4,276 research outputs found
Randomized benchmarking of single and multi-qubit control in liquid-state NMR quantum information processing
Being able to quantify the level of coherent control in a proposed device
implementing a quantum information processor (QIP) is an important task for
both comparing different devices and assessing a device's prospects with
regards to achieving fault-tolerant quantum control. We implement in a
liquid-state nuclear magnetic resonance QIP the randomized benchmarking
protocol presented by Knill et al (PRA 77: 012307 (2008)). We report an error
per randomized pulse of with a
single qubit QIP and show an experimentally relevant error model where the
randomized benchmarking gives a signature fidelity decay which is not possible
to interpret as a single error per gate. We explore and experimentally
investigate multi-qubit extensions of this protocol and report an average error
rate for one and two qubit gates of for a three
qubit QIP. We estimate that these error rates are still not decoherence limited
and thus can be improved with modifications to the control hardware and
software.Comment: 10 pages, 6 figures, submitted versio
The Quantum Mechanics of Hyperion
This paper is motivated by the suggestion [W. Zurek, Physica Scripta, T76,
186 (1998)] that the chaotic tumbling of the satellite Hyperion would become
non-classical within 20 years, but for the effects of environmental
decoherence. The dynamics of quantum and classical probability distributions
are compared for a satellite rotating perpendicular to its orbital plane,
driven by the gravitational gradient. The model is studied with and without
environmental decoherence. Without decoherence, the maximum quantum-classical
(QC) differences in its average angular momentum scale as hbar^{2/3} for
chaotic states, and as hbar^2 for non-chaotic states, leading to negligible QC
differences for a macroscopic object like Hyperion. The quantum probability
distributions do not approach their classical limit smoothly, having an
extremely fine oscillatory structure superimposed on the smooth classical
background. For a macroscopic object, this oscillatory structure is too fine to
be resolved by any realistic measurement. Either a small amount of smoothing
(due to the finite resolution of the apparatus) or a very small amount of
environmental decoherence is sufficient ensure the classical limit. Under
decoherence, the QC differences in the probability distributions scale as
(hbar^2/D)^{1/6}, where D is the momentum diffusion parameter. We conclude that
decoherence is not essential to explain the classical behavior of macroscopic
bodies.Comment: 17 pages, 24 figure
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The ConStratO model of handover: a tool to support technology design and evaluation
Handovers are a specific kind of multidisciplinary team meeting. Shift handovers and transfers are both regular features of hospital work but there is currently great variation in how such handovers are conducted, presenting a challenging for those seeking to develop technology to support handover. This paper presents the ConStratO model of handover, which captures aspects of the context that influence how the handover is conducted, a range of different handover strategies relating to different aspects of the handover, and possible outcomes of handover. The model is based on detailed data collection in a range of clinical settings. We present the model as a tool for developing and evaluating technology support for handover
Testing integrability with a single bit of quantum information
We show that deterministic quantum computing with a single bit (DQC1) can
determine whether the classical limit of a quantum system is chaotic or
integrable using O(N) physical resources, where is the dimension of the
Hilbert space of the system under study. This is a square root improvement over
all known classical procedures. Our study relies strictly on the random matrix
conjecture. We also present numerical results for the nonlinear kicked top.Comment: Minor changes taking into account Howard Wiseman's comment:
quant-ph/0305153. Accepted for publication in Phys. Rev.
