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Introduction Review known results Expansions of fluctuations Superamplitudes Conclusion and remarks Modular Forms of type IIB superstring theory, and U (1)-violating amplitudes Congkao Wen Queen Mary University of London To appear with


  1. Introduction Review known results Expansions of fluctuations Superamplitudes Conclusion and remarks Modular Forms of type IIB superstring theory, and U (1)-violating amplitudes Congkao Wen Queen Mary University of London To appear with Michael Green String Theory from a Worldsheet Perspective The Galileo Galilei Institute for Theoretical Physics 1 / 28

  2. Introduction Review known results Expansions of fluctuations Superamplitudes Conclusion and remarks Introduction We are interested in low-energy effective action of type IIB superstring theory. 0 ( τ ) R 4 + α ′ 5 F (2) L EFT ∼ R + α ′ 3 F (0) 0 ( τ ) d 4 R 4 0 ( τ ) d 6 R 4 + · · · · · · + α ′ 6 F (3) Good understanding on the modular functions of the coefficient of R 4 , d 4 R 4 and d 6 R 4 . see Michael’s talk. We want to extend our understanding for general BPS-terms. 2 / 28

  3. Introduction Review known results Expansions of fluctuations Superamplitudes Conclusion and remarks Outline Brief review on the known results. Derive these results from a different point of view: Using constraints from the consistency of superamplitudes. This allows us to extend the results to more general BPS interactions L ( p ) n i ∼ F ( p ) ( i ) P ( w ) w i ( τ ) d 2 p ( { Φ } ) , n where i denotes a possible degeneracy. 3 / 28

  4. Introduction Review known results Expansions of fluctuations Superamplitudes Conclusion and remarks Review on non-holomorphic modular forms Non-holomorphic modular forms are functions of τ : w , w ′ ( τ ) → ( c τ + d ) w ( c ¯ τ + d ) w ′ F ( p ) F ( p ) w , w ′ ( τ ) under SL (2 , Z ) transformation τ → a τ + b c τ + d . Covariant derivatives i τ 2 ∂ τ + w � � D w F ( p ) F ( p ) w , w ′ ( τ ) := F ( p ) w , w ′ ( τ ) := w +1 , w ′ − 1 ( τ ) , 2 � τ + w ′ � D w ′ F ( p ) ¯ F ( p ) w , w ′ ( τ ) := F ( p ) w , w ′ ( τ ) := − i τ 2 ∂ ¯ w − 1 , w ′ +1 ( τ ) . 2 We will only consider the cases with w ′ = − w 4 / 28

  5. Introduction Review known results Expansions of fluctuations Superamplitudes Conclusion and remarks Examples: Eisenstein series Well-known examples: non-holomorphic Eisenstein series � w τ s � m + n ¯ τ � 2 E w ( s , τ ) = | m + n τ | 2 s m + n τ ( m , n ) � =(0 , 0) It has weight ( w , − w ). Satisfies Laplace equation, ∆ ( w ) − E w ( s , τ ) := 4 D w − 1 ¯ D − w E w ( s , τ ) = ( s − w )( s + w − 1) E w ( s , τ ) or ∆ ( w ) + E w ( s , τ ) := 4 ¯ D − w − 1 D w E w ( s , τ ) = ( s + w )( s − w − 1) E w ( s , τ ) 5 / 28

  6. Introduction Review known results Expansions of fluctuations Superamplitudes Conclusion and remarks d 2 p R 4 terms R 4 and d 4 R 4 [Green, Gutperle + Vanhove][Green, Sethi][Basu][Pioline][Berkovits, Vafa]...... 2 , τ ) R 4 , 2 , τ ) d 4 R 4 E 0 ( 3 E 0 ( 5 Perturbative expansions in large τ 2 agree with explicit computations 3 − 1 E 0 ( 3 2 , τ ) = 2 ζ (3) τ 2 + 4 ζ (2) τ 2 2 + instantons 2 The coefficient of d 6 R 4 satisfies an inhomogeneous Laplace equation [Green, Vanhove][Yin, Wang] � � ∆ (0) F (3) 2 , τ ) 2 − − 12 0 ( τ ) = − E 0 ( 3 as a consequence of first-order differential equations we will derive. 6 / 28

