9,797 research outputs found
A Method to Separate Stochastic and Deterministic Information from Electrocardiograms
In this work we present a new idea to develop a method to separate stochastic
and deterministic information contained in an electrocardiogram, ECG, which may
provide new sources of information with diagnostic purposes. We assume that the
ECG has information corresponding to many different processes related with the
cardiac activity as well as contamination from different sources related with
the measurement procedure and the nature of the observed system itself. The
method starts with the application of an improuved archetypal analysis to
separate the mentioned stochastic and deterministic information. From the
stochastic point of view we analyze Renyi entropies, and with respect to the
deterministic perspective we calculate the autocorrelation function and the
corresponding correlation time. We show that healthy and pathologic information
may be stochastic and/or deterministic, can be identified by different measures
and located in different parts of the ECG.Comment: 4 pages, 6 figure
Primordial black hole evolution in two-fluid cosmology
Several processes in the early universe might lead to the formation of
primordial black holes with different masses. These black holes would interact
with the cosmic plasma through accretion and emission processes. Such
interactions might have affected the dynamics of the universe and generated a
considerable amount of entropy. In this paper we investigate the effects of the
presence of primordial black holes on the evolution of the early universe. We
adopt a two-fluid cosmological model with radiation and a primordial black hole
gas. The latter is modelled with different initial mass functions taking into
account the available constraints over the initial primordial black hole
abundances. We find that certain populations with narrow initial mass functions
are capable to produce significant changes in the scale factor and the entropy.Comment: 8 pages, 7 figures. Modified to match the published versio
Probing the ZZgamma and Zgammagamma Couplings Through the Process e+e- --> nu anti-nu gamma
We study the sensitivity for testing the anomalous triple gauge couplings
and via the process
at high energy linear colliders. For integrated luminosities of 500
and center of mass energies between 0.5 and 1.5 , we find that this
process can provide tests of the triple neutral gauge boson couplings of order
, one order of magnitude lower than the standard model prediction.Comment: 12 pages, 6 figure
The influence of massive stars in the interstellar medium of IC 1613: the supernova remnant S8 and the nebula S3 associated with a WO star
We present a detailed kinematical analysis of two selected nebulae in the
Local Group irregular galaxy IC 1613. The nebulae are: S8, the only known
supernova remnant in this galaxy, and S3, a Wolf-Rayet nebula associated with
the only WO star in this galaxy. For S8, we have obtained and analyzed its
radial velocity field, where we found complex profiles which can be fitted by
several velocity components. These profiles also show the presence of high
velocity, low density gas. From this, we have obtained the expansion velocity,
estimated the preshock density and calculated the basic kinematical parameters
of this SNR. We suggest that in S8 we are seing a SNR partially hidden by dust.
This suggestion comes from the fact that the SNR is located between two
superbubbles where a ridge of obscured material unveils the existence of dust.
Moreover, we show that this hypothesis prevails when energetic arguments are
taken into account. In the case of S3, this nebula shows bipolar structure. By
means of its kinematics, we have analyzed its two lobes, the ``waist'', as well
as its relation with the nearest superbubbles. For the first time we are able
to see closed the NW lobe, showing a clover leaf shape. This fact allows a
better quantitative knowledge of the nebula as a whole. Furthermore, we found
evidence of an expansion motion in the NW lobe. In the light of our results, we
can express that these nebulae are the product of very massive stellar
evolution. It is surprising the influence these stars still have in shaping
their surrounding gas, and on the energy liberation towards the interstellar
medium of this galaxy.Comment: Accepted for publication in the Astronomical Journal, July issue. 11
pages, 12 figures. High resolution figures can be found at
http://www.inaoep.mx/~mago/PAPERS/AJ
Soportes epigráficos de los Orgenomescos
Se presenta un ensayo multidisciplinar con el que se pretende arrojar luz sobre la epigrafÃa cántabra, mediante la recopilación y estudio, en este caso, de las inscripciones del pueblo de los orgenomescos. El principal objetivo de este trabajo es el análisis de los soportes epigráficos utilizados por los indÃgenas y su evolución durante la dominación romana mediante el análisis de las 16 inscripciones conocidas, halladas en las actuales provincias de Cantabria, Asturias, Palencia y Jaén. Se distingue una sociedad indÃgena mixta que presenta un mestizaje entre el mundo prerromano y romano con fuertes pervivencias en sus tradiciones, resultado de un proceso de aculturación e integración onomástica y social.This multidisciplinary essay aims to shed light on the Cantabrian epigraphy, by collecting and studying, in this case, the Orgenomesci people. The main goal of this research are the epigraphic supports used by the natives and their evolution during the roman dominion, by the study of the 16 epigraphic steles and inscriptions found in the actual provinces of Cantabria, Asturias, Palencia and Jaén. Hence, we can perceive a mixted native society with miscegenation between the preroman and roman world, alongside the survival of strong traditions, consequence of an acculturization process, onomastic and social integration
Bose-Einstein Condensate Driven by a Kicked Rotor in a Finite Box
We study the effect of different heating rates of a dilute Bose gas confined
in a quasi-1D finite, leaky box. An optical kicked-rotor is used to transfer
energy to the atoms while two repulsive optical beams are used to confine the
atoms. The average energy of the atoms is localized after a large number of
kicks and the system reaches a nonequilibrium steady state. A numerical
simulation of the experimental data suggests that the localization is due to
energetic atoms leaking over the barrier. Our data also indicates a correlation
between collisions and the destruction of the Bose-Einstein condensate
fraction.Comment: 7 pages, 8 figure
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