Investigacion acerca de las instituciones consagradas en la ley 20.406 de fecha 05-12-2009 a partir de la historia de su establecimiento

35 p. La siguiente tesis no es autorizada por el autor para su difusión en formato digitalPara la obtención de los recursos económicos de un país, sin duda alguna que los impuestos son una parte importante en la generación de estos. Con la ley 20.406, lo que se busca es una mayor acceso a la información bancaria de los contribuyentes con el objeto de evitar prácticas ilegales y evasivas, para esto se presento un proyecto de ley el cual después de una serie de modificaciones terminó convertido en los actuales artículos 62 y 62 bis de nuestro Código Tributario. El objetivo de este trabajo respecto a la creación de la ley, es conocer las modificaciones realizadas al proyecto y el porqué de estos tomando en consideración el respeto a las distintas garantías que poseen los contribuyentes./ ABSTRACT:To obtain the financial resources of a country, there is no doubt that taxes are an important part in generating these. Law 20,406 seeks greater access to bank information of taxpayers in order to prevent illegal and evasive practices, for this reason a bill was presented which, after a number of changes, became the current term items 62 and 62 bis of our Tax Code. The aim of this work, regarding the creation of law, is to assess changes made to the project and find out why these changes were made, taking into consideration the respect to the various garantees the taxpayers have

La Concentracion del Poder Economico. Libre Competencia y Ley Antimonopolio

52 p.Este trabajo pretende demostrar que el sistema o régimen antimonopolio en Chile, no prohíbe la concentración del poder económico, limitándose a controlar los abusos que se producen por el dominio de un poder de mercado o posición sobresaliente. Por esto, se sigue un estudio dogmático-jurídico, con el objeto de determinar los conceptos claves relacionados a la materia, sin dejar de lado lo que manifiesta la jurisprudencia, por ser ésta un pilar fundamental en el desarrollo de esta rama del derecho. Ante el problema propuesto y a lo largo de la exposición con que la estructura legislativa, efectivamente, no prohíbe la formación de posiciones dominantes (entre ellas el monopolio), sino que éstas, por el contrario, son protegidas, existiendo posiciones doctrinarias que aprueban la concentración, en razón a las externalidades positivas que esta posiciones puedan generar

Innovación y Emprendimiento en el Discurso Político Chileno

El objetivo de esta investigación es determinar el significado político que han adoptado las nociones de ‘innovación’ y ‘emprendimiento’ en las cuentas públicas presidenciales del 21 de mayo en Chile desde el año 1990 hasta 2016, con el fin de revelar tanto las construcciones discursivas asociadas a estos términos como la manera en que éstas se relacionan con las prácticas políticas a través del tiempo. Para lograrlo, se emplearon herramientas de la lingüística de corpus para realizar el análisis del discurso político. Los resultados arrojaron que tanto ‘innovación’ como ‘emprendimiento’ son conceptos que están asociados a aspectos económicos. Además, mientras el primero se comienza a usar de manera sistemática en los discursos del primer gobierno de Michelle Bachelet, el segundo es empleado principalmente en los discursos de Sebastián Piñera. En cuanto a los ámbitos temáticos, ‘innovación’ se entiende, en mayor medida, como un concepto esencial en el desarrollo productivo del país y ‘emprendimiento’ se entiende como un trabajo en sí

Formation of H2\text{H}_{2} on polycyclic aromatic hydrocarbons under conditions of the ISM: an ab initio molecular dynamics study

