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Luca Martucci On moduli and e ff ective theory of N=1 warped compactifications Based on: arXiv:0902.4031 15- ti European Workshop on S ts ing Ti eor y Z rich, 7-11 Sep tf mber 2009 Motivation: fluxes and


  1. Luca Martucci On moduli and e ff ective theory of N=1 warped compactifications Based on: arXiv:0902.4031 15- ti European Workshop on S ts ing Ti eor y Zü rich, 7-11 Sep tf mber 2009

  2. �������� ���� Motivation: fluxes and 4D physics In type II flux compactifications w the internal space is not CY

  3. �������� ���� Motivation: fluxes and 4D physics In type II flux compactifications w the internal space is not CY what is the 4D effective physics?

  4. �������� ���� Motivation: fluxes and 4D physics In type II flux compactifications w the internal space is not CY what is the 4D effective physics? Furthermore fluxes generically generate a non-trivial warping: with

  5. �������� ���� Motivation: fluxes and 4D physics In type II flux compactifications w the internal space is not CY what is the 4D effective physics? Furthermore fluxes generically generate a non-trivial warping: with Neglecting back-reaction: , 4D effective theory: (fluxless) CY spectrum (using standard CY tools) flux induced potential

  6. �������� ���� Motivation: fluxes and 4D physics In type II flux compactifications w the internal space is not CY what is the 4D effective physics? Furthermore fluxes generically generate a non-trivial warping: with What can we say about 4D effective theory of fully back-reacted vacua?

  7. Plan of the talk Type II (generalized complex) flux vacua Moduli, twisted cohomologies and 4D fields Kähler potential

  8. Type II (generalized complex) flux vacua

  9. ���� �������� Fluxes and SUSY w

  10. �������� ���� Fluxes and SUSY NS sector: w metric dilaton 3-form ( locally)

  11. �������� ���� Fluxes and SUSY NS sector: w metric dilaton 3-form ( locally) RR sector:

  12. �������� ���� Fluxes and SUSY NS sector: w metric dilaton 3-form ( locally) ( ) RR sector:

  13. �������� ���� Fluxes and SUSY NS sector: w metric dilaton 3-form ( locally) ( ) RR sector: � , with C = C k − 1 k

  14. ���� �������� Fluxes and SUSY Killing spinors: w

  15. �������� ���� Fluxes and SUSY Killing spinors: w Polyforms: ,

  16. �������� ���� Fluxes and SUSY Killing spinors: w Polyforms: , , IIA

  17. �������� ���� Fluxes and SUSY Killing spinors: w Polyforms: , , IIA , IIB

  18. �������� ���� Fluxes and SUSY Killing spinors: w Polyforms: , , IIA , IIB and are O(6,6) pure spinors!

  19. �������� ���� Fluxes and SUSY Killing spinors: w Polyforms: , they contain complete information about NS sector and SUSY

  20. �������� ���� Fluxes and SUSY Killing spinors: w Polyforms: , they contain complete information about NS sector and SUSY SUSY conditions Graña, Minasian, Petrini & Tomasiello `05 , ,

  21. �������� ���� Fluxes and SUSY Killing spinors: w Polyforms: , they contain complete information about NS sector and SUSY SUSY conditions Graña, Minasian, Petrini & Tomasiello `05 , , L.M. & Smyth `05 generalized calibrations precise interpretation in terms of: Koerber & L.M.`07 F- and D- flatness

  22. SUSY and GC geometry (F-flatness)

  23. SUSY and GC geometry integrable Hitchin `02 generalized complex structure (F-flatness)

  24. SUSY and GC geometry integrable Hitchin `02 generalized complex structure (F-flatness) symplectic (IIA) e.g. complex (IIB)

  25. SUSY and GC geometry integrable Hitchin `02 generalized complex structure (F-flatness) Induced polyform decomposition Gualtieri `04 6 3 � � Λ n T ∗ U k M = n =0 k = − 3

  26. SUSY and GC geometry integrable Hitchin `02 generalized complex structure (F-flatness) Induced polyform decomposition Gualtieri `04 6 3 � � Λ n T ∗ U k M = n =0 k = − 3

  27. SUSY and GC geometry integrable Hitchin `02 generalized complex structure (F-flatness) Induced polyform decomposition Gualtieri `04 6 3 � � Λ n T ∗ U k M = n =0 k = − 3 e.g. complex case

  28. SUSY and GC geometry integrable Hitchin `02; generalized complex structure (F-flatness) Induced polyform decomposition Gualtieri `04 6 3 � � Λ n T ∗ U k M = n =0 k = − 3 Integrability GC structure with

