Superstring theory and integration over the moduli space

Similar documents
N = 2 String Amplitudes *

Topological Holography and Chiral Algebras. Work in progress with Kevin Costello

Why Supersymmetry is Different

Twistor strings for N =8. supergravity

String Theory in a Nutshell. Elias Kiritsis

BPS non-local operators in AdS/CFT correspondence. Satoshi Yamaguchi (Seoul National University) E. Koh, SY, arxiv: to appear in JHEP

Instanton effective action in - background and D3/D(-1)-brane system in R-R background

Half BPS solutions in type IIB and M-theory

Heterotic Torsional Backgrounds, from Supergravity to CFT

Knot Homology from Refined Chern-Simons Theory

Anomalies, Conformal Manifolds, and Spheres

Rigid SUSY in Curved Superspace

Twistor Strings, Gauge Theory and Gravity. Abou Zeid, Hull and Mason hep-th/

Seminar in Wigner Research Centre for Physics. Minkyoo Kim (Sogang & Ewha University) 10th, May, 2013

M-theory S-Matrix from 3d SCFT

Refined Chern-Simons Theory, Topological Strings and Knot Homology

Intro to Geometry and Topology via G Physics and G 2 -manifolds. Bobby Samir Acharya. King s College London. and ICTP Trieste Ψ(1 γ 5 )Ψ

Exact Half-BPS Solutions in Type IIB and M-theory

Towards solution of string theory in AdS3 x S 3

Elements of Topological M-Theory

Superstrings and Supergeometry

* +, ...! Einstein. [1] Calabi-Yau [2] Calabi-Yau. :;æåø!! :; õ ø!!

On the BCOV Conjecture

The exact quantum corrected moduli space for the universal hypermultiplet

Recent Advances in SUSY

8.821 String Theory Fall 2008

Aspects of (0,2) theories

Bubbling Geometries for Half BPS Wilson Lines. Satoshi Yamaguchi (IHES) S. Yamaguchi, hep-th/ S. Yamaguchi, to appear

Smooth Wilson Loops and Yangian Symmetry in Planar N = 4 SYM

SCFTs, Compact CY 3-folds, and Topological Strings

Holographic Anyons in the ABJM theory

Generalized Teichmüller Spaces, Spin Structures and Ptolemy Transformations

Topological String Theory

Departement de Physique Theorique, Universite de Geneve, Abstract

BPS Black Holes Effective Actions and the Topological String ISM08 Indian Strings Meeting Pondicherry, 6-13 December 2008

Lecture 8: 1-loop closed string vacuum amplitude

Maximally Supersymmetric Solutions in Supergravity

Spectral Networks and Their Applications. Caltech, March, 2012

On Special Geometry of Generalized G Structures and Flux Compactifications. Hu Sen, USTC. Hangzhou-Zhengzhou, 2007

Complete action of open superstring field theory

LANDAU-GINZBURG MODEL FOR A CRITICAL TOPOLOGICAL STRING

CHY formalism and null string theory beyond tree level

Ambitwistor strings, the scattering equations, tree formulae and beyond

Twistor Strings, Gauge Theory and Gravity

Some Tools for Exploring Supersymmetric RG Flows

Rigid Holography and 6d N=(2,0) Theories on AdS 5 xs 1

Chern-Simons Theory and Its Applications. The 10 th Summer Institute for Theoretical Physics Ki-Myeong Lee

SUPERCONFORMAL FIELD THEORIES. John H. Schwarz. Abdus Salam ICTP 10 November 2010

Exact Solutions of 2d Supersymmetric gauge theories

RECENT DEVELOPMENTS IN FERMIONIZATION AND SUPERSTRING MODEL BUILDING

Quantum Fields in Curved Spacetime

Quantum Dynamics of Supergravity

Instantons in (deformed) gauge theories from strings

5d SCFTs and instanton partition functions

Sphere Partition Functions, Topology, the Zamolodchikov Metric

A Supergravity Dual for 4d SCFT s Universal Sector

Aspects of integrability in classical and quantum field theories

THE. Secret Life OF SCATTERING AMPLITUDES. based on work with Lionel Mason and with Mat Bullimore. David Skinner - Perimeter Institute

Anton M. Zeitlin. Columbia University, Department of Mathematics. Super-Teichmüller theory. Anton Zeitlin. Outline. Introduction. Cast of characters

