Presio ultzeren agerpen arriskua: Iritzi klinikoa eta balorazio eskalen arteko konparaketa

Presio ultzerak osasun publikoaren arazo bat dira, asaldura fisiko, psikologiko, ekonomiko eta sozial asko eragiten dituztelako. Ultzerak tratatzeko hainbat modu ezagutzen dira, baina argi dago tratamendu onena prebentzioa dela. Haien agerpena saihesteko ezinbestekoa da ultzera bat pairatzeko arriskua baloratzea. Hau egiteko profesionalek iritzi edo epaiketa klinikoa erabili dezakete (haien esperientziaren bitartez ultzera begi bistaz baloratu) edo eskala protokolizatuak erabili ditzakete. Lan honetan, berrikuspen bibliografiko baten bitartez, gehien erabiltzen diren balorazio eskalei buruzko informazioa lortu da. Beste aldetik, iritzi klinikoaren eta balorazio eskalen eraginkortasun klinikoa konparatu da. Azkenik, eskalak euren artean konparatu dira, bakoitzaren ezaugarriak aztertuz. Eskala asko argitaratu egin dira denboran zehar baina gehien balioztatuak eta erabilienak bost dira: Braden, Norton, EMINA, Waterlow eta Cubbin-Jackson. Eskalen artean Braden eta Norton dira eraginkorrenak (hurrenez hurren), Waterlow postu baxuago batean geratuz. EMINA gutxiago erabiltzen da, baina bere eraginkortasuna Braden-en antzekoa da. Dena den, hau baieztatzeko ikerketa gehiago behar dira. Cubbin-Jackson oso eraginkorra da ere baina bere erabilpena paziente akutuetan bereizita dago. Eskalen harrera profesionalen partetik nahiko ona izan da. Haien erabilpena erraza dela diote gehienek, eta ia erdiek metodo hau erabiltzen dute arriskua baloratzeko. %20ak epaiketa eta eskalak batera erabiltzen dituzte, eskalei garrantzia handiena emanez. Frogatu izan da eskalek epaiketa klinikoarekin konparatuz sentsibilitate altuagoa daukatela, hau da, arriskuan dauden paziente kopuru gehiago detektatuko dituztela, nahiz eta bi metodoen efikazia antzekoa izan. Eskalek beraz, faktore gehiago kontuan hartu eta pazientea modu zehatzago batean aztertzen dute. Orokorrean esan daiteke eskalak eraginkorrak direla baina ikerketa gehiago behar dira balidazio sakonago bat egiteko.

Finding needles in the haystack : a search for AM CVn systems using the Palomar Transient Factory

The AM CVn systems are a rare class of ultra-compact astrophysical binaries. With orbital periods of under an hour and as short as five minutes, they are among the closest known binary star systems and their evolution has direct relevance to the type Ia supernova rate and the white dwarf binary population. However, their faint and rare nature has made population studies of these systems difficult and several studies have found conflicting results.

I undertook a survey for AM CVn systems using the Palomar Transient Factory (PTF) astrophysical synoptic survey by exploiting the "outbursts" these systems undergo. Such events result in an increase in luminosity by a factor of up to two-hundred and are detectable in time-domain photometric data of AM CVn systems. My search resulted in the discovery of eight new systems, over 20% of the current known population. More importantly, this search was done in a systematic fashion, which allows for a population study properly accounting for biases.

Apart from the discovery of new systems, I used the time-domain data from the PTF and other synoptic surveys to better understand the long-term behavior of these systems. This analysis of the photometric behavior of the majority of known AM CVn systems has shown changes in their behavior at longer time scales than have previously been observed. This has allowed me to find relationships between the outburst properties of an individual system and its orbital period.

Even more importantly, the systematically selected sample together with these properties have allowed me to conduct a population study of the AM CVn systems. I have shown that the latest published estimates of the AM CVn system population, a factor of fifty below theoretical estimates, are consistent with the sample of systems presented here. This is particularly noteworthy since my population study is most sensitive to a different orbital period regime than earlier surveys. This confirmation of the population density will allow the AM CVn systems population to be used in the study of other areas of astrophysics.

Sormena bost urtko gelan. Musika, mugimendua eta jolasa.

