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Please use this identifier to cite or link to this item: http://repository.iitr.ac.in/handle/123456789/14117
Title: Moduli stabilization, large-volume dS minimum without over(D 3, -)-branes, (non-)supersymmetric black hole attractors and two-parameter Swiss cheese Calabi-Yau's
Authors: Misra, Aalok
Shukla P.
Published in: Nuclear Physics B
Abstract: We consider two sets of issues in this paper. The first has to do with moduli stabilization, existence of "area codes" [A. Giryavets, New attractors and area codes, JHEP 0603 (2006) 020, hep-th/0511215] and the possibility of getting a non-supersymmetric dS minimum without the addition of over(D 3, -)-branes as in KKLT for type II flux compactifications. The second has to do with the "inverse problem" [K. Saraikin, C. Vafa, Non-supersymmetric black holes and topological strings, hep-th/0703214] and "fake superpotentials" [A. Ceresole, G. Dall'Agata, Flow equations for non-BPS extremal black holes, JHEP 0703 (2007) 110, hep-th/0702088] for extremal (non-)supersymmetric black holes in type II compactifications. We use (orientifold of) a "Swiss cheese" Calabi-Yau [J.P. Conlon, F. Quevedo, K. Suruliz, Large-volume flux compactifications: Moduli spectrum and D3/D7 soft supersymmetry breaking, JHEP 0508 (2005) 007, hep-th/0505076] expressed as a degree-18 hypersurface in WCP4 [1, 1, 1, 6, 9] in the "large-volume-scenario" limit [V. Balasubramanian, P. Berglund, J.P. Conlon, F. Quevedo, Systematics of moduli stabilisation in Calabi-Yau flux compactifications, JHEP 0503 (2005) 007, hep-th/0502058]. The main result of our paper is that we show that by including non-perturbative α′ and instanton corrections in the Kähler potential and superpotential [T.W. Grimm, Non-perturbative corrections and modularity in N = 1 type IIB compactifications, arXiv: 0705.3253 [hep-th]], it may be possible to obtain a large-volume non-supersymmetric dS minimum without the addition of anti-D3 branes a la KKLT. The chosen Calabi-Yau has been of relevance also from the point of other studies of Kähler moduli stabilization via non-perturbative instanton contributions [F. Denef, M.R. Douglas, B. Florea, Building a better racetrack, JHEP 0406 (2004) 034, hep-th/0404257] and non-supersymmetric AdS vacua (and their subsequent dS-uplifts) using (α′)3 corrections to the Kähler potential [V. Balasubramanian, P. Berglund, J.P. Conlon, F. Quevedo, Systematics of moduli stabilisation in Calabi-Yau flux compactifications, JHEP 0503 (2005) 007, hep-th/0502058; K. Becker, M. Becker, M. Haack, J. Louis, Supersymmetry breaking and alpha'-corrections to flux induced potentials, JHEP 0206 (2002) 060, hep-th/0204254; A. Westphal, de Sitter string vacua from Kähler uplifting, JHEP 0703 (2007) 102, hep-th/0611332; V. Balasubramanian, P. Berglund, Stringy corrections to Kähler potentials, SUSY breaking, and the cosmological constant problem, JHEP 0411 (2004) 085, hep-th/0408054]. © 2008 Elsevier B.V. All rights reserved.
Citation: Nuclear Physics B (2008), 799(43862): 165-198
URI: https://doi.org/10.1016/j.nuclphysb.2008.03.001
http://repository.iitr.ac.in/handle/123456789/14117
Issue Date: 2008
ISSN: 5503213
Author Scopus IDs: 7402454182
56213746600
Author Affiliations: Misra, A., Department of Physics, Indian Institute of Technology, Roorkee, 247 667 Uttaranchal, India, Physics Department, Theory Unit, CERN, CH-1211 Geneva 23, Switzerland
Shukla, P., Department of Physics, Indian Institute of Technology, Roorkee, 247 667 Uttaranchal, India
Funding Details: P.S. is supported by a C.S.I.R., Government of India, (junior) research fellowship and the work of A.M. is partially supported by D.A.E. (Government of India) Young Scientist Award project grant. A.M. also thanks the CERN theory group for hospitality and the theoretical high energy physics groups at McGill University (specially Keshav Dasgupta), University of Pennsylvania (specially Vijay Balasubramanian), Ohio State University (specially Samir Mathur) and Columbia University (specially D. Kabat), for hospitality where part of this work was done and also where preliminary versions of this work were presented. A.M. also thanks Samir Mathur and Jeremy Michelson for interesting discussions, and Rajesh Gopakumar and Ashoke Sen for interesting questions (that helped improve the arguments of Section 4 ) during A.M.'s presentation of part of the material of this paper at ISM07, Harish-Chandra Research Institute, Allahabad.
Corresponding Author: Misra, A.; Department of Physics, Indian Institute of Technology, Roorkee, 247 667 Uttaranchal, India; email: aalokfph@iitr.ernet.in
Appears in Collections:Journal Publications [PH]

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