Imperial College London

ProfessorArkadyTseytlin

Faculty of Natural SciencesDepartment of Physics

Professor of Theoretical Physics
 
 
 
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Contact

 

+44 (0)20 7594 1890a.tseytlin Website

 
 
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Location

 

685Huxley BuildingSouth Kensington Campus

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Summary

 

Publications

Citation

BibTex format

@article{Tseytlin:2016:10.1007/JHEP06(2016)174,
author = {Tseytlin, AA and Wulff, L},
doi = {10.1007/JHEP06(2016)174},
journal = {Journal of High Energy Physics},
title = {Kappa-symmetry of superstring sigma model and generalized 10d supergravity equations},
url = {http://dx.doi.org/10.1007/JHEP06(2016)174},
volume = {2016},
year = {2016}
}

RIS format (EndNote, RefMan)

TY  - JOUR
AB - We determine the constraints imposed on the 10d target superspace geometry by the requirement of classical kappa-symmetry of the Green-Schwarz superstring. In the type I case we find that the background must satisfy a generalization of type I supergravity equations. These equations depend on an arbitrary vector X a and imply the one-loop scale invariance of the GS sigma model. In the special case when X a is the gradient of a scalar (dilaton) one recovers the standard type I equations equivalent to the 2d Weyl invariance conditions of the superstring sigma model. In the type II case we find a generalized version of the 10d supergravity equations the bosonic part of which was introduced in arXiv:1511.05795. These equations depend on two vectors X a and K a subject to 1st order differential relations (with the equations in the NS-NS sector depending only on the combination X a = X a + K a ). In the special case of K a = 0 one finds that X a = ∂ a and thus obtains the standard type II supergravity equations. New generalized solutions are found if K a is chosen to be a Killing vector (and thus they exist only if the metric admits an isometry). Non-trivial solutions of the generalized equations describe K-isometric backgrounds that can be mapped by T-duality to type II supergravity solutions with dilaton containing a linear isometry-breaking term. Examples of such backgrounds appeared recently in the context of integrable η-deformations of AdS n × S n sigma models. The classical kappa-symmetry thus does not, in general, imply the 2d Weyl invariance conditions for the GS sigma model (equivalent to type II supergravity equations) but only weaker scale invariance type conditions.
AU - Tseytlin,AA
AU - Wulff,L
DO - 10.1007/JHEP06(2016)174
PY - 2016///
SN - 1029-8479
TI - Kappa-symmetry of superstring sigma model and generalized 10d supergravity equations
T2 - Journal of High Energy Physics
UR - http://dx.doi.org/10.1007/JHEP06(2016)174
UR - http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000411289600004&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
UR - http://hdl.handle.net/10044/1/65970
VL - 2016
ER -