1,076 research outputs found

    Double resonant absorption measurement of acetylene symmetric vibrational states probed with cavity ring down spectroscopy

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    A novel mid-infrared/near-infrared double resonant absorption setup for studying infrared-inactive vibrational states is presented. A strong vibrational transition in the mid-infrared region is excited using an idler beam from a singly resonant continuous-wave optical parametric oscillator, to populate an intermediate vibrational state. High output power of the optical parametric oscillator and the strength of the mid-infrared transition result in efficient population transfer to the intermediate state, which allows measuring secondary transitions from this state with a high signal-to-noise ratio. A secondary, near-infrared transition from the intermediate state is probed using cavity ring down spectroscopy, which provides high sensitivity in this wavelength region. Due to the narrow linewidths of the excitation sources, the rovibrational lines of the secondary transition are measured with sub-Doppler resolution. The setup is used to access a previously unreported symmetric vibrational state of acetylene, ν1+ν2+ν3+ν41+ν51\nu_1+\nu_2+\nu_3+\nu_4^1+\nu_5^{-1} in the normal mode notation. Single-photon transitions to this state from the vibrational ground state are forbidden. Ten lines of the newly measured state are observed and fitted with the linear least-squares method to extract the band parameters. The vibrational term value was measured to be at 9775.0018(45) cm1\text{cm}^{-1}, the rotational parameter BB was 1.162222 cm1\text{cm}^{-1}, and the quartic centrifugal distortion parameter DD was 3.998(62)×106cm1\times 10^{-6} \text{cm}^{-1}, where the numbers in the parenthesis are one-standard errors in the least significant digits

    Fermi resonance-algebraic model for molecular vibrational spectra

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    A Fermi resonance-algebraic model is proposed for molecular vibrations, where a U(2) algebra is used for describing the vibrations of each bond, and Fermi resonances between stretching and bending modes are taken into account. The model for a bent molecule XY_2 and a molecule XY_3 is successfully applied to fit the recently observed vibrational spectrum of the water molecule and arsine (AsH_3), respectively, and results are compared with those of other models. Calculations show that algebraic approaches can be used as an effective method for describing molecular vibrations with small standard deviations

    Energy levels and far-infrared spectroscopy for two electrons in a semiconductor nanoring

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    The effects of electron-electron interaction of a two-electron nanoring on the energy levels and far-infrared (FIR) spectroscopy have been investigated based on a model calculation which is performed within the exactly numerical diagonalization. It is found that the interaction changes the energy spectra dramatically, and also shows significant influence on the FIR spectroscopy. The crossings between the lowest spin-singlet and triplet states induced by the coulomb interaction are clearly revealed. Our results are related to the experiment recently carried out by A. Lorke et al. [Phys. Rev. Lett. 84, 2223 (2000)].Comment: 17 pages, 6 figures, revised and accepted by Phys. Rev. B (Dec. 15

    A Proposed Master of Social Work Based in Indigenous Knowledges Program in Manitoba

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    This article focuses on an innovative proposed Master of Social Work based in Indigenous Knowledges program developed by an Indigenous Caucus within the Faculty of Social Work at the University of Manitoba in Canada. This culturally based program intends to ground students with a solid foundation in traditional Indigenous teachings and perspectives, and contemporary Indigenous philosophies, knowledges, concepts, critiques, and ways of being that stem from these traditions. The proposed Master of Social Work based in Indigenous Knowledges was developed as a lived program that builds community and social supports, and reclaims and re-energizes a sense of self, responsibility, self-sufficiency, self-determination, and self-government. The program’s aim is to deconstruct oppressive and colonialist structures and reconstruct, in a contemporary sense, what has been previously destroyed. An overview of the visions, objectives, program design, foundational themes and description of courses is provided, along with reflections on what teachings its development has provided

    Magnetic field dependence of the exciton energy in a quantum disk

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    The groundstate energy and binding energy of an exciton, confined in a^M quantum disk, are calculated as a function of an external magnetic field. The confinement potential is a hard wall of finite height. The diamagnetic shift is investigated for magnetic fields up to 40TT. Our results are applied to InyAl1yAs/AlxGa1xAsIn_{y}Al_{1-y}As/Al_{x}Ga_{1-x}As self-assembled quantum dots and very good agreement with experiments is obtained. Furthermore, we investigated the influence of the dot size on the diamagnetic shift by changing the disk radius. The exciton excited states are found as a function of the magnetic field. The relative angular momentum is not a quantum number and changes with the magnetic field strength.Comment: 10 pages, 17 figure

    Coulombically Interacting Electrons in a One-dimensional Quantum Dot

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    The spectral properties of up to four interacting electrons confined within a quasi one--dimensional system of finite length are determined by numerical diagonalization including the spin degree of freedom. The ground state energy is investigated as a function of the electron number and of the system length. The limitations of a description in terms of a capacitance are demonstrated. The energetically lowest lying excitations are physically explained as vibrational and tunneling modes. The limits of a dilute, Wigner-type arrangement of the electrons, and a dense, more homogeneous charge distribution are discussed.Comment: 10 pages (excl. Figures), Figures added in POSTSCRIPT, LaTe

    Infrared Excess in the Be Star Delta Scorpii

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    We present infrared photometric observations of the Be binary system delta Scorpii obtained in 2006. The J,H and K magnitudes are the same within the errors compared to observations taken 10 months earlier. We derive the infrared excess from the observation and compare this to the color excess predicted by a radiative equilibrium model of the primary star and its circumstellar disk. We use a non-LTE computational code to model the gaseous envelope concentrated in the star's equatorial plane and calculate the expected spectral energy distribution and Halpha emission profile of the star with its circumstellar disk. Using the observed infrared excess of delta Sco, as well as Halpha spectroscopy bracketing the IR observations in time, we place constraints on the radial density distribution in the circumstellar disk. Because the disk exhibits variability in its density distribution, this work will be helpful in understanding its dynamics.Comment: 12 pages, 14 figures, to be published in PASP May 200
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