Twistors, amplitudes and gravity

Instanton Calculus In R-R Background And The Topological String

Hidden Symmetry in Topological Gravity

Enumerative Geometry: from Classical to Modern

Geometry of the Calabi-Yau Moduli

Weyl Anomalies and D-brane Charges

Spinning strings and QED

Three-Charge Black Holes and ¼ BPS States in Little String Theory

A One-Loop Test of String Duality

Pietro Fre' SISSA-Trieste. Paolo Soriani University degli Studi di Milano. From Calabi-Yau manifolds to topological field theories

Recent developments in the construction of superstring field theory I

arxiv: v1 [hep-th] 4 Jul 2008

Thermodynamics of black branes as interacting branes

Recent Progress on Curvature Squared Supergravities in Five and Six Dimensions

AdS/CFT duality. Agnese Bissi. March 26, Fundamental Problems in Quantum Physics Erice. Mathematical Institute University of Oxford

Overview of classical mirror symmetry

Three-Charge Black Holes and ¼ BPS States in Little String Theory I

Topological reduction of supersymmetric gauge theories and S-duality

Some applications of light-cone superspace

The boundary state from open string fields. Yuji Okawa University of Tokyo, Komaba. March 9, 2009 at Nagoya

Superstrings in Graviphoton Background and N = Supersymmetry

Symmetries, Groups Theory and Lie Algebras in Physics

Non-Geometric Calabi- Yau Backgrounds

Holographic duals of interface theories and junctions of CFTs

Supersymmetric Gauge Theories, Matrix Models and Geometric Transitions

Yet Another Alternative to Compactification by Heterotic Five-branes

Non-Supersymmetric Seiberg duality Beyond the Planar Limit

Heterotic Geometry and Fluxes

Hexagons and 3pt functions

Quantum Entanglement of Baby Universes

e θ 1 4 [σ 1,σ 2 ] = e i θ 2 σ 3

Dualities and Topological Strings

If I only had a Brane

A Landscape of Field Theories

Introduction to AdS/CFT

Talk at the International Workshop RAQIS 12. Angers, France September 2012

Supertwistors, Chern-Simons And Super Gauge Theories

Superstring in the plane-wave background with RR-flux as a conformal field theory

N = 2 CHERN-SIMONS MATTER THEORIES: RG FLOWS AND IR BEHAVIOR. Silvia Penati. Perugia, 25/6/2010

Preprint typeset in JHEP style - HYPER VERSION. Special Geometry. Yang Zhang. Abstract: N = 2 Supergravity. based on hep-th/ , Boris PiolineA

Bobby Samir Acharya Kickoff Meeting for Simons Collaboration on Special Holonomy

Transcription:

Superstring theory and integration over the moduli space Kantaro Ohmori Hongo,The University of Tokyo Oct, 23rd, 2013 arxiv:1303.7299 [KO,Yuji Tachikawa] Todai/Riken joint workshop on Super Yang-Mills, solvable systems and related subjects

Section 1 introduction

Simplified history of the superstring theory

Simplified history of the superstring theory 70 s:bosonic string theory! supersymmetrize

Simplified history of the superstring theory 70 s:bosonic string theory! supersymmetrize 84 :1st superstring revolution

Simplified history of the superstring theory 70 s:bosonic string theory! supersymmetrize 84 :1st superstring revolution 86: Conformal Invariance, Supersymmetry, and String Theory [D.Friedan, E.Martinec, S.Shenker]

Simplified history of the superstring theory 70 s:bosonic string theory! supersymmetrize 84 :1st superstring revolution 86: Conformal Invariance, Supersymmetry, and String Theory [D.Friedan, E.Martinec, S.Shenker] 94 :2nd superstring revolution ) nonperturbative perspective

Simplified history of the superstring theory 70 s:bosonic string theory! supersymmetrize 84 :1st superstring revolution 86: Conformal Invariance, Supersymmetry, and String Theory [D.Friedan, E.Martinec, S.Shenker] 94 :2nd superstring revolution ) nonperturbative perspective 12: Superstring Perturbation Theory Revisited [E.Witten]: Superstring perturbation theory and supergeometry

Bosonic string theory

Bosonic string theory Action:S = R d2 zg ij @X i @X j

Bosonic string theory Action:S = R d2 zg ij @X i @X j ) Riemann Surface = 2d surface + metric

Bosonic string theory Action:S = R d2 zg ij @X i @X j ) Riemann Surface = 2d surface + metric Conformal symmetry ) bc ghost

Bosonic string theory Action:S = R d2 zg ij @X i @X j ) Riemann Surface = 2d surface + metric Conformal symmetry ) bc ghost )A= R M bos,g dmd mf (m, m)

Superstring theory

Superstring theory Action:S = R d2 zd 2 G ij D X i D X j

Superstring theory Action:S = R d2 zd 2 G ij D X i D X j ) Super Riemann Surface =2dsurface+supermetric =2dsurface+metric + gravitino θ θ θ θ θ θ θ θ θ

