ITAMP CALENDAR

2004

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January, 2004

Seminars

Visitors

 

Workshop

January 8-10, 2004, Ultracold Polar Molecules: Formation and Collisions, (Joint Workshop with Harvard/MIT Center for Ultracold Atoms), organized by John Doyle, Jeremy Hutson and Roman Krems

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February, 2004

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March, 2004

Seminars

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April, 2004

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May, 2004

Seminars

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May 10-12, 2004, Mesoscopic Physics, Quantum Optics, and Quantum Information, organized by Charles Marcus (Harvard University) and Hossein Sadeghour (ITAMP)

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June, 2004

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July, 2004

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August, 2004

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September, 2004

Seminars

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October, 2004

Seminars

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Workshop

October 4-6, 2004, Quantum Degenerate Gases in Low-Dimensionality, organized by Brett Esry (Kansas State), Maxim Olshanii (USC), Joerg Schmiedmayer (U. Heidelberg)

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November, 2004

Seminars

Visitors

Workshop

November 15-17, 2004, X-ray Diagnostics for Astrophysical Plasmas: Theory, Experiment, (Joint workshop sponsored by ITAMP, the CXC, the Con-X mission, and the Astro-E2 mission at NASA/Goddard) Scientific Organizing Committee: Randall Smith (NASA/GSFC and JHU), Jay Bookbinder (CfA), Nancy Brickhouse (CfA), Jelle Kaastra (SRON), Tim Kallman (NASA/GSFC), Kate Kirby (CfA), Duane Liedahl (LLNL), John Raymond (CfA), Claude Canizares, (MIT)

 

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December, 2004

Seminars

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 Lifshitz theory of the van der Waals and Casimir forces

G.L. Klimchitskaya and V.M. Mostepanenko

Universidade Federal da Paraiba-UFPB, Brazil

Monday, April 26, 2004
11:00, Classroom (A-101)
Harvard-Smithsonian Center for Astrophysics


The thermal Casimir force between real metals of finite conductivityis considered on the basis of the Lifshitz theory. The contradictions with the Nernst heat theorem arising when one substitutes the Drude model dielectric function into the Lifshitz formula are discussed. The reason for these contradictions is linked to the fact that the Drude dielectric function implies the energy transfer from the electromagnetic field to the phonons of lattice. We demonstrate that the Lifshitz formula expressed in terms of the surface impedance is free of contradictions and lays a reliable theoretical framework for the investigation of the thermal Casimir force. Recent precision measurements of the Casimir force by means of the microelectromechanical torsional oscillator are discussed bringing the experimental confirmation to the surface-impedance approach.

 

Casimir-Polder interaction between an atom and a cavity wall under the influence of real conditions


J.F.Babb, G.L.Klimchitskaya, and V.M. Mostepanenko

ITAMP and Universidade Federal da Paraiba-UFPB, Brazil

Friday, May 21, 2004
2:00 pm, Pratt Conference Room
Harvard-Smithsonian Center for Astrophysics

Abstract:
The Casimir-Polder interaction between an atom and a metal wall is investigated under the influence of real conditions including the dynamic polarizability of an atom, finite conductivity of a wall metal and nonzero temperature. Both analytical and numerical results for the free energy and force are obtained withing a wide separation range. Numerical computations are performed for Au wall and metastable He*, Na and Cs atoms. On the example of He* atom, we demonstrate that at short separations of about Au plasma wavelength at room temperature the free energy deviates up to 35% and force up to 57% from the classical Casimir-Polder result. So large deviations should be taken into account in precision experiments on atom-wall interaction. The combined account of different corrections to the Casimir-Polder interaction leads to the conclusion that at short separations the corrections due to the dynamic polarizability of an atom play a more important role than the corrections due to nonideality of a wall metal and leads to the suppression of the latter ones. By the comparison of the exact atomic polarizabilities with those in the framework of the single oscillator model, it is shown that the obtained asymptotic expressions give the possibility to calculate the free energy and force for atom-wall interaction under real conditions with a precision of one percent.