Ez da arraroa, egungo eskolan, nolabaiteko aukera eza aurkitzea Haur Hezkuntzako haurraren sormena garatzeko. Aukera eza honi erantzuna emateko asmoz sortu da proiektu hau. Hiru bitarteko nagusi uztartzea proposatzen da: alde batetik, musika, sormenaren garapenerako aukera anitz eskaintzen dituelako; bestetik, mugimendua, haurraren garapenen fisiko eta kognitiboan berebiziko garrantzia duen funtzioa; eta, azkenik, jolasa elementu integratzaile bezala, gizakiok haurtzaroan dugun oinarrizko jarduera. Ondoren proposatzen diren jolasak zehazki sortuak, aukeratuak eta moldatuak izan dira sormena era ludikoan garatzeko. Barakaldoko Alkartu Ikastola Publikoan praktikan jarri eta gero, esan dezakegu haurrek ia mugarik gabeko sormena garatu dezaketela, irakasleak bitarteko egokiak eskura jartzen badizkie.

Senezkotasuna hizkuntzan: Gramatika unibertsalaren inguruko gogoeta

Xabier Artiagoitia eta Joseba A. Lakarra (arg.)

Origin of Th/U variations in chondritic meteorites

Isotope dilution thorium and uranium analyses of the Harleton chondrite show a larger scatter than previously observed in equilibrated ordinary chondrites (EOC). The linear correlation of Th/U with 1/U in Harleton (and all EOC data) is produced by variation in the chlorapatite to merrillite mixing ratio. Apatite variations control the U concentrations. Phosphorus variations are compensated by inverse variations in U to preserve the Th/U vs. 1/U correlation. Because the Th/U variations reflect phosphate ampling, a weighted Th/U average should converge to an improved solar system Th/U. We obtain Th/U=3.53 (1_-mean=0.10), significantly lower and more precise than previous estimates.

To test whether apatite also produces Th/U variation in CI and CM chondrites, we performed P analyses on the solutions from leaching experiments of Orgueil and Murchison meteorites.

A linear Th/U vs. 1/U correlation in CI can be explained by redistribution of hexavalent U by aqueous fluids into carbonates and sulfates.

Unlike CI and EOC, whole rock Th/U variations in CMs are mostly due to Th variations. A Th/U vs. 1/U linear correlation suggested by previous data for CMs is not real. We distinguish 4 components responsible for the whole rock Th/U variations: (1) P and actinide-depleted matrix containing small amounts of U-rich carbonate/sulfate phases (similar to CIs); (2) CAIs and (3) chondrules are major reservoirs for actinides, (4) an easily leachable phase of high Th/U. likely carbonate produced by CAI alteration. Phosphates play a minor role as actinide and P carrier phases in CM chondrites.

Using our Th/U and minimum galactic ages from halo globular clusters, we calculate relative supernovae production rates for ²³²Th/²³⁸U and ²³⁵U/²³⁸U for different models of r-process nucleosynthesis. For uniform galactic production, the beginning of the r-process nucleosynthesis must be less than 13 Gyr. Exponentially decreasing production is also consistent with a 13 Gyr age, but very slow decay times are required (less than 35 Gyr), approaching the uniform production. The 15 Gyr Galaxy requires either a fast initial production growth (infall time constant less than 0.5 Gyr) followed by very low decrease (decay time constant greater than 100 Gyr), or the fastest possible decrease (≈8 Gyr) preceded by slow in fall (≈7.5 Gyr).

Análisis de la influencia de la orientación de las fibras metálicas en la resistencia de la matriz de hormigón de acuerdo al Ensayo Barcelona

[ES]El objetivo de este trabajo de fin de grado es analizar la influencia que tiene la cuantía y orientación de fibras metálicas presentes en el interior de probetas de hormigón autocompactante y cuyo objetivo es reforzar y aumentar la resistencia a tracción de este material. Se expondrán las propiedades que combina el HACRFA gracias a la autocompactación del hormigón y la inclusión de fibras en su interior y los beneficios que este nuevo material aporta. Por otro lado, se tratara de situar este estudio en un contexto, analizando a la vez cuál es el alcance y los objetivos más importantes que se han tenido en cuenta. A continuación, y a modo de complementación de su contexto, este trabajo tiene un estado del arte, en el que se mencionarán métodos y ensayos necesarios para llegar a un resultado que permita predecir cuál será la resistencia del material, y por tanto su tenacidad o capacidad de absorber energía, sin necesidad de emplear más que un método fácil y rápido, obviando el resto de ensayos destructivos utilizados en este trabajo. Para tal fin, se establece una metodología que, gracias a ensayos de laboratorio, permita establecer una relación entre el método sencillo que se ha mencionado, el método inductivo, y un resultado teórico de la tenacidad que presenta el HACRFA. Se observará cómo la desviación entre los ensayos experimentales y los resultados teóricos obtenidos es prácticamente nula, despreciando situaciones en las que se presenten comportamientos muy diferentes debido a fallos durante los ensayos.

