4,280,943 research outputs found
UCN Upscattering rates in a molecular deuterium crystal
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
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
It is a classical fact that the cotangent bundle T^* \M of a differentiable
manifold \M enjoys a canonical symplectic form . If
(\M,\j,g,\omega) is a pseudo-K\"ahler or para-K\"ahler -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 is
the pull-back by of and \G is a pseudo-Riemannian metric with
neutral signature . We investigate the curvature properties of the
pair (\J,\G) and prove that: \G is scalar-flat, is not Einstein unless
is flat, has nonpositive (resp.\ nonnegative) Ricci curvature if and only if
has nonpositive (resp.\ nonnegative) Ricci curvature as well, and is
locally conformally flat if and only if and has constant curvature,
or and is flat. We also check that (i) the holomorphic sectional
curvature of (\J,\G) is not constant unless is flat, and (ii) in
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
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
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
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 H collisions
Rate coefficients for state-to-state rotational transitions in CO induced by
both para- and ortho-H collisions are presented. The results were obtained
using the close-coupling method and the coupled-states approximation, with the
CO-H interaction potential of Jankowski & Szalewicz (2005). Rate
coefficients are presented for temperatures between 1 and 3000 K, and for
CO() quenching from to all lower levels. Comparisons
with previous calculations using an earlier potential show some discrepancies,
especially at low temperatures and for rotational transitions involving large
. 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
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