30,589 research outputs found
Restrictions over two-dimensional gauge models with Thirring-like interaction
Some years ago, it was shown how fermion self-interacting terms of the
Thirring-type impact the usual structure of massless two-dimensional gauge
theories [1]. In that work only the cases of pure vector and pure chiral gauge
couplings have been considered and the corresponding Thirring term was also
pure vector and pure chiral respectively, such that the vector (or chiral)
Schwinger model should not lose its chirality structure due to the addition of
the quartic interaction term. Here we extend this analysis to a generalized
vector and axial coupling both for the gauge interaction and the quartic
fermionic interactions. The idea is to perform quantization without losing the
original structure of the gauge coupling. In order to do that we make use of an
arbitrariness in the definition of the Thirring-like interaction.Comment: 9 pages, no figure
Medical education on fitness to drive : a survey of all UK medical schools
Aim: To identify the extent to which medical aspects of fitness to drive (FTD) are taught within UK medical schools.
Methods: A survey of all 32 UK medical schools. In-depth interviews with a range of staff at two medical schools; telephone survey of 30 schools.
Results: Two thirds of schools reported specific teaching on medical aspects of FTD but few covered it in any depth or in relation to specific medical conditions. Only one school taught FTD in relation to elderly medicine. FTD was an examination topic at only 12 schools.
Conclusion: Teaching on FTD is inconsistent across UK medical schools. Many new doctors will graduate with limited knowledge of medical aspects of FTD
Differential interferometric phases at high spectral resolution as a sensitive physical diagnostic of circumstellar disks
Context. The circumstellar disks ejected by many rapidly rotating B stars
(so-called Be stars) offer the rare opportunity of studying the structure and
dynamics of gaseous disks at high spectral as well as angular resolution. Aims.
This paper explores a newly identified effect in spectro-interferometric phase
that can be used for probing the inner regions of gaseous edge-on disks on a
scale of a few stellar radii. Methods. The origin of this effect (dubbed
central quasi-emission phase signature, CQE-PS) lies in the velocity-dependent
line absorption of photospheric radiation by the circumstellar disk. At high
spectral and marginal interferometric resolution, photocenter displacements
between star and isovelocity regions in the Keplerian disk reveal themselves
through small interferometric phase shifts. To investigate the diagnostic
potential of this effect, a series of models are presented, based on detailed
radiative transfer calculations in a viscous decretion disk. Results. Amplitude
and detailed shape of the CQE-PS depend sensitively on disk density and size
and on the radial distribution of the material with characteristic shapes in
differential phase diagrams. In addition, useful lower limits to the angular
size of the central stars can be derived even when the system is almost
unresolved. Conclusions. The full power of this diagnostic tool can be expected
if it can be applied to observations over a full life-cycle of a disk from
first ejection through final dispersal, over a full cycle of disk oscillations,
or over a full orbital period in a binary system
Vacuumless kinks systems from vacuum ones, an example
Some years ago, Cho and Vilenkin, introduced a model which presents
topological solutions, despite not having degenerate vacua as is usually
expected. Here we present a new model with topological defects, connecting
degenerate vacua but which in a certain limit recovers precisely the one
proposed originally by Cho and Vilenkin. In other words, we found a kind of
parent model for the so called vacuumless model. Then the idea is extended to a
model recently introduced by Bazeia et al. Finally, we trace some comments the
case of the Liouville model.Comment: 11 pages, 4 figure
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