  7. Introduction Review known results Expansions of fluctuations Superamplitudes Conclusion and remarks Fluctuations On-shell amplitudes and fluctuations To compute scattering amplitudes, we expand the effective action around a fixed background τ 0 . F ( τ 0 + δτ ) = F ( τ 0 ) − 2 i τ 2 ∂ τ F ( τ 0 )ˆ τ F ( τ 0 )¯ τ + 2 i τ 2 ∂ ¯ τ ˆ τ 2 + · · · τ 2 − 2¯ τ F ( τ 0 )¯ − 2 τ 2 2 ∂ 2 τ F ( τ 0 )ˆ τ 2 2 ∂ 2 ˆ ¯ τ := i δτ/ (2 τ 0 here ˆ 2 ). Example: if F (0) 0 ( τ 0 + δτ ) is the coefficient of R 4 , the expansion generates five and higher-point interactions: τ ˆ ˆ τ 7 / 28

  8. Introduction Review known results Expansions of fluctuations Superamplitudes Conclusion and remarks Fluctuations SL (2 , Z ) covariant derivatives Each vertex from expansion is in the form of simple derivatives instead of SL (2 , Z ) covariant derivatives: The fluctuation ˆ τ does not transform properly under U (1). Two-derivative classical action, when expanded around τ 0 contains infinity set of U (1)-violating vertices. e.g. ∂ µ τ∂ µ ¯ τ τ 2 + 2ˆ τ∂ µ ¯ τ + ¯ τ ¯ τ + ¯ � τ 2 ) + · · · � = ∂ µ ˆ ˆ τ 1 + 2(ˆ τ ) + 3(ˆ ˆ ˆ ˆ 4 τ 2 they are all vanishing on-shell, no U (1)-violating amplitudes in type IIB supergravity. 8 / 28

  9. Introduction Review known results Expansions of fluctuations Superamplitudes Conclusion and remarks Fluctuations SL (2 , Z ) covariant derivatives The 2-derivative U (1)-violating vertices do contribute to higher-derivative amplitudes, by attaching them to higher-derivative vertices: R 4 ˆ τ etc. τ ˆ ˆ τ These additional contributions precisely make the simple derivatives to be covariant derivatives. 9 / 28

  10. Introduction Review known results Expansions of fluctuations Superamplitudes Conclusion and remarks Field redefinition Field redefinitions A systematics: A field redefinition that removes all these on-shell vanishing vertices: τ = τ − τ 0 τ ˆ B = − 1 − ˆ τ − ¯ τ 0 the normal coordinate of the sigma model G / H . Used in [Schwarz, 83’] for SU (1 , 1) formulation of the classical theory. The field B kills two birds with one stone: The B field transforms linearly τ 0 + d � c ¯ � B → B . c τ 0 + d Removes all U (1)-violating (on-shell vanishing) vertices in the classical action. 10 / 28

  11. Introduction Review known results Expansions of fluctuations Superamplitudes Conclusion and remarks Field redefinition Field redefinition and covariant derivatives Expanded in terms of B fields: F ( τ 0 + δτ ) = F ( τ 0 ) − 2 i τ 2 ∂ τ F ( τ 0 )ˆ τ 2 + O (ˆ τ − 2 τ 2 2 ∂ 2 τ F ( τ 0 )ˆ τ 3 ) = F ( τ 0 ) − 2 i τ 2 ∂ τ F ( τ 0 ) B + B 2 + O ( B 3 ) − τ 2 2 ∂ 2 τ F ( τ 0 ) + i τ 2 ∂ τ F ( τ 0 ) � � + 2 Now each term is covariant derivatives i τ 2 ∂ τ F ( τ 0 ) = D 0 F ( τ 0 ) − τ 2 2 ∂ 2 τ F ( τ 0 ) + i τ 2 ∂ τ F ( τ 0 ) = D 1 D 0 F ( τ 0 ) 11 / 28

