9,296 research outputs found
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
Four-Probe Measurements of Carbon Nanotubes with Narrow Metal Contacts
We find that electrons in single-wall carbon nanotubes may propagate
substantial distances (tens of nanometers) under the metal contacts. We perform
four-probe transport measurements of the nanotube conductance and observe
significant deviations from the standard Kirchhoff's circuit rules. Most
noticeably, injecting current between two neighboring contacts on one end of
the nanotube, induces a non-zero voltage difference between two contacts on the
other end.Comment: 4 pages, 5 figures; submitte
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
Pauli-principle driven correlations in four-neutron nuclear decays
Mechanism of simultaneous non-sequential four-neutron () emission (or
`true' -decay) has been considered in phenomenological five-body approach.
This approach is analogous to the model of the direct decay to the continuum
often applied to - and -decays. It is demonstrated that -decay
fragments should have specific energy and angular correlations reflecting
strong spatial correlations of `valence' nucleons orbiting in their
-precursors. Due to the Pauli exclusion principle, the valence neutrons are
pushed to the symmetry-allowed configurations in the -precursor structure,
which causes a `Pauli focusing' effect. Prospects of the observation of the
Pauli focusing have been considered for the -precursors H and O.
Fingerprints of their nuclear structure or/and decay dynamics are predicted
- …