The topological recursion is a construction in algebraic geometry. It takes as initial data a spectral curve: the data of                               (          Σ          ,                      Σ                          0                                ,          x          ,                      ω                          0              ,              1                                ,                      ω                          0              ,              2                                )                        , where:                     x        :        Σ        →                  Σ                      0                                   is a covering of Riemann surfaces with ramification points;                               ω                      0            ,            1                                   is a meromorphic differential 1-form on                     Σ                , regular at the ramification points;                               ω                      0            ,            2                                   is a symmetric meromorphic bilinear differential form on                               Σ                      2                                   having a double pole on the diagonal and no residue.
The topological recursion is then a recursive definition of infinite sequences of symmetric meromorphic n-forms                               ω                      g            ,            n                                   on                               Σ                      n                                  , with poles at ramification points only, for integers g≥0 such that 2g-2+n>0. The definition is a recursion on the integer 2g-2+n.
In many applications, the n-form                               ω                      g            ,            n                                   is interpreted as a generating function that measures a set of surfaces of genus g and with n boundaries. The recursion is on 2-2g-n the Euler characteristics, whence the name "topological recursion".
The topological recursion was first discovered in random matrices. One main goal of random matrix theory, is to find the large size asymptotic expansion of n-point correlation functions, and in some suitable cases, the asymptotic expansion takes the form of a power series. The n-form                               ω                      g            ,            n                                   is then the gth coefficient in the asymptotic expansion of the n-point correlation function. It was found that the coefficients                               ω                      g            ,            n                                   always obey a same recursion on 2g-2+n. The idea to consider this universal recursion relation beyond random matrix theory, and to promote it as a definition of algebraic curves invariants, occurred in Eynard-Orantin 2007 who studied the main properties of those invariants.
An important application of topological recursion was to Gromov-Witten invariants. Marino and BKMP conjectured that Gromov-Witten invariants of a toric Calabi-Yau 3-fold                                           X                                   are the TR invariants of a spectral curve that is the mirror of                                           X                                  .
Since then, topological recursion has generated a lot of activity in particular in enumerative geometry. The link to Givental formalism and Frobenius manifolds has been established.
(Case of simple branch points. For higher order branchpoints, see the section Higher order ramifications below)
For                     n        ≥        1                 and                     2        g        −        2        +        n        >        0                :
                              ω                      g            ,            n                          (                  z                      1                          ,                  z                      2                          ,        …        ,                  z                      n                          )        =                  ∑                      a            =                          branchpoints                                                Res                      z            →            a                                  K        (                  z                      1                          ,        z        ,                  σ                      a                          (        z        )        )                              (                                    ω                      g            ,            n            +            1                          (        z        ,                  σ                      a                          (        z        )        ,                  z                      2                          ,        …        ,                  z                      n                          )        +                  ∑                                                                      I                                      1                                                  ⊎                                  I                                      2                                                  =                {                                  z                                      2                                                  ,                …                ,                                  z                                      n                                                  }                                                              g                                      1                                                  +                                  g                                      2                                                  =                g                                              ′                          ω                                    g                              1                                      ,            1            +            #                          I                              1                                                    (        z        ,                  I                      1                          )                  ω                                    g                              2                                      ,            1            +            #                          I                              2                                                    (                  σ                      a                          (        z        )        ,                  I                      2                          )                              )                                  
where                     K        (                  z                      1                          ,                  z                      2                          ,                  z                      3                          )                 is called the recursion kernel:                     K        (                  z                      1                          ,                  z                      2                          ,                  z                      3                          )        =                                                                              1                  2                                                            ∫                                                      z                    ′                                    =                                      z                                          3                                                                                                            z                                          2                                                                                                  ω                                  0                  ,                  2                                            (                              z                                  1                                            ,                              z                ′                            )                                                      ω                                  0                  ,                  1                                            (                              z                                  2                                            )              −                              ω                                  0                  ,                  1                                            (                              z                                  3                                            )                                              
and                               σ                      a                                   is the local Galois involution near a branch point                     a                , it is such that                     x        (                  σ                      a                          (        z        )        )        =        x        (        z        )                . The primed sum                               ∑          ′                         means excluding the two terms                     (                  g                      1                          ,                  I                      1                          )        =        (        0        ,        ∅        )                 and                     (                  g                      2                          ,                  I                      2                          )        =        (        0        ,        ∅        )                .
