1,013 research outputs found
Universal Reduction of Effective Coordination Number in the Quasi-One-Dimensional Ising Model
Critical temperature of quasi-one-dimensional general-spin Ising ferromagnets
is investigated by means of the cluster Monte Carlo method performed on
infinite-length strips, L times infty or L times L times infty. We find that in
the weak interchain coupling regime the critical temperature as a function of
the interchain coupling is well-described by a chain mean-field formula with a
reduced effective coordination number, as the quantum Heisenberg
antiferromagnets recently reported by Yasuda et al. [Phys. Rev. Lett. 94,
217201 (2005)]. It is also confirmed that the effective coordination number is
independent of the spin size. We show that in the weak interchain coupling
limit the effective coordination number is, irrespective of the spin size,
rigorously given by the quantum critical point of a spin-1/2 transverse-field
Ising model.Comment: 12 pages, 6 figures, minor modifications, final version published in
Phys. Rev.
The Playboy of the Western World
Synge explores how we view ourselves through the eyes of others with a character from the time of the The Troubles in Ireland. Presented in November, 1994.https://collected.jcu.edu/plays/1026/thumbnail.jp
On the differential geometry of curves in Minkowski space
We discuss some aspects of the differential geometry of curves in Minkowski
space. We establish the Serret-Frenet equations in Minkowski space and use them
to give a very simple proof of the fundamental theorem of curves in Minkowski
space. We also state and prove two other theorems which represent Minkowskian
versions of a very known theorem of the differential geometry of curves in
tridimensional Euclidean space. We discuss the general solution for torsionless
paths in Minkowki space. We then apply the four-dimensional Serret-Frenet
equations to describe the motion of a charged test particle in a constant and
uniform electromagnetic field and show how the curvature and the torsions of
the four-dimensional path of the particle contain information on the
electromagnetic field acting on the particle.Comment: 10 pages. Typeset using REVTE
IUCN—WWF Plant Advisory Group, First Meeting, held in the Missouri Botanical Garden, St Louis, Missouri, USA, during 17-18 December 1984
The Dumb Waiter; Riders to the Sea
The Dumb Waiter by Harold Pinter, and Riders to the Sea by John M. Synge were presented the John Carroll University\u27s Little Theatre Society in October of 1983.
A review of the performances appeared on page 8 of The Carroll News, October 26, 1983.https://collected.jcu.edu/plays/1095/thumbnail.jp
Quantum phase shift and neutrino oscillations in a stationary, weak gravitational field
A new method based on Synge's world function is developed for determining
within the WKB approximation the gravitationally induced quantum phase shift of
a particle propagating in a stationary spacetime. This method avoids any
calculation of geodesics. A detailed treatment is given for relativistic
particles within the weak field, linear approximation of any metric theory. The
method is applied to the calculation of the oscillation terms governing the
interference of neutrinos considered as a superposition of two eigenstates
having different masses. It is shown that the neutrino oscillations are not
sensitive to the gravitomagnetic components of the metric as long as the spin
contributions can be ignored. Explicit calculations are performed when the
source of the field is a spherical, homogeneous body. A comparison is made with
previous results obtained in Schwarzschild spacetime.Comment: 14 pages, no figure. Enlarged version; added references. In the
Schwarzschild case, our results on the non-radial propagation are compared
with the previous work
Energy Contents of Gravitational Waves in Teleparallel Gravity
The conserved quantities, that are, gravitational energy-momentum and its
relevant quantities are investigated for cylindrical and spherical
gravitational waves in the framework of teleparallel equivalent of General
Relativity using the Hamiltonian approach. For both cylindrical and spherical
gravitational waves, we obtain definite energy and constant momentum. The
constant momentum shows consistency with the results available in General
Relativity and teleparallel gravity. The angular momentum for cylindrical and
spherical gravitational waves also turn out to be constant. Further, we
evaluate their gravitational energy-momentum fluxes and gravitational pressure.Comment: 14 pages, accepted for publication in Mod. Phys. Lett.
Linear waves in sheared flows. Lower bound of the vorticity growth and propagation discontinuities in the parameters space
This study provides sufficient conditions for the temporal monotonic decay of
enstrophy for two-dimensional perturbations traveling in the incompressible,
viscous, plane Poiseuille and Couette flows. Extension of J. L. Synge's
procedure (1938) to the initial-value problem allowed us to find the region of
the wavenumber-Reynolds number map where the enstrophy of any initial
disturbance cannot grow. This region is wider than the kinetic energy's one. We
also show that the parameters space is split in two regions with clearly
distinct propagation and dispersion properties
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