m theory s matrix from 3d scft
play

M-theory S-Matrix from 3d SCFT Silviu S. Pufu, Princeton University - PowerPoint PPT Presentation

M-theory S-Matrix from 3d SCFT Silviu S. Pufu, Princeton University Based on: arXiv:1711.07343 with N. Agmon and S. Chester arXiv:1804.00949 with S. Chester and X. Yin arXiv:1808.10554 with D. Binder and S. Chester Also: arXiv:1406.4814 ,


  1. M-theory S-Matrix from 3d SCFT Silviu S. Pufu, Princeton University Based on: arXiv:1711.07343 with N. Agmon and S. Chester arXiv:1804.00949 with S. Chester and X. Yin arXiv:1808.10554 with D. Binder and S. Chester Also: arXiv:1406.4814 , arXiv:1412.0334 with S. Chester, J. Lee, and R. Yacoby arXiv:1610.00740 with M. Dedushenko and R. Yacoby Trieste, October 17, 2018 Silviu Pufu (Princeton University) 10-26-2018 1 / 32

  2. Silviu Pufu (Princeton University) 10-26-2018 1 / 32

  3. Motivation Learn about (reconstruct?) gravity / string theory / M-theory from CFT using AdS/CFT. Work toward a constructive proof of AdS/CFT. Most well-established examples: 4d SU ( N ) N = 4 SYM at large N and large ’t Hooft coupling / type IIB strings on AdS 5 × S 5 3d U ( N ) k × U ( N ) − k ABJM theory at large N / M-theory on AdS 4 × S 7 / Z k . Both have maximal SUSY (for ABJM only when k = 1 or 2). I’ll focus on the ABJM example in the case k = 1. Silviu Pufu (Princeton University) 10-26-2018 2 / 32

  4. Motivation Learn about (reconstruct?) gravity / string theory / M-theory from CFT using AdS/CFT. Work toward a constructive proof of AdS/CFT. Most well-established examples: 4d SU ( N ) N = 4 SYM at large N and large ’t Hooft coupling / type IIB strings on AdS 5 × S 5 3d U ( N ) k × U ( N ) − k ABJM theory at large N / M-theory on AdS 4 × S 7 / Z k . Both have maximal SUSY (for ABJM only when k = 1 or 2). I’ll focus on the ABJM example in the case k = 1. Silviu Pufu (Princeton University) 10-26-2018 2 / 32

  5. Motivation Last 10 years: progress in QFT calculations using supersymmetric localization; using conformal bootstrap in CFTs. Example: using SUSic loc., the S 3 partition function of ABJM theory can be written as a 2 N -dim’l integral [Kapustin, Willett, Yaakov ’09] i < j 4 sinh 2 ( λ i − λ j ) sinh 2 ( µ i − µ j ) � � i ) . e i k i ( λ 2 i − µ 2 d N λ d N µ � Z = π i , j cosh 2 ( λ i − µ j ) � √ 3 k 1 / 2 N 3 / 2 + O ( N 1 / 2 ) . Expand at large N to find F = − log Z = π 2 N 3 / 2 scaling matches # of d.o.f.’s on N coincident M2-branes as computed using 11d SUGRA. Subleading corrections contain info beyond 11d SUGRA. What exactly can we learn from them?? Silviu Pufu (Princeton University) 10-26-2018 3 / 32

  6. Motivation Last 10 years: progress in QFT calculations using supersymmetric localization; using conformal bootstrap in CFTs. Example: using SUSic loc., the S 3 partition function of ABJM theory can be written as a 2 N -dim’l integral [Kapustin, Willett, Yaakov ’09] i < j 4 sinh 2 ( λ i − λ j ) sinh 2 ( µ i − µ j ) � � i ) . e i k i ( λ 2 i − µ 2 d N λ d N µ � Z = π i , j cosh 2 ( λ i − µ j ) � √ 3 k 1 / 2 N 3 / 2 + O ( N 1 / 2 ) . Expand at large N to find F = − log Z = π 2 N 3 / 2 scaling matches # of d.o.f.’s on N coincident M2-branes as computed using 11d SUGRA. Subleading corrections contain info beyond 11d SUGRA. What exactly can we learn from them?? Silviu Pufu (Princeton University) 10-26-2018 3 / 32

