UTHEP- 773 The Fokker-Planck formalism for closed bosonic strings Nobuyuki Ishibashi

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UTHEP- 773
The Fokker-Planck formalism for closed bosonic strings
Nobuyuki Ishibashi
Tomonaga Center for the History of the Universe,
University of Tsukuba
Tsukuba, Ibaraki 305-8571, JAPAN
Abstract
Every Riemann surface with genus gand npunctures admits a hyperbolic metric, if 2g2+n>0. Such
a surface can be decomposed into pairs of pants whose boundaries are geodesics. We construct a string
field theory for closed bosonic strings based on this pants decomposition. In order to do so, we derive
a recursion relation satisfied by the off-shell amplitudes, using the Mirzakhani’s scheme for computing
integrals over the moduli space of bordered Riemann surfaces. The recursion relation can be turned into
a string field theory via the Fokker-Planck formalism. The Fokker-Planck Hamiltonian consists of kinetic
terms and three string vertices. Unfortunately, the worldsheet BRST symmetry is not manifest in the
theory thus constructed. We will show that the invariance can be made manifest by introducing auxiliary
fields.
e-mail: ishibashi.nobuyuk.ft@u.tsukuba.ac.jp
arXiv:2210.04134v2 [hep-th] 23 Jan 2023
1 Introduction
For constructing a string field theory (SFT), we should specify a rule to cut worldsheets into fundamental
building blocks, i.e. propagators and vertices. A few simple rules were proposed and SFTs for bosonic strings
were constructed following these rules [1–4]. Construction of an SFT for superstrings is more complicated
because of the spurious singularities [5].
The worldsheets of closed strings describing scattering amplitudes are punctured Riemann surfaces. In
mathematics, there exists a convenient way to decompose them into fundamental building blocks. On a
Riemann surface with genus gand nboundaries or punctures, one can introduce a metric with constant
negative curvature, if 2g2+n>0. Such a metric is called a hyperbolic metric and surfaces with hyperbolic
metrics are called hyperbolic surfaces. With a hyperbolic metric, one can decompose the surface into pairs of
pants with geodesic boundaries. It may be possible to consider the pair of pants as the fundamental building
block of the surface.
The hyperbolic metric was used to construct SFT in [6–8], in which the kinetic term of the action was
taken to be the conventional one Ψc
0QΨ,(1.1)
so that the propagators correspond to cylinders. The theories include infinitely many vertices besides the
three string vertex and the Feynman graphs have nothing to do with the pants decomposition. In this paper,
we would like to construct an SFT based on the pants decomposition. Namely, we will construct an SFT for
closed bosonic strings regarding the pair of pants as the three string vertex and the cylinders with vanishing
heights as the propagator, as depicted in Figure 1.
In such a theory, a state of string will correspond to a boundary of a pair of pants. Accordingly, the
string field should be labeled by an element of the Hilbert space of the first quantized strings and the length
Lof the boundary. The external states of the scattering amplitudes are regarded as the limit L0of such
states. The off-shell amplitudes may correspond to Riemann surfaces which have geodesic boundaries with
fixed lengths and will be expressed by integrals over the moduli spaces of such surfaces.
Unfortunately, such an approach suffers from a problem addressed in [9] (section IV. E). The three
string vertex will be given by the correlation function of the worldsheet theory on hyperbolic pants with
the boundary lengths specified. Suppose that one calculates the one loop one point function following
the conventional Feynman rules. The amplitude corresponds to the worldsheet in Figure 2 and we should
integrate over the length land the twist angle θ. By doing so, the fundamental domain of the modular group
is covered infinitely many times, as will be seen in section 4.3. The same happens for all the other amplitudes.
Therefore, the conventional Feynman rule with the vertex and the propagator in Figure 1 does not yield the
correct amplitudes.
In order to overcome this problem, we formulate the theory using the Mirzakhani’s scheme [10, 11] for
computing integrals over moduli space of bordered Riemann surfaces. Mirzakhani derived a recursion relation
for the volume of the moduli space. Applying her method to the off-shell amplitudes of closed bosonic strings,
we derive a recursion relation satisfied by these amplitudes.
