20,546 research outputs found
Quantum chaos with non-periodic, complex orbits in the Resonant Tunneling Diode
We show that a special type of orbits, which are non-periodic and complex,
'Saddle Orbits' (SOs) describe accurately the quantal and experimental current
oscillations in the Resonant Tunneling Diode in tilted fields. This is the
first demonstration that one needs to abandon the periodic orbits (POs)
paradigm in favour of this new and peculiar type of orbit. The SOs solve the
puzzle of broad regions of experimental oscillations where we find no real or
complex PO that can explain the data. The SOs succeeds in regimes involving
several non-isolated POs, where PO formulas fail.Comment: 3 pages, 5 figure
The possibility of determining open-cluster parameters from BVRI photometry
In the last decades we witnessed an increase in studies of open clusters of
the Galaxy, especially because of the good determination for a wide range of
values of parameters such as age, distance, reddening, and proper motion. The
reliable determination of the parameters strongly depends on the photometry
available and especially on the U filter, which is used to obtain the color
excess E(B-V) through the color-color diagram (U-B) by (B-V) by fitting a zero
age main-sequence. Owing to the difficulty of performing photometry in the U
band, many authors have tried to obtain E(B-V) without the filter. But because
of the near linearity of the color-color diagrams that use the other bands,
combined with the fact that most fitting procedures are highly subjective (many
done "by eye") the reliability of those results has always been questioned. Our
group has recently developed, a tool that performs isochrone fitting in
open-cluster photometric data with a global optimization algorithm, which
removes the need to visually perform the fits and thus removes most of the
related subjectivity. Here we apply our method to a set of synthetic clusters
and two observed open clusters (Trumpler 1 and Melotte 105) using only
photometry for the BVRI bands. Our results show that, considering the cluster
structural variance caused only by photometric and Poisson sampling errors, our
method is able to recover the synthetic cluster parameters with errors of less
than 10% for a wide range of ages, distances, and reddening, which clearly
demonstrates its potential. The results obtained for Trumpler 1 and Melotte 105
also agree well with previous literature values.Comment: 5 pages, 5 figures, accepted for publication in
Astronomy&Astrophysic
Tuning the Mott transition in a Bose-Einstein condensate by multi-photon absorption
We study the time-dependent dynamics of a Bose-Einstein condensate trapped in
an optical lattice. Modeling the system as a Bose-Hubbard model, we show how
applying a periodic driving field can induce coherent destruction of tunneling.
In the low-frequency regime, we obtain the novel result that the destruction of
tunneling displays extremely sharp peaks when the driving frequency is resonant
with the depth of the trapping potential (``multi-photon resonances''), which
allows the quantum phase transition between the Mott insulator and the
superfluid state to be controlled with high precision. We further show how the
waveform of the field can be chosen to maximize this effect.Comment: Minor changes, this version to be published in Phys. Rev. Let
From Growth Spurts to Sustained Growth: The Nature of Growth and Unified Growth Theory
The recent literature on unified growth theory has shed new light on the transition to sustained economic growth. Nevertheless, unified growth theory has not devoted a lot of attention to the nature of economic growth and its impact in the transition from Malthus to Solow. This research presents new evidence on the existence of pre-industrial growth spurts and provides new foundations concerning the nature of economic growth during the Malthus to Solow transition. Following previous research in unified growth theory, sustained economic growth arises due to complementarities between the triple engines of growth of technological development, human capital and the organization of the workplace. In this research, growth spurts are an intrinsic feature of the economy, but throughout history their effect on standards of living is mostly temporary. The rise in living standards only becomes sustained when the complementarity of the triple engines of growth emerges. In Malthusian economies, most technologies were basic and only require straightforward knowledge or human capital, and thus the skill-technology complementarity did not play a role in their development. As a consequence, most technological developments in Malthusian economies generated growth spurts that did not become sustained, although there was a temporary increase in standards of living. However, the increasing complexity of the epistemic knowledge base reported by the historical literature meant that investments in applied technology were progressively more significant, enhancing the role of human capital. After a certain threshold of the knowledge base was surpassed, more and more complex applied technologies were developed, and growth spurts became permanent features of the economy. This research thus captures some of the most important historical features concerning the nature of growth in the transition to sustained economic growth.growth spurts, unified growth theory, sustained economic growth
Update of membership and mean proper motion of open clusters from UCAC5 catalog
We present mean proper motions and membership probabilities of individual
stars for optically visible open clusters, which have been determined using
data from the UCAC5 catalog. This follows our previous studies with the UCAC2
and UCAC4 catalogs, but now using improved proper motions in the GAIA reference
frame. In the present study results were obtained for a sample of 1108 open
clusters. For five clusters, this is the first determination of mean proper
motion, and for the whole sample, we present results with a much larger number
of identified astrometric member stars than on previous studies. It is the last
update of our Open cluster Catalog based on proper motion data only. Future
updates will count on astrometric, photometric and spectroscopic GAIA data as
input for analyses.Comment: 7 pages, 3 figures, 2 tables, 4 equations; accepted for publication
in 2018 May 25 in the MNRA
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