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Supergravity was born in 1976 Supergravity was born in 1976 It has - PowerPoint PPT Presentation

Holography for N = 1 on S 4 Nikolay Bobev Instituut voor Theoretische Fysica KU Leuven Supergravity@40, GGI, Firenze October 27 2016 1311.1508 + 1605.00656 with Henriette Elvang, Daniel Freedman, Silviu Pufu Uri Kol, Tim Olson


  1. Holography for N = 1 ∗ on S 4 Nikolay Bobev Instituut voor Theoretische Fysica KU Leuven Supergravity@40, GGI, Firenze October 27 2016 1311.1508 + 1605.00656 with Henriette Elvang, Daniel Freedman, Silviu Pufu Uri Kol, Tim Olson

  2. Supergravity was born in 1976

  3. Supergravity was born in 1976 It has inspired many important developments in theoretical physics over the past 40 years!

  4. AdS/CFT Supersymmetric QFT on curved space

  5. 5d N = 8 gauged SO (6) supergravity

  6. Motivation ◮ Powerful exact results for supersymmetric field theories on curved manifolds using equivariant localization [Witten], [Nekrasov], [Pestun], ...

  7. Motivation ◮ Powerful exact results for supersymmetric field theories on curved manifolds using equivariant localization [Witten], [Nekrasov], [Pestun], ... ◮ Supersymmetric localization (sometimes) reduces the path integral of a gauge theory to a finite dimensional matrix integral. Still hard to evaluate explicitly in general!

  8. Motivation ◮ Powerful exact results for supersymmetric field theories on curved manifolds using equivariant localization [Witten], [Nekrasov], [Pestun], ... ◮ Supersymmetric localization (sometimes) reduces the path integral of a gauge theory to a finite dimensional matrix integral. Still hard to evaluate explicitly in general! ◮ Make progress by taking the planar limit for specific 4d N = 2 (non-conformal) gauge theories. [Russo], [Russo-Zarembo], [Buchel-Russo-Zarembo]

  9. Motivation ◮ Powerful exact results for supersymmetric field theories on curved manifolds using equivariant localization [Witten], [Nekrasov], [Pestun], ... ◮ Supersymmetric localization (sometimes) reduces the path integral of a gauge theory to a finite dimensional matrix integral. Still hard to evaluate explicitly in general! ◮ Make progress by taking the planar limit for specific 4d N = 2 (non-conformal) gauge theories. [Russo], [Russo-Zarembo], [Buchel-Russo-Zarembo] ◮ Evaluation of the partition function of planar SU ( N ) , N = 2 ∗ SYM on S 4 . An infinite number of quantum phase transitions as a function of λ ≡ g 2 YM N . [Russo-Zarembo]

  10. Motivation ◮ Powerful exact results for supersymmetric field theories on curved manifolds using equivariant localization [Witten], [Nekrasov], [Pestun], ... ◮ Supersymmetric localization (sometimes) reduces the path integral of a gauge theory to a finite dimensional matrix integral. Still hard to evaluate explicitly in general! ◮ Make progress by taking the planar limit for specific 4d N = 2 (non-conformal) gauge theories. [Russo], [Russo-Zarembo], [Buchel-Russo-Zarembo] ◮ Evaluation of the partition function of planar SU ( N ) , N = 2 ∗ SYM on S 4 . An infinite number of quantum phase transitions as a function of λ ≡ g 2 YM N . [Russo-Zarembo] ◮ Apply gauge/gravity duality to this setup and test holography in a non-conformal setup.

  11. Motivation ◮ Powerful exact results for supersymmetric field theories on curved manifolds using equivariant localization [Witten], [Nekrasov], [Pestun], ... ◮ Supersymmetric localization (sometimes) reduces the path integral of a gauge theory to a finite dimensional matrix integral. Still hard to evaluate explicitly in general! ◮ Make progress by taking the planar limit for specific 4d N = 2 (non-conformal) gauge theories. [Russo], [Russo-Zarembo], [Buchel-Russo-Zarembo] ◮ Evaluation of the partition function of planar SU ( N ) , N = 2 ∗ SYM on S 4 . An infinite number of quantum phase transitions as a function of λ ≡ g 2 YM N . [Russo-Zarembo] ◮ Apply gauge/gravity duality to this setup and test holography in a non-conformal setup. ◮ Study the dynamics of N = 1 theories holographically. Localization on S 4 has not been successful (so far!) for these theories!