As was pointed out in [12, 13], Mirzakhani’s recursion relation is related to the loop equation of minimal
string theory. On the other hand, the loop equations for minimal strings can be described by an SFT via
the Fokker-Planck formalism [14, 15]. We will show that the recursion relation of the off-shell amplitudes
can be described by an SFT using the Fokker-Planck formalism. The Fokker-Planck Hamiltonian consists of
kinetic terms and three string vertices. One can develop perturbation theory which does not suffer from the
above mentioned problem. Unfortunately, the worldsheet BRST symmetry is not manifest in the SFT thus
constructed. We will show that we can make the invariance manifest by introducing auxiliary fields.
The organization of this paper is as follows. In section 2, we define the off-shell amplitudes of closed
bosonic string theory based on the moduli space of bordered Riemann surfaces. In section 3, we derive
recursion relations satisfied by the off-shell amplitudes. In section 4, we prove that the off-shell amplitudes
defined in section 2 can be derived from the Fokker-Planck formalism for string fields. We show that the
solution of the recursion relations in section 3 satisfies the Schwinger-Dyson equation derived from the Fokker-
Planck Hamiltonian. In section 5, we modify the theory by introducing auxiliary fields and make it manifestly
1
Figure 1: A pants decomposition.
Figure 2: One loop one point function.
BRST invariant. Section 6 is devoted to discussions and comments. In Appendix A, we present formulas for
the local coordinates on hyperbolic pants. In appendix B, we prove the BRST identity.
2 Off-shell amplitudes
The off-shell amplitudes of the theory we will study should correspond to hyperbolic surfaces which have
geodesic boundaries with fixed lengths. In this section, we would like to define such amplitudes. The
formulation is a modification of the conventional ones [4, 16–18].
2.1 The moduli space Mg,n,L
Let Σg,n,Lwith L=(L1,, Ln)be a genus ghyperbolic surface with ngeodesic boundaries (labeled by an
index a=1,, n) whose lengths are L1,, Ln. Cutting the surface Σg,n,Lalong non-peripheral simple closed
geodesics, we can decompose it into pairs of pants Si(i=1,2g2+n). There are many choices for such
decomposition and here we pick one. The hyperbolic structure of the surface is specified by the lengths of
the non-peripheral simple closed geodesics and the way how boundaries of Si’s are identified. Therefore the
hyperbolic structure of Σg,n,Lcan be parametrized by the Fenchel-Nielsen coordinates (ls;τs)(s=1,,3g3+
n), where lsare the lengths of the nonperipheral boundaries of Siand τsdenotes the twist parameters which
specify how boundaries of different pairs of pants are identified. The Teichmüller space Tg,n,Lcorresponds to
the region 0<ls<,−∞<τs<. A volume form g,n,Lon Tg,n,Lcalled the Weil-Petersson volume form
2
is given by
g,n,L=3g3+n
s=1[dlss].
g,n,Ldoes not depend on the choice of the pants decomposition. The moduli space Mg,n,Lis defined as
Mg,n,LTg,n,LΓ,
where Γdenotes the mapping class group. The Fenchel-Nielsen coordinates (ls;τs)can be used as local
coordinates on Mg,n,L. We will define the off-shell amplitudes as integrals over Mg,n,L. The space of all
inequivalent hyperbolic structures on a surface is the same as that of the complex structures. Hence the
definition of the off-shell amplitudes here can be regarded as the traditional one for the case where the
lengths of the external strings are specified.
2.2 b-ghost insertions
Let us consider an element Σg,n,Lof Mg,n,L. One can attach a flat semi-infinite cylinder to each boundary [8]
as depicted in Figure 3 and obtain a punctured Riemann surface. The cylinder is conformally equivalent to a
disk with a puncture. Let wa(a=1,n)be a local coordinate on the a-th disk Dasuch that Dacorresponds
to the region wa1, the flat metric is given as
ds2=L2
a
(2π)2dwa2
wa2,
and the a-th puncture corresponds to wa=0. By these conditions, wais fixed up to a phase rotation. wacan
be expressed as a function wa(z)of a local coordinate zon Σg,n,L.wa(z)is holomorphic in a neighborhood
of Da.