  7. Motivation Last 10 years: progress in QFT calculations using supersymmetric localization; using conformal bootstrap in CFTs. Example: using SUSic loc., the S 3 partition function of ABJM theory can be written as a 2 N -dim’l integral [Kapustin, Willett, Yaakov ’09] i < j 4 sinh 2 ( λ i − λ j ) sinh 2 ( µ i − µ j ) � � i ) . e i k i ( λ 2 i − µ 2 d N λ d N µ � Z = π i , j cosh 2 ( λ i − µ j ) � √ 3 k 1 / 2 N 3 / 2 + O ( N 1 / 2 ) . Expand at large N to find F = − log Z = π 2 N 3 / 2 scaling matches # of d.o.f.’s on N coincident M2-branes as computed using 11d SUGRA. Subleading corrections contain info beyond 11d SUGRA. What exactly can we learn from them?? Silviu Pufu (Princeton University) 10-26-2018 3 / 32

  8. Motivation Last 10 years: progress in QFT calculations using supersymmetric localization; using conformal bootstrap in CFTs. Example: using SUSic loc., the S 3 partition function of ABJM theory can be written as a 2 N -dim’l integral [Kapustin, Willett, Yaakov ’09] i < j 4 sinh 2 ( λ i − λ j ) sinh 2 ( µ i − µ j ) � � i ) . e i k i ( λ 2 i − µ 2 d N λ d N µ � Z = π i , j cosh 2 ( λ i − µ j ) � √ 3 k 1 / 2 N 3 / 2 + O ( N 1 / 2 ) . Expand at large N to find F = − log Z = π 2 N 3 / 2 scaling matches # of d.o.f.’s on N coincident M2-branes as computed using 11d SUGRA. Subleading corrections contain info beyond 11d SUGRA. What exactly can we learn from them?? Silviu Pufu (Princeton University) 10-26-2018 3 / 32

  9. M-theory S-matrix This talk: Reconstruct M-theory S-matrix perturbatively at small momentum. scatter gravitons and superpartners in 11d. Equivalently, reconstruct the derivative expansion of the M-theory effective action. Schematically, d 11 x √ g � � R + Riem 4 + · · · + (SUSic completion) � S = . Restrict momenta to be in 4 out of the 11 dimensions. Silviu Pufu (Princeton University) 10-26-2018 4 / 32

  10. M-theory S-matrix This talk: Reconstruct M-theory S-matrix perturbatively at small momentum. scatter gravitons and superpartners in 11d. Equivalently, reconstruct the derivative expansion of the M-theory effective action. Schematically, d 11 x √ g � � R + Riem 4 + · · · + (SUSic completion) � S = . Restrict momenta to be in 4 out of the 11 dimensions. Silviu Pufu (Princeton University) 10-26-2018 4 / 32

  11. M-theory S-matrix This talk: Reconstruct M-theory S-matrix perturbatively at small momentum. scatter gravitons and superpartners in 11d. Equivalently, reconstruct the derivative expansion of the M-theory effective action. Schematically, d 11 x √ g � � R + Riem 4 + · · · + (SUSic completion) � S = . Restrict momenta to be in 4 out of the 11 dimensions. Silviu Pufu (Princeton University) 10-26-2018 4 / 32

  12. In 11d, we can scatter: gravitons, gravitini, 3-form gauge particles. ⇒ can use 4d N = 8 language. We scatter: Momenta within 4d = graviton (1); gravitinos (8); gravi-photons (28); gravi-photinos (56); scalars (70 = 35 + 35) At leading order in small momentum (i.e. p 2 ), scattering amplitudes are those in N = 8 SUGRA at tree level. Examples: A SUGRA, tree ( h − h − h + h + ) = � 12 � 4 [ 34 ] 4 , stu A SUGRA, tree ( S 1 S 1 S 2 S 2 ) = tu s , where s = ( p 1 + p 2 ) 2 , t = ( p 1 + p 4 ) 2 , u = ( p 1 + p 3 ) 2 . Amplitudes depend on the particles being scattered, but they’re all related by SUSY. (See Elvang & Huang’s book.) Silviu Pufu (Princeton University) 10-26-2018 5 / 32