For                     n        =        0                 and                     2        g        −        2        >        0                :
                              F                      g                          =                  ω                      g            ,            0                          =                              1                          2              −              2              g                                                         ∑                      a            =                          branchpoints                                                Res                      z            →            a                                            F                      0            ,            1                          (        z        )                  ω                      g            ,            1                          (        z        )                
with                     d                  F                      0            ,            1                          =                  ω                      0            ,            1                                   any antiderivative of                               ω                      0            ,            1                                  .
The definition of                               F                      0                          =                  ω                      0            ,            0                                   and                               F                      1                          =                  ω                      1            ,            0                                   is more involved and can be found in the original article of Eynard-Orantin.Main properties
Symmetry: each                               ω                      g            ,            n                                   is a symmetric                     n                -form on                               Σ                      n                                  .poles: each                               ω                      g            ,            n                                   is meromorphic, it has poles only at branchpoints, with vanishing residues.Homogeneity:                               ω                      g            ,            n                                   is homogeneous of degree                     2        −        2        g        −        n                . Under the change                               ω                      0            ,            1                          →        λ                  ω                      0            ,            1                                  , we have                               ω                      g            ,            n                          →                  λ                      2            −            2            g            −            n                                    ω                      g            ,            n                                  .Dilaton equation:                              ∑                      a            =                          branchpoints                                                Res                      z            →            a                                            F                      0            ,            1                          (        z        )                           ω                      g            ,            n            +            1                          (                  z                      1                          ,        …        ,                  z                      n                          ,        z        )        =        (        2        −        2        g        −        n        )                  ω                      g            ,            n                          (                  z                      1                          ,        …        ,                  z                      n                          )                
where                     d                  F                      0            ,            1                          =                  ω                      0            ,            1                                  .
Loop equations: The following forms have no poles at branchpoints                              ∑                      z            ∈                          x                              −                1                                      (            x            )                                    ω                      g            ,            n            +            1                          (        z        ,                  z                      1                          ,        …        ,                  z                      n                          )                
                              ∑                      {            z            ≠                          z              ′                        }            ⊂                          x                              −                1                                      (            x            )                                                (                                    ω                      g            ,            n            +            1                          (        z        ,                  z          ′                ,                  z                      2                          ,        …        ,                  z                      n                          )        +                  ∑                                                                      I                                      1                                                  ⊎                                  I                                      2                                                  =                {                                  z                                      2                                                  ,                …                ,                                  z                                      n                                                  }                                                              g                                      1                                                  +                                  g                                      2                                                  =                g                                                              ω                                    g                              1                                      ,            1            +            #                          I                              1                                                    (        z        ,                  I                      1                          )                  ω                                    g                              2                                      ,            1            +            #                          I                              2                                                    (                  z          ′                ,                  I                      2                          )                              )                                   where the sum has no prime, i.e. no term excluded.
Deformations: The                               ω                      g            ,            n                                   satisfy deformation equationsLimits: given a family of spectral curves                                                         S                                            t                                  , whose limit as                     t        →        0                 is a singular curve, resolved by rescaling by a power of                               t                      μ                                  , then                               lim                      t            →            0                                    t                      (            2            −            2            g            −            n            )            μ                                    ω                      g            ,            n                          (                                            S                                            t                          )        =                  ω                      g            ,            n                          (                  lim                      t            →            0                                    t                      μ                                                              S                                            t                          )                .Symplectic invariance: In the case where                     Σ                 is a compact algebraic curve with a marking of a symplectic basis of cycles,                     x                 is meromorphic and                               ω                      0            ,            1                          =        y        d        x                 is meromorphic and                               ω                      0            ,            2                          =        B                 is the fundamental second kind differential normalized on the marking, then the spectral curve                                           S                          =        (        Σ        ,                  C                ,        x        ,        y        d        x        ,        B        )                 and                                                                         S                            ~                                      =        (        Σ        ,                  C                ,        y        ,        −        x        d        y        ,        B        )                , have the same                               F                      g                                   shifted by some terms.Modular properties: In the case where                     Σ                 is a compact algebraic curve with a marking of a symplectic basis of cycles, and                               ω                      0            ,            2                          =        B                 is the fundamental second kind differential normalized on the marking, then the invariants                               ω                      g            ,            n                                   are quasi-modular forms under the modular group of marking changes. The invariants                               ω                      g            ,            n                                   satisfy BCOV equations.In case the branchpoints are not simple, the definition is amended as follows (simple branchpoints correspond to k=2):
