveu Dimitri Nanopoulos Holger Bech Nielsen Peter van Nieuwenhuizen Hirosi Ooguri Joseph Polchinski Alexander Polyakov Arvind Rajaraman Lisa Randall Seifallah Randjbar-Daemi Martin Roček John H. Schwarz Nathan Seiberg Ashoke Sen Steve Shenker Warren Siegel Eva Silverstein Matthias Staudacher Andrew Strominger Leonard Susskind Paul Townsend Sandip Trivedi Cumrun Vafa Gabriele Veneziano Erik Verlinde Herman Verlinde Edward Witten Tamiaki Yoneya Alexander Zamolodchikov Alexei Zamolodchikov Barton Zwiebach