  13. In 11d, we can scatter: gravitons, gravitini, 3-form gauge particles. ⇒ can use 4d N = 8 language. We scatter: Momenta within 4d = graviton (1); gravitinos (8); gravi-photons (28); gravi-photinos (56); scalars (70 = 35 + 35) At leading order in small momentum (i.e. p 2 ), scattering amplitudes are those in N = 8 SUGRA at tree level. Examples: A SUGRA, tree ( h − h − h + h + ) = � 12 � 4 [ 34 ] 4 , stu A SUGRA, tree ( S 1 S 1 S 2 S 2 ) = tu s , where s = ( p 1 + p 2 ) 2 , t = ( p 1 + p 4 ) 2 , u = ( p 1 + p 3 ) 2 . Amplitudes depend on the particles being scattered, but they’re all related by SUSY. (See Elvang & Huang’s book.) Silviu Pufu (Princeton University) 10-26-2018 5 / 32

  14. In 11d, we can scatter: gravitons, gravitini, 3-form gauge particles. ⇒ can use 4d N = 8 language. We scatter: Momenta within 4d = graviton (1); gravitinos (8); gravi-photons (28); gravi-photinos (56); scalars (70 = 35 + 35) At leading order in small momentum (i.e. p 2 ), scattering amplitudes are those in N = 8 SUGRA at tree level. Examples: A SUGRA, tree ( h − h − h + h + ) = � 12 � 4 [ 34 ] 4 , stu A SUGRA, tree ( S 1 S 1 S 2 S 2 ) = tu s , where s = ( p 1 + p 2 ) 2 , t = ( p 1 + p 4 ) 2 , u = ( p 1 + p 3 ) 2 . Amplitudes depend on the particles being scattered, but they’re all related by SUSY. (See Elvang & Huang’s book.) Silviu Pufu (Princeton University) 10-26-2018 5 / 32

  15. In 11d, we can scatter: gravitons, gravitini, 3-form gauge particles. ⇒ can use 4d N = 8 language. We scatter: Momenta within 4d = graviton (1); gravitinos (8); gravi-photons (28); gravi-photinos (56); scalars (70 = 35 + 35) At leading order in small momentum (i.e. p 2 ), scattering amplitudes are those in N = 8 SUGRA at tree level. Examples: A SUGRA, tree ( h − h − h + h + ) = � 12 � 4 [ 34 ] 4 , stu A SUGRA, tree ( S 1 S 1 S 2 S 2 ) = tu s , where s = ( p 1 + p 2 ) 2 , t = ( p 1 + p 4 ) 2 , u = ( p 1 + p 3 ) 2 . Amplitudes depend on the particles being scattered, but they’re all related by SUSY. (See Elvang & Huang’s book.) Silviu Pufu (Princeton University) 10-26-2018 5 / 32

  16. Momentum expansion Momentum expansion takes a universal form (independent of the type of particle): � 1 + ℓ 6 p f R 4 ( s , t ) + ℓ 9 A = A SUGRA, tree p f 1-loop ( s , t ) � + ℓ 12 p f D 6 R 4 ( s , t ) + ℓ 14 p f D 8 R 4 ( s , t ) + · · · . f D 2 n R 4 = symmetric polyn in s , t , u of degree n + 3 Known from type II string theory + SUSY [Green, Tseytlin, Gutperle, Vanhove, Russo, Pioline, . . . ] : f D 6 R 4 ( s , t ) = ( stu ) 2 stu f R 4 ( s , t ) = 3 · 2 7 , 15 · 2 15 . ℓ 10 p f D 4 R 4 allowed by SUSY, but known to vanish. This talk: Reproduce f R 4 and f D 4 R 4 = 0 from ABJM theory. Silviu Pufu (Princeton University) 10-26-2018 6 / 32

Download Presentation
Download Policy: The content available on the website is offered to you 'AS IS' for your personal information and use only. It cannot be commercialized, licensed, or distributed on other websites without prior consent from the author. To download a presentation, simply click this link. If you encounter any difficulties during the download process, it's possible that the publisher has removed the file from their server.

Recommend


More recommend