                              ω                      g            ,            n                          (                  z                      1                          ,                  z                      2                          ,        …        ,                  z                      n                          )        =                  ∑                      a            =                          branchpoints                                                Res                      z            →            a                                            ∑                      k            =            2                                                                                o                  r                  d                  e                  r                                                            x                                      (            a            )                                    ∑                      J            ⊂                          x                              −                1                                      (            x            (            z            )            )            ∖            {            z            }            ,                        #            J            =            k            −            1                                    K                      k                          (                  z                      1                          ,        z        ,        J        )                  ∑                                    J                              1                                      ,            …            ,                          J                              ℓ                                      ⊢            J            ∪            {            z            }                                    ∑                                                                      I                                      1                                                  ⊎                …                                  I                                      ℓ                                                  =                {                                  z                                      2                                                  ,                …                ,                                  z                                      n                                                  }                                                              g                                      1                                                  +                ⋯                +                                  g                                      ℓ                                                  =                g                +                ℓ                −                k                                              ′                          ∏                      i            =            1                                k                                    ω                                    g                              i                                      ,            #                          J                              i                                      +            #                          I                              i                                                    (                  J                      i                          ,                  I                      i                          )                
The first sum is over partitions                               J                      1                          ,        …        ,                  J                      ℓ                                   of                     J        ∪        {        z        }                 with non empty parts                               J                      i                          ≠        ∅                , and in the second sum, the prime means excluding all terms such that                     (                  g                      i                          ,        #                  J                      i                          +        #                  I                      i                          )        =        (        0        ,        1        )                .
                              K                      k                                   is called the recursion kernel:
                              K                      k                          (                  z                      0                          ,                  z                      1                          ,        …        ,                  z                      k                          )        =                                                            ∫                                                      z                    ′                                    =                  ∗                                                                      z                                          1                                                                                                  ω                                  0                  ,                  2                                            (                              z                                  0                                            ,                              z                ′                            )                                                      ∏                                  i                  =                  2                                                  k                                            (                              ω                                  0                  ,                  1                                            (                              z                                  1                                            )              −                              ω                                  0                  ,                  1                                            (                              z                                  i                                            )              )                                              
The base point * of the integral in the numerator can be chosen arbitrarily in a vicinity of the branchpoint, the invariants                               ω                      g            ,            n                                   will not depend on it.
Topological recursion invariants and intersection numbers
The invariants                               ω                      g            ,            n                                   can be written in terms of intersection numbers of tautological classes
(*)                               ω                      g            ,            n                          (                  z                      1                          ,        …        ,                  z                      n                          )        =                  2                      3            g            −            3            +            n                                    ∑                      G            =                          Graphs                                                            1                          #                              Aut                            (              G              )                                                ∫                                    (                              ∏                                  v                  =                                      vertices                                                                                                                                          M                                        ¯                                                                                        g                                          v                                                        ,                                      n                                          v                                                                                  )                                                                ∏                      v            =                          vertices                                                e                                    ∑                              k                                                                                                          t                    ^                                                                              σ                (                v                )                ,                k                                                    κ                              k                                                              ∏                      (            p            ,                          p              ′                        )            =                          nodal points                                                (                      ∑                          d              ,                              d                ′                                                          B                          σ              (              p              )              ,              2              d              ;              σ              (                              p                ′                            )              ,              2                              d                ′                                                          ψ                          p                                      d                                            ψ                                          p                ′                                                                    d                ′                                              )                          ∏                                    p                              i                                      =                          marked points                                    i            =            1            ,            …            ,            n                                    (                      ∑                                          d                                  i                                                                          ψ                                          p                                  i                                                                                    d                                  i                                                              d                      ξ                          σ              (                              p                                  i                                            )              ,                              d                                  i                                                              (                      z                          i                                )          )                        
