Mass- Radius Relation for Magnetized Strange Quarks Stars

We review the stability of magnetized strange quark matter (MSQM) within the phenomenological MIT bag model, taking into account the variation of the relevant input parameters, namely, the strange quark mass, baryon density, magnetic field and bag parameter. A comparison with magnetized asymmetric quark matter in beta-equilibrium as well as with strange quark matter (SQM) is presented. We obtain that the energy per baryon for MSQM decreases as the magnetic field increases, and its minimum value at vanishing pressure is lower than the value found for SQM, which implies that MSQM is more stable than non-magnetized SQM. The mass-radius relation for magnetized strange quark stars is also obtained in this framework.

Desenvolvimento de materiais poliméricos resistentes à radiação UV: determinação quantitativa de estabilizadores à radiação UV

A presente tese teve por objectivo principal o desenvolvimento de métodos que permitissem quantificar alguns aditivos HALS (Hindered Amine Ligth Stabilizers - Aminas Estericamente Impedidas Estabilizadoras à luz), tais como, Tinuvin 622®, Chimassorb 944® e Chimassorb 2020® presentes em amostras de corda sintética. Os métodos de quantificação compreenderam a hidrólise básica para o Tinuvin 622® e a hidrólise ácida para ambos os Chimassorbs, e a separação e identificação por HPLC-MS/MS dos produtos da mesma. Procedendo à realização do método com o respectivo padrão de cada aditivo foi possível obter-se uma curva de calibração para o Tinuvin 622® (y = 899733 X - 96173; r = 0,9979) e para o Chimassorb 944® (y = 44177 X - 18248; r = 0,9965). Relativamente ao Chimassorb 2020® foram realizados alguns ensaios preliminares fundamentais para o desenvolvimento de um método de quantificação para este aditivo. Para o Tinuvin 622® foram realizados ainda ensaios de forma a desenvolver-se um método em que a quantificação ocorresse exclusivamente pela separação do hidrolisado no HPLC com detector UV. Dado que o Tinuvin 622® não apresenta absorção no UV optou-se por realizar a derivatização fluorescente deste através da esterificação com PyCOOH (ácido pirenobutírico) em meio ácido. Nas amostras de corda foram realizados ensaios de envelhecimento e tracção, ensaios de brilho, ensaios de absorção, bem como a quantificação do Tinuvin 622® nas cordas com e sem tratamento de irradiação (envelhecimento). Comprovou-se que as amostras de corda contêm cerca de 0,2% de Tinuvin 622® e que a corda preta não contém aditivo HALS. Verificou-se que em cordas sujeitas à radiação UV, a tensão de ruptura é influenciada pela quantidade de Tinuvin 622® e que esta por sua vez depende do tempo de exposição a que a corda foi sujeita. Por outro lado, concluiu-se que a cor (pigmentos) e o brilho não apresentam influência significativa na resistência das cordas quando expostas à radiação UV.

Compact Stars and Magnetized CFL Matter

The stability of the color flavor locked phase in the presence of a strong magnetic field is investigated within the phenomenological MIT bag model. It is found that the minimum value of the energy per baryon in a color flavor locked state at vanishing pressure is lower than the corresponding one for unpaired magnetized strange quark matter and, as the magnetic field increases, the energy per baryon decreases. This implies that magnetized color flavor locked matter is more stable and could become the ground state inside neutron stars. The anisotropy of the pressures is discussed. The mass-radius relation for such stars is also studied.

Magnetized color flavor locked state and compact stars

The stability of the color flavor locked phase in the presence of a strong magnetic field is investigated within the phenomenological MIT bag model, taking into account the variation of the strange quark mass, the baryon density, the magnetic field, as well as the bag and gap parameters. It is found that the minimum value of the energy per baryon in a color flavor locked state at vanishing pressure is lower than the corresponding one for unpaired magnetized strange quark matter and, as the magnetic field increases, the energy per baryon decreases. This implies that magnetized colorflavor locked matter is more stable and could become the ground state inside neutron stars. The mass-radius relation for such stars is also studied.

Tunnig optical A-Sic/A-Si active filters by UV bias light in the visible and infrared spectral ranges

Visible range to telecom band spectral translation is accomplished using an amorphous SiC pi'n/pin wavelength selector under appropriate front and back optical light bias. Results show that background intensity works as selectors in the infrared region, shifting the sensor sensitivity. Low intensities select the near-infrared range while high intensities select the visible part according to its wavelength. Here, the optical gain is very high in the infrared/red range, decreases in the green range, stays close to one in the blue region and strongly decreases in the near-UV range. The transfer characteristics effects due to changes in steady state light intensity and wavelength backgrounds are presented. The relationship between the optical inputs and the output signal is established. A capacitive optoelectronic model is presented and tested using the experimental results. © 2014 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.

UV-Vis spectroscopic study preferential solvation and intermolecular interactions in methanol/1-propanol/acetonitrile by means of solvatochromic probes

Solvatochromic UV-Vis shifts of four indicators (4-nitroaniline, 4-nitroanisole, 4-nitrophenol and N,N-dimethy-1-4-nitro aniline) have been measured at 298.15 K in the ternary mixture methano1/1-propanol/acetonitrile (MeOH/1-PrOH/MeCN) in a total of 22 mole fractions, along with 18 additional mole fractions for each of the corresponding binary mixtures, MeOH/1-PrOH, 1-PrOH/MeCN and MeOH/MeCN. These values, combined with our previous experimental results for 2,6-dipheny1-4-(2,4,6-triphenylpyridinium-1-yl)phenolate (Reichardt's betaine dye) in the same mixtures, permitted the computation of the Kamlet-Taft solvent parameters, alpha, beta, and pi*. The rationalization of the spectroscopic behavior of each probe within each mixture's whole mole fraction range was achieved through the use of the Bosch and Roses preferential solvation model. The applied model allowed the identification of synergistic behaviors in MeCN/alcohol mixtures and thus to infer the existence of solvent complexes in solution. Also, the addition of small amounts of MeCN to the binary mixtures was seen to cause a significant variation in pi*, whereas the addition of alcohol to MeCN mixtures always lead to a sudden change in a and The behavior of these parameters in the ternary mixture was shown to be mainly determined by the contributions of the underlying binary mixtures. (C) 2014 Elsevier B.V. All rights reserved.

Rising stars: da ESTeSL para o mundo da radiologia

Serão apresentadas duas experiências que estudantes de radiologia da ESTeSL tiveram no estrangeiro: a experiência que as estudantes tiveram no seu ERASMUS em Viena de Áustria no 2º semestre de 2014/15 e o decorrer da Summer School OPTIMAX2015, em que as estudantes participaram em agosto de 2015, em Groningen, nos Países Baixos. Falar-se-á um pouco sobre os estudos em radiologia. Discutir-se-ão os desafios que são habitualmente apresentados a um estudante aquando da realização do seu artigo final de investigação, como se podem prevenir e ultrapassar esses obstáculos e construir um artigo científico de qualidade.