Understanding how the $\mathrm{H}_2$ molecule is formed under the chemical conditions of the interstellar media (ISM) is critical to the whole chemistry of it. Formation of $\mathrm{H}_2$ in the ISM requires a third body acting as a reservoir of energy. Polycyclic aromatic hydrocarbons (PAH's) are excellent candidates to play that role. In this work we simulated the collisions of hydrogen atoms with coronene to form $\mathrm{H}_2$ via the Eley-Rideal mechanism. To do so, we used Born-Oppenheimer (ab initio) Molecular Dynamics simulations. Our results show that that adsorption of H atoms and subsequent release of $\mathrm{H}_2$ readily happen on coronene for H atoms with kinetic energy as large as 1 eV. Special attention is paid to dissipation and partition of the energy released in the reactions. The capacity of coronene to dissipate collision and reaction energies depends varies with the reaction site. Inner sites dissipate energy easier and faster than edge sites, thus evidencing an interplay between the potential energy surface around the reaction center and its ability to cool the projectile. As for the the recombination of H atoms and the subsequent formation of $\mathrm{H}_{2}$, it is observed that $\sim 15\%$ of the energy is dissipated by the coronene molecule as vibrational energy and the remaining energy is carried by $\mathrm{H}_{2}$. The $\mathrm{H}_{2}$ molecules desorb from coronene with an excited vibrational state ($\upsilon \geq 3$), a large amount of translational kinetic energy ($\geq$ 0.4 eV) and with a small activation of the rotational degree of freedom.Comment: Accepted in MNRA

Medidas multi-influencia como medio para caracterizar la firma global de un buque y proteger el entorno marino

The overall signature of a vessel comprises acoustic, magnetic, electric-field, pressure, and seismic radiations. Over the past years, the international community’s efforts have mainly centered on reducing the acoustic influence with the dual aim of decreasing the vessel’s detectability and reducing the levels of acoustic pollution generated in the marine environment. Nowadays, the need to act not only on the acoustic radiation but against the overall set of the vessel’s radiations is becoming increasingly clear, both in the military and the civilian fields, based on aspects like vessel stealthiness, security of harbor and critical infrastructures, and environmental protection. As a key element to achieve this goal, it is greatly important to have at our disposal highly modular and adaptable measurement systems covering the overall set of the vessel’s radiations, with a high capacity of data transmission to base centers to have the capacity to make measurements in all kinds of marine environments.La firma global de un buque está compuesta por radiaciones: acústica, magnética, de campo eléctrico, de presión y sísmica. A lo largo de los últimos años, los esfuerzos de la comunidad internacional se han centrado principalmente en reducir la influencia acústica, con el doble objetivo de disminuir la detectabilidad del buque y reducir el nivel de contaminación acústica generada en el entorno marino. En la actualidad, se está constatando con claridad la necesidad de actuar no sólo sobre la radiación acústica, sino sobre el conjunto global de las radiaciones del buque, tanto en el ámbito militar como en el ámbito civil, basado en aspectos como: la discreción de los buques, la seguridad en puertos e infraestructuras críticas y la protección ambiental. Como elemento clave para alcanzar esta meta, es de gran importancia tener a nuestra disposición sistemas de medida adaptables y altamente modulares que cubran el conjunto total de las radiaciones de los buques, con alta capacidad de transmisión de datos a centros base, con el objeto de tener la capacidad de realizar medidas en toda clase de entornos marinos

¿Cambia mucho el tamaño de grano obtenido mediante tamizado manual frente al mecánico?

Los procesos erosivos en el litoral, junto con la importancia económica del turismo (Houston, 2008), hacen que las realimentaciones periódicas de nuestras playas sean sumamente frecuentes. Y el tamaño de la arena es uno de los más importantes parámetros a la hora proyectar este tipo de obras. La media o la desviación típica del tamaño de grano son imprescindibles para comprobar si la arena de préstamo (terrestre o sumergida) es adecuada para sustituir a la transportada previamente por el mar (Pranzini et al., 2018). Además, el conocimiento de la distribución granulométrica del sedimento hace posible prever la reacción del perfil transversal ante una tormenta (Larson y Kraus, 1991), o calcular la cantidad necesaria de arena para abordar una regeneración (USACE, 2002). Por otra parte, a la hora de tomar decisiones sobre la zona de vertido de una cántara llena de arena, el gestor precisa conocer los parámetros antes mencionados de manera casi inmediata. Eso significa que los análisis del sedimento deben efectuarse a bordo de la draga, mientras se desplaza de la zona de préstamo hacia la costa a regenerar. Sin embargo, debido a la habitual escasez de espacio, a la ausencia de un laboratorio adecuado y al no siempre fiable suministro eléctrico, los tamizados deben hacerse a mano. Ya se ha estudiado la influencia del tiempo de tamizado a la hora de analizar la distribución granulométrica de una arena de playa o de duna (Roman-Sierra et al., 2013). Sin embargo, hasta este momento no se ha analizado la posible diferencia en la media y la desviación típica de una arena tamizada de manera manual a bordo de una draga frente a una tamizadora mecánica en un laboratorio en tierra. Asímismo, para ahorrar espacio y esfuerzo físico, a bordo de la draga suelen usarse tamices de 10 cm de diámetro frente a los más habituales de 20 cm en laboratorio. Para dar respuesta a estas preguntas, se aprovechó una regeneración efectuada en Cádiz en el año 2017 para efectuar una serie de pruebas a bordo de la draga Njord. Los extrapolables y más que útiles resultados, así como la influencia y consecuencias que tienen las diferencias observadas en la dirección de obras de regeneración de playas, se expondrán durante la presentación oral