where the sum is over dual graphs of stable nodal Riemann surfaces of total arithmetic genus                     g                , and                     n                 smooth labeled marked points                               p                      1                          ,        …        ,                  p                      n                                  , and equipped with a map                     σ        :        {                  vertices                }        →        {                  branchpoints                }                .                               ψ                      p                          =                  c                      1                          (                                            L                                            p                          )                 is the Chern class of the cotangent line bundle                                                         L                                            p                                   whose fiber is the cotangent plane at                     p                .                               κ                      k                                   is the                     k                th Mumford's kappa class. The coefficients                                                                         t                ^                                                          a            ,            k                                  ,                               B                      a            ,            k            ;                          a              ′                        ,                          k              ′                                              ,                     d                  ξ                      a            ,            k                          (        z        )                , are the Taylor expansion coefficients of                               ω                      0            ,            1                                   and                               ω                      0            ,            2                                   in the vicinity of branchpoints as follows: in the vicinity of a branchpoint                     a                 (assumed simple), a local coordinate is                               ζ                      a                          (        z        )        =                              x            (            z            )            −            a                                  . The Taylor expansion of                               ω                      0            ,            2                          (        z        ,                  z          ′                )                 near branchpoints                     z        →        a                ,                               z          ′                →                  a          ′                         defines the coefficients                               B                      a            ,            d            ;                          a              ′                        ,                          d              ′                                              
                              ω                      0            ,            2                          (        z        ,                  z          ′                )                              ∼                                z            →            a            ,                                       z              ′                        →                          a              ′                                                        (                                                    δ                                  a                  ,                                      a                    ′                                                                              (                                  ζ                                      a                                                  (                z                )                −                                  ζ                                                            a                      ′                                                                      (                                  z                  ′                                )                                  )                                      2                                                                                +          2          π                      ∑                          d              ,                              d                ′                            =              0                                      ∞                                                                          B                                  a                  ,                  d                  ;                                      a                    ′                                    ,                                      d                    ′                                                                              Γ                (                                                                            d                      +                      1                                        2                                                  )                Γ                (                                                                                                    d                        ′                                            +                      1                                        2                                                  )                                                                    ζ                          a                                (          z                      )                          d                                            ζ                                          a                ′                                              (                      z            ′                                )                                          d                ′                                              )                d                  ζ                      a                          (        z        )        d                  ζ                                    a              ′                                      (                  z          ′                )                .
The Taylor expansion at                               z          ′                →        a                , defines the 1-forms coefficients                     d                  ξ                      a            ,            d                          (        z        )                
                    d                  ξ                      a            ,            d                          (        z        )        =                                            −              Γ              (              d              +                                                1                  2                                            )                                      Γ              (                                                1                  2                                            )                                                Res                                    z              ′                        →            a                                  (        x        (                  z          ′                )        −        a                  )                      −            d            −                                          1                2                                                              ω                      0            ,            2                          (        z        ,                  z          ′                )                 whose Taylor expansion near a branchpoint                               a          ′                         is
                    d                  ξ                      a            ,            d                          (        z        )                              ∼                                z            →                          a              ′                                                                                  −                              δ                                  a                  ,                                      a                    ′                                                              (              2              d              +              1              )              !              !              d                              ζ                                  a                                            (              z              )                                                      2                                  d                                                            ζ                                  a                                            (              z                              )                                  2                  d                  +                  2                                                                    +                  ∑                      k            =            0                                ∞                                                                              B                                  a                  ,                  2                  d                  ;                                      a                    ′                                    ,                  2                  k                                                            2                                  k                  +                  1                                                                    (              2              k              −              1              )              !              !                                                ζ                                    a              ′                                      (        z                  )                      2            k                          d                  ζ                                    a              ′                                      (        z        )                .
Write also the Taylor expansion of                               ω                      0            ,            1                                  
                              ω                      0            ,            1                          (        z        )                              ∼                                z            →            a                                            ∑                      k            =            0                                ∞                                    t                      a            ,            k                                                                       Γ              (                                                1                  2                                            )                                      (              k              +              1              )              Γ              (                                                                    k                    +                    1                                    2                                            )                                                         ζ                      a                          (        z                  )                      k                          d                  ζ                      a                          (        z        )                .
