17,884 research outputs found
Massive higher spins and holography
We review recent progress towards the understanding of higher spin gauge
symmetry breaking in AdS space from a holographic vantage point. According to
the AdS/CFT correspondence, N=4 SYM theory at vanishing coupling constant
should be dual to a theory in AdS which exhibits higher spin gauge symmetry
enhancement. When the SYM coupling is non-zero, all but a handful of HS
currents are violated by anomalies, and correspondingly local higher spin
symmetry in the bulk gets spontaneously broken. In agreement with previous
results and holographic expectations, we find that, barring one notable
exception (spin 1 eating spin 0), the Goldstone modes responsible for HS
symmetry breaking in AdS have non-vanishing mass even in the limit in which the
gauge symmetry is restored. We show that spontaneous breaking a' la
Stueckelberg implies that the mass of the relevant spin s'=s-1 Goldstone field
is exactly the one predicted by the correspondence.Comment: 8 pages, talk presented by M.B. at the "Fourth Meeting on Constrained
Dynamics and Quantum gravity" held in Cala Gonone (Sardinia, Italy),
September 12-16, 200
Type IIB Orientifolds with NS-NS Antisymmetric Tensor Backgrounds
We consider six dimensional N=1 space-time supersymmetric Type IIB
orientifolds with non-zero untwisted NS-NS sector B-field. The B-field is
quantized due to the requirement that the Type IIB spectrum be left-right
symmetric. The presence of the B-field results in rank reduction of both 99 and
55 open string sector gauge groups. We point out that in some of the models
with non-zero B-field there are extra tensor multiplets in the Z_2 twisted
closed string sector, and we explain their origin in a simple example. Also,
the 59 open string sector states come with a multiplicity that depends on the
B-field. These two facts are in accord with anomaly cancellation requirements.
We point out relations between various orientifolds with and without the
B-field, and also discuss the F-theory duals of these models.Comment: 13 pages, revtex, minor misprints correcte
Three-Point Functions of Quarter BPS Operators in N=4 SYM
In a recent paper hep-th/0109064, quarter-BPS chiral primaries were
constructed in the fully interacting four dimensional N=4 Super-Yang-Mills
theory with gauge group SU(N). These operators are annihilated by four
supercharges, and at order g^2 have protected scaling dimension and
normalization. Here, we compute three-point functions involving these
quarter-BPS operators along with half-BPS operators. The combinatorics of the
problem is rather involved, and we consider the following special cases: (1)
correlators of two half-BPS primaries with an arbitrary
chiral primary; (2) certain classes of and < quarter
quarter quarter > three-point functions; (3) three-point functions involving
the Delta
correlators with the special quarter-BPS operator made of single and double
trace operators only. The analysis in cases (1)-(3) is valid for general N,
while (4) is a large N approximation. Order g^2 corrections to all three-point
functions considered in this paper are found to vanish.
In the AdS/CFT correspondence, quarter-BPS chiral primaries are dual to
threshold bound states of elementary supergravity excitations. We present a
supergravity discussion of two- and three-point correlators involving these
bound states.Comment: 44 pages, Latex, eps figures, uses epsfig.sty; references adde
On the spectrum of AdS/CFT beyond supergravity
We test the spectrum of string theory on AdS_5 x S^5 derived in
hep-th/0305052 against that of single-trace gauge invariant operators in free
N=4 super Yang-Mills theory. Masses of string excitations at critical tension
are derived by extrapolating plane-wave frequencies at g_{YM}=0 down to finite
J. On the SYM side, we present a systematic description of the spectrum of
single-trace operators and its reduction to PSU(2,2|4) superconformal primaries
via a refined Eratostenes' supersieve. We perform the comparison of the
resulting SYM/string spectra of charges and multiplicities order by order in
the conformal dimension \Delta up to \Delta=10 and find perfect agreement.
