A climate terrorism assemblage? Exploring the politics of climate change-terrorism-radicalisation relations

Despite a series of claims from Bernie Sanders (2015), Barack Obama (2015), and others arguing that climate change, radicalisation, and terrorism are connected by complex causal relationships, there is very little academic examination of the politics of these claims. Building on DeLanda's (2006) account of assemblages and social complexity, this paper conceptualises climate change-terrorism-radicalisation relationships as a 'climate terrorism assemblage'. A 'climate terrorism assemblage' is a complex, emergent 'whole' formed from a heterogeneous range of interacting geopolitical components (e.g. climatic factors, migration, think tanks and academic publications, and a discourse of 'climate security'). Specifically, a climate terrorism assemblage is characterised by 'strategic territorialisations': context-specific, multi-scalar points at which political claims of causal links between climate change, terrorism, and radicalisation are crystallised. Strategic territorialisations are produced in two, interrelated contexts. First, using the case study of the Syrian Conflict, a climate terrorism assemblage reveals an intricate, contested politics of ‘drawing lines’ which link climate change, terrorism, and radicalisation. Secondly, the paper argues that, at the points at which causal links are constructed between climate change, terrorism and radicalisation, a climate terrorism assemblage territorialises around intersectional subject formations, in particular a young masculine subject vulnerable to potential radicalisation and terrorism. Overall, the paper concludes that a climate terrorism assemblage provides a productive analytic frame to investigate the contested power relations of climate change-radicalisation-terrorism connections

Star Clusters in Virgo and Fornax Dwarf Irregular Galaxies

We present the results of a search for clusters in dwarf irregular galaxies in the Virgo and Fornax Cluster using HST WFPC2 snapshot data. The galaxy sample includes 28 galaxies, 11 of which are confirmed members of the Virgo and Fornax clusters. In the 11 confirmed members, we detect 237 cluster candidates and determine their V magnitudes, V-I colors and core radii. After statistical subtraction of background galaxies and foreground stars, most of the cluster candidates have V-I colors of -0.2 and 1.4, V magnitudes lying between 20 and 25th magnitude and core radii between 0 and 6 pc. Using H-alpha observations, we find that 26% of the blue cluster candidates are most likely HII regions. The rest of the cluster candidates are most likely massive (>10^4 Msol) young and old clusters. A comparison between the red cluster candidates in our sample and the Milky Way globular clusters shows that they have similar luminosity distributions, but that the red cluster candidates typically have larger core radii. Assuming that the red cluster candidates are in fact globular clusters, we derive specific frequencies (S_N) ranging from ~0-9 for the galaxies. Although the values are uncertain, seven of the galaxies appear to have specific frequencies greater than 2. These values are more typical of ellipticals and nucleated dwarf ellipticals than they are of spirals or Local Group dwarf irregulars.Comment: 46 pages, 14 figures, 3 tables, accepted by AJ. Higher quality PS version of entire paper available at http://www.astro.washington.edu/seth/dirr_gcs.htm

Sensitivity of the superconducting state in thin films

For more than two decades, there have been reports on an unexpected metallic state separating the established superconducting and insulating phases of thin-film superconductors. To date, no theoretical explanation has been able to fully capture the existence of such a state for the large variety of superconductors exhibiting it. Here, we show that for two very different thin-film superconductors, amorphous indium oxide and a single crystal of 2H-NbSe2, this metallic state can be eliminated by adequately filtering external radiation. Our results show that the appearance of temperature-independent, metallic-like transport at low temperatures is sufficiently described by the extreme sensitivity of these superconducting films to external perturbations. We relate this sensitivity to the theoretical observation that, in two dimensions, superconductivity is only marginally stable