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We report on the different types of condensates possible in two-component atomic gas mixtures in one dimension involving both bosons and fermions. When the interactions are attractive, we show there is a rich variety of coherent ground-state phases that vary with their intrinsic and relative strength. We avoid any artifacts of lattice discretization by developing a novel implementation of a continuous matrix-product-state ansatz for mixtures that we first show to systematically converge towards exact results for the Lai-Yang-model integrable case.

he Review summarizes much of particle physics and cosmology. Using data from previous editions, plus 3,324 new measurements from 878 papers, we list, evaluate, and average measured properties of gauge bosons and the recently discovered Higgs boson, leptons, quarks, mesons, and baryons. We summarize searches for hypothetical particles such as supersymmetric particles, heavy bosons, axions, dark photons, etc. Particle properties and search limits are listed in Summary Tables. We give numerous tables, figures, formulae, and reviews of topics such as Higgs Boson Physics, Supersymmetry, Grand Unified Theories, Neutrino Mixing, Dark Energy, Dark Matter, Cosmology, Particle Detectors, Colliders, Probability and Statistics. Among the 120 reviews are many that are new or heavily revised, including a new review on High Energy Soft QCD and Diffraction and one on the Determination of CKM Angles from B Hadrons. The Review is divided into two volumes. Volume 1 includes the Summary Tables and 98 review articles. Volume 2 consists of the Particle Listings and contains also 22 reviews that address specific aspects of the data presented in the Listings. The complete Review (both volumes) is published online on the website of the Particle Data Group (pdg.lbl.gov) and in a journal. Volume 1 is available in print as the PDG Book. A Particle Physics Booklet with the Summary Tables and essential tables, figures, and equations from selected review articles is available in print and as a web version optimized for use on phones as well as an Android app.

We study two-component atomic gas mixtures in one dimension involving both bosons and fermions. When the inter-species interaction is attractive, we report a rich variety of coherent ground-state phases that vary with the intrinsic and relative strength of the interactions. We avoid any artifacts of lattice discretization by developing a novel implementation of a continuous matrix product state ansatz for mixtures and priorly demonstrate the validity of our approach on the integrable point that exists for mixtures with equal masses and interactions (Lai-Yang model) where we find that the ansatz correctly and systematically converges towards the exact results., Comment: 8 pages, 3 figures

We use the final data from the VIPERS redshift survey to extract an unparalleled sample of more than 2000 massive M > 10^11 M_sun passive galaxies (MPGs) at redshift 0.5 < z < 1.0, based on their NUVrK colours. This enables us to investigate how the population of these objects was built up over cosmic time. We find that the evolution of the number density depends on the galaxy mean surface stellar mass density, Sigma. In particular, dense (Sigma > 2000 M_sun pc^-2) MPGs show a constant comoving number density over this redshift range, whilst this increases by a factor ~ 4 for the least dense objects, defined as having Sigma < 1000 M_sun pc^-2. We estimate stellar ages for the MPG population both fitting the Spectral Energy Distribution (SED) and through the D4000_n index, obtaining results in good agreement. Our findings are consistent with passive ageing of the stellar content of dense MPGs. We show that at any redshift the less dense MPGs are younger than dense ones and that their stellar populations evolve at a slower rate than predicted by passive evolution. This points to a scenario in which the overall population of MPGs was built up over the cosmic time by continuous addition of less dense galaxies: on top of an initial population of dense objects that passively evolves, new, larger, and younger MPGs continuously join the population at later epochs. Finally, we demonstrate that the observed increase in the number density of MPGs is totally accounted for by the observed decrease in the number density of correspondingly massive star forming galaxies (i.e. all the non-passive M > 10^11 M_sun objects). Such systems observed at z ~ 1 in VIPERS, therefore, represent the most plausible progenitors of the subsequent emerging class of larger MPGs., 14 pages, 13 figures, submitted to A&A