The needle in the hundred square degree haystack: The hunt for binary neutron star mergers with LIGO and Palomar Transient Factory

The Advanced LIGO and Virgo experiments are poised to detect gravitational waves (GWs) directly for the first time this decade. The ultimate prize will be joint observation of a compact binary merger in both gravitational and electromagnetic channels. However, GW sky locations that are uncertain by hundreds of square degrees will pose a challenge. I describe a real-time detection pipeline and a rapid Bayesian parameter estimation code that will make it possible to search promptly for optical counterparts in Advanced LIGO. Having analyzed a comprehensive population of simulated GW sources, we describe the sky localization accuracy that the GW detector network will achieve as each detector comes online and progresses toward design sensitivity. Next, in preparation for the optical search with the intermediate Palomar Transient Factory (iPTF), we have developed a unique capability to detect optical afterglows of gamma-ray bursts (GRBs) detected by the Fermi Gamma-ray Burst Monitor (GBM). Its comparable error regions offer a close parallel to the Advanced LIGO problem, but Fermi's unique access to MeV-GeV photons and its near all-sky coverage may allow us to look at optical afterglows in a relatively unexplored part of the GRB parameter space. We present the discovery and broadband follow-up observations (X-ray, UV, optical, millimeter, and radio) of eight GBM-IPTF afterglows. Two of the bursts (GRB 130702A / iPTF13bxl and GRB 140606B / iPTF14bfu) are at low redshift (z=0.145 and z = 0.384, respectively), are sub-luminous with respect to "standard" cosmological bursts, and have spectroscopically confirmed broad-line type Ic supernovae. These two bursts are possibly consistent with mildly relativistic shocks breaking out from the progenitor envelopes rather than the standard mechanism of internal shocks within an ultra-relativistic jet. On a technical level, the GBM--IPTF effort is a prototype for locating and observing optical counterparts of GW events in Advanced LIGO with the Zwicky Transient Facility.

Avaliação tridimensional da via aérea superior de pacientes com apneia obstrutiva do sono que utilizaram aparelho de avanço mandibular

Os objetivos deste estudo foram avaliar o efeito do aparelho de avanço mandibular (Twin block - TB) no volume das vias aéreas superiores, por meio de tomografia computadorizada cone beam (CBCT); analisar, por meio da polissonografia, as mudanças no índice de apneia e hipopneia (IAH) e índice de apneia por hora de sono (IA), saturação de oxi-hemoglobina e eficiência do sono; e correlacionar o volume na CBCT e as polissonografias. Dezesseis pacientes portadores de apneia obstrutiva do sono, idade média de 47,06 anos, participaram deste estudo prospectivo, com acompanhamento médio de 7 meses. Foram feitas polissonografias iniciais (T1) e de acompanhamento (T2) com o TB em posição, e CBCT sem e com TB em posição. A segmentação e obtenção dos volumes das vias aéreas superiores foram realizadas e utilizados os testes t de Student pareado, de Wilcoxon e o índice de correlação de Spearman, com 5% de significância. Os resultados das polissonografias mostraram diferenças estatisticamente significativas entre T1 e T2 apenas para IAH (p<0,05). Houve aumento do volume da via aérea superior com TB quando comparado com o volume sem TB (p<0,05). Foi possível estabelecer-se correlação positiva entre volume da via aérea superior sem TB e IAH e IA em T1 (p<0,05), mas não houve correlação entre o volume da via aérea com TB e índices polissonográficos em T2. Pode-se concluir que, houve aumento de volume da via aérea superior com o TB e houve redução do IAH em T2 porém, sem correlação entre estes dados.