Superstring theory Action:S = R d2 zd 2 G ij D X i D X j ) Super Riemann Surface =2dsurface+supermetric =2dsurface+metric + gravitino θ θ θ θ θ θ θ θ θ Superconformal symmetry ) BC(bc ) superghost

Superstring theory Action:S = R d2 zd 2 G ij D X i D X j ) Super Riemann Surface =2dsurface+supermetric =2dsurface+metric + gravitino θ θ θ θ θ θ θ θ θ Superconformal symmetry ) BC(bc ) superghost )A= R M super,g dmd d md F (m, m,, )

Superstring theory Action:S = R d2 zd 2 G ij D X i D X j ) Super Riemann Surface =2dsurface+supermetric =2dsurface+metric + gravitino θ θ θ θ θ θ θ θ θ Superconformal symmetry ) BC(bc ) superghost )A= R M super,g dmd d md F (m, m,, )? )A= R M spin,g dmd mf 0 (m, m)

The bosonic and super moduli space M super 6=M spin odd direction M super M spin

The bosonic and super moduli space M super 6=M spin odd direction M super M spin Global integration on M super 6) Global integration on M spin (preserving holomorphic factorization)

The work of [KO,Tachikawa]

The work of [KO,Tachikawa] Global integration on M super 6) Global integration on M spin

The work of [KO,Tachikawa] Global integration on M super 6) Global integration on M spin We found special cases where Global integration on M super ) Global integration on M spin

The work of [KO,Tachikawa] (2)

The work of [KO,Tachikawa] (2) 2concreteexamples

The work of [KO,Tachikawa] (2) 2concreteexamples N =0 N =1embedding [N. Berkovits,C. Vafa 94]

The work of [KO,Tachikawa] (2) 2concreteexamples N =0 N =1embedding [N. Berkovits,C. Vafa 94] Topological amplitudes [I. Antoniadis, E. Gava, K.S. Narain, T.R. Taylor 94] [M. Bershadsky, S. Cecotti, H. Ooguri, C. Vafa 94]

1 introduction 2 Supergeometry and Superstring 3 Reduction to integration over bosonic moduli

Supermanifold

Supermanifold supermanifold = patched superspaces

Supermanifold supermanifold = patched superspaces M :supermanifoldofdimensionp q M 3 (x 1,, x p 1,, q ) i j = j i

Supermanifold supermanifold = patched superspaces M :supermanifoldofdimensionp q M 3 (x 1,, x p 1,, q ) i j = j i x 0 i = f i (x ) 0 µ = µ(x ) U α

Supermanifold supermanifold = patched superspaces M :supermanifoldofdimensionp q M 3 (x 1,, x p 1,, q ) i j = j i x 0 i = f i (x ) 0 µ = µ(x ) M red = {(x i,, x p )},! M U α

Supermoduli space Msuper

Supermoduli space M super Space of deformations of SRS (Super Riemann Surface)

Supermoduli space M super Space of deformations of SRS (Super Riemann Surface) even deformation: µ z z 2 H 1 ( red, T red )

Supermoduli space M super Space of deformations of SRS (Super Riemann Surface) even deformation: µ z z 2 H 1 ( red, T red ) odd deformation: z 2 H 1 ( red, T 1/2 red )

Supermoduli space M super Space of deformations of SRS (Super Riemann Surface) even deformation: µ z z 2 H 1 ( red, T red ) odd deformation: z 2 H 1 ( red, T 1/2 red ) { }: basisofgravitinob.g) =

Supermoduli space M super Space of deformations of SRS (Super Riemann Surface) even deformation: µ z z 2 H 1 ( red, T red ) odd deformation: z 2 H 1 ( red, T 1/2 red ) { }: basisofgravitinob.g) = dim M super = e o =3g 3 2g 2 (g 2)

Supermoduli space M super Space of deformations of SRS (Super Riemann Surface) even deformation: µ z z 2 H 1 ( red, T red ) odd deformation: z 2 H 1 ( red, T 1/2 red ) { }: basisofgravitinob.g) = dim M super = e o =3g 3 2g 2 (g 2) M super,red 'M spin

Supermoduli space of SRS with punctures

Supermoduli space of SRS with punctures n NS NS punctures and n R Rpunctures

Supermoduli space of SRS with punctures n NS NS punctures and n R Rpunctures dim M super = e o =3g 3+n NS +n R 2g 2+n NS +n R /2 (g 2)

