16,770 research outputs found

    Crossover from Single-Ion to Coherent Non-Fermi Liquid Behavior in Ce1x_{1-x}Lax_xNi9_9Ge4_4

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    We report specific heat and magneto-resistance studies on the compound Ce1x{}_{1-x}Lax{}_xNi9{}_9Ge4{}_4 for various concentrations over the entire stoichiometric range. Our data reveal single-ion scaling with Ce-concentration between x=0.1x = 0.1 and 0.95. Furthermore, CeNi9{}_9Ge4{}_4 turns out to have the largest ever recorded value of the electronic specific heat Δc/T\Delta c/T \approx 5.5 J K2mol1\rm K^{-2}mol^{-1} at T=0.08T=0.08 K which was found in Cerium f-electron lattice systems. In the doped samples Δc/T\Delta c/T increases logarithmically in the temperature range between 3 K and 50 mK typical for non-Fermi liquid (nFl) behavior, while ρ\rho exhibits a Kondo-like minimum around 30 K, followed by a single-ion local nFl behavior. In contrast to this, CeNi9{}_9Ge4{}_4 flattens out in Δc/T\Delta c/T below 300 mK and displays a pronounced maximum in the resistivity curve at 1.5 K indicating a coherent heavy fermion groundstate. These properties render the compound Ce1x{}_{1-x}Lax{}_xNi9{}_9Ge4{}_4 a unique system on the borderline between Fermi liquid and nFl physics.Comment: 2 pages, 3 figures, SCES0

    Exponential torsion growth for random 3-manifolds

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    We show that a random 3-manifold with positive first Betti number admits a tower of cyclic covers with exponential torsion growth

    Unusual Non-Fermi Liquid Behavior of Ce1x_{1-x}Lax_{x}Ni9_{9}Ge4_4 Analyzed in a Single Impurity Anderson Model with Crystal Field Effects

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    CeNi9_{9}Ge4_4 exhibits unusual non-Fermi liquid behavior with the largest ever recorded value of the electronic specific heat ΔC/T5.5\Delta C/T \cong 5.5 JK2^{-2}mol1^{-1} without showing any evidence of magnetic order. Specific heat measurements show that the logarithmic increase of the Sommerfeld coefficient flattens off below 200 mK. In marked contrast, the local susceptibility Δχ\Delta\chi levels off well above 200 mK and already becomes constant below 1 K. Furthermore, the entropy reaches 2RRln2 below 20 K corresponding to a four level system. An analysis of CC and χ\chi was performed in terms of an SU(N=4)SU(N=4) single impurity Anderson model with additional crystal electric field (CEF) splitting. Numerical renormalization group calculations point to a possible consistent description of the different low temperature scales in Δc\Delta c and Δχ\Delta \chi stemming from the interplay of Kondo effect and crystal field splitting.Comment: 2 pages, 2 figure

    X-ray Properties of the Abell 644 Cluster of Galaxies

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    We use new ASCA observations and archival ROSAT Position Sensitive Proportional Counter (PSPC) data to determine the X-ray spectral properties of the intracluster gas in Abell 644. From the overall spectrum, we determine the average gas temperature to be 8.64 (+0.67,-0.56) keV, and an abundance of 0.32 (+/-0.04) ZZ_{\odot}. The global ASCA and ROSAT spectra imply a cooling rate of 214 (+100,-91) MM_{\odot} yr1^{-1}. The PSPC X-ray surface brightness profile and the ASCA data suggest a somewhat higher cooling rate. We determine the gravitational mass and gas mass as a function of radius. The total gravitating mass within 1.2 Mpc is 6.2×10146.2\times10^{14} MM_{\odot}, of which 20% is in the form of hot gas. There is a region of elevated temperature 1.5-5 arcmin to the west of the cluster center. The south-southwest region of the cluster also shows excess emission in the ROSAT PSPC X-ray image, aligned with the major axis of the optical cD galaxy in the center of the cluster. We argue that the cluster is undergoing or has recently undergone a minor merger. The combination of a fairly strong cooling flow and evidence for a merger make this cluster an interesting case to test the disruption of cooling flow in mergers.Comment: 26 pages LaTeX including 9 eps figures + 4 pages LaTeX tables (landscape); accepted to ApJ, uses aaspp

    Thin film evolution equations from (evaporating) dewetting liquid layers to epitaxial growth

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    In the present contribution we review basic mathematical results for three physical systems involving self-organising solid or liquid films at solid surfaces. The films may undergo a structuring process by dewetting, evaporation/condensation or epitaxial growth, respectively. We highlight similarities and differences of the three systems based on the observation that in certain limits all of them may be described using models of similar form, i.e., time evolution equations for the film thickness profile. Those equations represent gradient dynamics characterized by mobility functions and an underlying energy functional. Two basic steps of mathematical analysis are used to compare the different system. First, we discuss the linear stability of homogeneous steady states, i.e., flat films; and second the systematics of non-trivial steady states, i.e., drop/hole states for dewetting films and quantum dot states in epitaxial growth, respectively. Our aim is to illustrate that the underlying solution structure might be very complex as in the case of epitaxial growth but can be better understood when comparing to the much simpler results for the dewetting liquid film. We furthermore show that the numerical continuation techniques employed can shed some light on this structure in a more convenient way than time-stepping methods. Finally we discuss that the usage of the employed general formulation does not only relate seemingly not related physical systems mathematically, but does as well allow to discuss model extensions in a more unified way

