8,670 research outputs found
Optical tomography using the SCIRun problem solving environment: Preliminary results for three-dimensional geometries and parallel processing
We present a 3D implementation of the UCL imaging package for absorption and scatter reconstruction from time-resolved data (TOAST), embedded in the SCIRun interactive simulation and visualization package developed at the University of Utah. SCIRun is a scientific programming environment that allows the interactive construction, debugging, and steering of large-scale scientific computations. While the capabilities of SCIRun's interactive approach are not yet fully exploited in the current TOAST implementation, an immediate benefit of the combined TOAST/SCIRun package is the availability of optimized parallel finite element forward solvers, and the use of SCIRun's existing 3D visualisation tools. A reconstruction of a segmented 3D head model is used as an example for demonstrating the capability of TOAST/SCIRun of simulating anatomically shaped meshes
Exploring manifestation and nature of a dineutron in two-neutron emission using a dynamical dineutron model
Emission of two neutrons or two protons in reactions and decays is often
discussed in terms of "dineutron" or "diproton" emission. The discussion often
leans intuitively on something described by Migdal-Watson approximation. In
this work we propose a way to formalize situations of dineutron emission. It is
demonstrated that properly formally defined dineutron emission may reveal
properties which are drastically different from those traditionally expected,
and properties which are actually observed in three-body decays.Comment: 11 pages, 11 Figure
Thomas-Ehrman effect in a three-body model: Ne case
The dynamic mechanism of the Thomas-Ehrman shift is studied in three-cluster
systems by example of Ne and C isobaric mirror partners. We
predict configuration mixings for and states in Ne and
C. Large isospin symmetry breaking on the level of wave function
component weights is demonstrated for these states and discussed as three-body
mechanism of Thomas-Ehrman shift. It is shown that the description of the
Coulomb displacement energies requires a consistency among three parameters:
the Ne decay energy , the F ground state energy , and
the configuration mixing parameters for the Ne/C and
states. Basing on this analysis we infer the F ground state
energy to be MeV.Comment: 10 pages 8 figure
High precision studies of soft dipole mode in two-neutron halo nuclei: He case
The "soft dipole" E1 strength function is calculated for the transition from
the He ground state to the continuum He++. The
calculations were performed within the hyperspherical harmonics formalism. The
sensitivity of the results to the He ground state structure and to final
state interactions, are analyzed. The large-basis calculations show the
reliably converged results for soft dipole strength function and for momentum
correlations of the ^{6}\mbox{He} \rightarrow \, ^{4}He++ dissociation
products. Transition mechanisms are analyzed based on the momentum
correlations. The comparison with experimental data is provided.Comment: 16 pages, 17 figure
Low polarized emission from the core of coronal mass ejections
In white-light coronagraph images, cool prominence material is sometimes
observed as bright patches in the core of coronal mass ejections (CMEs). If, as
generally assumed, this emission is caused by Thomson-scattered light from the
solar surface, it should be strongly polarised tangentially to the solar limb.
However, the observations of a CME made with the SECCHI/STEREO coronagraphs on
31 August 2007 show that the emission from these bright core patches is
exceptionally low polarised. We used the polarisation ratio method of Moran and
Davila (2004) to localise the barycentre of the CME cloud. By analysing the
data from both STEREO spacecraft we could resolve the plane-of-the-sky
ambiguity this method usually suffers from. Stereoscopic triangulation was used
to independently localise the low-polarisation patch relative to the cloud. We
demonstrated for the first time that the bright core material is located close
to the centre of the CME cloud. We show that the major part of the CME core
emission, more than 85% in our case, is H radiation and only a small
fraction is Thomson-scattered light. Recent calculations also imply that the
plasma density in the patch is 8 10 cm or more compared to 2.6
10 cm for the Thomson-scattering CME environment surrounding the
core material.Comment: 5 pages, 3 figure
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