3,531 research outputs found
Comparing league formats with respect to match importance in Belgian football
Recently, most clubs in the highest Belgian football division have become convinced that the format of their league should be changed. Moreover, the TV station that broadcasts the league is pleading for a more attractive competition. However, the clubs have not been able to agree on a new league format, mainly because they have conflicting interests. In this paper, we compare the current league format, and three other formats that have been considered by the Royal Belgian Football Association. We simulate the course of each of these league formats, based on historical match results. We assume that the attractiveness of a format is determined by the importance of its games; our importance measure for a game is based on the number of teams for which this game can be decisive to reach a given goal. Furthermore, we provide an overview of how each league format aligns with the expectations and interests of each type of club
Crystal field splitting and correlation effect on the electronic structure of A2IrO3
The electronic structure of the honeycomb lattice iridates Na2IrO3 and
Li2IrO3 has been investigated using resonant inelastic x-ray scattering (RIXS).
Crystal-field split d-d excitations are resolved in the high-resolution RIXS
spectra. In particular, the splitting due to non-cubic crystal fields, derived
from the splitting of j_eff=3/2 states, is much smaller than the typical
spin-orbit energy scale in iridates, validating the applicability of j_eff
physics in A2IrO3. We also find excitonic enhancement of the particle-hole
excitation gap around 0.4 eV, indicating that the nearest-neighbor Coulomb
interaction could be large. These findings suggest that both Na2IrO3 and
Li2IrO3 can be described as spin-orbit Mott insulators, similar to the square
lattice iridate Sr2IrO4
RXTE observations of the first transient Z source XTE J1701-462: shedding new light on mass accretion in luminous neutron star LMXBs
(Abridged) We report on ten weeks of RXTE observations of the X-ray transient
XTE J1701-462. Comparisons with other sources suggest it had all the
characteristics of the neutron star Z sources (the brightest persistent neutron
star LMXBs). These include Z tracks in X-ray color diagrams and typical
variability components detected in the power spectra. XTE J1701-462 is the
first transient Z source and provides unique insights into mass accretion rate
(Mdot) and luminosity dependencies in neutron star LMXBs. As its overall
luminosity decreased, we observed a switch between two types of Z-source
behavior, with most of the branches of the Z-track changing their shape and/or
orientation. We interpret this switch as an extreme case of the longterm
changes seen in the persistent Z sources and suggest that these result from
changes in Mdot. We also suggest that the Cyg-like Z sources (Cyg X-2, GX 5-1,
and GX 340+0) might be more luminous (> 50%) than the Sco-like Z sources (Sco
X-1, GX 17+2, and GX 349+2). Adopting a possible explanation for the behavior
of kHz QPOs, which involves a prompt as well as a filtered response to changes
in Mdot, we propose that changes in Mdot can explain both movement along the Z
track and changes in the shape of the Z track. We discuss some consequences of
this and consider the possibility that the branches of the Z will evolve into
the branches observed in the X-ray color diagrams of the less luminous atoll
sources, but not in a way that was previously suggested.Comment: Accepted for publication in ApJ, 11 page
RXTE observations of the neutron star low-mass X-ray binary GX 17+2: correlated X-ray spectral and timing behavior
We have analyzed ~600 ks of Rossi X-ray Timing Explorer data of the neutron
star low-mass X-ray binary and Z source GX 17+2. A study was performed of the
properties of the noise components and quasi-periodic oscillations (QPOs) as a
function of the spectral properties, with the main goal to study the relation
between the frequencies of the horizontal branch and upper kHz QPOs. It was
found that when the upper kHz QPO frequency is below 1030 Hz these frequencies
correlate, whereas above 1030 Hz they anti-correlate. GX 17+2 is the first
source in which this is observed. We also found that the frequency difference
of the high frequency QPOs was not constant and that the quality factors (Q
values) of the HBO, its second harmonic, and the kHz QPOs are similar, and vary
almost hand in hand by a factor of more than three. Observations of the normal
branch oscillations during two type I X-ray bursts showed that their absolute
amplitude decreased as the flux from the neutron star became stronger. We
discuss these and other findings in terms of models that have been proposed for
these phenomena. We also compare the behavior of GX 17+2 and other Z sources
with that of black hole sources and consider the possibility that the mass
accretion rate might not be driving force behind all spectral and variability
changes.Comment: 35 pages, including 14 figures. Accepted for publication in ApJ.
Revised discussion, one new figure, and some minor figure changes with
respect to old versio
Photoemission spectra of LaMnO3 controlled by orbital excitations
We investigate the spectral function of a hole moving in the orbital-ordered
ferromagnetic planes of LaMnO, and show that it depends critically on the
type of orbital ordering. While the hole does not couple to the spin
excitations, it interacts strongly with the excitations of orbitals
(orbitons), leading to new type of quasiparticles with a dispersion on the
orbiton energy scale and with strongly enhanced mass and reduced weight.
Therefore we predict a large redistribution of spectral weight with respect to
the bands found in local density approximation (LDA) or in LDA+U.Comment: 4 pages, 4 figures, 3 figures embedded, figure 3 correcte
Investigation of the Domain Wall Fermion Approach to Chiral Gauge Theories on the Lattice
We investigate a recent proposal to construct chiral gauge theories on the
lattice using domain wall fermions. We restrict ourselves to the finite volume
case, in which two domain walls are present, with modes of opposite chirality
on each of them. We couple the chiral fermions on only one of the domain walls
to a gauge field. In order to preserve gauge invariance, we have to add a
scalar field, which gives rise to additional light mirror fermion and scalar
modes. We argue that in an anomaly free model these extra modes would decouple
if our model possesses a so-called strong coupling symmetric phase. However,
our numerical results indicate that such a phase most probably does not exist.
---- Note: 9 Postscript figures are appended as uuencoded compressed tar file.Comment: 27p. Latex; UCSD/PTH 93-28, Wash. U. HEP/93-6
Low temperature transport in AC-driven Quantum Dots in the Kondo regime
We present a fully nonequilibrium calculation of the low temperature
transport properties of a quantum dot in the Kondo regime when an AC potential
is applied to the gate voltage. We solve a time dependent Anderson model with
finite on-site Coulomb interaction. The interaction self-energy is calculated
up to second order in perturbation theory in the on-site interaction, in the
context of the Keldysh non-equilibrium technique, and the effect of the AC
voltage is taken into account exactly for all ranges of AC frequencies and AC
intensities. The obtained linear conductance and time-averaged density of
states of the quantum dot evolve in a non trivial way as a function of the AC
frequency and AC intensity of the harmonic modulation.Comment: 30 pages,7 figure
Orbital excitations in LaMnO
We study the recently observed orbital excitations, orbitons, and treat
electron-electron correlations and lattice dynamics on equal footing. It is
shown that the orbiton energy and dispersion are determined by both
correlations and lattice-vibrations. The electron-phonon coupling causes
satellite structures in the orbiton spectral function and the elementary
excitations of the system are mixed modes with both orbital and phonon
character. It is proposed that the satellite structures observed in recent
Raman-scattering experiments on LaMnO are actually orbiton derived
satellites in the phonon spectral function, caused by the phonon-orbiton
interaction.Comment: 4 pages, 3 figures embedde
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