This chapter explores the role of the Bangladeshi immigrant woman in Britain and the effects of patriarchy in the Bangladeshi community on the immigrant female as noted by the life of the protagonist Nazneen and other female characters in the novel titled, Brick Lane by Monica Ali. Further the essay also compares and contrasts South Asian immigrant women to show how one group (a woman from India) is affected differently from her South Asian sister from Bangladesh. To understand the difference between the two groups of immigrant women, Monica Ali's novel was contrasted with Tarquin Hall's heroine from his novel Salam Brick Lane. By examining the role of South Asian immigrant women in Britain, other issues about immigrant culture was also brought to the forefront, such as religion, specifically Islam to show its effect on the lives of immigrant women in countries outside their own.

Synopsis We present new interpretations of Digital Elevation Model (DEM) data and marine fossils collected from three sites on the Rhins of Galloway which, contrary to recent proposals, suggest that the landforms and deposits of the region do not represent evidence for a readvance during the Lateglacial Period. Rather we suggest that the high-arctic fauna found in the region are representative of an earlier, colder part of a Middle Devensian ice-free interval. The predominantly streamlined topography, and distinct lack of identifiable discrete moraine limits argues for only minor, local glacial advances, in combination with widespread rapid retreat across the peninsula at the end of the Lateglacial.

Summary Sixty ASA 1 and 2 children aged between 2 and 16 years who required tracheal intubation as part of anaesthesia for elective surgery were studied. We evaluated intubating conditions, haemodynamic responses and duration of apnoea following propofol 4 mg.kg−1 combined with either remifentanil 1.25 μg.kg−1 (group R), or suxamethonium 1 mg.kg−1 (group S). Tracheal intubation was graded as excellent, good or poor according to ease of laryngoscopy, vocal cord position, coughing, and jaw relaxation and limb movement. Thirty of group S and 28 of group R children were successfully intubated on the first attempt. Overall, intubation conditions were excellent or good in 26/30 (87%) patients in group S and 20/30 (67%) in group R (p

A computer screen-based simulator has been developed to simulate the administration of intravenous and analgesic drugs. It merges on-line measurements (such as systolic arterial pressure (SAP) and heart rate (HR)) and nonnumerical clinical signs (such as sweating, lacrimation and pupil response), using anaesthetists' experience or self-organizing fuzzy logic control (SOFLC) algorithms to administer drugs into a patient. The hierarchical control architecture includes five parts, which are: monitoring depth of anaesthesia (DOA), drug controller, deciding the sensitivity of the patient, narcotic supplementation and recovery time. It has been developed to predict drug profiles, control the drug levels and assess recovery time during anaesthesia. Meanwhile, linguistic rules and fuzzy set theory have been used to model a patient's SAP and HR during induction and maintenance stages. Successful simulation results have given confidence to perform on-line clinical trials in operating theatre.

Background and purpose Treatment-induced arm lymphoedema is a common and distressing complication of curative surgery and radiotherapy for early breast cancer. A number of studies testing alpha-tocopherol (vitamin E) and pentoxifylline suggest evidence of clinical regression of superficial radiation-induced fibrosis but there is only very limited evidence from randomised trials. Arm lymphoedema after lymphatic radiotherapy and surgery has been used in the present study as a clinical system for testing these drugs in a double-blind placebo-controlled randomised phase II trial. Patients and methods Sixty-eight eligible research volunteers with a minimum 20% increase in arm volume at a median 15.5 years (range 2–41) after axillary/supraclavicular radiotherapy (plus axillary surgery in 51/68 (75%) cases) were randomised to active drugs or placebo. All volunteers were given dl-alpha tocopheryl acetate 500mg twice a day orally plus pentoxifylline 400mg twice a day orally, or corresponding placebos, for 6 months. The primary endpoint was volume of the ipsilateral limb measured opto-electronically using a perometer and expressed as a percentage of the contralateral limb volume. Results At 12 months post-randomisation, there was no significant difference between treatment and control groups in terms of arm volume. Absolute change in arm volume at 12 months was 2.5% (95% CI −0.40 to 5.3) in the treatment group compared to 1.2% (95% CI −2.8 to 5.1) in the placebo group. The difference in mean volume change between randomisation groups at 12 months was not statistically significant ( P =0.6), −1.3% (95% CI −6.1 to 3.5), nor was there a significant difference in response at 6 months ( P =0.7), where mean change in arm volume from baseline in the treatment and placebo groups was −2.3% (95% CI −7.9 to 3.4) and −1.1% (95% CI −3.9 to 1.7), respectively. There were no significant differences between randomised groups in terms of secondary endpoints, including tissue induration (fibrosis) in the irradiated breast or chest wall, pectoral fold or supraclavicular fossa, change in photographic breast/chest wall appearance or patient self-assessment of function and Quality of Life at either 6 or 12 months. Conclusions The study fails to demonstrate efficacy of dl-alpha tocopheryl acetate plus pentoxifylline in patients with arm lymphoedema following axillary surgery and lymphatic radiotherapy, nor does it suggest any benefits of these drugs in radiation-induced induration (fibrosis) in the breast, chest wall, pectoral fold, axilla or supraclavicular fossa.