Equivalently, the coefficients                               t                      a            ,            k                                   can be found from expansion coefficients of the Laplace transform, and the coefficients                                                                         t                ^                                                          a            ,            k                                   are the expansion coefficients of the log of the Laplace transform
                              ∫                      x            (            z            )            −            x            (            a            )            ∈                                          R                                            +                                                              ω                      0            ,            1                          (        z        )                  e                      −            u            x            (            z            )                          =                                                            e                                  −                  u                  x                  (                  a                  )                                                                              π                                                                    2                              u                                  3                                      /                                    2                                                                              ∑                      k            =            0                                ∞                                    t                      a            ,            k                                    u                      −            k                          =                                                            e                                  −                  u                  x                  (                  a                  )                                                                              π                                                                    2                              u                                  3                                      /                                    2                                                                              e                      −                          ∑                              k                =                0                                            ∞                                                                                                          t                    ^                                                                              a                ,                k                                                    u                              −                k                                                             .
For example, we have
                              ω                      0            ,            3                          (                  z                      1                          ,                  z                      2                          ,                  z                      3                          )        =                  ∑                      a                                    e                                                                                          t                    ^                                                                              a                ,                0                                                    d                  ξ                      a            ,            0                          (                  z                      1                          )        d                  ξ                      a            ,            0                          (                  z                      2                          )        d                  ξ                      a            ,            0                          (                  z                      3                          )        .                
                              ω                      1            ,            1                          (        z        )        =        2                  ∑                      a                                    e                                                                                          t                    ^                                                                              a                ,                0                                                              (                                    1              24                                d                      ξ                          a              ,              1                                (          z          )          +                                                                                                                t                      ^                                                                                        a                  ,                  1                                            24                                d                      ξ                          a              ,              0                                (          z          )          +                                    1              2                                            B                          a              ,              0              ;              a              ,              0                                d                      ξ                          a              ,              0                                (          z          )          )                .                
The formula (*) generalizes ELSV formula as well as Mumford's formula and Mariño-Vafa formula.
M. Mirzakhani's recursion for hyperbolic volumes of moduli spaces is an instance of topological recursion. For the choice of spectral curve                               (                      C                    ;                                 C                    ;                     x          :          z          ↦                      z                          2                                ;                                 ω                          0              ,              1                                (          z          )          =                                    4              π                                z          sin                                (            π            z            )                    d          z          ;                                ω                          0              ,              2                                (                      z                          1                                ,                      z                          2                                )          =                                                    d                                  z                                      1                                                  d                                  z                                      2                                                                              (                                  z                                      1                                                  −                                  z                                      2                                                                    )                                      2                                                                                )                        
the n-form                               ω                      g            ,            n                          =                  d                      1                          …                  d                      n                                    F                      g            ,            n                                   is the Laplace transform of the Weil-Petersson volume
                              F                      g            ,            n                          (                  z                      1                          ,        …        ,                  z                      n                          )        =                  ∫                      0                                ∞                                    e                      −                          z                              1                                                    L                              1                                                    d                  L                      1                          …                  ∫                      0                                ∞                                    e                      −                          z                              n                                                    L                              n                                                    d                  L                      n                                            ∫                                                                      M                                                            g                ,                n                                      (                          L                              1                                      ,            …            ,                          L                              n                                      )                          w                
where                                                         M                                            g            ,            n                          (                  L                      1                          ,        …        ,                  L                      n                          )                 is the moduli space of hyperbolic surfaces of genus g with n geodesic boundaries of respective lengths                               L                      1                          ,        …        ,                  L                      n                                  , and                     w                 is the Weil-Petersson volume form.
The topological recursion for the n-forms                               ω                      g            ,            n                          (                  z                      1                          ,        …        ,                  z                      n                          )                , is then equivalent to Mirzakhani's recursion.
For the choice of spectral curve                               (                      C                    ;                                 C                    ;                     x          :          z          ↦                      z                          2                                ;                                 ω                          0              ,              1                                (          z          )          =          2                      z                          2                                d          z          ;                                ω                          0              ,              2                                (                      z                          1                                ,                      z                          2                                )          =                                                    d                                  z                                      1                                                  d                                  z                                      2                                                                              (                                  z                                      1                                                  −                                  z                                      2                                                                    )                                      2                                                                                )                        
the n-form                               ω                      g            ,            n                          =                  d                      1                          …                  d                      n                                    F                      g            ,            n                                   is
                              F                      g            ,            n                          (                  z                      1                          ,        …        ,                  z                      n                          )        =                  2                      2            −            2            g            −            n                                    ∑                                    d                              1                                      +            ⋯            +                          d                              n                                      =            3            g            −            3            +            n                                    ∏                      i            =            1                                n                                                              (              2                              d                                  i                                            −              1              )              !              !                                      z                              i                                            2                                  d                                      i                                                  +                1                                                                                  ⟨                          τ                                                d                                      1                                                                        …                          τ                                                d                                      n                                                                        ⟩                                g                                  
where                                           ⟨                          τ                                                d                                      1                                                                        …                          τ                                                d                                      n                                                                        ⟩                                g                                   is the Witten-Kontsevich intersection number of Chern classes of cotangent line bundles in the compactified moduli space of Riemann surfaces of genus g with n smooth marked points.