QUIJOTE scientific results - IV. A northern sky survey in intensity and polarization at 10-20-GHz with the multifrequency instrument

We present QUIJOTE intensity and polarization maps in four frequency bands centred around 11, 13, 17, and 19-GHz, and covering approximately 29?000?deg2, including most of the northern sky region. These maps result from 9000?h of observations taken between May 2013 and June 2018 with the first QUIJOTE multifrequency instrument (MFI), and have angular resolutions of around 1°, and sensitivities in polarization within the range 35?40?µK per 1° beam, being a factor ?2?4 worse in intensity. We discuss the data processing pipeline employed, and the basic characteristics of the maps in terms of real space statistics and angular power spectra. A number of validation tests have been applied to characterize the accuracy of the calibration and the residual level of systematic effects, finding a conservative overall calibration uncertainty of 5 per?cent. We also discuss flux densities for four bright celestial sources (Tau A, Cas A, Cyg A, and 3C274), which are often used as calibrators at microwave frequencies. The polarization signal in our maps is dominated by synchrotron emission. The distribution of spectral index values between the 11?GHz and WMAP 23?GHz map peaks at [Beta] = -3.09 with a standard deviation of 0.14. The measured BB/EE ratio at scales of [L lower case+ = 80 is 0.26 ± 0.07 for a Galactic cut |b| > 10°. We find a positive TE correlation for 11?GHz at large angular scales ([L lower case+ [less than or equivalent to] 50), while the EB and TB signals are consistent with zero in the multipole range 30 [less than or equivalent to] [L lower case+ [less than or equivalent to] 150. The maps discussed in this paper are publicly available.We thank the staff of the Teide Observatory for invaluable assistance in the commissioning and operation of QUIJOTE. The QUIJOTE experiment is being developed by the Instituto de Astrofisica de Canarias (IAC), the Instituto de Fisica de Cantabria (IFCA), and the Universities of Cantabria, Manchester and Cambridge. Partial finan- cial support was provided by the Spanish Ministry of Science and Innovation under the projects AYA2007-68058-C03-01, AYA2007- 68058-C03-02, AYA2010-21766-C03-01, AYA2010-21766-C03-02, AYA2014-60438-P, ESP2015-70646-C2-1-R, AYA2017-84185-P, ESP2017-83921-C2-1-R, AYA2017-90675-REDC (co-funded with EU FEDER funds), PGC2018-101814-B-I00, PID2019-110610RB- C21, PID2020-120514GB-I00, IACA13-3E-2336, IACA15-BE- 3707, EQC2018-004918-P, the Severo Ochoa Programs SEV-2015- 0548 and CEX2019-000920-S, the Maria de Maeztu Program MDM- 2017-0765, and by the Consolider-Ingenio project CSD2010-00064 (EPI: Exploring the Physics of Inflation). We acknowledge support from the ACIISI, Consejeria de Economia, Conocimiento y Empleo del Gobierno de Canarias and the European Regional Development Fund (ERDF) under grant with reference ProID2020010108. This project has received funding from the European Union’s Horizon 2020 - Research and Innovation Framework Programme under grant agreement number 687312 (RADIOFOREGROUNDS). This research made use of computing time available on the high-performance computing systems at the IAC. We thankfully acknowledge the technical expertise and assistance provided by the Spanish Supercomputing Network (Red Espa ˜ nola de Supercom- putaci ´on), as well as the computer resources used: the Deimos/Di v a Supercomputer, located at the IAC. This research used resources of the National Energy Research Scientific Computing Center, which is supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. The PWV data used in the tests presented in Section 4 comes from the Iza ˜ na Atmospheric Observatory (IZO), and have been made available to us by the Iza ˜ na Atmospheric Research Center (AEMET). SEH and CD acknowledge support from the STFC Consolidated Grant (ST/P000649/1). FP acknowledges support from the Spanish State Research Agency (AEI) under grant number PID2019-105552RB- C43. DT acknowledges the support from the Chinese Academy of Sciences (CAS) President’s International Fellowship Initiative (PIFI) with Grant N. 2020PM0042. Some of the presented results are based on observations obtained with Planck ( http:// www.esa.int/ Planck), an ESA science mission with instruments and contributions directly funded by ESA Member States, NASA, and Canada. We acknowl- edge the use of the Le gac y Archiv e for Microwav e Background Data Analysis (LAMBDA). Support for LAMBDA is provided by the NASA Office of Space Science. Some of the results in this paper have been derived using the HEALPIX (G ´orski et al. 2005 ) and HEALPY (Zonca et al. 2019 ) packages. We also use Numpy (Harris et al. 2020 ), Matplotlib (Hunter 2007 ), and the SKLEARN module (Pedregosa et al. 2011 )

