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Coherent modeling of mortality patterns for age-specific subgroups
The recent actuarial literature has shown that mortality patterns and trajectories in closely related populations are similar in some respects and that small differences are unlikely to increase in the long run. The common feeling is that mortality forecasts for individual countries could be improved by taking into account the patterns from a larger group. Starting from this consideration, we apply the three-way Lee–Carter model to a group of countries, by extending the bilinear LC model to a three-way structure, which incorporates a further component in the decomposition of the log-mortality rates. From a methodological point of view, there are several issues to deal with when focusing on such kind of data. In the presence of a three-way data structure, several choices on the pretreatment of the data could affect the whole modeling process. This kind of analysis is useful to assess the source of variation in the raw mortality data, before the extraction of the rank-one components by the LC model. The proposed procedure is used to extract an ad hoc time mortality trend parameter for age-specific subgroups. The results show that the proposed strategy leads to a more coherent description of mortality for age-specific subgroups
A Geometric Monte Carlo Algorithm for the Antiferromagnetic Ising model with "Topological" Term at
In this work we study the two and three-dimensional antiferromagnetic Ising
model with an imaginary magnetic field at . In order to
perform numerical simulations of the system we introduce a new geometric
algorithm not affected by the sign problem. Our results for the model are
in agreement with the analytical solutions. We also present new results for the
model which are qualitatively in agreement with mean-field predictions
Signatures of rotating binaries in micro-lensing experiments
Gravitational microlensing offers a powerful method with which to probe a
variety of binary-lens systems, as the binarity of the lens introduces
deviations from the typical (single-lens) Paczy\'nski behaviour in the event
light curves. Generally, a static binary lens is considered to fit the observed
light curve and, when the orbital motion is taken into account, an
oversimplified model is usually employed. In this paper, we treat the
binary-lens motion in a realistic way and focus on simulated events that are
fitted well by a Paczy\'nski curve. We show that an accurate timing analysis of
the residuals (calculated with respect to the best-fitting Paczy\'nski model)
is usually sufficient to infer the orbital period of the binary lens. It goes
without saying that the independently estimated period may be used to further
constrain the orbital parameters obtained by the best-fitting procedure, which
often gives degenerate solutions. We also present a preliminary analysis of the
event OGLE-2011-BLG-1127 / MOA-2011-BLG-322, which has been recognized to be
the result of a binary lens. The period analysis results in a periodicity of
\simeq 12 days, which confirms the oscillation of the observed data around the
best-fitting model. The estimated periodicity is probably associated with an
intrinsic variability of the source star, and therefore there is an opportunity
to use this technique to investigate either the intrinsic variability of the
source or the effects induced by the binary-lens orbital motion.Comment: In press on MNRAS, 2014. 8 pages, 4 figures. On-line material
available on the Journal web-pag
A Voltage Calibration Chain for Meters Used in Measurements of EV Inductive Power Charging
The inductive charging of electric vehicles requires specific measurement and
calibration systems. In fact, the measurement of power on board involves DC
signals, which are superimposed to a significant AC ripple up to or over 150
kHz, depending on the type of charging system. A calibration method that makes
use of a phantom power, based on two independent but synchronized circuits, is
considered, simulating the charging voltage and current. This paper describes
in detail a solution in the realization of the voltage calibration chain, based
on the use of a DC voltage calibrator, an injector and a voltage divider.Comment: 2 pages, Conference on Precision Electromagnetic Measurements (CPEM
2018), Paris
Identification of the Coronal Sources of the Fast Solar Wind
The present spectroscopic study of the ultraviolet coronal emission in a
polar hole, detected on April 6-9, 1996 with the Ultraviolet Coronagraph
Spectrometer aboard the SOHO spacecraft, identifies the inter-plume lanes and
background coronal hole regions as the channels where the fast solar wind is
preferentially accelerated. In inter-plume lanes, at heliocentric distance 1.7
\rsun, the corona expands at a rate between 105 km/s and 150 km/s, that is,
much faster than in plumes where the outflow velocity is between 0 km/s and 65
km/s. The wind velocity is inferred from the Doppler dimming of the O VI
1032, 1037 \AA lines, within a range of values, whose lower
and upper limit corresponds to anisotropic and isotropic velocity distribution
of the oxygen coronal ions, respectively.Comment: 14 pages, 4 figures, 3 tables, Accepted by ApJ Letter
Anderson transition and multifractals in the spectrum of the Dirac operator of Quantum Chromodynamics at high temperature
We investigate the Anderson transition found in the spectrum of the Dirac
operator of Quantum Chromodynamics (QCD) at high temperature, studying the
properties of the critical quark eigenfunctions. Applying multifractal
finite-size scaling we determine the critical point and the critical exponent
of the transition, finding agreement with previous results, and with available
results for the unitary Anderson model. We estimate several multifractal
exponents, finding also in this case agreement with a recent determination for
the unitary Anderson model. Our results confirm the presence of a true Anderson
localization-delocalization transition in the spectrum of the quark Dirac
operator at high-temperature, and further support that it belongs to the 3D
unitary Anderson model class.Comment: 10 pages, 6 figure
Phase structure of a generalized Nambu Jona-Lasinio model with Wilson fermions in the mean field or large -expansion
We analyze the vacuum structure of a generalized lattice Nambu--Jona-Lasinio
model with two flavors of Wilson fermions, such that its continuum action is
the most general four-fermion action with 'trivial' color interactions, and
having a symmetry in the chiral limit. The phase structure
of this model in the space of the two four-fermion couplings shows, in addition
to the standard Aoki phases, new phases with , in
close analogy to similar results recently suggested by some of us for lattice
QCD with two degenerate Wilson fermions. This result shows how the phase
structure of an effective model for low energy QCD cannot be entirely
understood from Wilson Chiral Perturbation Theory, based on the standard QCD
chiral effective Lagrangian approach.Comment: 24 pages, 3 figures, sent to Nuclear Physics
A catalogue sample of low mass galaxies observed in X-rays with central candidate black holes
We present a sample of -ray selected candidate black holes in 51 low mass
galaxies with {and mass up to M} obtained by
cross-correlating the NASA-SLOAN Atlas with the 3XMM catalogue. {We have also
searched in the available catalogues for radio counterparts of the black hole
candidates and find that 19 of the previously selected sources have also a
radio counterpart.} Our results show that about of the galaxies of our
sample host { an -ray source} (associated to a radio counterpart) spatially
coincident with the galaxy center, in agreement with { other recent works}. For
these {\it nuclear} sources, the -ray/radio fundamental plane relation
allows one to estimate the mass of the (central) candidate black holes which
results to be in the range M (with median
value of M and eight candidates having mass
below M). This result, while suggesting that -ray
emitting black holes in low-mass galaxies may have had a key role in the
evolution of such systems, makes even more urgent to explain how such massive
objects formed in galaxies. {Of course, dedicated follow-up observations both
in the -ray and radio bands, as well as in the optical, are necessary in
order to confirm our resultsComment: 15 Pages, 2 Figures, 3 Table
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