The European Convention on Human Rights and the United Kingdom's Supreme Court

This article reviews the attitudes displayed by the UK's Supreme Court towards claims based on human rights law.

The International Protection of Refugees and Asylum Seekers: the Role of Article 3 of the European Convention on Human Rights

This book presents a comprehensive assessment of regional responses to the crisis in the asylum/refugee system and critically examines how different regions tackle the problem. The chapters consider the fundamental challenges which undermine an effective asylum process as well as regional difficulties with the various circumstances surrounding asylum seekers. With contributions on Africa, Europe, Latin America, South Asia and the Middle East, and the Pacific, the collection strives to appreciate what informs each region’s approach to the asylum process and asks if there are issues common to every region and if regions can learn from one another. The book seeks an understanding of the existing legal regime for the protection of asylum seekers and how regional institutions such as human rights commissions and regional courts enforce and adjudicate the law.

On the diversity of superluminous supernovae: ejected mass as the dominant factor

We assemble a sample of 24 hydrogen-poor superluminous supernovae(SLSNe). Parameterizing the light-curve shape through rise and declinetime-scales shows that the two are highly correlated. Magnetar-poweredmodels can reproduce the correlation, with the diversity in rise anddecline rates driven by the diffusion time-scale. Circumstellarinteraction models can exhibit a similar rise-decline relation, but onlyfor a narrow range of densities, which may be problematic for thesemodels. We find that SLSNe are approximately 3.5 mag brighter and havelight curves three times broader than SNe Ibc, but that the intrinsicshapes are similar. There are a number of SLSNe with particularly broadlight curves, possibly indicating two progenitor channels, butstatistical tests do not cleanly separate two populations. The generalspectral evolution is also presented. Velocities measured from Fe II aresimilar for SLSNe and SNe Ibc, suggesting that diffusion timedifferences are dominated by mass or opacity. Flat velocity evolution inmost SLSNe suggests a dense shell of ejecta. If opacities in SLSNe aresimilar to other SNe Ibc, the average ejected mass is higher by a factor2-3. Assuming κ = 0.1 cm2 g-1, we estimate amean (median) SLSN ejecta mass of 10 M⊙ (6M⊙), with a range of 3-30 M⊙. Doubling theassumed opacity brings the masses closer to normal SNe Ibc, but with ahigh-mass tail. The most probable mechanism for generating SLSNe seemsto be the core collapse of a very massive hydrogen-poor star, forming amillisecond magnetar.