2,385 research outputs found

    Spin dynamics in copper metaborate CuB2O4CuB_2 O_4 studied by muon spin relaxation

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    Copper metaborate CuB2_2O4_{4} was studied by muon spin relaxation measurements in order to clarify its static and dynamic magnetic properties. The time spectra of muon spin depolarization suggest that the local fields at the muon site contain both static and fluctuating components in all ordered phases down to 0.3 K. In the weak ferromagnetic phase (20 K~>T>>T>~9.3 K), the static component is dominant. On the other hand, upon cooling the fluctuating component becomes dominant in the incommensurate helix phase (9.3K > T > 1.4K). The dynamical fluctuations of the local fields persist down to 0.3K, where a new incommensurate phase (T < 1.4K) is expected to appear. This result suggests that spins fluctuate even at T \to 0. We propose two possible origins of the remnant dynamical spin fluctuations: frustration of the exchange interactions and the dynamic behavior of the soliton lattice

    Gamow-Teller transitions and deformation in the proton-neutron random phase approximation

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    We investigate reliability of Gamow-Teller transition strengths computed in the proton-neutron random phase approximation, comparing with exact results from diagonalization in full 0ω0\hbar\omega shell-model spaces. By allowing the Hartree-Fock state to be deformed, we obtain good results for a wide variety of nuclides, even though we do not project onto good angular momentum. We suggest that deformation is as important or more so than pairing for Gamow-Teller transitions.Comment: 8 pages, 5 figures; added references, clarified discussion with regards to stabilit

    Exploring Emerging Occupational Therapy Identity and the Development of Graduate Attributes Among Occupational Therapy Students

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    Introduction: Strong professional identity allows for appropriate representation and promotion of occupational therapy. Academic education assists in the development of occupational therapy identity. This study aims to explore the development of occupational therapy identity and graduate attributes in occupational therapy students after the first year of a revised curriculum. Method: Occupational therapy students (n¼58) were surveyed at the commencement of the second year. Data analysis used descriptive statistics and inferential statistics (v2 for trend). Results: A total of 54 students (93.1%) completed the survey. Students progressively developed occupational therapy identity over time. There were no significant associations between main factors influencing the original decision to study occupational therapy and when occupational therapy identity developed. However, there were significant associations between main factors influencing students’ decision to continue studying and when identity developed. Most students agreed the curriculum equipped them to develop graduate attributes, although this was not significantly associated with factors that either influenced students to study, or continue studying, occupational therapy. There was significant association between development of graduate attributes and occupational therapy identity over time. Conclusion: This study showed an emergence of occupational therapy identity and graduate attributes in students, demonstrating the importance of first year curriculum in the development of these factors

    Nearly Bi-Maximal Neutrino Mixing, Muon g-2 Anomaly and Lepton-Flavor-Violating Processes

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    We interpret the newly observed muon g-2 anomaly in the framework of a leptonic Higgs doublet model with nearly degenerate neutrino masses and nearly bi-maximal neutrino mixing. Useful constraints are obtained on the rates of lepton-flavor-violating rare decays τμγ\tau \to \mu \gamma, μeγ\mu \to e \gamma and τeγ\tau \to e \gamma as well as the μ\mu-ee conversion ratio RμeR_{\mu e}. We find that Γ(μeγ)\Gamma (\mu \to e \gamma), Γ(τeγ)\Gamma (\tau \to e \gamma) and RμeR_{\mu e} depend crucially on possible non-zero but samll values of the neutrino mixing matrix element Ve3V_{e3}, and they are also sensitive to the Dirac-type CP-violating phase. In particular, we show that Γ(τμγ)/mτ5\Gamma (\tau \to \mu \gamma)/m^5_\tau, Γ(μeγ)/mμ5\Gamma (\mu \to e \gamma)/m^5_\mu and Γ(τeγ)/mτ5\Gamma (\tau \to e \gamma)/m^5_\tau are approximately in the ratio 1:2Ve32:2Ve321: 2|V_{e3}|^2: 2|V_{e3}|^2 if Ve3|V_{e3}| is much larger than O(102){\cal O}(10^{-2}), and in the ratio 2(Δmatm2)2:(Δmsun2)2:(Δmsun2)22 (\Delta m^2_{\rm atm})^2: (\Delta m^2_{\rm sun})^2:(\Delta m^2_{\rm sun})^2 if Ve3|V_{e3}| is much lower than O(103){\cal O}(10^{-3}), where Δmatm2\Delta m^2_{\rm atm} and Δmsun2\Delta m^2_{\rm sun} are the corresponding mass-squared differences of atmospheric and solar neutrino oscillations.Comment: LaTex 6 pages (2 PS figures). Phys. Rev. D (in printing

