Detecting the Transverse Proximity Effect: Radiative Feedback from QSOs

We present results of a search for absorbers close to QSOs near the line of sight of background quasars based on sensitive Keck/HIRES observations of the QSO triplet KP76, KP77, and KP78 (z=2.466, 2.535, and 2.615), with separations of 2-3 arcmin on the plane plane of the sky. Through the use of a high resolution spectra, together with accurate systemic redshifts of the QSOs using near-IR spectroscopy, we quantify the state of the IGM gas at the redshifts of the foreground QSOs. The inferred ionizing flux at the proper transverse distances probed is up to 100 times greater than the UV background. We show that the state of the gas has been significantly affected by the UV radiation from the foreground QSOs

Polytropic equation of state and primordial quantum fluctuations

We study the primordial Universe in a cosmological model where inflation is driven by a fluid with a polytropic equation of state $p = \alpha\rho + k\rho^{1 + 1/n}$. We calculate the dynamics of the scalar factor and build a Universe with constant density at the origin. We also find the equivalent scalar field that could create such equation of state and calculate the corresponding slow-roll parameters. We calculate the scalar perturbations, the scalar power spectrum and the spectral index.Comment: 16 pages, 4 figure

No-horizon theorem for spacetimes with spacelike G1 isometry groups

We consider four-dimensional spacetimes $(M,{\mathbf g})$ which obey the Einstein equations ${\mathbf G}={\mathbf T}$, and admit a global spacelike $G_{1}={\mathbb R}$ isometry group. By means of dimensional reduction and local analyis on the reduced (2+1) spacetime, we obtain a sufficient condition on ${\mathbf T}$ which guarantees that $(M,{\mathbf g})$ cannot contain apparent horizons. Given any (3+1) spacetime with spacelike translational isometry, the no-horizon condition can be readily tested without the need for dimensional reduction. This provides thus a useful and encompassing apparent horizon test for $G_{1}$-symmetric spacetimes. We argue that this adds further evidence towards the validity of the hoop conjecture, and signals possible violations of strong cosmic censorship.Comment: 8 pages, LaTeX, uses IOP package; published in Class. Quantum Gra

A note on the cylindrical collapse of counter-rotating dust

We find analytical solutions describing the collapse of an infinitely long cylindrical shell of counter-rotating dust. We show that--for the classes of solutions discussed herein--from regular initial data a curvature singularity inevitably develops, and no apparent horizons form, thus in accord with the spirit of the hoop conjecture.Comment: 8 pages, LaTeX, ijmpd macros (included), 1 eps figure; accepted for publication in Int. J. Mod. Phys.

Analgesia e Anestesia Obstétricas na Maternidade do Hospital D. Estefânia: Estudo Retrospectivo

Resumo: Por intermédio deste estudo, pretendeu-se verificar qual a realidade em termos de analgesia e anestesia obstétricas na Maternidade do Hospital D. Estefânia, ao longo de 4 anos. Para isso, foi realizado um estudo retrospectivo no período entre Janeiro de 2005 e Dezembro de 2008. Foram avaliados a classificação ASA das parturientes, o número total de partos, o número de parturientes submetidas a técnicas locorregionais e suas complicações, número de cesarianas e a necessidade de conversão de técnica regional para anestesia geral. No período do estudo, houve um total de 8291 partos, maioritariamente em mulheres ASA I, dos quais 2643 foram cesarianas. A maioria das parturientes (77%) foi submetida a uma técnica locorregional, para analgesia de trabalho de parto ou anestesia para cesariana, com baixa taxa de complicações (2,9%) e com rara necessidade de conversão para anestesia geral (3,5%). As autoras concluiram que, na Maternidade do Hospital D. Estefânia, a epidural continua a ser a técnica gold standard para analgesia do trabalho de parto, com raras complicações e permitindo a fácil conversão para anestesia para cesariana

Strong curvature singularities in quasispherical asymptotically de Sitter dust collapse

We study the occurrence, visibility, and curvature strength of singularities in dust-containing Szekeres spacetimes (which possess no Killing vectors) with a positive cosmological constant. We find that such singularities can be locally naked, Tipler strong, and develop from a non-zero-measure set of regular initial data. When examined along timelike geodesics, the singularity's curvature strength is found to be independent of the initial data.Comment: 16 pages, LaTeX, uses IOP package, 2 eps figures; accepted for publication in Class. Quantum Gra