Interestingly, the SYM/string massive spectrum exhibits a hidden symmetry
structure larger than expected, with bosonic subgroup SO(10,2) and thirty-two
supercharges.Comment: 28 pages, LaTeX2
A Chiral N=1 Type I Vacuum in Four Dimensions and Its Heterotic Dual
In this paper we consider Type I string theory compactified on a Z_7
orbifold. The model has N=1 supersymmetry, a U(4) \otimes U(4) \otimes U(4)
\otimes SO(8) gauge group, and chiral matter. There are only D9-branes (for
which we discuss tadpole cancellation conditions) in this model corresponding
to a perturbative heterotic description in a certain region of the moduli
space. We construct the heterotic dual, match the perturbative type I and
heterotic tree-level massless spectra via giving certain scalars appropriate
vevs, and point out the crucial role of the perturbative superpotential (on the
heterotic side) for this matching. The relevant couplings in this
superpotential turn out to be non-renormalizable (unlike the Z-orbifold case
discussed in Ref [1], where Yukawa couplings sufficed for duality matching). We
also discuss the role of the anomalous U(1) gauge symmetry present in both type
I and heterotic models. In the perturbative regime we match the (tree-level)
moduli spaces of these models. We point out possible generalizations of the Z_3
and Z_7 cases to include D5-branes which would help in understanding
non-perturbative five-brane dynamics on the heterotic side.Comment: Revtex 3.0, 23 pages, 1 eps figure (to appear in Phys. Rev. D
Simplifying one-loop amplitudes in superstring theory
We show that 4-point vector boson one-loop amplitudes, computed in ref.[1] in
the RNS formalism, around vacuum configurations with open unoriented strings,
preserving at least N=1 SUSY in D=4, satisfy the correct supersymmetry Ward
identities, in that they vanish for non MHV configurations (++++) and (-+++).
In the MHV case (--++) we drastically simplify their expressions. We then study
factorisation and the limiting IR and UV behaviour and find some unexpected
results. In particular no massless poles are exposed at generic values of the
modular parameter. Relying on the supersymmetric properties of our bosonic
amplitudes, we extend them to manifestly supersymmetric super-amplitudes and
compare our results with those obtained in the D=4 hybrid formalism, pointing
out difficulties in reconciling the two approaches for contributions from N=1,2
sectors.Comment: 38 pages plus appendice
Cooperative damping mechanism of the resonance in the nuclear photoabsorption
We propose a resonance damping mechanism to explain the disappearance of the
peaks around the position of the resonances higher than the resonance
in the nuclear photoabsorption. This phenomenon is understood by taking into
account the cooperative effect of the collision broadening of and
, the pion distortion and the interference in the two-pion
photoproduction processes in the nuclear medium.Comment: 11 pages, uses revtex.sty. To appear in Phys. Rev. Let
On Exact Symmetries and Massless Vectors in Holographic Flows and other Flux Vacua
We analyze the isometries of Type IIB flux vacua based on the
Papadopolous-Tseytlin ansatz and identify the related massless bulk vector
fields. To this end we devise a general ansatz, valid in any flux
compactification, for the fluctuations of the metric and p-forms that
diagonalizes the coupled equations. We then illustrate the procedure in the
simple case of holographic flows driven by the RR 3-form flux only.
Specifically we study the fate of the isometries of the Maldacena-Nunez
solution associated to wrapped D5-branes.Comment: 23 page
Multiwavelength campaign on Mrk 509: testing realistic comptonization models
Mrk 509 was observed by XMM-Newton and INTEGRAL in October/November 2009, with one observation every four days for a total of ten observations. Each observation has been fitted with a realistic thermal Comptonization model for the continuum emission. Prompted by the correlation between the UV and soft X-ray flux, we used a thermal Comptonization component for the soft X-ray excess. The UV to X-ray/gamma-ray emission of Mrk 509 can be well fitted by these components, pointing to the existence of a hot (kT ⌠100 keV), optically-thin (Ï âŒ 0.5) corona producing the primary continuum. In contrast, the soft X-ray component requires a warm (kT ⌠1 keV), optically-thick (Ï âŒ 10-20) plasma. Estimates of the amplification ratio for this warm plasma support a configuration relatively close to the âtheoreticalâ configuration of a slab corona above a passive disk. This plasma could be the warm upper layer of the accretion disk. In contrast, the hot corona has a more photon-starved geometry. The high temperature (⌠100 eV) of the soft-photon field entering and cooling it favors a localization of the hot corona in the inner flow. This soft-photon field could be part of the comptonized emission produced by the warm plasma
Three-Family Supersymmetric Standard-like Models from Intersecting Brane Worlds
We construct the first three family N=1 supersymmetric string model with
Standard Model gauge group SU(3)_C x SU(2)_L x U(1)_Y from an orientifold of
type IIA theory on T^6/(Z_2 x Z_2) and D6-branes intersecting at angles. In
addition to the minimal supersymmetric Standard Model particles, the model
contains right-handed neutrinos, a chiral (but anomaly-free) set of exotic
multiplets, and extra vector-like multiplets. We discuss some phenomenological
features of this model.Comment: 4 pages, minor typos correcte
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