4,280,943 research outputs found

    UCN Upscattering rates in a molecular deuterium crystal

    Full text link
    A calculation of ultra-cold neutron (UCN) upscattering rates in molecular deuterium solids has been carried out, taking into account intra-molecular exictations and phonons. The different moelcular species ortho-D2 (with even rotational quantum number J) and para-D2 (with odd J) exhibit significantly different UCN-phonon annihilation cross-sections. Para- to ortho-D2 conversion, furthermore, couples UCN to an energy bath of excited rotational states without mediating phonons. This anomalous upscattering mechanism restricts the UCN lifetime to 4.6 msec in a normal-D2 solid with 33% para content.Comment: 3 pages, one figur

    On the kernel of a singular integral operator with non-carleman shift and conjugation

    Get PDF
    On the Hilbert space (L) over tilde (2)(T) the singular integral operator with non-Carleman shift and conjugation K = P+ +(aI + AC)P- is considered, where P-+/- are the Cauchy projectors, A = (m)Sigma(j=0) a(j)U(j), a, a(j), j = (1, m) over bar, are continuous functions on the unit circle T, U is the shift operator and C is the operator of complex conjugation. Some estimates for the dimension of the kernel of the operator K are obtained.Fundacao para a Ciencia e Tecnologia (Portugal) through Centro de Analise Funcional e Aplicacoes of Instituto Superior Tecnicoinfo:eu-repo/semantics/publishedVersio

    A canonical structure on the tangent bundle of a pseudo- or para-K\"ahler manifold

    Full text link
    It is a classical fact that the cotangent bundle T^* \M of a differentiable manifold \M enjoys a canonical symplectic form Ω∗\Omega^*. If (\M,\j,g,\omega) is a pseudo-K\"ahler or para-K\"ahler 2n2n-dimensional manifold, we prove that the tangent bundle T\M also enjoys a natural pseudo-K\"ahler or para-K\"ahler structure (\J,\G,\Omega), where Ω\Omega is the pull-back by gg of Ω∗\Omega^* and \G is a pseudo-Riemannian metric with neutral signature (2n,2n)(2n,2n). We investigate the curvature properties of the pair (\J,\G) and prove that: \G is scalar-flat, is not Einstein unless gg is flat, has nonpositive (resp.\ nonnegative) Ricci curvature if and only if gg has nonpositive (resp.\ nonnegative) Ricci curvature as well, and is locally conformally flat if and only if n=1n=1 and gg has constant curvature, or n>2n>2 and gg is flat. We also check that (i) the holomorphic sectional curvature of (\J,\G) is not constant unless gg is flat, and (ii) in n=1n=1 case, that \G is never anti-self-dual, unless conformally flat.Comment: Clarified the statements on the cotangent bundle. Corrected various typo

    Extended chiral algebras and the emergence of SU(2) quantum numbers in the Coulomb gas

    Get PDF
    We study a set of chiral symmetries contained in degenerate operators beyond the `minimal' sector of the c(p,q) models. For the operators h_{(2j+2)q-1,1}=h_{1,(2j+2)p-1} at conformal weight [ (j+1)p-1 ][ (j+1)q -1 ], for every 2j \in N, we find 2j+1 chiral operators which have quantum numbers of a spin j representation of SU(2). We give a free-field construction of these operators which makes this structure explicit and allows their OPEs to be calculated directly without any use of screening charges. The first non-trivial chiral field in this series, at j=1/2, is a fermionic or para-fermionic doublet. The three chiral bosonic fields, at j=1, generate a closed W-algebra and we calculate the vacuum character of these triplet models.Comment: 23 pages Late

    Interstellar H2 toward HD 147888

    Full text link
    The ultraviolet and far--ultraviolet spectra of HD 147888 allows to access the v=0 as well as higher vibrational levels of the ground H2 electronic level. We have determined column densities of the H2 molecule on vibrational levels v=0-5 and rotational levels J=0-6. The ortho to para H2 ratio for the excited vibrational states equals to 1.2. For the lowest vibrational state v=0 and rotational level J=1 the ortho to para H2 ratio is only 0.16. The temperature of ortho-para thermodynamical equilibrium is T_OP=43+-3 K. The large number of H2 absorption lines in the HST spectra allows to determine column densities even from a noisy spectra. The measurements of H2 column densities on excited vibrational levels (from the HST spectra) leads to constrains of radiation field in photon-dominated regions (PDR) models of interstellar cloud towards HD 147888

    Two fermion relativistic bound states

    Get PDF
    We consider the relativistic quantum mechanics of a two interacting fermions system. We first present a covariant formulation of the kinematics of the problem and give a short outline of the classical results. We then quantize the system with a general interaction potential and deduce the explicit equations in a spherical basis. The case of the Coulomb interaction is studied in detail by numerical methods, solving the eigenvalue problem for J=0, J=1, J=2 and determining the spectral curves for a varying ratio of the mass of the interacting particles. Details of the computations, together with a perturbative approach in the mass ratio and an extended description of the ground states of the Para- and Orthopositronium are given in Appendix.Comment: 26 pages, 6 figure

    Rotational quenching of CO due to H2_2 collisions

    Full text link
    Rate coefficients for state-to-state rotational transitions in CO induced by both para- and ortho-H2_2 collisions are presented. The results were obtained using the close-coupling method and the coupled-states approximation, with the CO-H2_2 interaction potential of Jankowski & Szalewicz (2005). Rate coefficients are presented for temperatures between 1 and 3000 K, and for CO(v=0,jv=0,j) quenching from j=1−40j=1-40 to all lower j′j^\prime levels. Comparisons with previous calculations using an earlier potential show some discrepancies, especially at low temperatures and for rotational transitions involving large ∣Δj∣|\Delta j|. The differences in the well depths of the van der Waals interactions in the two potential surfaces lead to different resonance structures in the energy dependence of the cross sections which influence the low temperature rate coefficients. Applications to far infrared observations of astrophysical environments are briefly discussed.Comment: 28 pages, 10 figure
    • …
    corecore