  12. Synopsis ◮ N = 1 ∗ SYM is a theory of an N = 1 vector multiplet and 3 massive chiral multiplets in the adjoint of the gauge group. It is a massive deformation of N = 4 SYM. There is a unique supersymmetric Lagrangian on S 4 . [Pestun], [Festuccia-Seiberg], [NB-Elvang-Freedman-Pufu]

  13. Synopsis ◮ N = 1 ∗ SYM is a theory of an N = 1 vector multiplet and 3 massive chiral multiplets in the adjoint of the gauge group. It is a massive deformation of N = 4 SYM. There is a unique supersymmetric Lagrangian on S 4 . [Pestun], [Festuccia-Seiberg], [NB-Elvang-Freedman-Pufu] ◮ The result from localization for N , λ ≫ 1 for N = 2 ∗ is [Russo-Zarembo] 2 (1 + ( mR ) 2 ) log λ (1 + ( mR ) 2 ) e 2 γ + 1 = − N 2 2 F N =2 ∗ = − log Z N =2 ∗ , S 4 S 4 16 π 2 For N = 1 ∗ hard to calculate the partition function in the field theory.

  14. Synopsis ◮ N = 1 ∗ SYM is a theory of an N = 1 vector multiplet and 3 massive chiral multiplets in the adjoint of the gauge group. It is a massive deformation of N = 4 SYM. There is a unique supersymmetric Lagrangian on S 4 . [Pestun], [Festuccia-Seiberg], [NB-Elvang-Freedman-Pufu] ◮ The result from localization for N , λ ≫ 1 for N = 2 ∗ is [Russo-Zarembo] 2 (1 + ( mR ) 2 ) log λ (1 + ( mR ) 2 ) e 2 γ + 1 = − N 2 2 F N =2 ∗ = − log Z N =2 ∗ , S 4 S 4 16 π 2 For N = 1 ∗ hard to calculate the partition function in the field theory. ◮ The goal is to calculate F N =2 ∗ and F N =1 ∗ holographically. S 4 S 4

  15. Synopsis ◮ N = 1 ∗ SYM is a theory of an N = 1 vector multiplet and 3 massive chiral multiplets in the adjoint of the gauge group. It is a massive deformation of N = 4 SYM. There is a unique supersymmetric Lagrangian on S 4 . [Pestun], [Festuccia-Seiberg], [NB-Elvang-Freedman-Pufu] ◮ The result from localization for N , λ ≫ 1 for N = 2 ∗ is [Russo-Zarembo] 2 (1 + ( mR ) 2 ) log λ (1 + ( mR ) 2 ) e 2 γ + 1 = − N 2 2 F N =2 ∗ = − log Z N =2 ∗ , S 4 S 4 16 π 2 For N = 1 ∗ hard to calculate the partition function in the field theory. ◮ The goal is to calculate F N =2 ∗ and F N =1 ∗ holographically. S 4 S 4 ◮ Precision test of holography! In AdS 5 / CFT 4 one typically compares numbers. Here we have a whole function to match.

  16. Synopsis ◮ N = 1 ∗ SYM is a theory of an N = 1 vector multiplet and 3 massive chiral multiplets in the adjoint of the gauge group. It is a massive deformation of N = 4 SYM. There is a unique supersymmetric Lagrangian on S 4 . [Pestun], [Festuccia-Seiberg], [NB-Elvang-Freedman-Pufu] ◮ The result from localization for N , λ ≫ 1 for N = 2 ∗ is [Russo-Zarembo] 2 (1 + ( mR ) 2 ) log λ (1 + ( mR ) 2 ) e 2 γ + 1 = − N 2 2 F N =2 ∗ = − log Z N =2 ∗ , S 4 S 4 16 π 2 For N = 1 ∗ hard to calculate the partition function in the field theory. ◮ The goal is to calculate F N =2 ∗ and F N =1 ∗ holographically. S 4 S 4 ◮ Precision test of holography! In AdS 5 / CFT 4 one typically compares numbers. Here we have a whole function to match. ◮ Previous results from holography for N = 1 ∗ and N = 2 ∗ on R 4 . [Freedman-Gubser-Pilch-Warner], [Girardello-Petrini-Porrati-Zaffaroni], [Pilch-Warner], [Buchel-Peet-Polchinski], [Evans-Johnson-Petrini], [Polchinski-Strassler], ... On S 4 the holographic construction is more involved.

