Coulomb Drag Between Parallel Ballistic Quantum Wires

The Coulomb drag between parallel, {\it ballistic} quantum wires is studied theoretically in the presence of a perpendicular magnetic field B. The transresistance R_D shows peaks as a function of the Fermi level and splitting energy between the 1D subbands of the wires. The sharpest peaks appear when the Fermi level crosses the subband extrema so that the Fermi momenta are small. Two other kinds of peaks appear when either {\it intra}- or {\it inter}-subband transitions of electrons have maximum probability; the {\it intra}-subband transitions correspond to a small splitting energy. R_D depends on the field B in a nonmonotonic fashion: it decreases with B, as a result of the suppression of backscattering, and increases sharply when the Fermi level approaches the subband bottoms and the suppression is outbalanced by the increase of the Coulomb matrix elements and of the density of states.Comment: Text 14 pages in Latex/Revtex format, 4 Postscript figures. Phys. Rev. B,in pres

(μ-Formato-κ 2 O:O′)bis­[dicarbon­yl(η 5-cyclo­penta­dien­yl)iron(II)] tetra­fluoridoborate

In the structure of the title compound [Fe2(C5H5)2(CHO2)(CO)4]BF4, each FeII atom is coordinated in a pseudo-octa­hedral three-legged piano-stool fashion. The cyclo­penta­dienyl ligand occupies three fac coordination sites while the two carbonyl ligands and formate O atom occupy the remaining three sites

Amelioration of photic injury in rat retina by ascorbic acid: a histopathologic

It has been postulated that ascorbic acid may help to protect the retina from oxidative insult by light. To confirm this hypothesis, the authors compared light-damaged retinas of rats with or without ascorbate supplement by morphologic and morphometric studies at different time periods after light exposure. No dramatic morphologic differences were observed in the photoreceptor-retinal pigment epithelium complex between the two groups six hr after light exposure to 200 to 250-foot candles of visible light. Six to 13 days after 24 hr of exposure, the retina of rats that received ascorbate supplement showed significantly less severe damage than the retina of unsupplemented rats. The superior and temporal quadrants of the retina appeared to be most susceptible to the light damage when comparing rats with or without ascorbate supplement. These findings suggested that ascorbate ameliorates the photic injury in rat retina. Invest Ophthalmol Vis Sci 26: [1589][1590][1591][1592][1593][1594][1595][1596][1597][1598] 1985 Although the mechanisms of photic injury to the retina have not been determined definitely, oxidative reaction is believed to play an important role. 1 ' 2 Light acts on some photo-excitable components in the retina to produce superoxide radicals, which may induce plasma membrane injury. It is postulated that, as a natural antioxidant, ascorbic acid may neutralize these superoxide radicals and provide protection for the retina 3 " 5 and other tissues such as lens and brain, which contain abundant ascorbic acid. 6 ' 7 In a previous report, we exposed guinea pig and baboon retinas to light and observed that the reduced ascorbate in the retina was decreased, Materials and Methods Sixteen 21-day-old albino rats were kept in a 12-hr cycle of 5-foot candle light and darkness and were fed a normal diet adlibitum for 30 days before the experiment. Before exposure to intense visible light, rats were dark adapted for 16 to 18 hr. Eight rats were injected intraperitoneally with a dose of 0.5 g/kg of ascorbic acid 24 hr before and just before intense light exposure. Six rats fed a normal diet and six rats that received ascorbic acid supplement were exposed to green-filtered fluorescent light (Plexiglas #2092 filter; Polycast Technology Corp.; Stamford; CT) of 200 to 250 foot candles for 24 hr. Normal rat were paired with ascorbate-treated rat during light exposure. Following light exposure, the animals were returned to a totally dark environment. Four rats, two fed a normal diet and two that received ascorbic acid supplement, were kept in a cyclic light environment as controls. The rats were killed six hr, six days, and 13 days after light exposure. The right eyes were removed for rhodopsin measurement

Efficient multiscale imaging of subsurface resistivity with uncertainty quantification using ensemble Kalman inversion