Preliminary results for RR Lyrae stars and Classical Cepheids from the Vista Magellanic Cloud (VMC) Survey
The Vista Magellanic Cloud (VMC, PI M.R. Cioni) survey is collecting
-band time series photometry of the system formed by the two Magellanic
Clouds (MC) and the "bridge" that connects them. These data are used to build
-band light curves of the MC RR Lyrae stars and Classical Cepheids and
determine absolute distances and the 3D geometry of the whole system using the
-band period luminosity (), the period - luminosity - color ()
and the Wesenhiet relations applicable to these types of variables. As an
example of the survey potential we present results from the VMC observations of
two fields centered respectively on the South Ecliptic Pole and the 30 Doradus
star forming region of the Large Magellanic Cloud. The VMC -band light
curves of the RR Lyrae stars in these two regions have very good photometric
quality with typical errors for the individual data points in the range of
0.02 to 0.05 mag. The Cepheids have excellent light curves (typical
errors of 0.01 mag). The average magnitudes derived for both types
of variables were used to derive relations that are in general good
agreement within the errors with the literature data, and show a smaller
scatter than previous studies.Comment: 7 pages, 6 figure. Accepted for publication in Astrophysics and Space
Science. Following a presentation at the conference "The Fundamental Cosmic
Distance Scale: State of the Art and the Gaia Perspective", Naples, May 201
DA495 - an aging pulsar wind nebula
We present a radio continuum study of the pulsar wind nebula (PWN) DA 495
(G65.7+1.2), including images of total intensity and linear polarization from
408 to 10550 MHz based on the Canadian Galactic Plane Survey and observations
with the Effelsberg 100-m Radio Telescope. Removal of flux density
contributions from a superimposed \ion{H}{2} region and from compact
extragalactic sources reveals a break in the spectrum of DA 495 at 1.3 GHz,
with a spectral index below the break and
above it (). The
spectral break is more than three times lower in frequency than the lowest
break detected in any other PWN. The break in the spectrum is likely the result
of synchrotron cooling, and DA 495, at an age of 20,000 yr, may have
evolved from an object similar to the Vela X nebula, with a similarly energetic
pulsar. We find a magnetic field of 1.3 mG inside the nebula. After
correcting for the resulting high internal rotation measure, the magnetic field
structure is quite simple, resembling the inner part of a dipole field
projected onto the plane of the sky, although a toroidal component is likely
also present. The dipole field axis, which should be parallel to the spin axis
of the putative pulsar, lies at an angle of {\sim}50\degr east of the North
Celestial Pole and is pointing away from us towards the south-west. The upper
limit for the radio surface brightness of any shell-type supernova remnant
emission around DA 495 is OAWatt
m Hz sr (assuming a radio spectral index of ), lower than the faintest shell-type remnant known to date.Comment: 25 pages, accepted by Ap
INFLUÊNCIA DA PRECIPITAÇÃO NOS MANGUEZAIS DA BARRA DO RIBEIRA – IGUAPE/SP
The mangrove, coastal ecosystem defined as a transition between terrestrialand marine environment is characterized as a salinized environment with aconstant flooding caused by tides. Emphasizing the System area CoastalCananéia - Iguape, its importance is related to the biomass production, insertedinto the natural bioenergetics system, increasing the productivity of the coastalzone with the introduction of organic particles. This means vegetal communitiesare adapted to many physical conditionants the active in the coastal zones,including the climate conditionants. This article is part of a larger work, whichpurpose is contributes to the comprehension of variability of the climaticattributes and their influence on the mangrove vegetation. Here are presentedthe data and analysis of the precipitation and interception of rain by the canopyof the mangrove forest located in Barra do Ribeira-Iguape/SP. A microclimatictower was installed with two meteorological stations and each one had raingauge to obtain an analysis of the variation of precipitation above and below thecanopy of mangrove. More sixteen rain gauges were installed in an area of 400m². Our research results shows that in microclimatic scales the main control forthe variation of climatic attributes