Despite extensive observational efforts, the brightest sub-mm source in the Hubble Deep Field, HDF850.1, has failed to yield a convincing optical/infrared identifica- tion almost 4 years after its discovery. This failure is all the more notable given the availability of supporting multi-frequency data of unparalleled depth, and sub-arcsec positional accuracy for the sub-mm/mm source. Consequently, HDF850.1 has become a test case of the possibility that the most violently star-forming objects in the universe are too red and/or distant to be seen in the deepest optical images. Here we report the discovery of the host galaxy of HDF850.1. This object has been revealed by careful analysis of a new, deep Kimage of the HDF obtained with the Subaru 8.2-m telescope. Its reality is confirmed by a similar analysis of the HST NICMOS F160W image of the same region. This object is extremely faint (K ≃ 23.5), clumpy (on sub-arcsec scales) and very red (I − K > 5.2; H − K = 1.4 ± 0.35). The likelihood that it is the correct identification is strongly reinforced by a reanalysis of the combined MERLIN+VLA 1.4-GHz map of the field which provides a new radio detection of HDF850.1 only 0.1arcsec from the new near-infrared counterpart, and with sufficient positional accuracy to exclude all previously considered alternative optical candidates. We have calculated new confidence limits on the estimated redshift of HDF850.1 in the light of the new radio detection, and find z = 4.1±0.5. We have also determined the scale-length, and hence estimated the mass of the apparently nearby (0.5arcsec distant) z ≃ 1 elliptical galaxy 3-586.0. From this we calculate that the flux density of HDF850.1 has been boosted by a factor of ≃ 3 through gravitational lensing by this intervening elliptical, consistent with predictions that a small but significant fraction of blank-field sub-mm sources are lensed by foreground galaxies. We discuss the wider implications of these results for the sub-mm population and cosmic star-formation history.

Propulsive movements of the caudal oscillating flukes produce large forces chat could induce equally large recoil forces at the cranial end of the animal, and, thus, affect stability. To examine these vertical oscillations, video analysis was used to measure the motions of the rostrum, pectoral flipper, caudal peduncle, and fluke tip for seven odonrocere cetaceans: Delphinapterus leucas, Globicepbala melaena, Lagenvrhyncbus obliquidens, O~cinus orra, Pseudorca crassidens, Stenella plagiodon, and TarJiops truncatus. Animals swam over a range of speeds of 1.4-7.3 mlsec. For each species, oscillatory frequency of the fluke tip increased linearly with swimming speed. Peak-to-peak amplitude at each body position remained constanc with respect ro swimming speed for all species. Mean peak-to-peak amplitude ranged from 0.02 to 0.06 body length at the rostrum and from 0.17 to 0.25 body length at the fluke tip. The phase relationships between the various body components remain constant with respect to swimming speed. Oscillations of the rostrum were nearly in phase with the fluke tip with phase differences out of -9.4"-33.0" of a cycle period of 360". Pectoral flipper oscillations trailed fluke oscillations by 60.9°-123.40. The lower range in amplitude at the rostrum compared co rhe fluke rip reflects increased resistance to vertical oscillation at the cranial end, which enhances the animal's stability. This resistance is likely due to both active and passive increased body stiffness, resistance on the flippers, phased movements of body components, and use of a lift-based propulsion. Collectively, these mechanisms srabilize the body of cetaceans during active swimming, which can reduce locomotor energy expenditure and reduce excessive motions of the head affecting sensory capabilities.

