Sociology, Science and Sustainability: Developing Relationships in Scotland

This paper considers the application of the sociological imagination during the analysis of data collected during an ethnographic study of an environmental regulator, the Scottish Environment Protection Agency (SEPA). SEPA is tasked with implementing the European Water Framework Directive (WFD) in Scotland, which will radically alter the regulation of water use. Applying a sociological imagination allowed the researcher to advocate for a more interdisciplinary and equitable understanding of sustainable water use when feeding back initial research results at the end of the data collection period. The researchers introduced socialised definitions of the environment, which linked social justice and ecological concerns. These insights provided a challenge to the traditional bio-physical science focus of the organisational participants, for whom sustainability is a relatively new addition to their duties. The paper concludes by discussing the importance of developing these interdisciplinary relationships in the future.Sociological Imagination, Water Framework Directive, Sustainability Science, Consumer-Citizens

On Spectral and Temporal Variability in Blazars and Gamma Ray Bursts

A simple model for variability in relativistic plasma outflows is studied, in which nonthermal electrons are continuously and uniformly injected in the comoving frame over a time interval dt. The evolution of the electron distribution is assumed to be dominated by synchrotron losses, and the energy- and time-dependence of the synchrotron and synchrotron self-Compton (SSC) fluxes are calculated for a power-law electron injection function with index s = 2. The mean time of a flare or pulse measured at photon energy E with respect to the onset of the injection event varies as E^{-1/2} and E^{-1/4} for synchrotron and SSC processes, respectively, until the time approaches the limiting intrinsic mean time (1+z)dt/(2 D), where z is the redshift and D is the Doppler factor. This dependence is in accord with recent analyses of blazar and GRB emissions, and suggests a method to discriminate between external Compton and SSC models of high-energy gamma radiation from blazars and GRBs. The qualititative behavior of the X-ray spectral index/flux relation observed from BL Lac objects can be explained with this model. This demonstrates that synchrotron losses are primarily responsible for the X-ray variability behavior and strengthens a new test for beaming from correlated hard X-ray/TeV observations.Comment: 10 pages, 2 figures, accepted for publication in Astrophysical Journal Letters; uses aaspp4.sty, epsf.st

Fluid Velocity Fluctuations in a Suspension of Swimming Protists

In dilute suspensions of swimming microorganisms the local fluid velocity is a random superposition of the flow fields set up by the individual organisms, which in turn have multipole contributions decaying as inverse powers of distance from the organism. Here we show that the conditions under which the central limit theorem guarantees a Gaussian probability distribution function of velocities are satisfied when the leading force singularity is a Stokeslet, but are not when it is any higher multipole. These results are confirmed by numerical studies and by experiments on suspensions of the alga Volvox carteri, which show that deviations from Gaussianity arise from near-field effects.Comment: 4 pages, 3 figure

Hydromagnetic constraints on deep zonal flow in the giant planets

The observed zonal flows of the giant planets will, if they penetrate below the visible atmosphere, interact significantly with the planetary magnetic field outside the metallized core. The appropriate measure of this interaction is the Chandrasekhar number Q = H^2 /4πρνα^2 λ (H = radial component of the magnetic field, ν = eddy viscosity, λ = magnetic diffusivity, α^-1 = length scale on which λ varies); at depths where Q ≳ 1, the velocity will be forced to oscillate on a small length scale or decay to zero. We estimate the conductivity due to semiconduction in H_2 (Jupiter, Saturn) and ionization in H_(2)0 (Uranus, Neptune) as a function of depth; the value λ ≈ 10^10 cm^2 s^-1 needed for Q = 1 is readily obtained well outside the metallic core (where A ≈ 10^2 cm^2 s^-1). These assertions are quantified by a simple model of the equatorial zonal jet in which the flow is assumed uniform on cylinders concentric with the spin axis, and viscous and magnetic torques on each cylinder are balanced. We solve this "Taylor constraint" simultaneously with the dynamo equation to obtain the velocity and magnetic field in the equatorial plane. With this model we reproduce the widely differing jet widths of Jupiter and Saturn (though not the flow at very high or low latitudes) using v = 2500 cm^2 s^-1, consistent with the requirement that viscous dissipation not exceed the specific luminosity. A model Uranian jet consistent with the limited Voyager data can also be constructed, with appropriately smaller v, but only if one assumes a two-layer interior. We tentatively predict a wide Neptunian jet. For Saturn (but not Jupiter or Uranus) the model has a large magnetic Reynolds number where Q = 1 and hence exhibits substantial axisymmetrization of the field in the equatorial plane. This effect may or may not persist at higher latitudes. The one-dimensional model presented is only a first step. Variation of the velocity and magnetic field parallel to the spin axis must be modeled in order to answer several important questions, including: (1) What is the behavior of flows at high latitudes, whose Taylor cylinders are interrupted by the region with Q > 1? (2) To what extent is differential rotation in the envelope responsible for the spinaxisymmetry of Saturn's magnetic field

