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String cosmology and String cosmology and String cosmology and the - PowerPoint PPT Presentation

String cosmology and String cosmology and String cosmology and the index of the Dirac Dirac operator operator the index of the Dirac operator the index of the Renata Kallosh Kallosh Renata Kallosh Renata Stanford Stanford Strings and


  1. String cosmology and String cosmology and String cosmology and the index of the Dirac Dirac operator operator the index of the Dirac operator the index of the Renata Kallosh Kallosh Renata Kallosh Renata Stanford Stanford Strings and Fields Strings and Fields YITP, August 20 2005 , August 20 2005 YITP

  2. Outline Outline � String Cosmology, Flux � String Cosmology, Flux Compactification Compactification, Stabilization of , Stabilization of Moduli, Metastable Metastable de Sitter Space, de Sitter Space, KKLT KKLT construction construction Moduli, � When stabilizing instanton corrections are possible? � When stabilizing instanton corrections are possible? How fluxes affect the standard condition ? How fluxes affect the standard condition ? � Index of a � Index of a Dirac Dirac operator on Euclidean M5 operator on Euclidean M5 brane brane and D3 brane brane with background fluxes: with background fluxes: and D3 general condition for existence of instanton instanton corrections corrections general condition for existence of � An example of fixing of all � An example of fixing of all moduli moduli: M : M- -theory on theory on and IIB IIB on : on : D3/D7 D3/D7 cosmological model cosmological model and Work with Aspinwall Aspinwall, Bergshoeff, , Bergshoeff, Kashani Kashani- -Poor, Poor, Sorokin,Tomasiello Sorokin,Tomasiello Work with hep-th/0501081, hep-th/0503138, hep-th/0506014, hep-th/0507069

  3. Our Universe is an Ultimate Test of Fundamental Physics � High High- -energy accelerators will probe the scale energy accelerators will probe the scale � of energies way below GUT scale of energies way below GUT scale � Cosmology and astrophysics are sources of data in the gravitational sector of the fundamental physics (above GUT, near Planck scale)

  4. Impact of the discovery of the current acceleration of the universe Until recently, string theory could not describe acceleration of the early universe (inflation) The discovery of current acceleration made the problem even more severe, but also helped to identify the root of the problem

  5. String Theory and Cosmology String Theory and Cosmology String Theory and Cosmology How to get the 4d 4d near de Sitter near de Sitter and/or and/or de Sitter de Sitter space space How to get the from the compactified 10d string theory or 11d M-theory?

  6. No- -Go Theorems for 4d de Sitter Space Go Theorems for 4d de Sitter Space No from 10/11d string/M theory from 10/11d string/M theory • Gibbons 1985 1985 • de Wit, Smit, Hari Dass, 1987 1987 • Maldacena, Nunez, 2001 2001 How to go around the conditions for How to go around the conditions for de Sitter no- -go theorems? go theorems? de Sitter no How to perform a compactification compactification from from How to perform a 10/11 dimensions to 4 dimensions and 10/11 dimensions to 4 dimensions and stabilize the moduli? stabilize the moduli?

  7. First proposal First proposal Towards cosmology in type IIB string theory string theory Towards cosmology in type IIB Dilaton and complex structure stabilization Dilaton Dilaton and complex structure stabilization and complex structure stabilization Giddings, Kachru and Polchinski Giddings, Kachru and Polchinski Volume stabilization, KKLT Kachru, R.K., Linde, Trivedi Kachru, R.K., Linde, Trivedi 2003 2003 construction of de Sitter space Maloney, Silverstein, Strominger, in non-critical string theory Kachru, R. K., Maldacena, McAllister, Linde, Trivedi INFLATION INFLATION

  8. FLUX COMPACTIFICATION COMPACTIFICATION and and FLUX MODULI STABILIZATION STABILIZATION MODULI FLUXES small numbers FLUXES small numbers in string theory for cosmology in string theory for cosmology � Best understood example: resolved conifold K and M are integer fluxes K and M are integer fluxes

  9. The throat geometry has a highly warped region Redshift in the throat in the throat Redshift

  10. Flux compactification and moduli stabilization in IIB string theory (supergravity + local sources) The potential with respect to dilaton dilaton and volume is very steep, and volume is very steep, moduli moduli run down run down The potential with respect to and V vanishes, the space tends to decompactify decompactify to 10d and string coupling to 10d and string coupling and V vanishes, the space tends to tends to vanish, unless both are stabilized at some finite values. s. tends to vanish, unless both are stabilized at some finite value Dilaton stabilization Dilaton stabilization Dilaton stabilization Warping fixed by local sources (tadpole condition) and non- vanishing ISD fluxes This equation fixes the shape of CY and the dilaton- axion