Coupling between gravitino and SCFT

Coupling between gravitino and SCFT S = 1 R 2 d 2 z T F

Coupling between gravitino and SCFT S = 1 R 2 d 2 z T F S e = 1 R 2 d 2 z e TF e

Coupling between gravitino and SCFT S = 1 R 2 d 2 z T F S e = 1 R 2 d 2 z e TF e S e = R d 2 z ea A / µ e µ (Flat background)

Coupling between gravitino and SCFT S = 1 R 2 d 2 z T F S e = 1 R 2 d 2 z e TF e S e = R d 2 z ea A / µ e µ (Flat background) c.f. D µ D µ 3 A µ A µ

Scattering amplitudes of superstring

Scattering amplitudes of superstring V i :Vertexop.pic.number 1 (NS) or 1/2 (R)

Scattering amplitudes of superstring V i :Vertexop.pic.number 1 (NS) or 1/2 (R) A V,g = R M super dmd d md F V,g (m,, m, )

Scattering amplitudes of superstring V i :Vertexop.pic.number 1 (NS) or 1/2 (R) A V,g = R M super dmd d md F V,g (m,, m, ) FD V,g (m,, m, ) = Q i V Q e i a=1 (R red d 2 zbµ a ) Q e b=1 (R red d 2 zb e eµ b ) Q o=1 ( R d2 red z ) Q e o =1 ( R red d 2 z e e ) exp( S S e S e )i m

Scattering amplitudes of superstring V i :Vertexop.pic.number 1 (NS) or 1/2 (R) A V,g = R M super dmd d md F V,g (m,, m, ) FD V,g (m,, m, ) = Q i V Q e i a=1 (R red d 2 zbµ a ) Q e b=1 (R red d 2 zb e eµ b ) Q o=1 ( R d2 red z ) Q e o =1 ( R red d 2 z e e ) exp( S S e S e )i m S = P R o =1 2 red d 2 z T F

Scattering amplitudes of superstring V i :Vertexop.pic.number 1 (NS) or 1/2 (R) A V,g = R M super dmd d md F V,g (m,, m, ) FD V,g (m,, m, ) = Q i V Q e i a=1 (R red d 2 zbµ a ) Q e b=1 (R red d 2 zb e eµ b ) Q o=1 ( R d2 red z ) Q e o =1 ( R red d 2 z e e ) exp( S S e S e )i m S = P R o =1 2 red d 2 z T F We get result of FMS when = (z p ) and int. out. s.

Integration over a supermanifold

Integration over a supermanifold E = {(m 1, 2 )}/ m m + + 1 2 m +1

Integration over a supermanifold E = {(m 1, 2 )}/ m m + + 1 2 m +1 R E (a + b 1 2 )dmdmd 1 d 2 = b= + p 1a/2

Integration over a supermanifold E = {(m 1, 2 )}/ m m + + 1 2 m +1 R E (a + b 1 2 )dmdmd 1 d 2 = b= + p 1a/2 1 2 mixed with m

Projectedness of supermanifolds

Projectedness of supermanifolds M:projected, an atlas in which x 0 = f (x) for all gluing ) naive integrations with s are allowed

Projectedness of supermanifolds M:projected, an atlas in which x 0 = f (x) for all gluing ) naive integrations with s are allowed, p : M! M red exists

Projectedness of supermanifolds M:projected, an atlas in which x 0 = f (x) for all gluing ) naive integrations with s are allowed, p : M! M red exists R M! = R M red p (!)

Projectedness of supermanifolds M:projected, an atlas in which x 0 = f (x) for all gluing ) naive integrations with s are allowed, p : M! M red exists R M! = R M red p (!) All supermanifolds are projected in smooth sense.

Projectedness of supermanifolds M:projected, an atlas in which x 0 = f (x) for all gluing ) naive integrations with s are allowed, p : M! M red exists R M! = R M red p (!) All supermanifolds are projected in smooth sense. Complex supermanifolds are not projected in holomorphic sense in general.

Supermoduli Space is not projected [R.Donagi, E.Witten, arxiv:1304.7798]

Supermoduli Space is not projected [R.Donagi, E.Witten, arxiv:1304.7798] M super,red 'M spin i : M spin,! M super

Supermoduli Space is not projected [R.Donagi, E.Witten, arxiv:1304.7798] M super,red 'M spin i : M spin,! M super p : M super!m spin does not exists. (g 5, non-holomorphiconeexists)

Supermoduli Space is not projected [R.Donagi, E.Witten, arxiv:1304.7798] M super,red 'M spin i : M spin,! M super p : M super!m spin does not exists. (g 5, non-holomorphiconeexists) Global integration on M super 6) Global integration on M spin (preserving holomorphic factorization)