Electrical resistivity tomography (ERT) is widely used to image the Earth's subsurface and has proven to be an extremely useful tool in application to hydrological problems. Conventional smoothness-constrained inversion of ERT data is efficient and robust, and consequently very popular. However, it does not resolve well sharp interfaces of a resistivity field and tends to reduce and smooth resistivity variations. These issues can be problematic in a range of hydrological or near-surface studies, for example mapping regolith-bedrock interfaces. While fully Bayesian approaches, such as those using Markov chain Monte Carlo sampling, can address the above issues, their very high computation cost makes them impractical for many applications. Ensemble Kalman inversion (EKI) offers a computationally efficient alternative by approximating the Bayesian posterior distribution in a derivative-free manner, which means only a relatively small number of 'black-box' model runs are required. Although common limitations for ensemble Kalman filter-type methods apply to EKI, it is both efficient and generally captures uncertainty patterns correctly. We propose the use of a new EKI-based framework for ERT which estimates a resistivity model and its uncertainty at a modest computational cost. Our EKI framework uses a level-set parametrization of the unknown resistivity to allow efficient estimation of discontinuous resistivity fields. Instead of estimating level-set parameters directly, we introduce a second step to characterize the spatial variability of the resistivity field and infer length scale hyperparameters directly. We demonstrate these features by applying the method to a series of synthetic and field examples. We also benchmark our results by comparing them to those obtained from standard smoothness-constrained inversion. Resultant resistivity images from EKI successfully capture arbitrarily shaped interfaces between resistivity zones and the inverted resistivities are close to the true values in synthetic cases. We highlight its readiness and applicability to similar problems in geophysics

Scaling Laws and Transient Times in 3He Induced Nuclear Fission

Fission excitation functions of compound nuclei in a mass region where shell effects are expected to be very strong are shown to scale exactly according to the transition state prediction once these shell effects are accounted for. The fact that no deviations from the transition state method have been observed within the experimentally investigated excitation energy regime allows one to assign an upper limit for the transient time of 10 zs.Comment: 7 pages, TeX type, psfig, submitted to Phys. Rev. C, also available at http://csa5.lbl.gov/moretto/ps/he3_paper.p

A statistical interpretation of the correlation between intermediate mass fragment multiplicity and transverse energy

Multifragment emission following Xe+Au collisions at 30, 40, 50 and 60 AMeV has been studied with multidetector systems covering nearly 4-pi in solid angle. The correlations of both the intermediate mass fragment and light charged particle multiplicities with the transverse energy are explored. A comparison is made with results from a similar system, Xe+Bi at 28 AMeV. The experimental trends are compared to statistical model predictions.Comment: 7 pages, submitted to Phys. Rev.

Spontaneous Coherence and Collective Modes in Double-Layer Quantum Dot Systems

We study the ground state and the collective excitations of parabolically-confined double-layer quantum dot systems in a strong magnetic field. We identify parameter regimes where electrons form maximum density droplet states, quantum-dot analogs of the incompressible states of the bulk integer quantum Hall effect. In these regimes the Hartree-Fock approximation and the time-dependent Hartree-Fock approximations can be used to describe the ground state and collective excitations respectively. We comment on the relationship between edge excitations of dots and edge magneto-plasmon excitations of bulk double-layer systems.Comment: 20 pages (figures included) and also available at http://fangio.magnet.fsu.edu/~jhu/Paper/qdot_cond.ps, replaced to fix figure

Tag-Aware Recommender Systems: A State-of-the-art Survey

In the past decade, Social Tagging Systems have attracted increasing attention from both physical and computer science communities. Besides the underlying structure and dynamics of tagging systems, many efforts have been addressed to unify tagging information to reveal user behaviors and preferences, extract the latent semantic relations among items, make recommendations, and so on. Specifically, this article summarizes recent progress about tag-aware recommender systems, emphasizing on the contributions from three mainstream perspectives and approaches: network-based methods, tensor-based methods, and the topic-based methods. Finally, we outline some other tag-related works and future challenges of tag-aware recommendation algorithms.Comment: 19 pages, 3 figure

First narrow-band search for continuous gravitational waves from known pulsars in advanced detector data

Spinning neutron stars asymmetric with respect to their rotation axis are potential sources of continuous gravitational waves for ground-based interferometric detectors. In the case of known pulsars a fully coherent search, based on matched filtering, which uses the position and rotational parameters obtained from electromagnetic observations, can be carried out. Matched filtering maximizes the signalto- noise (SNR) ratio, but a large sensitivity loss is expected in case of even a very small mismatch between the assumed and the true signal parameters. For this reason, narrow-band analysis methods have been developed, allowing a fully coherent search for gravitational waves from known pulsars over a fraction of a hertz and several spin-down values. In this paper we describe a narrow-band search of 11 pulsars using data from Advanced LIGO’s first observing run. Although we have found several initial outliers, further studies show no significant evidence for the presence of a gravitational wave signal. Finally, we have placed upper limits on the signal strain amplitude lower than the spin-down limit for 5 of the 11 targets over the bands searched; in the case of J1813-1749 the spin-down limit has been beaten for the first time. For an additional 3 targets, the median upper limit across the search bands is below the spin-down limit. This is the most sensitive narrow-band search for continuous gravitational waves carried out so far