Pain neuroscience education in patients with chronic musculoskeletal pain: an umbrella review

IntroductionIn recent years, pain neuroscience education (PNE) has been the focus of extensive research in the scientific literature in the field of physical therapy, but the results obtained are controversial and its clinical application remains unclear. The main aim of this umbrella review was to assess the effectiveness of PNE in patients with chronic musculoskeletal pain (CMP).MethodsWe searched systematically in PubMed (Medline), PEDro, EMBASE, CINAHL and PsycINFO. Methodological quality was analyzed using AMSTAR-2 scale and overlapping analysis using GROOVE tool.Results16 systematic reviews were included. A qualitative synthesis was performed for the following sets of patients with CMP: overall CMP, chronic spinal pain, patients with fibromyalgia and patients with osteoarthritis. In general terms, it seems that the addition of the PNE-based intervention to other treatments, mostly exercise-based interventions although we might refer to it in terms of a multimodal approach, leads to greater clinical improvements than the multimodal approach alone. We have found this especially in the reduction of the influence of psychosocial variables. However, it seems that studies testing the effectiveness of PNE in isolation, systematic reviews with or without meta-analysis did not show statistically significant improvements overall in terms of pain intensity, disability levels or psychosocial variables.DiscussionThere is a great heterogeneity in the results obtained and the PNE protocols used, a critically low quality in the reviews included and a very high overlap, so there is a need to improve the studies in this field before clinical application.Systematic review registrationPROSPERO (CRD42022355634)

QUIJOTE scientific results - VIII. Diffuse polarized foregrounds from component separation with QUIJOTE-MFI