  29. SUSY and GC geometry integrable Hitchin `02; generalized complex structure (F-flatness) Induced polyform decomposition Gualtieri `04 6 3 � � Λ n T ∗ U k M = n =0 k = − 3 Integrability GC structure with Generalized Hodge decomposition (assuming -lemma) Cavalcanti `05

  30. Moduli, twisted cohomologies and 4D fields

  31. Moduli and polyforms

  32. Moduli and polyforms The full closed string information is stored in Koerber & L.M.`07 see also: Grañã, Louis & Waldram `05;`06 Benmachiche and Grimm `06 ,

  33. Moduli and polyforms The full closed string information is stored in Koerber & L.M.`07 see also: Grañã, Louis & Waldram `05;`06 Benmachiche and Grimm `06 , `half’ of NS degrees of freedom

  34. Moduli and polyforms The full closed string information is stored in Koerber & L.M.`07 see also: Grañã, Louis & Waldram `05;`06 Benmachiche and Grimm `06 , information encoded in `half’ of NS degrees of freedom (second `half’ of NS degrees of freedom)

  35. Moduli and polyforms The full closed string information is stored in Koerber & L.M.`07 see also: Grañã, Louis & Waldram `05;`06 Benmachiche and Grimm `06 , information encoded in `half’ of NS degrees RR degrees of of freedom freedom (second `half’ of NS degrees of freedom)

  36. Moduli and polyforms The full closed string information is stored in Koerber & L.M.`07 see also: Grañã, Louis & Waldram `05;`06 Benmachiche and Grimm `06 , information encoded in `half’ of NS degrees RR degrees of of freedom freedom (second `half’ of NS degrees of freedom) The and moduli are associated to twisted cohomology classes of: ,

  37. Moduli and 4D fields

  38. Moduli and 4D fields moduli space of Hitchin `02;

  39. Moduli and 4D fields moduli space of Hitchin `02;

  40. Moduli and 4D fields In principle, all -moduli can be lifted (up to rescaling) moduli space of Hitchin `02;

  41. Moduli and 4D fields In principle, all -moduli can be lifted (up to rescaling) moduli space of Hitchin `02; ( ) assuming for minimal SUSY

  42. Moduli and 4D fields In principle, all -moduli can be lifted (up to rescaling) moduli space of Hitchin `02; ( ) assuming for minimal SUSY , -moduli RR axionic shift

  43. Moduli and 4D fields In principle, all -moduli can be lifted (up to rescaling) moduli space of Hitchin `02; ( ) assuming for minimal SUSY , -moduli RR axionic shift and will be 4D chiral fields of 4D superconformal theory see e.g.: Kallosh, Kofman, Linde & Van Proeyen`00 Weyl-chiral weights:

  44. Dual picture: linear multiplets

  45. Dual picture: linear multiplets D-flatness condition

  46. Dual picture: linear multiplets D-flatness condition

  47. Dual picture: linear multiplets D-flatness condition Expand: , bosonic components of linear multiplets dual to

  48. Dual picture: linear multiplets D-flatness condition Expand: , bosonic components of linear multiplets dual to Linear-chiral functional dependence explicit form depends on microscopical details

  49. Grañã & Polchinski; Example: IIB warped CY Gubser `00 Giddings, Kachru & Polchinski `01

  50. Grañã & Polchinski; Example: IIB warped CY Gubser `00 Giddings, Kachru & Polchinski `01

  51. Grañã & Polchinski; Example: IIB warped CY Gubser `00 Giddings, Kachru & Polchinski `01

  52. Grañã & Polchinski; Example: IIB warped CY Gubser `00 Giddings, Kachru & Polchinski `01 complex structure moduli, lifted up to conformal compensator

  53. Grañã & Polchinski; Example: IIB warped CY Gubser `00 Giddings, Kachru & Polchinski `01 complex structure moduli, lifted up to conformal compensator

  54. Grañã & Polchinski; Example: IIB warped CY Gubser `00 Giddings, Kachru & Polchinski `01 complex structure moduli, lifted up to conformal compensator

  55. Grañã & Polchinski; Example: IIB warped CY Gubser `00 Giddings, Kachru & Polchinski `01 complex structure moduli, lifted up to conformal compensator Chiral fields:

  56. Grañã & Polchinski; Example: IIB warped CY Gubser `00 Giddings, Kachru & Polchinski `01 complex structure moduli, lifted up to conformal compensator Chiral fields: removed axion-dilaton

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