6,439 research outputs found
Large scale EPR correlations and cosmic gravitational waves
We study how quantum correlations survive at large scales in spite of their
exposition to stochastic backgrounds of gravitational waves. We consider
Einstein-Podolski-Rosen (EPR) correlations built up on the polarizations of
photon pairs and evaluate how they are affected by the cosmic gravitational
wave background (CGWB). We evaluate the quantum decoherence of the EPR
correlations in terms of a reduction of the violation of the Bell inequality as
written by Clauser, Horne, Shimony and Holt (CHSH). We show that this
decoherence remains small and that EPR correlations can in principle survive up
to the largest cosmic scales.Comment: 5 figure
Insights on the dynamical history of the Fomalhaut system - Investigating the Fom c hypothesis
The eccentric shape of the debris disk observed around Fomalhaut was first
attributed to Fom b, a companion detected near the belt inner-edge, but new
constraints on its orbit revealed that it is belt-crossing, highly eccentric
, and can hardly account for the shape of the belt. The best
scenario to explain this paradox is that there is another massive body in this
system, Fom c, which drives the debris disk shape. The resulting planetary
system is highly unstable, which hints at a dynamical scenario involving a
recent scattering of Fom b on its current orbit, potentially with the putative
Fom c.
Our goal is to give insights on the probability for Fom b to have been set on
its highly eccentric orbit by a close-encounter with the putative Fom c. We aim
to study in particular the part played by mean-motion resonances with Fom c,
which could have brought Fom b sufficiently close to Fom c for it to be
scattered on its current orbit, but also delay this scattering event.
Using N-body simulations, we found that the generation of orbits similar to
that of Fom b, either in term of dimensions or orientation, is a robust process
involving a scattering event and a further secular evolution of inner material
with an eccentric massive body such as the putative Fom c. We found in
particular that mean-motion resonances can delay scattering events, and thus
the production of Fom b-like orbits, on timescales comparable to the age of the
system, thus explaining the witnessing of an unstable configuration.
We conclude that Fom b probably originated from an inner resonance with Fom
c, which is at least Neptune-Saturn size, and was set on its current orbit by a
scattering event with Fom c. Since Fom b could not have formed from material in
resonance, our scenario also hints at former migration processes in this
planetary system
Herschel/PACS photometry of transiting-planet host stars with candidate warm debris disks
Dust in debris disks is produced by colliding or evaporating planetesimals,
remnants of the planet formation process. Warm dust disks, known by their
emission at < 24 micron, are rare (4% of FGK main sequence stars) and
especially interesting because they trace material in the region likely to host
terrestrial planets, where the dust has a very short dynamical lifetime.
Statistical analyses of the source counts of excesses as found with the mid-IR
Wide Field Infrared Survey Explorer (WISE) suggest that warm-dust candidates
found for the Kepler transiting-planet host-star candidates can be explained by
extragalactic or galactic background emission aligned by chance with the target
stars. These statistical analyses do not exclude the possibility that a given
WISE excess could be due to a transient dust population associated with the
target. Here we report Herschel/PACS 100 and 160 micron follow-up observations
of a sample of Kepler and non-Kepler transiting-planet candidates' host stars,
with candidate WISE warm debris disks, aimed at detecting a possible cold
debris disk in any of them. No clear detections were found in any one of the
objects at either wavelength. Our upper limits confirm that most objects in the
sample do not have a massive debris disk like that in beta Pic. We also show
that the planet-hosting star WASP-33 does not have a debris disk comparable to
the one around eta Crv. Although the data cannot be used to rule out rare warm
disks around the Kepler planet-hosting candidates, the lack of detections and
the characteristics of neighboring emission found at far-IR wavelengths support
an earlier result suggesting that most of the WISE-selected IR excesses around
Kepler candidate host stars are likely due to either chance alignment with
background IR-bright galaxies and/or to interstellar emission.Comment: 8 pages, 3 figures, accepted for publication at Astronomy &
Astrophysics on 4 August 201
Developing the Technique of Measurements of Magnetic Field in the CMS Steel Yoke Elements With Flux-Loops and Hall Probes
Compact muon solenoid (CMS) is a general-purpose detector designed to run at
the highest luminosity at the CERN large hadron collider (LHC). Its distinctive
features include a 4 T superconducting solenoid with 6 m diameter by 12.5 m
long free bore, enclosed inside a 10000-ton return yoke made of construction
steel. Accurate characterization of the magnetic field everywhere in
theCMSdetector, including the large ferromagnetic parts of the yoke, is
required. To measure the field in and around ferromagnetic parts, a set of
flux-loops and Hall probe sensors will be installed on several of the steel
pieces. Fast discharges of the solenoid during system commissioning tests will
be used to induce voltages in the flux-loops that can be integrated to measure
the flux in the steel at full excitation of the solenoid. The Hall sensors will
give supplementary information on the axial magnetic field and permit
estimation of the remanent field in the steel after the fast discharge. An
experimental R&D program has been undertaken, using a test flux-loop, two Hall
sensors, and sample disks made from the same construction steel used for the
CMS magnet yoke. A sample disc, assembled with the test flux-loop and the Hall
sensors, was inserted between the pole tips of a dipole electromagnet equipped
with a computer-controlled power supply to measure the excitation of the steel
from full saturation to zero field. The results of the measurements are
presented and discussed.Comment: 6 pages, 8 figures, 6 reference
Dynamic instabilities of fracture under biaxial strain using a phase field model
We present a phase field model of the propagation of fracture under plane
strain. This model, based on simple physical considerations, is able to
accurately reproduce the different behavior of cracks (the principle of local
symmetry, the Griffith and Irwin criteria, and mode-I branching). In addition,
we test our model against recent experimental findings showing the presence of
oscillating cracks under bi-axial load. Our model again reproduces well
observed supercritical Hopf bifurcation, and is therefore the first simulation
which does so
Measuring the Magnetic Flux Density in the CMS Steel Yoke
The Compact Muon Solenoid (CMS) is a general purpose detector, designed to
run at the highest luminosity at the CERN Large Hadron Collider (LHC). Its
distinctive features include a 4 T superconducting solenoid with 6-m-diameter
by 12.5-m-length free bore, enclosed inside a 10000-ton return yoke made of
construction steel. The return yoke consists of five dodecagonal three-layered
barrel wheels and four end-cap disks at each end comprised of steel blocks up
to 620 mm thick, which serve as the absorber plates of the muon detection
system. Accurate characterization of the magnetic field everywhere in the CMS
detector is required. To measure the field in and around the steel, a system of
22 flux-loops and 82 3-D Hall sensors is installed on the return yoke blocks.
