1,811 research outputs found

    Biharmonic pattern selection

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    A new model to describe fractal growth is discussed which includes effects due to long-range coupling between displacements uu. The model is based on the biharmonic equation 4u=0\nabla^{4}u =0 in two-dimensional isotropic defect-free media as follows from the Kuramoto-Sivashinsky equation for pattern formation -or, alternatively, from the theory of elasticity. As a difference with Laplacian and Poisson growth models, in the new model the Laplacian of uu is neither zero nor proportional to uu. Its discretization allows to reproduce a transition from dense to multibranched growth at a point in which the growth velocity exhibits a minimum similarly to what occurs within Poisson growth in planar geometry. Furthermore, in circular geometry the transition point is estimated for the simplest case from the relation rL/e1/2r_{\ell}\approx L/e^{1/2} such that the trajectories become stable at the growing surfaces in a continuous limit. Hence, within the biharmonic growth model, this transition depends only on the system size LL and occurs approximately at a distance 60%60 \% far from a central seed particle. The influence of biharmonic patterns on the growth probability for each lattice site is also analysed.Comment: To appear in Phys. Rev. E. Copies upon request to [email protected]

    Incarceration history and risk of HIV and hepatitis C virus acquisition among people who inject drugs: a systematic review and meta-analysis

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    Background People who inject drugs (PWID) experience a high prevalence of incarceration and might be at high risk of HIV and hepatitis C virus (HCV) infection during or after incarceration. We aimed to assess whether incarceration history elevates HIV or HCV acquisition risk among PWID. Methods In this systematic review and meta-analysis, we searched MEDLINE, Embase, and PsycINFO databases for studies in any language published from Jan 1, 2000 until June 13, 2017 assessing HIV or HCV incidence among PWID. We included studies that measured HIV or HCV incidence among community-recruited PWID. We included only studies reporting original results and excluded studies that evaluated incident infections by self-report. We contacted authors of cohort studies that met the inclusion or exclusion criteria, but that did not report on the outcomes of interest, to request data. We extracted and pooled data from the included studies using random-effects meta-analyses to quantify the associations between recent (past 3, 6, or 12 months or since last follow-up) or past incarceration and HIV or HCV acquisition (primary infection or reinfection) risk among PWID. We assessed the risk of bias of included studies using the Newcastle-Ottawa Scale. Between-study heterogeneity was evaluated using the I2 statistic and the P-value for heterogeneity. Findings We included published results from 20 studies and unpublished results from 21 studies. These studies originated from Australasia, western and eastern Europe, North and Latin America, and east and southeast Asia. Recent incarceration was associated with an 81% (relative risk [RR] 1·81, 95% CI 1·40–2·34) increase in HIV acquisition risk, with moderate heterogeneity between studies (I2=63·5%; p=0·001), and a 62% (RR 1·62, 95% CI 1·28–2·05) increase in HCV acquisition risk, also with moderate heterogeneity between studies (I2=57·3%; p=0·002). Past incarceration was associated with a 25% increase in HIV (RR 1·25, 95% CI 0·94–1·65) and a 21% increase in HCV (1·21, 1·02–1·43) acquisition risk. Interpretation Incarceration is associated with substantial short-term increases in HIV and HCV acquisition risk among PWID and could be a significant driver of HCV and HIV transmission among PWID. These findings support the need for developing novel interventions to minimise the risk of HCV and HIV acquisition, including addressing structural risks associated with drug laws and excessive incarceration of PWID

    Plasma Electronics

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    Contains reports on twelve research projects.United States Atomic Energy Commission (Contract AT(30-1)-3285)United States Atomic Energy Commission under Contract AT(30-1)-3221National Science Foundation (Grant GK-57

    Natural Inflation: Particle Physics Models, Power Law Spectra for Large Scale Structure, and Constraints from COBE

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    A pseudo-Nambu-Goldstone boson, with a potential of the form V(ϕ)=Λ4[1±cos(ϕ/f)],naturallygivesrisetoinflationifV(\phi) = \Lambda^4[1 \pm \cos(\phi/f)], naturally gives rise to inflation if f \sim M_{Pl}and and \Lambda \sim M_{GUT}.Weshowhowthiscanariseintechnicolorlikeandsuperstringmodels,andworkoutanexplicitstringexampleinthecontextofmultiplegauginocondensationmodels.Westudythecosmologyofthismodelindetail,andfindthatsufficientreheatingtoensurethatbaryogenesiscantakeplacerequires. We show how this can arise in technicolor-like and superstring models, and work out an explicit string example in the context of multiple gaugino condensation models. We study the cosmology of this model in detail, and find that sufficient reheating to ensure that baryogenesis can take place requires f > 0.3 M_{Pl}.Theprimordialdensityfluctuationspectrumgeneratedisanonscaleinvariantpowerlaw,. The primordial density fluctuation spectrum generated is a non-scale-invariant power law, P(k) \propto k^{n_s},with, with n_s \simeq 1 - (M^2_{Pl}/8\pi f^2),leadingtomorepoweronlargelengthscalesthanthe, leading to more power on large length scales than the n_s = 1HarrisonZeldovichspectrum.ThestandardCDMmodelwith Harrison-Zeldovich spectrum. The standard CDM model with 0 \la n_s \la 0.6-0.7couldinprincipleexplainthelargescaleclusteringobservedintheAPMandIRASgalaxysurveysaswellaslargescaleflows,buttheCOBEmicrowaveanisotropyimpliessuchlowamplitudes(orhighbiasfactors, could in principle explain the large-scale clustering observed in the APM and IRAS galaxy surveys as well as large-scale flows, but the COBE microwave anisotropy implies such low amplitudes (or high bias factors, b>2)fortheseCDMmodelsthatgalaxyformationoccurstoolatetobeviable;combiningCOBEwithsufficientlyearlygalaxyformationorthelargescaleflowsleadsto) for these CDM models that galaxy formation occurs too late to be viable; combining COBE with sufficiently early galaxy formation or the large-scale flows leads to n_s >0.6,or, or f > 0.3 M_{Pl}aswell.Forextendedandpowerlawinflationmodels,thisconstraintiseventighter, as well. For extended and power law inflation models, this constraint is even tighter, n_s > 0.7$; combined with other bounds on large bubbles in extended inflation, this leaves little room for most extended models.Comment: 42 pages, (12 figures not included but available from the authors

    Plasmas and Controlled Nuclear Fusion

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    Contains research objectives and reports on four research projects.National Science Foundation (Grant GK-614)National Science Foundation (Grant GK-57
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