Unilateral Humanitarian Intervention and International Law

Este artigo deve ser visto como uma tentativa de participação no debate actual sobre a legitimidade das intervenções humanitárias, através da análise dos desafios morais e legais postos pelas acções unilaterais. Em particular, o autor examina a sugestão de Hedley Bull de que se as intervenções unilaterais exprimirem a “vontade colectiva da sociedade internacional”, então não constituem nenhuma ameaça à ordem internacional. Para discutir devidamente esta observação, é necessário, ante de mais, considerar o significado da expressão, “vontade colectiva da sociedade internacional”. Deve reduzir-se esta vontade colectiva à autoridade das Nações Unidas? Ou existem outros locais de legitimização das intervenções humanitárias? Qualquer discussão sobre o papel da ONU no caso das intervenções humanitárias tem que incluir o tema do direito de veto dos membros permanentes do Conselho de Segurança. Está na altura de rever o direito de veto, limitando-o nos casos de emergências humanitárias? Estas são as questões discutidas pelo artigo

NMR implementation of Quantum Delayed-Choice Experiment

We report the first experimental demonstration of quantum delayed-choice experiment via nuclear magnetic resonance techniques. An ensemble of molecules each with two spin-1/2 nuclei are used as target and the ancilla qubits to perform the quantum circuit corresponding the delayed-choice setup. As expected in theory, our experiments clearly demonstrate the continuous morphing of the target qubit between particle-like and wave-like behaviors. The experimental visibility of the interference patterns shows good agreement with the theory.Comment: Revised text, more figures adde

A Flexible Bayesian Model for Studying Gene–Environment Interaction

An important follow-up step after genetic markers are found to be associated with a disease outcome is a more detailed analysis investigating how the implicated gene or chromosomal region and an established environment risk factor interact to influence the disease risk. The standard approach to this study of gene–environment interaction considers one genetic marker at a time and therefore could misrepresent and underestimate the genetic contribution to the joint effect when one or more functional loci, some of which might not be genotyped, exist in the region and interact with the environment risk factor in a complex way. We develop a more global approach based on a Bayesian model that uses a latent genetic profile variable to capture all of the genetic variation in the entire targeted region and allows the environment effect to vary across different genetic profile categories. We also propose a resampling-based test derived from the developed Bayesian model for the detection of gene–environment interaction. Using data collected in the Environment and Genetics in Lung Cancer Etiology (EAGLE) study, we apply the Bayesian model to evaluate the joint effect of smoking intensity and genetic variants in the 15q25.1 region, which contains a cluster of nicotinic acetylcholine receptor genes and has been shown to be associated with both lung cancer and smoking behavior. We find evidence for gene–environment interaction (P-value = 0.016), with the smoking effect appearing to be stronger in subjects with a genetic profile associated with a higher lung cancer risk; the conventional test of gene–environment interaction based on the single-marker approach is far from significant

Hubble Space Telescope Spectroscopic Observations of the Ejecta of SN 1987A at 2000 Days

We have used the Faint Object Spectrograph on the Hubble Space Telescope to observe the spectra of SN 1987A over the wavelength range 2000 -- 8000\ \AA\ on dates 1862 and 2210 days after the supernova outburst. Even these pre-COSTAR observations avoid much of the contamination from the bright stars nearby and provide a very useful set of line strengths and shapes for analysis. The spectrum is formed in an unusual physical setting: cold gas which is excited and ionized by energetic electrons from the radioactive debris of the supernova explosion. The spectra of SN 1987A at this phase are surprisingly similar to those of the nova shells of CP Puppis and T Pyxidis decades after outburst. SN 1987A and the novae are characterized by emission from material with electron temperatures of only a few hundred degrees Kelvin, and show narrow Balmer continuum emission and strong emission lines from O$^+$. The Balmer continuum shape requires the electron temperature in the supernova ejecta to be as low as 500 K on day 1862 and 400 K on day 2210 after outburst. The \OIIUV\ doublet is surprisingly strong and is plausibly powered by collisional ionization of neutral oxygen to excited states of O$^+$. The line intensity ratio of the \OID\ doublet obtained from Gaussian fits of the line profiles is 1.8$\pm0.2$, contrary to the optically thin limit of 3. This ratio is {\it not} due to an optical depth effect, but rather is an artifact of assuming a Gaussian profile to fit the \OID\ doublet profile. Specifying the line ratio $R\, = \, F([{\rm OI}]6300)/F([{\rm OI}]6364)$ = 3 is consistent with the data and allows a calculation of the decomposed line profile. All the observed strong lines are found to be blueshifted by a similar amountComment: 26 pages, 8 Postcript figures availlable at ftp://tycho.as.utexas.edu/pub/users/lwang/SN87ASIN