903 research outputs found
Charge-Transfer Excitations in the Model Superconductor HgBaCuO
We report a Cu -edge resonant inelastic x-ray scattering (RIXS) study of
charge-transfer excitations in the 2-8 eV range in the structurally simple
compound HgBaCuO at optimal doping ( K).
The spectra exhibit a significant dependence on the incident photon energy
which we carefully utilize to resolve a multiplet of weakly-dispersive ( eV) electron-hole excitations, including a mode at 2 eV. The observation
of this 2 eV excitation suggests the existence of a charge-transfer pseudogap
deep in the superconducting phase. Quite generally, our data demonstrate the
importance of exploring the incident photon energy dependence of the RIXS cross
section.Comment: 5 pages, 3 figure
Nuclear break-up of 11Be
The break-up of 11Be was studied at 41AMeV using a secondary beam of 11Be
from the GANIL facility on a 48Ti target by measuring correlations between the
10Be core, the emitted neutrons and gamma rays. The nuclear break-up leading to
the emission of a neutron at large angle in the laboratory frame is identified
with the towing mode through its characteristic n-fragment correlation. The
experimental spectra are compared with a model where the time dependent
Schrodinger equation (TDSE) is solved for the neutron initially in the 11 Be. A
good agreement is found between experiment and theory for the shapes of neutron
experimental energies and angular distributions. The spectroscopic factor of
the 2s orbital is tentatively extracted to be 0.46+-0.15. The neutron emission
from the 1p and 1d orbitals is also studied
The global clonal complexity of the murine blood system declines throughout life and after serial transplantation.
Although many recent studies describe the emergence and prevalence of "clonal hematopoiesis of indeterminate potential" in aged human populations, a systematic analysis of the numbers of clones supporting steady-state hematopoiesis throughout mammalian life is lacking. Previous efforts relied on transplantation of "barcoded" hematopoietic stem cells (HSCs) to track the contribution of HSC clones to reconstituted blood. However, ex vivo manipulation and transplantation alter HSC function and thus may not reflect the biology of steady-state hematopoiesis. Using a noninvasive in vivo color-labeling system, we report the first comprehensive analysis of the changing global clonal complexity of steady-state hematopoiesis during the natural murine lifespan. We observed that the number of clones (ie, clonal complexity) supporting the major blood and bone marrow hematopoietic compartments decline with age by ∼30% and ∼60%, respectively. Aging dramatically reduced HSC in vivo-repopulating activity and lymphoid potential while increasing functional heterogeneity. Continuous challenge of the hematopoietic system by serial transplantation provoked the clonal collapse of both young and aged hematopoietic systems. Whole-exome sequencing of serially transplanted aged and young hematopoietic clones confirmed oligoclonal hematopoiesis and revealed mutations in at least 27 genes, including nonsense, missense, and deletion mutations in Bcl11b, Hist1h2ac, Npy2r, Notch3, Ptprr, and Top2b
Charge and current-sensitive preamplifiers for pulse shape discrimination techniques with silicon detectors
New charge and current-sensitive preamplifiers coupled to silicon detectors
and devoted to studies in nuclear structure and dynamics have been developed
and tested. For the first time shapes of current pulses from light charged
particles and carbon ions are presented. Capabilities for pulse shape
discrimination techniques are demonstrated.Comment: 14 pages, 12 figures, to be published in Nucl. Inst. Meth.
Resonant inelastic x-ray scattering in electronically quasi-zero-dimensional CuB2O4
We explore the general phenomenology of resonant inelastic scattering (RIXS)
using CuB2O4, a network of CuO4 plaquettes electronically isolated by B+3 ions.
