73 research outputs found
On integrability of strings on symmetric spaces
In the absence of NSNS three-form flux the bosonic string on a symmetric
space is described by a symmetric space coset sigma-model. Such models are
known to be classically integrable. We show that the integrability extends also
to cases with non-zero NSNS flux (respecting the isometries) provided that the
flux satisfies a condition of the form H_{abc}H^{cde}~R_{ab}^{de}. We then turn
our attention to the type II Green-Schwarz superstring on a symmetric space. We
prove that if the space preserves some supersymmetry there exists a truncation
of the full superspace to a supercoset space and derive the general form of the
superisometry algebra. In the case of vanishing NSNS flux the corresponding
supercoset sigma-model for the string is known to be integrable. We prove that
the integrability extends to the full string by augmenting the supercoset Lax
connection with terms involving the fermions which are not captured by the
supercoset model. The construction is carried out to quadratic order in these
fermions. This proves the integrability of strings on symmetric spaces
supported by RR flux which preserve any non-zero amount of supersymmetry.
Finally we also construct Lax connections for some supercoset models with
non-zero NSNS flux describing strings in AdS(2,3) x S(2,3) x S(2,3) x T(2,3,4)
backgrounds preserving eight supersymmetries.Comment: 34 pages; v3: Minor clarifications, matches published version; v4:
Missing local Lorentz transformation added in eqs. (2.14), (2.15) and (4.64
Trivial solutions of generalized supergravity vs non-abelian T-duality anomaly
The equations that follow from kappa symmetry of the type II Green-Schwarz
string are a certain deformation, by a Killing vector field , of the type II
supergravity equations. We analyze under what conditions solutions of these
`generalized' supergravity equations are trivial in the sense that they solve
also the standard supergravity equations. We argue that for this to happen
must be null and satisfy with the NSNS three-form field
strength. Non-trivial examples are provided by symmetric pp-wave solutions. We
then analyze the consequences for non-abelian T-duality and the closely related
homogenous Yang-Baxter sigma models. When one performs non-abelian T-duality of
a string sigma model on a non-unimodular (sub)algebra one generates a
non-vanishing proportional to the trace of the structure constants. This is
expected to lead to an anomaly but we show that when satisfies the same
conditions the anomaly in fact goes away leading to more possibilities for
non-anomalous non-abelian T-duality.Comment: 11 pages; v2: Important clarifications in sec 5 and projections fixed
there. References added. v3: Typos fixed and eq. (5.13) with the general form
of the anomaly in terms of K and X adde
Classifying integrable symmetric space strings via factorized scattering
All symmetric space solutions of type II supergravity have recently
been found for . For the supersymmetric solutions (and their T-duals) it
is known that the Green-Schwarz string is classically integrable. We complete
the classification by ruling out integrability for the remaining
non-supersymmetric solutions. This is achieved by showing that tree-level
scattering on the worldsheet of a GKP or BMN string fails to factorize for
these cases.Comment: 17 pages; v2: Improvements to sec 1, results now summarized in Tab 1.
Matches published versio
Constraining integrable AdS/CFT with factorized scattering
We consider (warped) AdS string backgrounds which allow for a GKP spinning
string/null cusp solution. Integrability implies that the worldsheet S-matrix
should factorize, which in turn constrains the form of the warp factor as a
function of the coordinates of the internal space. This constraint is argued to
rule out integrability for all supersymmetric AdS7 and AdS6 backgrounds as well
as AdS5 Gaiotto-Maldacena backgrounds and a few highly supersymmetric AdS4 and
AdS3 backgrounds.Comment: 19 pages; v2: Further clarifications in sec 4 and 5. Published
versio
Worldsheet scattering in AdS(3)/CFT(2)
We confront the recently proposed exact S-matrices for AdS(3)/CFT(2) with
direct worldsheet calculations. Utilizing the BMN and Near Flat Space (NFS)
expansions for strings on AdS(3) x S(3) x S(3) x S(1) and AdS(3) x S(3) x T(4)
we compute both tree-level and one-loop scattering amplitudes. Up to some minor
issues we find nice agreement in the tree-level sector. At the one-loop level
however we find that certain non-zero tree-level processes, which are not
visible in the exact solution, contribute, via the optical theorem, and give an
apparent mismatch for certain amplitudes. Furthermore we find that a proposed
one-loop modification of the dressing phase correctly reproduces the worldsheet
calculation while the standard Hernandez-Lopez phase does not. We also compute
several massless to massless processes.Comment: 20 pages, 1 figure; v2: Some clarifications in comparison to
literatur
The AdS(n) x S(n) x T(10-2n) BMN string at two loops
We calculate the two-loop correction to the dispersion relation for
worldsheet modes of the BMN string in AdS(n) x S(n) x T(10-2n) for n=2,3,5. For
the massive modes the result agrees with the exact dispersion relation derived
from symmetry considerations with no correction to the interpolating function
h. For the massless modes in AdS(3) x S(3) x T(4) however our result does not
match what one expects from the corresponding symmetry based analysis. We also
derive the S-matrix for massless modes up to the one-loop order. The scattering
phase is given by the massless limit of the Hernandez-Lopez phase. In addition
we compute a certain massless S-matrix element at two loops and show that it
vanishes suggesting that the two-loop phase in the massless sector is zero.Comment: 30 pages, 6 figures; v2: References and comment on type IIB added,
acknowledgements updated; v3: Comparison to proposed exact massless S-matrix
in sec 5.3 corrected. Only non-trivial phase appears at one loop. Additional
minor clarification
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