Synopsis The Late Devensian arctic marine deposits (Errol Clay Formation) at the Gallowflat Claypit between Perth and Dundee are correlated with the type succession at nearby Inchcoonans, but include an expanded basal glaciomarine unit with rhythms interpreted as symmict varves. Laminated silt–clay couplets are thought to be tidal. Conditions were fully marine by 13.8 ka bp (based on new radiocarbon dates and a 400 a reservoir age). Following recession of the Tay–Forth glacier from its advanced Late Devensian position at the Wee Bankie Terminal Moraine, it is inferred that deglaciation of the middle Tay estuary some 100 km to the west took place between 14.5 and 14 ka bp. The possibility that there was a readvance of ice in the Tay and Forth estuaries during or close to the Heinrich iceberg discharge event H1 is briefly discussed.

In the Arabian Peninsula, rangeland biodiversity and animal production exist in a delicate balance. Increases in the small ruminant population has meant that the palatable indigenous plant species have been severely overgrazed. Exotic species are now being grown for fodder, however these use large volumes of irrigation water, and the practice is not sustainable. One approach to the conservation of biological diversity and the promotion of sustainable animal production is the conservation and utilization of these indigenous plant species. Seeds of three priority grasses have been collected, multiplied and evaluations for their water use efficiency and nutritive values made.

We present a comparison between the observed properties of damped Lyman alpha systems (DLAs) and the predictions of simple models for the evolution of present day disk galaxies, including both low and high surface brightness galaxies. We focus in particular on the number density, column density distribution and gas density of DLAs, which have now been measured in relatively large samples of absorbers. From the comparison we estimate the contribution of present day disk galaxies to the population of DLAs, and how it varies with redshift. Based on the differences between the models and the observations, we also speculate on the nature of the fraction of DLAs which apparently do not arise in disk galaxies.

Background and purpose : Small proportions of patients receiving radiotherapy develop marked long-term radiation damage. It is thought that this is due, at least in part, to intrinsic differences in cellular radiosensitivity, but the underlying mechanism is unknown. Reactive oxygen species are involved in cellular radiation damage, hence inter-individual differences in free radical detoxification may be related to radiosensitivity. Within mitochondria manganese superoxide dismutase (MnSOD) provides a major defence against oxidative damage by reactive oxygen species. MnSOD has been linked to expression of malignant phenotype and apoptosis and polymorphic variation in the gene, SOD2 to risk of breast cancer. Materials and methods : Forty-one breast cancer patients developing marked changes in breast appearance after radiotherapy and 39 patients who showed no clinically detectable reaction after radiotherapy were analyzed for germline sequence variation in SOD2 . Results : The Ala-9Val polymorphism was detected, but no other sequence variants were detected in SOD2 . Both alleles of the Ala-9Val polymorphism were equally distributed between the two patient groups. Conclusions : Sequence variation in SOD2 is not the major cause of radiotherapy complications in women with breast cancer.