  11. 4d description * SUSY at scale 1/R(CY) N=1 effective action * Specify the Kahler potential, superpotential and gauge couplings Add the superpotential due to fluxes Add the superpotential due to fluxes � � Solve equations * Solve equations The complex structure fields and the axion-dilaton are fixed. The overall volume still has a runaway potential The overall volume still has a runaway potential

  12. Shape moduli Shape moduli fixed by fluxes fixed by fluxes σ σ Total volume not fixed by fluxes Total volume not fixed by fluxes

  13. Potential Potential No- -scale scale supergravity supergravity No No potential for the volume moduli. Dilaton and shape No potential for the volume moduli. Dilaton and shape moduli are generically fixed in are generically fixed in Minkowski Minkowski space! space! moduli *** Kahler moduli problem (in particular, overall volume) *** Kahler moduli problem (in particular, overall volume) ***KKLT proposal ***KKLT proposal i) non- -perturbative perturbative superpotential from Euclidean D3 superpotential from Euclidean D3- - i) non branes wrapped on special 4- -cycles cycles branes wrapped on special 4 ii) non-perturbative superpotential from pure SYM on a stack of D7’s on

  14. Effective theory for the volume moduli theory for the volume moduli Effective Solve Solve the volume is stabilized in the volume is stabilized in AdS critical point in the regime of validity of AdS critical point in the regime of validity of calculations! calculations!

  15. Volume stabilization Volume stabilization Volume stabilization Basic steps: Basic steps: Warped geometry of the compactified space and nonperturbative nonperturbative effects effects Warped geometry of the compactified space and instantons ) lead to condensation, instantons (gaugino gaugino condensation, ) lead to AdS AdS space space ( negative vacuum energy) with unbroken SUSY and stabilized volume negative vacuum energy) with unbroken SUSY and stabilized volume Uplifting AdS space to a metastable metastable dS space (positive vacuum energy) by dS space (positive vacuum energy) by Uplifting AdS space to a adding anti- -D3 brane at the tip of the D3 brane at the tip of the conifold conifold (or D7 brane with fluxes) (or D7 brane with fluxes) adding anti AdS minimum AdS minimum Metastable dS minimum Metastable dS minimum

  16. in KS warped geometry Metastable Metastable dS vacua vacua V(AdS) + V(anti-D3)= V(dS) dS

  17. RECENT DRAMATIC PROGRESS in moduli stabilization in string theory � KKLT scenario, 2003 � Building a better racetrack , Denef, Douglas, Florea, 2004 � Fixing all moduli in an F-theory compactification, Denef, Douglas, Florea, Grassi, Kachru, 2005 � Fluxes and gaugings, Derendinger, Kounnas, Petropoulos, Zwirner, 2005 � Type IIA moduli stabilization, DeWolfe, Giryavets, Kachru, Taylor, 2005 � Fixing all moduli in M-theory on K3xK3, Aspinwall, R.K. 2005 � On de Sitter vacua in type IIA, Saueressig, Theis, Vandoren, 2005

  18. IIB string compactified on K3x A natural space for D3/D7 cosmological model Dasgupta, Herdeiro, Hirano, R.K; Koyama, Tachikawa and Watari � Flux vacua in this model were studied by Trivedi, Tripathy in string theory, and by Angelantonj, D'Auria, Ferrara, Trigiante in string theory and 4d gauged supergravity. Kähler moduli remained non-fixed. � The minimal remaining moduli space is Hypers Vectors KKLT stabilization Is KKLT stabilization possible is possible for the ? for the volume of volume of K3!

  19. KKLT 1: gaugino condensation. Works only for vector multiplets, does not work for hypers. KKLT 2: 2: instantons instantons from Euclidean 3 from Euclidean 3- -branes wrapped branes wrapped KKLT on 4- -cycles cycles. . May work for vector on 4 May work for vector multiplets multiplets and and hypers hypers. . � On K3 x there are 4-cycles which may or may not lead to non-vanishing instantons Status in 2004 Status in 2004 According to the old rules ( established before fluxes were introduced ), the relevant M-theory divisors in our model have an arithmetic genus 2 . Therefore one could incorrectly conclude that there are no stabilizing instantons for our favorite cosmological model .

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