  12. Introduction Review known results Expansions of fluctuations Superamplitudes Conclusion and remarks Field redefinition Field redefinition: other fields Similar field redefinition for other fields in theory. Example: a fermionic term Q µ = ∂ µ τ 1 Λ a γ µ ( ∂ µ + iq Λ Q µ )¯ Λ a , . with 2 τ 2 The redefined field � q Λ / 2 � 1 − B Λ ′ a = Λ a . 1 − ¯ B 12 / 28

  13. Introduction Review known results Expansions of fluctuations Superamplitudes Conclusion and remarks Superamplitudes Summary: All interactions are manifestly SL (2 , Z ) invariant, with appropriate choices of the fluctuation fields. Ready to study scattering amplitudes: 10D spinor helicity and type IIB SUSY: [Boels and O’Connell] massless momentum p BA := ( γ µ ) BA p µ = λ Ba λ A a . A = 1 , . . . , 16 is the spinor of SO (9 , 1) and a = 1 , . . . , 8 the SO (8) little group index. Supercharges n n ∂ � ¯ � λ A , a Q A λ A i , a η a Q A n = i , n = . i ∂η a i i =1 i =1 13 / 28

  14. Introduction Review known results Expansions of fluctuations Superamplitudes Conclusion and remarks Superamplitudes The on-shell massless states: a + 1 2! η a η b φ ab + · · · + 1 8!( η ) 8 ¯ Φ( η ) = B + η a Λ ′ B . a = − 3 B = 2, and q η = − 1 q B = − 2 , q Λ ′ 2 , · · · , q h = 0 , · · · , q ¯ 2 . The super amplitudes � � n A n = δ 10 � δ 16 ( Q n ) ˆ Q A ¯ n ˆ A n ( η, λ ) , A n ( η, λ ) = 0 , p r with r =1 U (1)-conserved amplitudes ˆ A n ∼ η 4( n − 4) . 14 / 28

  15. Introduction Review known results Expansions of fluctuations Superamplitudes Conclusion and remarks Superamplitudes: maximal U (1)-violating Maximal U (1)-violating amplitudes [Boels] A ( p ) n , i = F ( p ) A ( p ) n − 4 , i ( τ ) δ 16 ( Q n ) ˆ n , i ( s ij ) , where i denotes a possible degeneracy. The maximal U (1)-violating amplitudes have no poles. A ( p ) Therefore ˆ n , i ( s ij ) is a degree- p symmetric polynomial of s ij . They are super vertices. In 4D, they are KLT of MHV ⊗ MHV . 15 / 28

  16. Introduction Review known results Expansions of fluctuations Superamplitudes Conclusion and remarks Superamplitudes: maximal U (1)-violating Higher-point amplitudes are related to the lower-point ones by soft limits. The coefficients are related by covariant derivatives, F ( p ) n − 4 , i ( τ ) ∼ D n − 5 F ( p ) n − 5 , i ( τ ) The kinematics are related by soft limits (soft B field) A ( p ) A ( p ) ˆ p n → 0 → ˆ � n , i ( s ij ) n − 1 , i ( s ij ) � Covariant derivative is a result of combination of soft dilaton ( τ 2 ∂ τ 2 A n ) [Di Vecchia][Di Vecchia, Marotta, Mojaza, Nohle] and soft axion limit ( w � i R i A n ). 16 / 28

  17. Introduction Review known results Expansions of fluctuations Superamplitudes Conclusion and remarks Superamplitudes: maximal U (1)-violating A (0) ˆ n , i ( s ij ) = 1 is for dimension-8 interactions, related to R 4 , (no degeneracy) F (0) n − 4 ( τ ) ∼ D n − 5 · · · D 0 E ( 3 2 , τ ) ∼ E n − 4 ( 3 2 , τ ) A (2) ˆ i < j s 2 n , i ( s ij ) = � ij is for dimension-12 interactions, related to d 4 R 4 , (no degeneracy) F (2) n − 4 ( τ ) ∼ D n − 5 · · · D 0 E ( 5 2 , τ ) ∼ E n − 4 ( 5 2 , τ ) 17 / 28

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