    All-Sky Near Infrared Space Astrometry

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    Gaia is currently revolutionizing modern astronomy. However, much of the Galactic plane, center and the spiral arm regions are obscured by interstellar extinction, rendering them inaccessible because Gaia is an optical instrument. An all-sky near infrared (NIR) space observatory operating in the optical NIR, separated in time from the original Gaia would provide microarcsecond NIR astrometry and millimag photometry to penetrate obscured regions unraveling the internal dynamics of the Galaxy.Comment: 7 page

    Discovery of magnetic fields in the very young, massive stars W601 (NGC 6611) and OI 201 (NGC 2244)

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    Context: Recent spectropolarimetric observations of Herbig Ae/Be stars have yielded new arguments in favour of a fossil origin for the magnetic fields of intermediate mass stars. Aims: To study the evolution of these magnetic fields, and their impact on the evolution of the angular momentum of these stars during the pre-main sequence phase, we observed Herbig Ae/Be members of young open clusters of various ages. Methods: We obtained high-resolution spectropolarimetric observations of Herbig Ae/Be stars belonging to the young open clusters NGC 6611 (< 6 Myr), NGC 2244 (~1.9 Myr), and NGC 2264 (~8 Myr), using ESPaDOnS at theCanada-France-Hawaii Telescope. Results: Here we report the discovery of strong magnetic fields in two massive pre-main sequence cluster stars. We detected, for the first time, a magnetic field in a pre-main sequence rapid rotator: the 10.2 Msun Herbig B1.5e star W601 (NGC 6611; v sin i ~ 190 km/s). Our spectropolarimetric observations yield a longitudinal magnetic field larger than 1 kG, and imply a rotational period shorter than 1.7 days. The spectrum of this very young object (age ~ 0.017 Myr) shows strong and variable lines of He and Si. We also detected a magnetic field in the 12.1 Msun B1 star OI 201 (NGC 2244; v sin i = 23.5 km/s). The Stokes V profile of this star does not vary over 5 days, suggesting a long rotational period, a pole-on orientation, or aligned magnetic and rotation axes. OI 201 is situtated near the Zero-Age Main Sequence on the HR diagram, and exhibits normal chemical abundances and no spectrum variability.Comment: Accepted for publication as a letter in A&

    Quantifying Dynamics in Tropical Peat Swamp Forest Biomass with Multi- Temporal LiDAR Datasets

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    Tropical peat swamp forests in Indonesia store huge amounts of carbon and are responsible for enormous carbon emissions every year due to forest degradation and deforestation. These forest areas are in the focus of REDD+ (reducing emissions from deforestation, forest degradation, and the role of conservation, sustainable management of forests and enhancement of forest carbon stocks) projects, which require an accurate monitoring of their carbon stocks or aboveground biomass (AGB). Our study objective was to evaluate multi-temporal LiDAR measurements of a tropical forested peatland area in Central Kalimantan on Borneo. Canopy height and AGB dynamics were quantified with a special focus on unaffected, selective logged and burned forests. More than 11,000 ha were surveyed with airborne LiDAR in 2007 and 2011. In a first step, the comparability of these datasets was examined and canopy height models were created. Novel AGB regression models were developed on the basis of field inventory measurements and LiDAR derived height histograms for 2007 (r(2) = 0.77, n = 79) and 2011 (r(2) = 0.81, n = 53), taking the different point densities into account. Changes in peat swamp forests were identified by analyzing multispectral imagery. Unaffected forests accumulated on average 20 t/ha AGB with a canopy height increase of 2.3 m over the four year time period. Selective logged forests experienced an average AGB loss of 55 t/ha within 30 m and 42 t/ha within 50 m of detected logging trails, although the mean canopy height increased by 0.5 m and 1.0 m, respectively. Burned forests lost 92% of the initial biomass. These results demonstrate the great potential of repetitive airborne LiDAR surveys to precisely quantify even small scale AGB and canopy height dynamics in remote tropical forests, thereby featuring the needs of REDD+
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