Synopsis Multidisciplinary investigations of a radiocarbon dated isostatically raised, shallow marine sequence have enabled environmental parameters, including estimates of relative sea level and water temperatures, to be reconstructed for the Windermere Interstadial (WI) in the western Forth valley. Detailed faunal (ostracod and macrofauna) and sedimentological (particle size and micromorphology) examination of the 2.28 m sequence at Moss-side of Boquhapple suggests the existence of a shallow fjord-style margin environment at the site. Comparisons between recent faunal analogues and the fossil record suggest that WI relative sea levels can be limited to between +15 and +30 m OD. Additional regional stratigraphical and geomorphological investigations augment this interpretation. New AMS 14 C dates suggest that marine accumulation at the site was established by c. 12.8 ka bp, and continued to probably after c. 11.5 ka bp. Palaeotemperature reconstructions from the macrofauna and ostracod records show some divergence, but suggest temperatures were lower than present. The upper 0.50 m of the sequence shows significant reworking, and micromorphological analysis of one sample from this marine deposit discloses a limited number of features consistent with subaerial (possibly periglacial) processes. The final lowering in relative sea level, possibly to below +7 m OD, is believed to have occurred during the Loch Lomond (Younger Dryas) Stadial.

We use very large cosmological N--body simulations to obtain accurate predictions for the two-point correlations and power spectra of mass-limited samples of galaxy clusters. We consider two currently popular cold dark matter (CDM) cosmogonies, a critical density model ($\tau$CDM) and a flat low density model with a cosmological constant ($\Lambda$CDM). Our simulations each use $10^9$ particles to follow the mass distribution within cubes of side $2h^{-1}$Gpc ($\tau$CDM) and $3h^{-1}$Gpc ($\Lambda$CDM) with a force resolution better than $10^{-4}$ of the cube side. We investigate how the predicted cluster correlations increase for samples of increasing mass and decreasing abundance. Very similar behaviour is found in the two cases. The correlation length increases from $r_0=12$ -- 13$h^{-1}$Mpc for samples with mean separation $d_{\rm c}=30h^{-1}$Mpc to $r_0=22$-- 27$h^{-1}$Mpc for samples with $d_{\rm c}=100h^{-1}$Mpc. The lower value here corresponds to $\tau$CDM and the upper to $\Lambda$CDM. The power spectra of these cluster samples are accurately parallel to those of the mass over more than a decade in scale. Both correlation lengths and power spectrum biases can be predicted to better than 10% using the simple model of Sheth, Mo & Tormen (2000). This prediction requires only the linear mass power spectrum and has no adjustable parameters. We compare our predictions with published results for the APM cluster sample. The observed variation of correlation length with richness agrees well with the models, particularly for $\Lambda$CDM. The observed power spectrum (for a cluster sample of mean separation $d_{\rm c}=31h^{-1}$Mpc) lies significantly above the predictions of both models.

Molecular biology, combined with Mendelian and quantitative genetics in quantitative trait locus (QTL) mapping and marker-assisted selection (MAS), provides powerful new tools to facilitate efficient genetic manipulation by plant breeders of complex traits such as drought tolerance and phosphorus (P) acquisition ability. This paper examines current opportunities for genetically manipulating the ability of crop plants to more efficiently acquire (i.e. access and take up) essential soil nutrients, using as examples P and several of the crops in the genetic improvement mandate of the International Crops Research Institute for the Semi-Arid Tropics (ICRISAT) – chickpea (Cicer arietinum L.), groundnut (Arachis hypogaea L.), pearl millet [Pennisetum glaucum (L.) R. Br.], pigeonpea [Cajanus cajan(L.) Millsp.], and sorghum [Sorghum bicolor (L.) Moench]. It is concluded that for at least some of these important, but often academically and economically orphaned tropical food, forage and feed-grain crops, the genetic variation and molecular tools that we will need already exist or can be expected to become available in the very near future. With appropriate, targeted research, these tools can permit empirical exploration of the potential for marker-facilitated mapping and manipulation of major genes that can contribute to enhanced ability of these crops to acquire P from sources with limited availability. With these tools, delivery of new versions of currently popular high-yielding, high quality, disease resistant crop cultivars, having genetically improved ability to acquire P currently in soils but unavailable for crop growth, could take as little as five to seven years. Sustainable use of such improved cultivars would require their utilization as components of integrated soil fertility management systems.

