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Dmitri Sorokin, INFN Padova Section based on arXiv:1511.03024 with I. Bandos, L. Martucci and M. Tonin VII Round Table Italy-Russia, Dubna, 25-27 November 2015
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Recent(2014-15) burst of interest In applications to cosmology and inflation (S. Ferrara talk). Recent (2014-15) burst of interest in the study of spontaneous breaking of local supersymmetry and the emergence of positive cosmological constant due to Volkov- Akulov goldstini in D=4 sugra. In applications to cosmology and inflation (S. Ferrara talk). One of the aims: One of the aims: provide a solid 4D effective field theory ground for cosmological models constructed in the framework of 10D string theory (e.g. KKLT-like models involving anti- D3-branes to generate dS vacua) Most of the constructions of D=4 sugra with spontaneously broken susy use constrained (nilpotent) superfield description of the Volkov-Akulov goldstini (scalar partners are composed of goldstino bilinears) Antoniadis, Dudas, Ferrara, Kehagias, Farakos, Kallosh, Linde, Porrati, Sagnotti, dall’Agata, Zwirner; Bergshoeff, Freedman, Kallosh, Van Proeyen; Hasegawa,Yamada; Kuzenko; Antoniadis, Markou;… Earlier related studies Earlier related studies of local susy breaking & super-Braut-Englert-Higgs effect in sugra: Volkov & Soroka ‘73, Deser & Zumino ‘77,…, Lindstrom & Rocek ‘79, Samuel & Wess ‘83, Ivanov & Kapustnikov ’84 -’90,… Our goal: Our goal: to generate susy breaking by coupling supergravity to the original VA model which is the most straightforwardly related to the 3-brane constructions 2
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ORIGINAL VOLKOV-AKULOV MODEL ’72 AS A 3-BRANE Goldstino as the manifestation of susy breaking 3 Volkov-Akulov superspace SUSY transform. SUSY invariant VA 1-form: spinor field appears on the brane worldvolume non-linear susy transform. Consider a 4d worldvolume (of a 3-brane) placed in superspace susy breaking parameter 3-brane tesnion (Hughes & Polchinski ‘86, Kallosh ’98)
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volume of 4d surface in superspace 4 From general theory of non-linear realizations it follows (Ivanov & Kapustnikov ’77) that the VA model is universal: all models of spontaneous susy breaking involving goldstino should be related to the VA model by a non-linear transformation of Kuzenko & Tyler 10’-11’ whose general form was obtained only quite ricently Kuzenko & Tyler 10’-11’ Constrained superfield realization of the VA goldstino (Ivanov, Kapustnikov ’77; Rocek 78’,…,Samuel, Wess ‘83; Casalbuoni et al. 89’,…, Komargodski, Seiberg 09’,..) chiral superfield constrained by: Example:
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Volkov -Soroka model ‘73 Deser, Zumino ‘77,…, Lindstrom, Rocek ’79; Ferrara et al; Samuel, Wess ’83; Ivanov, Kapustnikov ’84 -’90,… 5 2014-15 2014-15 Antoniadis, Dudas, Ferrara, Kehagias, Farakos, Kallosh, Linde, Porrati, Sagnotti, dall’Agata, Zwirner: Bergshoeff, Freedman, Kallosh, Van Proeyen; Hasegawa,Yamada; Kuzenko; Antoniadis, Markou;…, Schillo, van der Woerd, Wrase Recent constructions are mainly based on the superconformal approach to supergravity () (see Freedman and Van Proeyen Book for a review) e.g. Samuel, Wess’83 Alternatively, one can use «Poincarè» superspace and superfield forlmalism ( e.g. Samuel, Wess’83 ) Kahler potentialsuperpotential chiral measure SYM kin.term Lagrange multiplier - sugra constraints
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component pure supergravity + VA goldstino to the second order in χ (upon integrating out the auxiliary fields) (Bergshoeff at. all; Hasegawa,Yamada ‘15) 6 AdS sugra action ( Townsend ‘77 ) In the unitary gauge the remaining first line in the action describes a massive gravitino field coupled to gravity with the cosmological constant
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For finding a more direct relation of 4D effective theories with spontaneously broken local susy to 10D stringy constructions which use anti-D3-branes to induce a de Sitter vacuum, it may be useful to couple to supergravity the original Volkov-Akulov 3-brane model, without resorting to the constrained superfields The action has a suggestive geometric form of the sum of three different volumes in N=1, D=4 curved superspace 7 pullback on 3-brane worldvolume in the static gauge for worldvolume diffeomorphisms: All the couplings of VA goldstino to sugra fields is encoded in. In the WZ gauge we obtain:
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8 differ from constrained superfield action superfield action, but should be related by non-linear field redefinitions a la Kuzenko & Tyler
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9 1973 Volkov & Soroka o in 1973 Volkov & Soroka gauged non-linearly realized super-Poincaré group Introduced gauge fields associated with local super-Poincarè generators Constructed translation and susy invariant objects with the use of Stueckelberg-like fields: generalization of VA one-form Volkov-Soroka action: ω - is independent field → constant c can be absorbed by Ψ → cΨ= Ψ’ = “de Sitter sugra“ action - does not transform under susy
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Freedman, van Nieuwenhuizen & Ferrara ‘76 Deser & Zumino ‘76 10 SYSY transformations: The constructed models of local susy breaking demonstrate that coupling of N=1 D=4 supergravity to Volkov-Akulov goldstino in one way or another results (in the unitary gauge) in the Volkov-Soroka action
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We have reviewed models of matter coupled N=1, D=4 supergravity with spontaneously broken supersymmetry triggered by the presence of VA goldstini. Spontaneous SUSY breaking generates a positive contribution to the vacuum energy thus allowing for the appearance of de Sitter vacua in the theory. This makes these supergravity models useful and relevant for cosmological and inflationary model building The realization of the local susy breaking with the use o the space-filling Volkov-Akulov 3-brane coupled to gravity and matter supermultiplets may by useful for finding a more direct connection of these 4d effective field theories to string theory constructions involving anti-D3-branes, like the KKLT model and its refinings 11
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