Fast discharges of the solenoid (190 s time-constant) made during the CMS
magnet surface commissioning test at the solenoid central fields of 2.64, 3.16,
3.68 and 4.01 T were used to induce voltages in the flux-loops. The voltages
are measured on-line and integrated off-line to obtain the magnetic flux in the
steel yoke close to the muon chambers at full excitations of the solenoid. The
3-D Hall sensors installed on the steel-air interfaces give supplementary
information on the components of magnetic field and permit to estimate the
remanent field in steel to be added to the magnetic flux density obtained by
the voltages integration. A TOSCA 3-D model of the CMS magnet is developed to
describe the magnetic field everywhere outside the tracking volume measured
with the field-mapping machine. The results of the measurements and
calculations are presented, compared and discussed.Comment: 9 pages, 7 figures, 16 references, presented at the III International
Conference on Superconductivity and Magnetism (ICSM-2012), Kumburgaz,
Istanbul, Turkey, 29 April - 4 May 201
Measuring the Magnetic Flux Density with Flux Loops and Hall Probes in the CMS Magnet Flux Return Yoke
The Compact Muon Solenoid (CMS) is a general purpose detector, designed to
run at the highest luminosity at the CERN Large Hadron Collider (LHC). Its
distinctive features include a 4 T superconducting solenoid with 6-m-diameter
by 12.5-m-length free bore, enclosed inside a 10,000-ton return yoke made of
construction steel. The flux return yoke consists of five dodecagonal
three-layered barrel wheels and four end-cap disks at each end comprised of
steel blocks up to 620 mm thick, which serve as the absorber plates of the muon
detection system. To measure the field in and around the steel, a system of 22
flux loops and 82 3-D Hall sensors is installed on the return yoke blocks. A
TOSCA 3-D model of the CMS magnet is developed to describe the magnetic field
everywhere outside the tracking volume that was measured with the field-mapping
machine. The voltages induced in the flux loops by the magnetic flux changing
during the CMS magnet standard ramps down are measured with six 16-bit DAQ
modules. The off-line integration of the induced voltages reconstructs the
magnetic flux density in the yoke steel blocks at the operational magnet
current of 18.164 kA. The results of the flux loop measurements during three
magnet ramps down are presented and discussed.Comment: 3 pages, 6 figures, presented at the IEEE Nuclear Science Symposium
2016 (NSS) in Strasbourg, France on November 3, 2016. arXiv admin note: text
overlap with arXiv:1605.0877
Flux Loop Measurements of the Magnetic Flux Density in the CMS Magnet Yoke
The Compact Muon Solenoid (CMS) is a general purpose detector, designed to
run at the highest luminosity at the CERN Large Hadron Collider (LHC). Its
distinctive features include a 4 T superconducting solenoid with 6-m-diameter
by 12.5-m-length free bore, enclosed inside a 10,000-ton return yoke made of
construction steel. The return yoke consists of five dodecagonal three-layered
barrel wheels and four end-cap disks at each end comprised of steel blocks up
to 620 mm thick, which serve as the absorber plates of the muon detection
system. To measure the field in and around the steel, a system of 22 flux loops
and 82 3-D Hall sensors is installed on the return yoke blocks. A TOSCA 3-D
model of the CMS magnet is developed to describe the magnetic field everywhere
outside the tracking volume measured with the field-mapping machine. The first
attempt is made to measure the magnetic flux density in the steel blocks of the
CMS magnet yoke using the standard magnet discharge with the current ramp down
speed of 1.5 A/s.Comment: 7 pages, 5 figures, presented at ISCM2016 - 5th International
Conference on Superconductivity and Magnetism on April 28, 2016 at Fethiye,
Turke
Adding Salt to an Aqueous Solution of t-Butanol: Is Hydrophobic Association Enhanced or Reduced?
Recent neutron scattering experiments on aqueous salt solutions of
amphiphilic t-butanol by Bowron and Finney [Phys. Rev. Lett. {\bf 89}, 215508
(2002); J. Chem. Phys. {\bf 118}, 8357 (2003)] suggest the formation of
t-butanol pairs, bridged by a chloride ion via
hydrogen-bonds, and leading to a reduced number of intermolecular hydrophobic
butanol-butanol contacts. Here we present a joint experimental/theoretical
study on the same system, using a combination of molecular dynamics simulations
and nuclear magnetic relaxation measurements. Both theory and experiment
clearly support the more intuitive scenario of an enhanced number of
hydrophobic contacts in the presence of the salt, as it would be expected for
purely hydrophobic solutes [J. Phys. Chem. B {\bf 107}, 612 (2003)]. Although
our conclusions arrive at a structurally completely distinct scenario, the
molecular dynamics simulation results are within the experimental errorbars of
the Bowron and Finney work.Comment: 15 pages twocolumn revtex, 11 figure
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