20,854 research outputs found
Dephasing of Mollow Triplet Sideband Emission of a Resonantly Driven Quantum Dot in a Microcavity
Detailed properties of resonance fluorescence from a single quantum dot in a
micropillar cavity are investigated, with particular focus on emission
coherence in dependence on optical driving field power and detuning.
Power-dependent series over a wide range could trace characteristic Mollow
triplet spectra with large Rabi splittings of GHz. In
particular, the effect of dephasing in terms of systematic spectral broadening
of the Mollow sidebands is observed as a strong fingerprint
of excitation-induced dephasing. Our results are in excellent agreement with
predictions of a recently presented model on phonon-dressed QD Mollow triplet
emission in the cavity-QED regime
Indistinguishable photons from the resonance fluorescence of a single quantum dot in a microcavity
We demonstrate purely resonant continuous-wave optical laser excitation to
coherently prepare an excitonic state of a single semiconductor quantum dot
(QDs) inside a high quality pillar microcavity. As a direct proof of QD
resonance fluorescence, the evolution from a single emission line to the
characteristic Mollow triplet10 is observed under increasing pump power. By
controlled utilization of weak coupling between the emitter and the fundamental
cavity mode through Purcell-enhancement of the radiative decay, a strong
suppression of pure dephasing is achieved, which reflects in close to Fourier
transform-limited and highly indistinguishable photons with a visibility
contrast of 90%. Our experiments reveal the model-like character of the coupled
QD-microcavity system as a promising source for the generation of ideal photons
at the quantum limit. From a technological perspective, the vertical cavity
symmetry -- with optional dynamic tunability -- provides strongly directed
light emission which appears very desirable for future integrated emitter
devices.Comment: 24 pages, 6 figure
The Geometry and Ionization Structure of the Wind in the Eclipsing Nova-like Variables RW Tri and UX UMa
The UV spectra of nova-like variables are dominated by emission from the
accretion disk, modified by scattering in a wind emanating from the disk. Here
we model the spectra of RW Tri and UX UMa, the only two eclipsing nova-likes
which have been observed with the Hubble Space Telescope in the
far-ultraviolet, in an attempt to constrain the geometry and the ionization
structure of their winds. Using our Monte Carlo radiative transfer code we
computed spectra for simply-parameterized axisymmetric biconical outflow models
and were able to find plausible models for both systems. These reproduce the
primary UV resonance lines - N V, Si IV, and C IV - in the observed spectra in
and out of eclipse. The distribution of these ions in the wind models is
similar in both cases as is the extent of the primary scattering regions in
which these lines are formed. The inferred mass loss rates are 6% to 8% of the
mass accretion rates for the systems. We discuss the implication of our point
models for our understanding of accretion disk winds in cataclysmic variables.Comment: 13 pages, 15 figures and 4 tables. Published in Ap
200 A GeV Au+Au collisions serve a nearly perfect quark-gluon liquid
The specific shear viscosity (eta/s)_QGP of a Quark-Gluon-Plasma (QGP) at
temperatures T_c < T < 2T_c is extracted from the centrality dependence of the
eccentricity-scaled elliptic flow measured in ultra-relativistic heavy-ion
collisions. Coupling viscous fluid dynamics for the QGP with a microscopic
transport model for hadronic freeze-out we find that the eccentricity-scaled
elliptic flow is a universal function of charged multiplicity per unit overlap
area, (1/S)(dN_ch/dy), that depends only on the viscosity but not on the model
used for computing the initial fireball eccentricity. Comparing with
measurements we find 1 < (4pi)(eta/s)_QGP < 2.5 where the uncertainty range is
dominated by model uncertainties for the eccentricity values used to normalize
the measured elliptic flow.Comment: 4 pages, 2 figures, accepted by PR
Event-by-event shape and flow fluctuations of relativistic heavy-ion collision fireballs
Heavy-ion collisions create deformed quark-gluon plasma (QGP) fireballs which
explode anisotropically. The viscosity of the fireball matter determines its
ability to convert the initial spatial deformation into momentum anisotropies
that can be measured in the final hadron spectra. A quantitatively precise
empirical extraction of the QGP viscosity thus requires a good understanding of
the initial fireball deformation. This deformation fluctuates from event to
event, and so does the finally observed momentum anisotropy. We present a
harmonic decomposition of the initial fluctuations in shape and orientation of
the fireball and perform event-by-event ideal fluid dynamical simulations to
extract the resulting fluctuations in the magnitude and direction of the
corresponding harmonic components of the final anisotropic flow at midrapidity.
The final harmonic flow coefficients are found to depend non-linearly on the
initial harmonic eccentricity coefficients. We show that, on average, initial
density fluctuations suppress the buildup of elliptic flow relative to what one
obtains from a smooth initial profile of the same eccentricity, and discuss
implications for the phenomenological extraction of the QGP shear viscosity
from experimental elliptic flow data.Comment: 22 pages, 17 figures. Relative to [v2], minor changes in text. Fig. 9
redrawn. This version accepted by Phys. Rev.
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