Exploring the Dynamic Radio Sky: The Search for Slow Transients with the VLA

While synoptic surveys in the optical and at high energies have revealed a rich discovery phase space of slow transients, a similar yield is still awaited in the radio. Majority of the past blind surveys, carried out with radio interferometers, have suffered from a low yield of slow transients, ambiguous transient classifications, and contamination by false positives. The newly-refurbished Karl G. Jansky Array (Jansky VLA) offers wider bandwidths for accurate RFI excision as well as substantially-improved sensitivity and survey speed compared with the old VLA. The Jansky VLA thus eliminates the pitfalls of interferometric transient search by facilitating sensitive, wide-field, and near-real-time radio surveys and enabling a systematic exploration of the dynamic radio sky. This thesis aims at carrying out blind Jansky VLA surveys for characterizing the radio variable and transient sources at frequencies of a few GHz and on timescales between days and years. Through joint radio and optical surveys, the thesis addresses outstanding questions pertaining to the rates of slow radio transients (e.g. radio supernovae, tidal disruption events, binary neutron star mergers, stellar flares, etc.), the false-positive foreground relevant for the radio and optical counterpart searches of gravitational wave sources, and the beaming factor of gamma-ray bursts. The need for rapid processing of the Jansky VLA data and near-real-time radio transient search has enabled the development of state-of-the-art software infrastructure. This thesis has successfully demonstrated the Jansky VLA as a powerful transient search instrument, and it serves as a pathfinder for the transient surveys planned for the SKA-mid pathfinder facilities, viz. ASKAP, MeerKAT, and WSRT/Apertif.

Solar System Small-Body Demographics with the Palomar Transient Factory Survey

Observational studies of our solar system's small-body populations (asteroids and comets) offer insight into the history of our planetary system, as these minor planets represent the left-over building blocks from its formation. The Palomar Transient Factory (PTF) survey began in 2009 as the latest wide-field sky-survey program to be conducted on the 1.2-meter Samuel Oschin telescope at Palomar Observatory. Though its main science program has been the discovery of high-energy extragalactic sources (such as supernovae), during its first five years PTF has collected nearly five million observations of over half a million unique solar system small bodies. This thesis begins to analyze this vast data set to address key population-level science topics, including: the detection rates of rare main-belt comets and small near-Earth asteroids, the spin and shape properties of asteroids as inferred from their lightcurves, the applicability of this visible light data to the interpretation of ultraviolet asteroid observations, and a comparison of the physical properties of main-belt and Jovian Trojan asteroids. Future sky-surveys would benefit from application of the analytical techniques presented herein, which include novel modeling methods and unique applications of machine-learning classification. The PTF asteroid small-body data produced in the course of this thesis work should remain a fertile source of solar system science and discovery for years to come.

A influência da linguagem para o raciocínio de crenças falsas em Teoria da Mente: uma análise em pacientes afásicos agramáticos

