2,666 research outputs found
Efficient Coherent Control by Optimized Sequences of Pulses of Finite Duration
Reliable long-time storage of arbitrary quantum states is a key element for
quantum information processing. In order to dynamically decouple a spin or
quantum bit from a dephasing environment, we introduce an optimized sequence of
control pulses of finite durations \tau\pp and finite amplitudes. The
properties of this sequence of length stem from a mathematically rigorous
derivation. Corrections occur only in order and \tau\pp^3 without
mixed terms such as T^N\tau\pp or T^N\tau\pp^2. Based on existing
experiments, a concrete setup for the verification of the properties of the
advocated realistic sequence is proposed.Comment: 8 pages, 1 figur
A low-density hot Jupiter in a near-aligned, 4.5-day orbit around a = 10.8, F5V star
We report the independent discovery and characterisation of a hot Jupiter in
a 4.5-d, transiting orbit around the star TYC 7282-1298-1 ( = 10.8, F5V).
The planet has been pursued by the NGTS team as NGTS-2b and by ourselves as
WASP-179b. We characterised the system using a combination of photometry from
WASP-South and TRAPPIST-South, and spectra from CORALIE (around the orbit) and
HARPS (through the transit). We find the planet's orbit to be nearly aligned
with its star's spin. From a detection of the Rossiter-McLaughlin effect, we
measure a projected stellar obliquity of . From
line-profile tomography of the same spectra, we measure . We find the planet to have a low density ( = 0.67
0.09 , = 1.54 0.06 ), which, along
with its moderately bright host star, makes it a good target for transmission
spectroscopy. We find a lower stellar mass ( = )
than reported by the NGTS team ( = ), though the
difference is only .Comment: Submitted to AJ. 9 pages, 6 figures, 5 table
Aspects of higher curvature terms and U-duality
We discuss various aspects of dimensional reduction of gravity with the
Einstein-Hilbert action supplemented by a lowest order deformation formed as
the Riemann tensor raised to powers two, three or four. In the case of R^2 we
give an explicit expression, and discuss the possibility of extended coset
symmetries, especially SL(n+1,Z) for reduction on an n-torus to three
dimensions. Then we start an investigation of the dimensional reduction of R^3
and R^4 by calculating some terms relevant for the coset formulation, aiming in
particular towards E_8(8)/(Spin(16)/Z_2) in three dimensions and an
investigation of the derivative structure. We emphasise some issues concerning
the need for the introduction of non-scalar automorphic forms in order to
realise certain expected enhanced symmetries.Comment: 26 pp., 15 figs., plain te
SU(2) Yang-Mills Theory with extended Supersymmetry in a Background Magnetic Field
The vacuum structure of N=2 (and N=4) SUSY Yang-Mills theory is analyzed in
detail by considering the effective potential for constant background scalar-
magnetic fields within different approximations. We compare the one-loop
approximation with- or without instanton improved effective coupling with the
one-loop result in the dual desription. For N=2 we find that non-perturbative
monopole degrees of freedom remove the non-trivial minima present in the
(improved) one-loop potential in the strong-coupling regime. The combination of
Yang-Mills and dual desription leads to a self-consistent effective potential
over the full range of background fields.Comment: 15 pages, Revtex, 3 figures, References added, section two shortened,
some minor remarks and corrections adde
WASP-189b: an ultra-hot Jupiter transiting the bright A star HR 5599 in a polar orbit
We report the discovery of WASP-189b: an ultra-hot Jupiter in a 2.72-d
transiting orbit around the A star WASP-189 (HR 5599). We detected
periodic dimmings in the star's lightcurve, first with the WASP-South survey
facility then with the TRAPPIST-South telescope. We confirmed that a planet is
the cause of those dimmings via line-profile tomography and radial-velocity
measurements using the HARPS and CORALIE spectrographs. Those reveal WASP-189b
to be an ultra-hot Jupiter ( = 2.13 0.28 ;
= 1.374 0.082 ) in a polar orbit (; ) around a rapidly rotating
A6IV-V star ( = 8000 100 K; 100
km\, s). We calculate a predicted equilibrium temperature of = 2641 34 K, assuming zero albedo and efficient redistribution,
which is the third hottest for the known exoplanets. WASP-189 is the brightest
known host of a transiting hot Jupiter and the third-brightest known host of
any transiting exoplanet. We note that of the eight hot-Jupiter systems with
7000 K, seven have strongly misaligned orbits, and two of the
three systems with 8000 K have polar orbits (the third is
aligned).Comment: Submitted to MNRAS. 10 pages, 9 figures, 3 table
Fractional oscillator process with two indices
We introduce a new fractional oscillator process which can be obtained as
solution of a stochastic differential equation with two fractional orders.
Basic properties such as fractal dimension and short range dependence of the
process are studied by considering the asymptotic properties of its covariance
function. The fluctuation--dissipation relation of the process is investigated.