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Relaxation rates for vibrationally excited molecular hydrogen, 50-2000 K

Ronald J. Bieniek

Physics Department and LEAD Program
University of Missouri - Rolla

Monday, June 21, 2004
2:00 pm, Tea Room
Harvard-Smithsonian Center for Astrophysics

Abstract:
A quantum mechanical "breathing sphere" approach to molecular collisions that changes vibrational-translational states yields a simple analytic expression for thermally averaged relaxation rates that accurately models relaxation rates for OH(v), NO(v), and N2(v) over a range of vibrational excitations. Although H2 should be the worst molecule for the breathing-sphere approximation because of its large rotational-energy spacing, the rates predicted by the analytic expression for H2(v=1)+H2 -> H2(v=0)+H2 for temperatures 50-2000 K are in very good agreement with experimental values and more complicated theoretical computations. As in the N2 case, the predicted temperature dependence successfully follows the five-orders-of-magnitude change in relaxation rate with temperature. Rates for v=2 and v=3 initial excitations will also be discussed.

 

Absolute Cross Section for Electron Impact Excitation of the C III 117.6 nm Multiplet


Mr. Adrian Daw

CfA, Appalachian State University

Wednesday, July 7, 2004
12:30 pm, Pratt Conference Room
Harvard-Smithsonian Center for Astrophysics


We report the latest results from Ion Beam Experiment at the CfA: We have measured the cross section for Electron Impact Excitation (EIE) of C III 117.6 nm for energies below threshold to 17 eV above. Using the unique capabilities of the inclined-beams with photon-detection technique, this work provides the first measurement of the EIE cross section for C III 117.6 nm that covers the energy range required to determine rate coefficients for density diagnostics of the Sun, cool stars, CV binaries and planetary nebulae. This is the first result with the new 5 GHz electron-cyclotron-resonance ion source, which produces useful currents ( >30 nA) of charge states up to 5+. Following the final radiometric calibration, rate coefficients from this work will have an uncertainty of 10% or less.

 

The variable phase method used to calculate and correct scattering lengths


Michael J Jamieson


Department of Computing Science
University of Glasgow

Wednesday, August 4, 2004
12:00 pm, Phillips Auditorium
Harvard-Smithsonian Center for Astrophysics

Abstract:
I will show how the scattering length can be obtained from the equation satisfied by the phase in variable phase theory and how the variable phase equation can be used to predict upper and lower bounds for the long range correction to the scattering length. I will describe a numerical example.

 Gas - surface interactions in star-forming regions

David Williams

University College London

Friday, 15 October 2004
10:00 am, Pratt Conference Room
Harvard-Smithsonian Center for Astrophysics

Abstract:

In denser regions of interstellar space, such as those in star-forming regions, the interactions between gas atoms and molecules with dust grain surfaces become more significant. An example of this is the growth of ice coatings on dust grains by the hydrogenation of oxygen atoms on surfaces in regions above a certain critical visual extinction. Surface processes may in some circumstances dominate gas-phase processes. There is a need for reliable information on adsorption, desorption, reaction, and also on the solid-state processing of amorphous ices. In my talk I shall describe recent studies of situations in which the gas-surface interactions are likely to be important. These may include hot cores in regions of massive star formation, clumpy models of molecular clouds in regions of low mass star formation, and the interaction of stellar jets with dense cores within clumpy clouds.

 

Collision-induced non-adiabatic transitions in the ion-pair states of iodine molecule

Alexei A. Buchachenko


Laboratory of Quantum Mechanics and Molecular Structure
Moscow State University

Friday, 29 October 2004
10:00 am, Pratt Conference Room
Harvard-Smithsonian Center for Astrophysics

Abstract:

Ion-pair electronic states of the iodine molecule lie above the manifold of the valence electronic states and form clusters, or tiers, of closely spaced strongly bound potential
energy curves. Collisions of iodine molecules excited to the ion-pair states with rare gas atoms or molecular partners provide an interesting model for understanding the propensities of non-adibatic electronic energy transfer with respect to the symmetry of the electronic states involved, energy gap and Franck-Condon factor between initial and final rovibronic levels. The results of the quantum scattering calculations of the cross sections and rate constants for the non-adiabatic transitions will be discussed and an overview of experimental studies will be given.

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