  17. Plan ◮ N = 1 ∗ SYM theory on S 4 ◮ The supergravity dual ◮ Holographic calculations ◮ Outlook

  18. N = 1 ∗ SYM theory on S 4

  19. N = 1 ∗ SYM on R 4 The field content of N = 4 SYM is A µ , X 1 , 2 , 3 , 4 , 5 , 6 , λ 1 , 2 , 3 , 4 .

  20. N = 1 ∗ SYM on R 4 The field content of N = 4 SYM is A µ , X 1 , 2 , 3 , 4 , 5 , 6 , λ 1 , 2 , 3 , 4 . Organize this into an N = 1 vector multiplet A µ , ψ 1 ≡ λ 4 , and 3 chiral multiplets 1 � � χ j = λ j , Z j = √ X j + iX j +3 , j = 1 , 2 , 3 . 2 Only SU (3) × U (1) R of the SO (6) R-symmetry is manifest.

  21. N = 1 ∗ SYM on R 4 The field content of N = 4 SYM is A µ , X 1 , 2 , 3 , 4 , 5 , 6 , λ 1 , 2 , 3 , 4 . Organize this into an N = 1 vector multiplet A µ , ψ 1 ≡ λ 4 , and 3 chiral multiplets 1 � � χ j = λ j , Z j = √ X j + iX j +3 , j = 1 , 2 , 3 . 2 Only SU (3) × U (1) R of the SO (6) R-symmetry is manifest. The N = 1 ∗ theory is obtained by turning on (independent) mass terms for the chiral multiplets.

  22. N = 1 ∗ SYM on S 4 The theory is no longer conformal so it is not obvious how to put it on S 4 .

  23. N = 1 ∗ SYM on S 4 The theory is no longer conformal so it is not obvious how to put it on S 4 . When there is a will there is a way! [Pestun], [Festuccia-Seiberg], ...

  24. N = 1 ∗ SYM on S 4 The theory is no longer conformal so it is not obvious how to put it on S 4 . When there is a will there is a way! [Pestun], [Festuccia-Seiberg], ... L S 4 N =1 ∗ = L S 4 N =4 + 2 Z 1 ˜ Z 1 + Z 2 ˜ Z 2 + Z 3 ˜ R 2 tr � � Z 3 + tr � m 1 Z 1 ˜ m 2 Z 2 ˜ m 3 Z 3 ˜ � m 1 ˜ Z 1 + m 2 ˜ Z 2 + m 3 ˜ Z 3 − 1 2 tr ( m 1 χ 1 χ 1 + m 2 χ 2 χ 2 + m 3 χ 3 χ 3 + ˜ m 1 ˜ χ 1 ˜ χ 1 + ˜ m 2 ˜ χ 2 ˜ χ 2 + ˜ m 3 ˜ χ 3 ˜ χ 3 ) − 1 m i ǫ ijk ˜ m i ǫ ijk Z i ˜ Z j ˜ tr � � √ Z k + ˜ Z i Z j Z k 2 i 2 + ˜ 2 + ˜ � 2 � m 1 Z 2 1 + m 2 Z 2 2 + m 3 Z 2 m 1 ˜ m 2 ˜ m 3 ˜ + 2 R tr 3 + ˜ Z 1 Z 2 Z 3 . 15 (real) relevant operators in the Lagrangian + 1 complex gaugino vev + 1 complexified gauge coupling. Only 18 of these operators are visible as modes in IIB supergravity. m we get the N = 2 ∗ For m 3 = ˜ m 3 = 0 , m 1 = m 2 ≡ m and ˜ m 1 = ˜ m 2 ≡ ˜ theory.

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