    Finite-Width Effects in Top Quark Production at Hadron Colliders

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    Production cross sections for t\bar{t} and t\bar{t}j events at hadron colliders are calculated, including finite width effects and off resonance contributions for the entire decay chain, t --> bW --> b\ell\nu, for both top quarks. Resulting background rates to Higgs search at the CERN LHC are updated for inclusive H --> WW studies and for H --> \tau\tau and H --> WW decays in weak boson fusion events. Finite width effects are large, increasing t\bar{t}(j) rates by 20% or more, after typical cuts which are employed for top-background rejection.Comment: 32 pages, 11 figures, 7 tables; minor changes, reference added, to be published in Phys. Rev.

    Discovery of magnetic fields in hot subdwarfs

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    We present initial results of a project to measure mean longitudinal magnetic fields in a group of sdB/OB/O stars. The project was inspired by the discovery of three super-metal-rich sdOB stars, each having metals (e.g. Ti, V) enhanced by factors of 10^3 to 10^5. Similar behaviour is observed in chemically peculiar A stars, where strong magnetic fields are responsible for the enrichment. With this in mind, we obtained circularly polarised spectra of two of the super-metal-rich sdOBs, two "normal" sdBs and two sdOs using FORS1 on the ESO/VLT. By examining circular polarisation in the hydrogen Balmer lines and in helium lines, we have detected magnetic fields with strengths of 1-2 kG in most of our targets. This suggests that such fields are relatively common in hot subdwarfs.Comment: 4 pages, to appear in White Dwarfs, eds. D. Koester, S. Moehler, ASP Conf. serie

    Size effect on magnetism of Fe thin films in Fe/Ir superlattices

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    In ferromagnetic thin films, the Curie temperature variation with the thickness is always considered as continuous when the thickness is varied from nn to n+1n+1 atomic planes. We show that it is not the case for Fe in Fe/Ir superlattices. For an integer number of atomic planes, a unique magnetic transition is observed by susceptibility measurements, whereas two magnetic transitions are observed for fractional numbers of planes. This behavior is attributed to successive transitions of areas with nn and n+1n+1 atomic planes, for which the TcT_c's are not the same. Indeed, the magnetic correlation length is presumably shorter than the average size of the terraces. Monte carlo simulations are performed to support this explanation.Comment: LaTeX file with Revtex, 5 pages, 5 eps figures, to appear in Phys. Rev. Let

    Pharmacokinetics of Pamidronate in Patients With Bone Metastases

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    Background: Pamidronate is a secondgeneration bisphosphonate used in the treatment of tumor-induced hypercalcemia and in the management of bone metastases from breast cancer, myeloma, or prostate cancer. The pharmacokinetics of pamidronate is unknown in cancer patients. Purpose: To determine the influence of the rate of administration and of bone metabolism, we studied the pharmacokinetics of pamidronate at three different infusion rates in 37 patients with bone metastases. Methods: Three groups of 11-14 patients were given 60 mg pamidronate as an intravenous infusion over a period of 1, 4, or 24 hours. Urine samples were collected in the three groups of patients. Plasma samples were obtained only in the 1-hour infusion group. The assay of pamidronate in plasma and urine was performed by high-performance liquid chromatography with fluorescence detection after the derivatization of pamidronate with fluorescamine. Results: The body retention (BR) at 0-24 hours of pamidronate represented 60%-70% of the administered dose and was not significantly modified by the infusion rate. In particular, the BR at 0-24 hours was not reduced at the fastest infusion rate. Among patients, a threefold variability in BR at 0-24 hours occurred, which was related directly to the number of bone metastases and, to some extent, to creatinine clearance. At 60 mg/hour, the plasma kinetics followed a multiexponential course characterized by a short distribution phase. The mean (±SD) half-life of the distribution phase was 0.8 hour (±0.3), the mean (±SD) of the area under the curve for drug concentration in plasma × time at 0-24 hours was 22.0 × 8.8 μmol/L × hours, and the mean (±SD) of the maximum plasma concentration was 9.7 μmol/L (±3.2). Pharmacokinetic variables remained unchanged after repeated infusions applied to four patients. Clinically, the three infusion rates were equally well tolerated without significant toxicity. Conclusions: The 1-hour infusion rate could be proposed as kinetically appropriate for the administration of pamidronate to patients with metastatic bone diseases. [J Natl Cancer Inst 84: 788-792, 1992

    Construction and Test of MDT Chambers for the ATLAS Muon Spectrometer

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    The Monitored Drift Tube (MDT) chambers for the muon spectrometer of the AT- LAS detector at the Large Hadron Collider (LHC) consist of 3-4 layers of pressurized drift tubes on either side of a space frame carrying an optical monitoring system to correct for deformations. The full-scale prototype of a large MDT chamber has been constructed with methods suitable for large-scale production. X-ray measurements at CERN showed a positioning accuracy of the sense wires in the chamber of better than the required 20 ?microns (rms). The performance of the chamber was studied in a muon beam at CERN. Chamber production for ATLAS now has started
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