We derive linearly polarized astrophysical component maps in the Northern Sky from the QUIJOTE-MFI data at 11 and 13?GHz in combination with the Wilkinson Microwave Anisotropy Probe K and Ka bands (23 and 33?GHz) and all Planck polarized channels (30-353-GHz), using the parametric component separation method B-SeCRET. The addition of QUIJOTE-MFI data significantly improves the parameter estimation of the low-frequency foregrounds, especially the estimation of the synchrotron spectral index, [beta]s. We present the first detailed ?s map of the Northern Celestial Hemisphere at a smoothing scale of 2°. We find statistically significant spatial variability across the sky. We obtain an average value of ?3.08 and a dispersion of 0.13, considering only pixels with reliable goodness of fit. The power-law model of the synchrotron emission provides a good fit to the data outside the Galactic plane but fails to track the complexity within this region. Moreover, when we assume a synchrotron model with uniform curvature, cs, we find a value of cs = ?0.0797 ± 0.0012. However, there is insufficient statistical significance to determine which model is favoured, either the power law or the power law with uniform curvature. Furthermore, we estimate the thermal dust spectral parameters in polarization. Our cosmic microwave background, synchrotron, and thermal dust maps are highly correlated with the corresponding products of the PR4 Planck release, although some large-scale differences are observed in the synchrotron emission. Finally, we find that the ?s estimation in the high signal-to-noise synchrotron emission areas is prior-independent, while, outside these regions, the prior governs the [beta]s estimation.We thank the staff of the Teide Observatory for invaluable assistance in the commissioning and operation of QUIJOTE. The QUIJOTE experiment is being developed by the Instituto de Astrofisica de Canarias (IAC), the Instituto de Fisica de Cantabria (IFCA), and the Universities of Cantabria, Manchester, and Cambridge. Partial financial support was provided by the Spanish Ministry of Science and Innovation under the projects AYA2007-68058-C03-01, AYA2007- 68058-C03-02, AYA2010-21766-C03-01, AYA2010-21766-C03-02, AYA2014-60438-P, ESP2015-70646-C2-1-R, AYA2017-84185-P, ESP2017-83921-C2-1-R, AYA2017-90675-REDC (co-funded with EU FEDER funds), PGC2018-101814-B-I00, PID2019-110610RBC21, PID2020-120514GB-I00, IACA13-3E-2336, IACA15-BE3707, EQC2018-004918-P, the Severo Ochoa Programs SEV-2015- 0548 and CEX2019-000920-S, the Maria de Maeztu Program MDM2017-0765, and by the Consolider-Ingenio project CSD2010-00064 (EPI: Exploring the Physics of Inflation). We acknowledge support from the ACIISI, Consejeria de Economia, Conocimiento y Empleo del Gobierno de Canarias, and the European Regional Development Fund (ERDF) under grant with reference ProID2020010108. This project has received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement number 687312 (RADIOFOREGROUNDS). EdlH acknowledges financial support from the Concepcion´ Arenal Programme of the Universidad de Cantabria. DT acknowledges the support from the Chinese Academy of Sciences (CAS) President’s International Fellowship Initiative (PIFI) with grant no. 2020PM0042. FP acknowledges support from the Spanish State Research Agency (AEI) under grant number PID2019-105552RB-C43. The authors acknowledge the computer resources, technical expertise, and assistance provided by the Spanish Supercomputing Network (RES) node at Universidad de Cantabria. Some of the presented results are based on observations obtained with Planck (http://www.esa.int/Planck), an ESA science mission with instruments and contributions directly funded by ESA Member States, NASA, and Canada. We acknowledge the use of the Legacy Archive for Microwave Background Data Analysis (LAMBDA) and the Planck Legacy Archive (PLA). Support for LAMBDA is provided by the NASA Office of Space Science. Some of the results in this paper have been derived using the HEALPIX package (Gorski ´ et al. 2005), and the HEALPY (Zonca et al. 2019), NUMPY (Harris et al. 2020), EMCEE (ForemanMackey et al. 2013), and MATPLOTLIB (Hunter 2007) PYTHON packages

Detección y caracterización automáticas basadas en tratamiento digital de imágenes y redes neuronales de señales tonales emitidas por cetáceos

Se presenta un nuevo método para la detección y caracterización de señales tonales emitidas por cetáceos. Las señales son atuomáticamente detectadas a partir del espectrograma, aisladas mediante un proceso de segmentación basado en regiones, extraídas tras un proceso de resolución de cruces y caracterizadas automáticamente mediante un número fijo de coeficientes derivados de la aplicación de redes neuronales de funciones de base radial. Estos coeficientes pueden ser empelados para una posterior clasificación de las señales basada en sus características. Las presentaciones del método han sido extensivamente evaluadas a partir de señales simuladas y registros de grabaciones en la mar