The fractional oscillator process can be regarded as one-dimensional fractional
Euclidean Klein-Gordon field, which can be obtained by applying the Parisi-Wu
stochastic quantization method to a nonlocal Euclidean action. The Casimir
energy associated with the fractional field at positive temperature is
calculated by using the zeta function regularization technique.Comment: 32 page
Circulating Antinuclear Antibodies in Patients with Pelvic Masses Are Associated with Malignancy and Decreased Survival
BACKGROUND: Circulating autoantibodies occur more frequently in cancer patients than in patients without cancer. METHODS AND FINDINGS: We examined sera from patients referred for pelvic mass symptoms to a tertiary university clinic. A total of 127 were diagnosed with epithelial ovarian cancer while 386 had a benign condition. A screen for IgG anti-nuclear antibodies (ANA) by indirect immunofluorescence on HEp-2 cells confirmed a highly significant overrepresentation of ANA in the cancer group where 40% had detectable (i.e., a titer ≥160) ANA compared with less than 12% in the benign group. The overrepresentation of ANA in the cancer group persisted (p<0.0001) after matching the age-profile of the benign group with the ovarian cancer group. Only 19 out of 127 patients in the age-matched benign subgroup were positive for ANA corresponding to an 85% specificity at 40% sensitivity of ANA as the only marker for malignancy. No correlation of ANA positivity in either group with specific bands in immunoblots could be demonstrated even though immunoblot positivity was clearly increased in the malignant group (41% vs. 3%). The presence, strength, and type of ANA did not correlate with serum CA-125 values or with staging, and ANA outcome did not contribute with independent diagnostic information. However, survival was significantly shorter in ANA-positive compared with ANA-negative cancer patients and patients with CA-125 below the median CA-125 value in the cancer group had a significantly decreased survival when positive for ANA. ANA status made no difference in the group with CA-125 values above the median. Also, there was a significant correlation between speckled ANA-strength and histological tumor grade. CONCLUSIONS: Circulating antibodies are a promising source for new biomarkers in cancer. Characterization of epitope specificities and measurements of consecutive samples will be important for further elucidating the role of ANA in evaluating ovarian cancer patients
Parental transfer of the antimicrobial protein LBP/BPI protects Biomphalaria glabrata eggs against oomycete infections
Copyright: © 2013 Baron et al. This is an open-access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited. Funding: This work was funded by ANR (ANR-07-BLAN-0214 and ANR-12-EMMA-00O7-01), CNRS and INRA. PvW was financially supported by the BBSRC. The funders had no role in study design, data collection and analysis, decision to publish, or preparation of the manuscript.Peer reviewedPublisher PD
Decoherence-protected quantum gates for a hybrid solid-state spin register
Protecting the dynamics of coupled quantum systems from decoherence by the
environment is a key challenge for solid-state quantum information processing.
An idle qubit can be efficiently insulated from the outside world via dynamical
decoupling, as has recently been demonstrated for individual solid-state
qubits. However, protection of qubit coherence during a multi-qubit gate poses
a non-trivial problem: in general the decoupling disrupts the inter-qubit
dynamics, and hence conflicts with gate operation. This problem is particularly
salient for hybrid systems, wherein different types of qubits evolve and
decohere at vastly different rates. Here we present the integration of
dynamical decoupling into quantum gates for a paradigmatic hybrid system, the
electron-nuclear spin register. Our design harnesses the internal resonance in
the coupled-spin system to resolve the conflict between gate operation and
decoupling. We experimentally demonstrate these gates on a two-qubit register
in diamond operating at room temperature. Quantum tomography reveals that the
qubits involved in the gate operation are protected as accurately as idle
qubits. We further illustrate the power of our design by executing Grover's
quantum search algorithm, achieving fidelities above 90% even though the
execution time exceeds the electron spin dephasing time by two orders of
magnitude. Our results directly enable decoherence-protected interface gates
between different types of promising solid-state qubits. Ultimately, quantum
gates with integrated decoupling may enable reaching the accuracy threshold for
fault-tolerant quantum information processing with solid-state devices.Comment: This is original submitted version of the paper. The revised and
finalized version is in print, and is subjected to the embargo and other
editorial restrictions of the Nature journa
Galileons as Wess-Zumino Terms
We show that the galileons can be thought of as Wess-Zumino terms for the
spontaneous breaking of space-time symmetries. Wess-Zumino terms are terms
which are not captured by the coset construction for phenomenological
Lagrangians with broken symmetries. Rather they are, in d space-time
dimensions, d-form potentials for (d+1)-forms which are non-trivial co-cycles
in Lie algebra cohomology of the full symmetry group relative to the unbroken
symmetry group. We introduce the galileon algebras and construct the
non-trivial (d+1)-form co-cycles, showing that the presence of galileons and
multi-galileons in all dimensions is counted by the dimensions of particular
Lie algebra cohomology groups. We also discuss the DBI and conformal galileons
from this point of view, showing that they are not Wess-Zumino terms, with one
exception in each case.Comment: 49 pages. v2 minor changes, version appearing in JHE
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