53 research outputs found

    Planar lattice gases with nearest-neighbour exclusion

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    We discuss the hard-hexagon and hard-square problems, as well as the corresponding problem on the honeycomb lattice. The case when the activity is unity is of interest to combinatorialists, being the problem of counting binary matrices with no two adjacent 1's. For this case we use the powerful corner transfer matrix method to numerically evaluate the partition function per site, density and some near-neighbour correlations to high accuracy. In particular for the square lattice we obtain the partition function per site to 43 decimal places.Comment: 16 pages, 2 built-in Latex figures, 4 table

    Observation of hard scattering in photoproduction events with a large rapidity gap at HERA

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    Events with a large rapidity gap and total transverse energy greater than 5 GeV have been observed in quasi-real photoproduction at HERA with the ZEUS detector. The distribution of these events as a function of the γp\gamma p centre of mass energy is consistent with diffractive scattering. For total transverse energies above 12 GeV, the hadronic final states show predominantly a two-jet structure with each jet having a transverse energy greater than 4 GeV. For the two-jet events, little energy flow is found outside the jets. This observation is consistent with the hard scattering of a quasi-real photon with a colourless object in the proton.Comment: 19 pages, latex, 4 figures appended as uuencoded fil

    An Observational Overview of Solar Flares

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    We present an overview of solar flares and associated phenomena, drawing upon a wide range of observational data primarily from the RHESSI era. Following an introductory discussion and overview of the status of observational capabilities, the article is split into topical sections which deal with different areas of flare phenomena (footpoints and ribbons, coronal sources, relationship to coronal mass ejections) and their interconnections. We also discuss flare soft X-ray spectroscopy and the energetics of the process. The emphasis is to describe the observations from multiple points of view, while bearing in mind the models that link them to each other and to theory. The present theoretical and observational understanding of solar flares is far from complete, so we conclude with a brief discussion of models, and a list of missing but important observations.Comment: This is an article for a monograph on the physics of solar flares, inspired by RHESSI observations. The individual articles are to appear in Space Science Reviews (2011

    Observation of Events with an Energetic Forward Neutron in Deep Inelastic Scattering at HERA

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    In deep inelastic neutral current scattering of positrons and protons at the center of mass energy of 300 GeV, we observe, with the ZEUS detector, events with a high energy neutron produced at very small scattering angles with respect to the proton direction. The events constitute a fixed fraction of the deep inelastic, neutral current event sample independent of Bjorken x and Q2 in the range 3 · 10-4 \u3c xBJ \u3c 6 · 10-3 and 10 \u3c Q2 \u3c 100 GeV2

    Whole genome sequence analysis of pulmonary function and COPD in 19,996 multi-ethnic participants

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    Chronic obstructive pulmonary disease (COPD), diagnosed by reduced lung function, is a leading cause of morbidity and mortality. We performed whole genome sequence (WGS) analysis of lung function and COPD in a multi-ethnic sample of 11,497 participants from population- and family-based studies, and 8499 individuals from COPD-enriched studies in the NHLBI Trans-Omics for Precision Medicine (TOPMed) Program. We identify at genome-wide significance 10 known GWAS loci and 22 distinct, previously unreported loci, including two common variant signals from stratified analysis of African Americans. Four novel common variants within the regions of PIAS1, RGN (two variants) and FTO show evidence of replication in the UK Biobank (European ancestry n ~ 320,000), while colocalization analyses leveraging multi-omic data from GTEx and TOPMed identify potential molecular mechanisms underlying four of the 22 novel loci. Our study demonstrates the value of performing WGS analyses and multi-omic follow-up in cohorts of diverse ancestry

    Extraction of the gluon density of the proton at x

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    Restaurant Waste Treatment and Management

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    © 2017 by Taylor & Francis Group, LLC. Restaurant waste is composed of solid and liquid waste. The solid waste stream includes food waste, plastics, paper and paperboard, while the liquid waste stream includes fats, oils, and grease (FOG). In the United States, in 2012, 36 million tons of food waste was generated and only 1.7 million tons were recycled. Approximately 20% of the prepared food in the United States ends up as waste. Of the total waste stream from restaurants, over 50% is food waste. This chapter discusses how restaurant waste can be reduced or recycled. Solid restaurant waste can be reduced through food recovery techniques such as food source recovery, food donation, food scraps for animal food, and food scraps for industrial uses. Food waste from restaurant can be used to produce methane from anaerobic digestion (two-stage and 184single high-rate digesters including egg-shape digesters), synthetic gas (syngas) from biomass gasification (fixed bed, fluidized bed, and plasma processes), and hydrogen by fermentation (biohydrogen production). Another industrial use of food waste is the production of compost through windrows or forced air composting processes. Restaurant and hotels generate over 3 billion gallons of waste cooking oil per year. Ideally, the waste oil can be collected and converted to biodiesel fuel by transesterification process. Some restaurant wastes from cruise ships can also be recycled for reuse. The current restaurant waste treatment and management practice on board modern cruise ships is introduced in this chapter
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