20 research outputs found

    Comprehensive rate coefficients for electron collision induced transitions in hydrogen

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    Energy-changing electron-hydrogen atom collisions are crucial to regulating the energy balance in astrophysical and laboratory plasmas and relevant to the formation of stellar atmospheres, recombination in H-II clouds, primordial recombination, three-body recombination and heating in ultracold and fusion plasmas. Computational modeling of electron-hydrogen collision has been attempted through quantum mechanical scattering state-to-state calculations of transitions involving low-lying energy levels in hydrogen (with principal quantum number n < 7) and at large principal quantum numbers using classical trajectory techniques. Analytical expressions are proposed which interpolates the current quantum mechanical and classical trajectory results for electron-hydrogen scattering in the entire range of energy levels, for nearly all temperature range of interest in astrophysical environments. An asymptotic expression for the Born cross-section is interpolated with a modified expression derived previously for electron-hydrogen scattering in the Rydberg regime using classical trajectory Monte Carlo simulations. The derived formula is compared to existing numerical data for transitions involving low principal quantum numbers, and the dependence of the deviations upon temperature is discussed.Comment: To appear in The Astrophysical Journa

    Non-Maxwellian rate coefficients for electron and ion collisions in Rydberg plasmas: implications for excitation and ionization

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    Scattering phenomena between charged particles and highly excited Rydberg atoms are of critical importance in many processes in plasma physics and astrophysics. While a Maxwell-Boltzmann (MB) energy distribution for the charged particles is often assumed for calculations of collisional rate coefficients, in this contribution we relax this assumption and use two different energy distributions, a bimodal MB distribution and a Îș\kappa-distribution. Both variants share a high-energy tails occurring with higher probability than the corresponding MB distribution. The high energy tail may significantly affect rate coefficients for various processes. We focus the analysis to specific situations by showing the dependence of the rate coefficients on the principal quantum number of hydrogen atoms in n-changing collisions with electrons in the excitation and ionization channels and in a temperature range relevant to the divertor region of a tokamak device. We finally discuss the implications for diagnostics of laboratory plasmas.Comment: 14 pages, 4 figures, Journal of Plasma Physics collection on 'Laboratory and Astrophysical Plasmas: New Perspectives

    Many-body quantum chaos in stroboscopically-driven cold atoms

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    Seeking signatures of quantum chaos in experimentally realizable many-body systems is of vigorous interest. In such systems, the spectral form factor (SFF), defined as the Fourier transform of two-level spectral correlation function, is known to exhibit random matrix theory (RMT) behaviors, namely a 'ramp' followed by a 'plateau' in sufficiently late time. Recently, a generic early-time deviation from the RMT behavior, which we call the 'bump', has been shown to exist in random quantum circuits and spin chains as toy models for many-body quantum chaotic systems. Here we demonstrate the existence of the 'bump-ramp-plateau' behavior in the SFF for a number of paradigmatic, stroboscopically-driven cold atom models of interacting bosons in optical lattices and spinor condensates. We find that the scaling of the many-body Thouless time tTht_{\text{Th}} -- the time of the onset of the (RMT) ramp behavior -- and the increase of the bump amplitude in atom number are significantly slower in (effectively 0D) chaotic spinor gases than in 1D optical lattices, demonstrating the role of locality in many-body quantum chaos. Moreover, tTht_{\text{Th}} scaling and the bump amplitude are more sensitive to variations in atom number than the system size regardless of the hyperfine structure, the symmetry classes, or the choice of the driving protocol. We obtain scaling functions of SFF which suggest power-law behavior for the bump regime in quantum chaotic cold-atom systems. Finally, we propose an interference measurement protocol to probe SFF in the laboratory.Comment: 10 pages, 7 figures, supplementary materia
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