In this way, from Σg,n,L, we obtain a punctured Riemann surface Σg,n with local coordinates around
punctures, which are specified up to phase rotations. To Σg,n thus obtained, one can associate a surface
state, picking a local coordinate waas above for each Da. Let us denote this surface state by Σg,n,L. By
definition, we have Σg,n,LΨ1Ψn=n
a=1
w1
aOΨa(0)Σg,n ,(2.1)
where OΨadenotes the operator corresponding to the state Ψaand Σg,n denotes the correlation function
on Σg,n. Under a phase rotation waeawa,Σg,n,Ltransforms as
Σg,n,LΣg,n,L
a
ea(L(a)
0¯
L(a)
0).
The correlation function Σg,n,LΨ1Ψnis invariant under the phase rotation, if
(L0¯
L0)Ψa=0.
In order to define the amplitudes, we need to construct a top form on the moduli space Mg,n,Lfrom
the b-ghost. A deformation of the hyperbolic structure of a surface induces that of the complex structure.
Therefore we can construct the b-ghost insertion corresponding to a tangent vector of Mg,n,L, following the
procedure given in [4,16,18,19]. Let zibe a local coordinate on the pair of pants Si, such that the hyperbolic
metric on Siis in the form
ds2=eϕdzi2.
Each boundary of Siis either shared by another pair of pants Sj(ji)or is equal to one of the boundaries
of Σg,n,L. In the former case, the local coordinate zjon Sjand ziare related by
zi=Fij (zj),(2.2)
3
Figure 3: Attaching flat semi-infinite cylinders to Σg,n,L.
in a neighborhood of SiSj=Cij . If the boundary of Sicoincides with Da,ziand waare related by
zi=fia(wa),(2.3)
in a neighborhood of Da. The transition functions Fij , fia describe the moduli of Σg,n,L.
Suppose that under an infinitesimal change of moduli, zi, wa, Fij , fia change as
zizi+εvi,
wawa,
Fij Fij +δFij ,
fia fia +δfia .
Eqs. (2.2), (2.3) imply
zi+εvi=(Fij +δFij )(zj+εvj).
zi+εvi=(fia +δfia)(wa),
and we obtain
ε(vidzi
dzj
vj)=δFij (zj),
εvi=δfia(wa),
in a neighborhood of Cij , ∂Darespectively. One can take vito be holomorphic in neighborhoods of boundaries
of Siand smooth inside. For such vi, we define
b(v)
iSi
dzi
2πi vi(zi)b(zi)Si
d¯zi
2πi ¯vi(¯zi)¯
b(¯zi).(2.4)
Here the integration contours are taken so that they run along Sikeeping Sion the left for zi.
For our purpose, we need to make the formulas (2.2), (2.3) and (2.4) more explicit. Siitself is a hyperbolic
surface with three boundaries and by attaching flat semi-infinite cylinders to the boundaries as above, we
get a three punctured sphere with local coordinates Wk(k=1,2,3). Therefore Siis conformally equivalent
to C3
k=1Dkwhere Dkare the disks corresponding to the cylinders. We choose the local coordinate zion
Sito be the complex coordinate zon Csuch that the three punctures are at z=0,1,. The explicit forms
of Wk(zi)are given in [20, 21], which are presented in appendix A. There is a freedom in choosing which of
Dkcorresponds to each boundary of Si, but (A.3) implies Wk(zi)’s are related by SL(2,C)transformation
of ziand a phase rotation and the choice does not change the result. If the boundary Daof Σg,n,Lcoincides
with Wk(zi)=1, we can take wato be equal to Wk(zi). Then the explicit form of (2.3) becomes
zi=W1
k(wa).(2.5)
4
摘要:

UTHEP-773TheFokker-PlanckformalismforclosedbosonicstringsNobuyukiIshibashi*TomonagaCenterfortheHistoryoftheUniverse,UniversityofTsukubaTsukuba,Ibaraki305-8571,JAPANAbstractEveryRiemannsurfacewithgenusgandnpuncturesadmitsahyperbolicmetric,if2g2nA0.Suchasurfacecanbedecomposedintopairsofpantswhosebou...

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