is the canopy, mainly in rainfall distributionbelow the canopy, which consequently influences in the distribution ofvegetables species in the environment. It was found also that the amount ofrainfall that effectively reaches the ground and how this is redistributed withinthe environment depends on the density of the canopy and its twigs and trunks.To the mangrove this process is important because the amount of rain thateffectively reaches the soil helps to reduce salinity in the environment and isdeterminant for the type of predominant species in the mangrove. This projectcounted on the financing of the CNPq, process referring number 470434/2006-6to the proclamation MCT/CNPq 02/2006 - Universal.O manguezal, definido como um ecossistema costeiro de transição entre osambientes terrestres e marinhos caracteriza-se por ambiente salinizado e pelaconstante inundação causada por marés. Com destaque na área do SistemaCosteiro Cananéia – Iguape, sua importância maior está relacionada à produçãode biomassa, inserida no sistema bioenergético natural, aumentando aprodutividade da zona costeira com a introdução de particulados orgânicos.Representam comunidades vegetais adaptadas a várias condicionantes físicasatuantes nas zonas costeiras, entre elas, as climáticas. O presente artigo fazparte de um trabalho maior, que tem como objetivo contribuir com oentendimento da variação dos atributos climáticos e sua influência na vegetaçãodo manguezal. No entanto, aqui serão apresentados os dados e as análises doatributo precipitação, bem como a interceptação da precipitação pelo dossel domanguezal, localizado na Barra do Ribeira-Iguape/SP. Para isso, foi instaladauma torre microclimática contendo duas estações meteorológicas, com umpluviômetro cada, de forma a obter uma análise da variação da precipitaçãoacima e abaixo do dossel de manguezal. Além de 16 pluviômetros totalizadoresao longo de uma área de 400 m². Verificou-se que, na escala de trabalhomicroclimática, o dossel é o principal controle para a variação dos atributosclimáticos, principalmente na distribuição pluviométrica abaixo desse dossel, oque, consequentemente, influencia na distribuição das espécies vegetais doambiente. Constatou-se que a quantidade de precipitação que efetivamenteatinge o solo e a forma com que ela é redistribuída dentro do ambiente dependeda densidade do dossel e de suas ramificações de galhos e caule. Para omanguezal esse processo é importante, visto que a quantidade de chuva queefetivamente atinge o solo contribuir para a diminuição da salinidade presenteno ambiente, sendo determinante para o tipo de espécie predominante no manguezal. Esse projeto foi financiamento pelo CNPq, processo número470434/2006-6 referente ao edital MCT/CNPq 02/2006 – Universal
Doping dependence of phonon and quasiparticle heat transport of pure and Dy-doped Bi_2Sr_2CaCu_2O_{8+\delta} single crystals
The temperature and magnetic-field (H) dependences of thermal conductivity
(\kappa) of Bi_2Sr_2CaCu_2O_{8+\delta} (Bi2212) are systematically measured for
a broad doping range by using both pure Bi2212 single crystals with tuned
oxygen contents and Bi_2Sr_2Ca_{1-x}Dy_xCu_2O_{8+\delta} (Dy-Bi2212) single
crystals with different Dy contents x. In the underdoped samples, the
quasiparticle (QP) peak below T_c is strongly suppressed, indicating strong QP
scattering by impurities or oxygen defects, whereas the phonon conductivity is
enhanced in moderately Dy-doped samples and a phonon peak at 10 K is observed
for the first time in Bi2212 system, which means Dy^{3+} ions not only
introduce the impurities or point defects but also stabilize the crystal
lattice. The subkelvin data show that the QP heat conductivity gradually
decreases upon lowering the hole doping level. The magnetic-field dependence of
\kappa at temperature above 5 K is mainly due to the QP scattering off
vortices. While the underdoped pure Bi2212 show very weak field dependence of
\kappa, the Dy-doped samples present an additional "dip"-like term of \kappa(H)
at low field, which is discussed to be related to the phonon scattering by free
spins of Dy^{3+} ions. For non-superconducting Dy-Bi2212 samples with x \simeq
0.50, an interesting "plateau" feature shows up in the low-T \kappa(H)
isotherms with characteristic field at 1 -- 2 T, for which we discuss the
possible revlevance of magnon excitations.Comment: 11 pages, 11 figures, accepted for publication in Phys. Rev.
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