Kappa-symmetry of superstring sigma model and generalized 10d supergravity equations
A bstract 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...
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Published in | The journal of high energy physics Vol. 2016; no. 6; pp. 1 - 28 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
Berlin/Heidelberg
Springer Berlin Heidelberg
01.06.2016
Springer Nature B.V |
Subjects | |
Online Access | Get full text |
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Summary: | A
bstract
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
ϕ
(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
ϕ
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. |
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Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 14 content type line 23 |
ISSN: | 1029-8479 1029-8479 |
DOI: | 10.1007/JHEP06(2016)174 |