O termo Teoria da Mente diz respeito à habilidade que os seres humanos adquirem de compreender seus próprios estados mentais e os dos outros e predizer ações e comportamentos dentro de uma interação social. As principais questões da pesquisa em Teoria da Mente são: determinar qual o tipo de conhecimento que sustenta essa habilidade, qual sua origem e desenvolvimento e em que momento se manifesta. (Astington e Gopnik, 1991). Ao levar em consideração que a língua pode ser vista como instrumento da cognição (Spelke, 2003), através da qual o falante adquire suporte para o planejamento de ações, contribuindo para o desempenho de tarefas cognitivas complexas (Corrêa, 2006), de Villiers (2004, 2005, 2007 e subsequentes), no que diz respeito à Teoria da Mente, argumenta que o seu desenvolvimento depende do desenvolvimento linguístico, estando diretamente ligado à aquisição de verbos de estado mental, como pensar, por exemplo, pelo fato de que esses verbos subcategorizam uma sentença encaixada. Para ela, o domínio dessa estrutura possibilita que o raciocínio de crenças falsas da Teoria da Mente seja efetivamente realizado. A presente dissertação tem como objetivo verificar em que medida há uma influência direta e necessária da linguagem para a condução de tarefas de Teoria da Mente. Para tanto, focamos nossa atenção em pessoas que estão, por algum motivo, destituídas parcialmente da capacidade linguística, mas que mantêm intacta a capacidade cognitiva, os afásicos. Por meio de uma pesquisa realizada com dois pacientes afásicos de Broca, selecionados pelos critérios clássicos, procuramos entender se a habilidade de predizer ações está intacta nestes pacientes ou se tal habilidade foi perdida, assim como a linguagem. Para tanto, aplicamos dois testes de crença falsa em Teoria da Mente. O primeiro utilizou-se de suporte verbal, uma narração de eventos e expectativas dos personagens envolvidos. A pergunta-teste foi manipulada em função do grau de complexidade por meio do cruzamento de dois fatores: sentenças simples ou complexas e QU-in situ ou movido. O segundo teste seguiu o padrão não-verbal, sendo constituído de uma sequência de imagens, sendo que o sujeito deveria decidir entre duas últimas imagens apresentadas, aquela que coerentemente finalizava a história. Uma vez que houvesse influência direta da linguagem na condução de tarefas de Teoria da Mente, esperar-se-ia que a dificuldade no teste verbal refletisse o grau de complexidade das questões apresentadas. Adicionalmente, o desempenho no teste não-verbal também deveria ser insatisfatório, dado o comprometimento linguístico apresentado pelos sujeitos testados. Para o primeiro teste, o desempenho dos pacientes foi aleatório e inferior ao do grupo controle, já para o segundo teste, o aproveitamento foi de 100%. Em geral, os resultados sugerem que o raciocínio de crenças falsas em Teoria da Mente é alcançado por esses sujeitos, haja vista o desempenho plenamente satisfatório no teste não-verbal. Os resultados do teste verbal, por outro lado, atestam tão somente a dificuldade linguística característica dessa população. Desse modo, conclui-se que uma vez desenvolvida a habilidade em Teoria da Mente, esta permanece intacta na mente destes pacientes, mesmo que destituídos parcialmente da capacidade linguística

Bicyclo[3.2.0]hepta-1,4,6-triene: synthesis, thermal rearrangement, and anion formation

In order to determine the properties of the bicycloheptatrienyl anion (Ia) (predicted to be conjugatively stabilized by Hückel Molecular Orbital Theory) the neutral precursor, bicyclo[3. 2. 0] hepta-1, 4, 6-triene (I) was prepared by the following route.

Reaction of I with potassium-t-butoxide, potassium, or lithium dicyclohexylamide gave anion Ia in very low yield. Reprotonation of I was found to occur solely at the 1 or 5 position to give triene II, isolated as to its dimers.

A study of the acidity of I and of other conjugated hydrocarbons by means of ion cyclotron resonance spectroscopy resulted in determination of the following order of relative acidities:

H₂S ˃ C₅H₆ ˃ CH₃NO₂ ˃ 1, 4- C₅H₈ ˃ I ˃ C₂H₅OH ˃ H₂O; cyclo-C₇H₈ ˃ C₂ H₅OH; фCH₃ ˃ CH₃OH

In addition, limits for the proton affinities of the conjugate bases were determined:

350 kcal/mole ˂ PA(C₅ H₅^-) ˂ 360 kcal/mole

362 kcal/mole ˂ PA(C₅H₇^-, Ia, cyclo-C₇H₇^-) ˂ 377 kcal/mole PA(фCH₂^-) ˂ 385 kcal/mole

Gas phase kinetics of the trans-XVIII to I transformation gave the following activation parameters: E_a = 43.0 kcal/mole, log A = 15.53 and ∆S^ǂ (220°) = 9.6 cu. The results were interpreted as indicating initial 1,2 bond cleavage to give the 1,3-diradical which closed to I. Similar studies on cis-XVIII gave results consistent with a surface component to the reaction (E_a = 22.7 kcal/mole; log A = 9.23, ∆S^ǂ (119°) = -18.9 eu).

The low pressure (0.01 to 1 torr) pyrolysis of trans-XVIII gave in addition to I, fulvenallene (LV), ethynylcyclopentadiene (LVI) and heptafulvalene (LVII). The relative ratios of the C₇H₆ isomers were found to be dependent upon temperature and pressure, higher relative pressure and lower temperatures favoring formation of I. The results were found to be consistent with the intermediacy of vibrationally excited I and subsequent reaction to give LV and LVI.