55 research outputs found
Baryons and String Creation from the Fivebrane Worldvolume Action
We construct BPS-exact solutions of the worldvolume Born-Infeld plus WZW
action of a D5-brane in the background of N D3-branes. The non-trivial
background metric and RR five-form field strength play a crucial role in the
solution. When a D5-brane is dragged across a stack of N D3-branes a bundle of
N fundamental strings joining the two types of branes is created, as in the
Hanany-Witten effect. Our solutions give a detailed description of this bundle
in terms of a D5-brane wrapped on a sphere. We discuss extensions of these
solutions which have an interpretation in terms of gauge theory multi-quark
states via the AdS/CFT correspondence.Comment: LaTeX, 18 pages, 5 eps figures; v2: added reference which had been
inadvertently omitte
A prototype for dS/CFT
We consider dS_2/CFT_1 where the asymptotic symmetry group of the de Sitter
spacetime contains the Virasoro algebra. We construct representations of the
Virasoro algebra realized in the Fock space of a massive scalar field in de
Sitter, built as excitations of the Euclidean vacuum state. These
representations are unitary, without highest weight, and have vanishing central
charge. They provide a prototype for a new class of conformal field theories
dual to de Sitter backgrounds in string theory. The mapping of operators in the
CFT to bulk quantities is described in detail. We comment on the extension to
dS_3/CFT_2.Comment: 17 pages, revtex
Baryons and Flux Tubes in Confining Gauge Theories from Brane Actions
We study baryon configurations in large N non-supersymmetric SU(N) gauge
theories, applying the AdS/CFT correspondence. Using the D5-brane worldvolume
theory in the near-horizon geometry of non-extremal D3-branes, we find
embeddings which describe baryonic states in three-dimensional QCD. In
particular, we construct solutions corresponding to a baryon made of N quarks,
and study what happens when some fraction of the total number of quarks
are bodily moved to a large spatial separation from the others. The individual
clumps of quarks are represented by Born-Infeld string tubes obtained from a
D5-brane whose spatial section has topology . They are connected
by a confining color flux tube, described by a portion of the fivebrane that
runs very close and parallel to the horizon. We find that this flux tube has a
tension with a nontrivial -dependence (not previously obtained by other
methods). A similar picture is presented for the four-dimensional case.Comment: LaTeX, 20 pages, 6 eps figures; v2: added reference, corrected
numerical error in Eqs. (13) and (23
Physical parameters of a relativistic jet at very high redshift: the case of the blazar J1430+4204
Context. The high-redshift (z = 4.72) blazar J1430+4204 produced a major
radio outburst in 2005. Such outbursts are usually associated with the
emergence of a new component in the inner radio jet. Aims. We searched for
possible changes in the radio structure on milli-arcsecond angular scales, to
determine physical parameters that characterise the relativistic jet ejected
from the centre of this source. Methods. We analysed 15-GHz radio
interferometric images obtained with the Very Long Baseline Array (VLBA) before
and after the peak of the outburst. Results. We did not identify any
significant new jet component over a period of 569 days. We estimated the
Doppler factor, the Lorentz factor, and the apparent transverse speed of a
putative jet component using three different methods. The likely small jet
angle to the line of sight and our values of the apparent transverse speed are
consistent with not detecting a new jet feature.Comment: (6 pages, 4 figures) accepted for publication in Astronomy and
Astrophysic
Multifrequency VLBA Monitoring of 3C 273 during the INTEGRAL Campaign in 2003 - I. Kinematics of the Parsec Scale Jet from 43 GHz Data
In this first of a series of papers describing polarimetric multifrequency
Very Long Baseline Array (VLBA) monitoring of 3C 273 during a simultaneous
campaign with the INTEGRAL gamma-ray satellite in 2003, we present 5 Stokes I
images and source models at 7 mm. We show that a part of the inner jet (1-2
milliarcseconds from the core) is resolved in a direction transverse to the
flow, and we analyse the kinematics of the jet within the first 10 mas. Based
on the VLBA data and simultaneous single-dish flux density monitoring, we
determine an accurate value for the Doppler factor of the parsec scale jet, and
using this value with observed proper motions, we calculate the Lorentz factors
and the viewing angles for the emission components in the jet. Our data
indicates a significant velocity gradient across the jet with the components
travelling near the southern edge being faster than the components with more
northern path. We discuss our observations in the light of jet precession model
and growing plasma instabilities.Comment: Accepted for publication in Astronomy & Astrophysics, 16 pages, 15
figure
Blazar sequence - an artefact of Doppler boosting
The blazar sequence is a scenario in which the bolometric luminosity of the
blazar governs the appearance of its spectral energy distribution. The most
prominent result is the significant negative correlation between the
synchrotron peak frequencies and the synchrotron peak luminosities of the
blazar population. Observational studies of the blazar sequence have, in
general, neglected the effect of Doppler boosting. We study the dependence of
both the synchrotron peak frequency and luminosity with Doppler-corrected
quantities. We determine the spectral energy distributions of 135 radio-bright
AGN and find the best-fit parabolic function for the distribution to quantify
their synchrotron emission. The corresponding measurements of synchrotron peak
luminosities and frequencies are Doppler-corrected with a new set of Doppler
factors calculated from variability data. The relevant correlations for the
blazar sequence are determined for these intrinsic quantities. The Doppler
factor depends strongly on the synchrotron peak frequency, the lower energy
sources being more boosted. Applying the Doppler correction to the peak
frequencies and luminosities annuls the negative correlation between the two
quantities, which becomes positive. For BL Lacertae objects, the positive
correlation is particularly strong. The blazar sequence, when defined as the
anticorrelation between the peak frequency and luminosity of the synchrotron
component of the spectral energy distribution, disappears when the intrinsic,
Doppler-corrected values are used. It is an observational phenomenon created by
variable Doppler boosting across the synchrotron peak frequency range.Comment: 9 pages, 5 figures + 2 tables. The published version with minor
changes, the main conclusions are unchange
The milliarcsecond-scale jet of PKS 0735+178 during quiescence
We present polarimetric 5 GHz to 43 GHz VLBI observations of the BL Lacertae
object PKS 0735+178, spanning March 1996 to May 2000. Comparison with previous
and later observations suggests that the overall kinematic and structural
properties of the jet are greatly influenced by its activity. Time intervals of
enhanced activity, as reported before 1993 and after 2000 by other studies, are
followed by highly superluminal motion along a rectilinear jet. In contrast the
less active state in which we performed our observations, shows subluminal or
slow superluminal jet features propagating through a twisted jet with two sharp
bends of about 90 deg. within the innermost three-milliarcsecond jet structure.
Proper motion estimates from the data presented here allow us to constrain the
jet viewing angle to values < 9 deg., and the bulk Lorentz factor to be between
2 and 4.Comment: 11 pages, 12 figures. Accepted for publication in A&
Statistical entropy of three-dimensional q-deformed Kerr-de Sitter space
A quantum deformation of three-dimensional de Sitter space was proposed in
hep-th/0407188. We use this to calculate the entropy of Kerr-de Sitter space,
using a canonical ensemble, and find agreement with the semiclassical result.Comment: 11 pages, revtex, (v2, reference added
- âŠ