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Автор Joseph P. Conlon
Автор Daniel Cremades
Автор Fernando Quevedo
Дата выпуска 2007-01-01
dc.description The Kähler potential is the least understood part of effective N = 1 supersymmetric theories derived from string compactifications. Even at tree-level, the Kähler potential for the physical matter fields, as a function of the moduli fields, is unknown for generic Calabi-Yau compactifications and has only been computed for simple toroidal orientifolds. In this paper we describe how the modular dependence of matter metrics may be extracted in a perturbative expansion in the Kähler moduli. Scaling arguments, locality and knowledge of the structure of the physical Yukawa couplings are sufficient to find the relevant Kähler potential. Using these techniques we compute the `modular weights' for bifundamental matter on wrapped D7 branes for large-volume IIB Calabi-Yau flux compactifications. We also apply our techniques to the case of toroidal compactifications, obtaining results consistent with those present in the literature. Our techniques do not provide the complex structure moduli dependence of the Kähler potential, but are sufficient to extract relevant information about the canonically normalised matter fields and the soft supersymmetry breaking terms in gravity mediated scenarios.
Формат application.pdf
Издатель Institute of Physics Publishing
Название Kähler potentials of chiral matter fields for Calabi-Yau string compactifications
Тип paper
DOI 10.1088/1126-6708/2007/01/022
Electronic ISSN 1029- 8479
Print ISSN 1126-6708
Журнал Journal of High Energy Physics
Том 2007
Первая страница 22
Последняя страница 022
Аффилиация Joseph P. Conlon; DAMTP, Centre for Mathematical Sciences, Wilberforce Road, Cambridge, CB3 0WA, U.K.
Аффилиация Daniel Cremades; DAMTP, Centre for Mathematical Sciences, Wilberforce Road, Cambridge, CB3 0WA, U.K.
Аффилиация Fernando Quevedo; DAMTP, Centre for Mathematical Sciences, Wilberforce Road, Cambridge, CB3 0WA, U.K.
Выпуск 01

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