Section 3 Reduction to integration over bosonic moduli

Reduction condition

Reduction condition Global integration on M super ) Global integration on M spin in special cases F (m, m,, ) =G(m, m) Q all i i (saturations of s)

Reduction condition Global integration on M super ) Global integration on M spin in special cases F (m, m,, ) =G(m, m) Q all i i (saturations of s) mixing of m and (m 0 = m + 1 2 )doesnot changes F

Reduction condition Global integration on M super ) Global integration on M spin in special cases F (m, m,, ) =G(m, m) Q all i i (saturations of s) mixing of m and (m 0 = m + 1 2 )doesnot changes F F does not depend on the locations of picture changing operators

Topological amplitudes in string theory [I. Antoniadis, E. Gava, K.S. Narain, T.R. Taylor 94] [M. Bershadsky, S. Cecotti, H. Ooguri, C. Vafa 94]

Topological amplitudes in string theory [I. Antoniadis, E. Gava, K.S. Narain, T.R. Taylor 94] [M. Bershadsky, S. Cecotti, H. Ooguri, C. Vafa 94] Type II string on CY (N =(2, 2)SCFT) R 1,3 ) 4d N =2supergravity model

Topological amplitudes in string theory [I. Antoniadis, E. Gava, K.S. Narain, T.R. Taylor 94] [M. Bershadsky, S. Cecotti, H. Ooguri, C. Vafa 94] Type II string on CY (N =(2, 2)SCFT) R 1,3 ) 4d N =2supergravity model F-term of 4d e ective field theory is related to topological string.

Reduction to topological string Type II string on CY(6d) R 1,3 ) 4d N =2supergravity model

Reduction to topological string Type II string on CY(6d) R 1,3 ) 4d N =2supergravity model A g :zeromomentalimitofg loop amplitude of 2g 2 graviphotons (RR) and 2 gravitons (NSNS)

Reduction to topological string Type II string on CY(6d) R 1,3 ) 4d N =2supergravity model A g :zeromomentalimitofg loop amplitude of 2g 2 graviphotons (RR) and 2 gravitons (NSNS) A g = R M super

Reduction to topological string Type II string on CY(6d) R 1,3 ) 4d N =2supergravity model A g :zeromomentalimitofg loop amplitude of 2g 2 graviphotons (RR) and 2 gravitons (NSNS) A g = R M super A g =(g!) 2 F g = R M bos

Vertex operators

Vertex operators Graviphoton: V T = spacetime (ghost) p = exp(i 3 2 (H(z) H(z))) e H : U(1) R boson : U(1) R charge (3/2, 3/2)

Vertex operators Graviphoton: V T = spacetime (ghost) p = exp(i 3 2 (H(z) H(z))) e H : U(1) R boson : U(1) R charge (3/2, 3/2) Graviton: V R = R red spacetime,ghost

Saturation of s

Saturation of s A g = R D Q 2g 2 i =1 (x i ) U(1) R :(3g 3, 3g 3) (spacetime) (bc) Q o=1 ( R d2 red z ) Q e o =1 ( R red d 2 z e e ) R exp( red (T F + T e E F e + A e )) m

Saturation of s A g = R D Q 2g 2 i =1 (x i ) U(1) R :(3g 3, 3g 3) (spacetime) (bc) Q o=1 ( R d2 red z ) Q e o =1 ( R red d 2 z e e ) R exp( red (T F + T e E F e + A e )) m nonzero contribution ) 3g 3 and 3g 3e

Saturation of s A g = R D Q 2g 2 i =1 (x i ) U(1) R :(3g 3, 3g 3) (spacetime) (bc) Q o=1 ( R d2 red z ) Q e o =1 ( R red d 2 z e e ) R exp( red (T F + T e E F e + A e )) m nonzero contribution ) 3g 3 and 3g 3e There are only 3g 3 and 3g 3 e

Saturation of s A g = R D Q 2g 2 i =1 (x i ) U(1) R :(3g 3, 3g 3) (spacetime) (bc) Q o=1 ( R d2 red z ) Q e o =1 ( R red d 2 z e e ) R exp( red (T F + T e E F e + A e )) m nonzero contribution ) 3g 3 and 3g 3e There are only 3g 3 and 3g 3 e The correlation function does not depend of the choice of

Conclusion

Conclusion Superstring amplitude cannot be represent as integration over M spin in general

Conclusion Superstring amplitude cannot be represent as integration over M spin in general Special cases exist.

Conclusion Superstring amplitude cannot be represent as integration over M spin in general Special cases exist. Amplitudes which is equivalent topological amplitudes are the case.

End.