For the choice of spectral curve                               (                      C                    ;                                 C                    ;                     x          :          −          z          +          ln                                z                    ;                                 ω                          0              ,              1                                (          z          )          =          (          1          −          z          )          d          z          ;                                ω                          0              ,              2                                (                      z                          1                                ,                      z                          2                                )          =                                                    d                                  z                                      1                                                  d                                  z                                      2                                                                              (                                  z                                      1                                                  −                                  z                                      2                                                                    )                                      2                                                                                )                        
the n-form                               ω                      g            ,            n                          =                  d                      1                          …                  d                      n                                    F                      g            ,            n                                   is
                              F                      g            ,            n                          (                  z                      1                          ,        …        ,                  z                      n                          )        =                  ∑                      ℓ            (            μ            )            ≤            n                                    m                      μ                          (                  e                      x            (                          z                              1                                      )                          ,        …        ,                  e                      x            (                          z                              n                                      )                          )                          h                      g            ,                          μ                              1                                      ,            …            ,                          μ                              n                                                            
where                               h                      g            ,            μ                                   is the connected simple Hurwitz number of genus g with ramification $mu=(mu_1,dots,mu_n)$: the number of branch covers of the Riemann sphere by a genus g connected surface, with 2g-2+n simple ramification points, and one point with ramification profile given by the partition                     μ                .
Gromov-Witten numbers and the BKMP conjecture
Let                                           X                                   a toric Calabi-Yau 3-fold, with Kähler moduli                               t                      1                          ,        …        ,                  t                                    b                              2                                      (                                          X                                      )                                  . Its mirror manifold is singular over a complex plane curve                     Σ                 given by a polynomial equation                     P        (                  e                      x                          ,                  e                      y                          )        =        0                , whose coefficients are functions of the Kähler moduli. For the choice of spectral curve                               (          Σ          ;                                               C                                      ∗                                ;                     x          ;                                 ω                          0              ,              1                                =          y          d          x          ;                                ω                          0              ,              2                                )                         with                               ω                      0            ,            2                                   the fundamental second kind differential on                     Σ                ,
According to the BKMP conjecture, the n-form                               ω                      g            ,            n                          =                  d                      1                          …                  d                      n                                    F                      g            ,            n                                   is
                              F                      g            ,            n                          (                  z                      1                          ,        …        ,                  z                      n                          )        =                  ∑                                    d                        ∈                          H                              2                                      (                                          X                                      ,                          Z                        )                                    ∑                                    μ                              1                                      ,            …            ,                          μ                              n                                      ∈                          H                              1                                      (                                          L                                      ,                          Z                        )                                    t                      d                                    ∏                      i            =            1                                n                                    e                      x            (                          z                              i                                      )                                                              N                                            g                          (                              X                          ,                              L                          ;                  d                ,                  μ                      1                          ,        …        ,                  μ                      n                          )                
where                                                         N                                            g                          (                              X                          ,                              L                          ;                  d                ,                  μ                      1                          ,        …        ,                  μ                      n                          )        =                  ∫                      [                                                                                M                                    ¯                                                            g                ,                n                                      (                                          X                                      ,                                          L                                      ,                          d                        ,                          μ                              1                                      ,            …            ,                          μ                              n                                      )                          ]                                                v                  i                  r                                                                    1                
is the genus g Gromov-Witten number, representing the number of holomorphic maps of a surface of genus g into                                           X                                  , with n boundaries mapped to a special Lagrangian submanifold                                           L                                  .                               d                =        (                  d                      1                          ,        …        ,                  d                                    b                              2                                      (                                          X                                      )                          )                 is the 2nd relative homology class of the surface's image, and                               μ                      i                          ∈                  H                      1                          (                              L                          ,                  Z                )                 are homology classes (winding number) of the boundary images.
The BKMP conjecture has since then been proved.