Postoperative analgesia in patients who receive regular oral opioids pre-operatively is frequently suboptimal. To improve management we introduced a regimen using subcutaneous diamorphine infusions with incremental doses. Infusion doses were calculated as half the daily pre-operative dose of oral morphine with the increments as one-sixth of the infusion dose. Results were recorded on the first two postoperative days before (n = 13) and after (n = 23) commencing the new regimen. The percentage of patients reporting severe pain at rest and on movement were significantly reduced by the new regimen (54% and 69% vs. 13% and 40%, respectively) since the opioid dose as a percentage of the pre-operative dose was significantly higher (160% vs. 352%). There were no instances of excessive sedation or slow respiratory rate in any patient. The use of the regimen has resulted in greater doses of opioids being administered with fewer patients in severe pain without significant complications.

A multi-sensor fusion system for monitoring and control of depth of anaesthesia in the operating theatre is described. Two types of anaesthesia measures are considered, the first being based on auditory evoked responses, while the second measure is based on cardiovascular system signals. The first measure is based on analysis of the signal using wavelets and a neuro-fuzzy system, while the second measure is based on analysis of the measurements using a rule-based fuzzy logic system. The two measures are combined to give a final level of depth of anaesthesia using another rule-based fuzzy logic system. The depth of anaesthesia level is fed back to a target controlled infusion system (TCI) to control the infusion of the drug propofol for maintaining a constant level of depth of anaesthesia.

Fibrosis in normal tissues is a common and dose-limiting late complication of radiotherapy at many cancer sites, but its pathogenesis is poorly understood. We undertook a controlled study of the effect of irradiation on the collagen production of fibroblasts cultured from skin biopsies taken from patients undergoing radiotherapy treatment. Eight weeks after a single 8 Gy fraction using 300 kV X-rays, five patients treated at the Royal Marsden Hospital underwent biopsy of the irradiated site and of the contralateral, unirradiated body site. Fibroblasts from irradiated and control, unirradiated sites were cultured in vitro, and collagen production rates were measured during a 48-hour incubation under standardized conditions and in the presence and absence of transforming growth factor β1(TGF β1), 1 ng/ml, using HPLC. Collagen production was elevated in cells cultured from irradiated skin; median collagen production rates 61.16 pmoles hydroxyproline/105cells/hour in irradiated cells, 39.78 pmoles hydroxyproline/105cells/hour in unirradiated cells, P = 0.016 (Mann–Whitney U-test). In fibroblasts from unirradiated sites, collagen production rates were increased by the addition of TGF β1; however, in three of the cell lines cultured from irradiated sites this effect of TGF β1 on collagen production was not observed. © 2000 Cancer Research Campaign

The glacial deposits at the Boyne Bay Limestone Quarry near Portsoy, a key Quaternary Site of Special Scientific Interest, comprise (i) a sandy, partly weathered diamicton (Craig of Boyne Till Formation, CBTF) resting on decomposed bedrock, (ii) a central, variably glaciotectonised assemblage of dark clay, diamicton and sand, with rafts of sand and weathered diamicton (Whitehills Glacigenic Formation, WGF), and (iii) an upper dark sandy diamicton (Old Hythe Till Formation, OHTF). The CBTF was probably derived from the west or southwest, and the WGF from seawards. Structures within the OHTF conform to deposition by east- or southeast-moving ice from the Moray Firth, but some erratics indicate derivation from the south. The CBTF is believed to pre-date the last (lpswichian) interglacial, but the WGF and OHTF both post-date the early Middle Devensian, and are probably of Late Devensian age. It is proposed that the OHTF was deposited by ice from inland which was directed eastwards near the coast by a vigorous glacier in the Moray Firth, and that the complex, Late Devensian glacial history of the south coast of the Moray Firth as a whole is the result of the interplay of these two contemporary ice-masses. British Geological Survey. © NERC 2000.