Spectra show a small number of well-separated features, and we exploit the
simple electronic structure to explore RIXS phenomenology by developing a
calculation which allows for intermediate-state effects ignored in standard
approaches. These effects are found to be non-negligible and good
correspondence between our model and experiment leads to a simple picture of
such phenomenology as the genesis of d-d excitations at the K edge and
intermediate-state interference effects.Comment: Phys. Rev. B 80, 092509 (2009
Ion stopping in dense plasma target for high energy density physics
The basic physics of nonrelativistic and electromagnetic ion stopping in hot and ionized plasma targets is thoroughly updated. Corresponding projectile-target interactions involve enhanced projectile ionization and coupling with target free electrons leading to significantly larger energy losses in hot targets when contrasted to their cold homologues. Standard stoppping formalism is framed around the most economical extrapolation of high velocity stopping in cold matter. Further elaborations pay attention to target electron coupling and nonlinearities due to enhanced projectile charge state, as well. Scaling rules are then used to optimize the enhanced stopping of MeV/amu ions in plasmas with electron linear densities nel ~ 10 18 -10 20 cm -2 . The synchronous firing of dense and strongly ionized plasmas with the time structure of bunched and energetic multicharged ion beam then allow to probe, for the first time, the long searched enhanced plasma stopping and projectile charge at target exit. Laser ablated plasmas (SPQR1) and dense linear plasma columns (SPQR2) show up as targets of choice in providing accurate and on line measurements of plasma parameters. Corresponding stopping results are of a central significance in asserting the validity of intense ion beam scenarios for driving thermonuclear pellets. Other applications of note feature thorium induced fission, novel ion sources and specific material processing through low energy ion beams. Last but not least, the given ion beam-plasma target interaction physics is likely to pave a way to the production and diagnostics of warm dense matter (WDM)
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Impact of particles on the Planck HFI detectors: Ground-based measurements and physical interpretation
The Planck High Frequency Instrument (HFI) surveyed the sky continuously from
August 2009 to January 2012. Its noise and sensitivity performance were
excellent, but the rate of cosmic ray impacts on the HFI detectors was
unexpectedly high. Furthermore, collisions of cosmic rays with the focal plane
produced transient signals in the data (glitches) with a wide range of
characteristics. A study of cosmic ray impacts on the HFI detector modules has
been undertaken to categorize and characterize the glitches, to correct the HFI
time-ordered data, and understand the residual effects on Planck maps and data
products. This paper presents an evaluation of the physical origins of glitches
observed by the HFI detectors. In order to better understand the glitches
observed by HFI in flight, several ground-based experiments were conducted with
flight-spare HFI bolometer modules. The experiments were conducted between 2010
and 2013 with HFI test bolometers in different configurations using varying
particles and impact energies. The bolometer modules were exposed to 23 MeV
protons from the Orsay IPN TANDEM accelerator, and to Am and Cm
-particle and Fe radioactive X-ray sources. The calibration data
from the HFI ground-based preflight tests were used to further characterize the
glitches and compare glitch rates with statistical expectations under
laboratory conditions. Test results provide strong evidence that the dominant
family of glitches observed in flight are due to cosmic ray absorption by the
silicon die substrate on which the HFI detectors reside. Glitch energy is
propagated to the thermistor by ballistic phonons, while there is also a
thermal diffusion contribution. The implications of these results for future
satellite missions, especially those in the far-infrared to sub-millimetre and
millimetre regions of the electromagnetic spectrum, are discussed.Comment: 11 pages, 13 figure
Collision statistics in a dilute granular gas fluidized by vibrations in low gravity
We report an experimental study of a dilute "gas" of inelastically colliding
particles excited by vibrations in low gravity. We show that recording the
collision frequency together with the impulses on a wall of the container gives
access to several quantities of interest. We observe that the mean collision
frequency does not scale linearly with the number N of particles in the
container. This is due to the dissipative nature of the collisions and is also
directly related to the non extensive behaviour of the kinetic energy (the
granular temperature is not intensive).Comment: to be pubished in Europhysics Letters (May/June 2006
Heavy ion irradiation of crystalline water ice
Under cosmic irradiation, the interstellar water ice mantles evolve towards a
compact amorphous state. Crystalline ice amorphisation was previously monitored
mainly in the keV to hundreds of keV ion energies. We experimentally
investigate heavy ion irradiation amorphisation of crystalline ice, at high
energies closer to true cosmic rays, and explore the water-ice sputtering
yield. We irradiated thin crystalline ice films with MeV to GeV swift ion
beams, produced at the GANIL accelerator. The ice infrared spectral evolution
as a function of fluence is monitored with in-situ infrared spectroscopy
(induced amorphisation of the initial crystalline state into a compact
amorphous phase). The crystalline ice amorphisation cross-section is measured
in the high electronic stopping-power range for different temperatures. At
large fluence, the ice sputtering is measured on the infrared spectra, and the
fitted sputtering-yield dependence, combined with previous measurements, is
quadratic over three decades of electronic stopping power. The final state of
cosmic ray irradiation for porous amorphous and crystalline ice, as monitored
by infrared spectroscopy, is the same, but with a large difference in
cross-section, hence in time scale in an astrophysical context. The cosmic ray
water-ice sputtering rates compete with the UV photodesorption yields reported
in the literature. The prevalence of direct cosmic ray sputtering over
cosmic-ray induced photons photodesorption may be particularly true for ices
strongly bonded to the ice mantles surfaces, such as hydrogen-bonded ice
structures or more generally the so-called polar ices.Comment: 22pages, 11 figures, accepted in A&
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