Neuralized Mouse Embryonic Stem Cells Develop Neural Rosette-Like Structures in Response to Retinoic Acid and Produce Teratomas in the Brains of Syngeneic Mice

Several induction protocols can direct differentiation of mouse embryonic stem cells (ESCs) to become neural cells. The B5 and B6 mouse ESC lines display different growth patterns in vitro, and when grown as adherent cultures, the B6 ESCs proliferated at a significantly lower rate than B5 ESCs. Remarkably, after a neural induction protocol that includes removal of LIF and addition of retinoic acid (RA), mature B6 embryoid bodies (EBs) displayed a unique neural rosette-like morphology. On Day 8 of neural induction, B6 EBs revealed mature neuronal markers localized primarily to cells in the center of the EBs and glial markers expressed both in centrally and peripherally located cells. In contrast to B5 cells, when neuralized Day 8 B6 EB cells were dissociated and transplanted into the left striatum of syngeneic C57BL/6 mouse brains, teratomas formed. In addition, teratomas established from undifferentiated B6 cells grew more rapidly and achieved larger volumes when compared to those produced by Day 8, neuralized B6 EBs. The slow growth rate of B6 cells in vitro may have contributed to incomplete neuralization, formation of neural rosette-like structures, and a propensity to form teratomas

Prolific pair production with high-power lasers

Prolific electron-positron pair production is possible at laser intensities approaching 10^{24} W/cm^2 at a wavelength of 1 micron. An analysis of electron trajectories and interactions at the nodes (B=0) of two counter-propagating, circularly polarised laser beams shows that a cascade of gamma-rays and pairs develops. The geometry is generalised qualitatively to linear polarisation and laser beams incident on a solid target.Comment: 4 pages, 1 figure, minor revisions, accepted for publication in Physical Review Letter

Growth rates of the Weibel and tearing mode instabilities in a relativistic pair plasma

We present an algorithm for solving the linear dispersion relation in an inhomogeneous, magnetised, relativistic plasma. The method is a generalisation of a previously reported algorithm that was limited to the homogeneous case. The extension involves projecting the spatial dependence of the perturbations onto a set of basis functions that satisfy the boundary conditions (spectral Galerkin method). To test this algorithm in the homogeneous case, we derive an analytical expression for the growth rate of the Weibel instability for a relativistic Maxwellian distribution and compare it with the numerical results. In the inhomogeneous case, we present solutions of the dispersion relation for the relativistic tearing mode, making no assumption about the thickness of the current sheet, and check the numerical method against the analytical expression.Comment: Accepted by PPC

Studies Of The Mechanism of Epidermal Injury By A Staphylococcal Epidermolytic Toxin

Experimental animal models of the two forms of toxic epidermal necrolysis have been reviewed: a murine model of staphylococcal-induced epidermolysis and a hamster model of graft-versus-host disease. In the former, a protein exotoxin, epidermolysin, has been purified and characterized. The exotoxin has a molecular weight of approximately 30,000 and causes a split beneath the granular layer. It is effective at 3 × 10-12 moles. Epidermolysin does not require an intact complement system for its action since B10D2 mice deficient in C5 or mice injected with the decomplementing agent in cobra venom factor were susceptible to its epidermolytic effects. Neither are immunocompetent thymocytes required for the action of the toxin since hairless, athymic adult (nu/nu) mice are susceptible. A few reports of epidermolysis due to an exotoxin of group I Staphylococcus aureus have appeared. This toxin is antigenically different from the exotoxin of group II organisms.A model of drug-induced toxic epidermal necrolysis has been described in hamsters, but the toxic principle released from sensitized lymphoid cells has not yet been characterized