Test station to characterize the emission of a LiDAR

A test station setup devised to measure the emission characteristics and beam propagation parameters of a light detection and ranging (LiDAR) system is presented. The main blocks of the station to measure the accessible emission, wavelength peak and FWHM, pulse duration, pulse repetition rate, horizontal and vertical angular resolution, field of view, beam propagation factor M 2, beam waist size, waist location, and divergence are described. The performance of this test station was demonstrated using a commercial spinning LiDAR, a Velodyne VLP-16, which successfully enables these measurements for a laser beam with a wavelength of 913 nm.

Comparison of the use of life cycle assessment and ecological footprint methods for evaluating environmental performances in dairy production

One popular methodology for assessing the environmental impact of livestock sector is Life Cycle Assessment (LCA), that quantifies the environmental impact of a product. Ecological Footprint (EF) performs an environmental sustainability assessment, by comparing the demand for natural capital by an economic activity with the offer of such capital within a certain territory. The aim of the study was the comparison between LCA and EF in assessing the environmental performances of milk production, assuming as case study three cattle farms with increasing levels of production intensity. Different metrics and functional units (FU) (i.e., fat and protein corrected milk, FPCM and hectare) were adopted for LCA analysis, considering some of the major impact categories. For greenhouse gases emissions, the Global Warming Potential (GWP) and the Global Temperature Potential (GTP) were considered. Both metrics were calculated assuming or not the distinction between biogenic and fossil methane. Adopting GWP as a metric, the results per kg of FPCM provided by the LCA highlighted a different trade off compared to the EF method: the farm with the highest productive intensity produced the least impactful milk in terms of GWP but had the most negative Ecological Balance (EB). The same occurred for the other impact categories. When GTP was adopted, or the hectare was considered as FU, the least intensive farm, characterized by greater feed self-sufficiency, became the one that produced the least impactful milk and had the least negative EB. The study highlighted the scientific significance of the integration between the two approaches for creating a comprehensive representation of the effects of human activities on the environment. The LCA method evaluates impacts intensity referred to a specific functional unit and its results are strongly influenced by productive efficiency; the EF method evaluates environmental sustainability of productions in relation to the territory that supports them.

Volume fraction determination of microgel composed of interpenetrating polymer networks of PNIPAM and polyacrylic acid

Interpenetrated polymer network microgels, composed of crosslinked networks of poly(N-isopropylacrylamide) and polyacrylic acid (PAAc), have been investigated through rheological measurements at four different amounts of PAAc. Both PAAc content and crosslinking degree modify particle dimensions, mass and softness, thereby strongly affecting the volume fraction and the system viscosity. Here the volume fraction is derived from the flow curves at low concentrations by fitting the zero-shear viscosity with the Einstein-Batchelor equation which provides a parameterkto shift weight concentration to volume fraction. We find that particles with higher PAAc content and crosslinker are characterized by a greater value ofkand therefore by larger volume fractions when compared to softer particles. The packing fractions obtained from rheological measurements are compared with those from static light scattering for two PAAc contents revealing a good agreement. Moreover, the behaviour of the viscosity as a function of packing fraction, at room temperature, has highlighted an Arrhenius dependence for microgels synthesized with low PAAc content and a Vogel-Fulcher-Tammann dependence for the highest investigated PAAc concentration. A comparison with the hard spheres behaviour indicates a steepest increase of the viscosity with decreasing particles softness. Finally, the volume fraction dependence of the viscosity at a fixed PAAc and at two different temperatures, below and above the volume phase transition, shows a quantitative agreement with the structural relaxation time measured through dynamic light scattering indicating that interpenetrated polymer network microgels softness can be tuned with PAAc and temperature and that, depending on particle softness, two different routes are followed.

Apparatus for simultaneous dynamic light scattering-small angle neutron scattering investigations of dynamics and structure in soft matter

Dynamic Light Scattering (DLS) and Small-Angle Neutron Scattering (SANS) are two key tools to probe the dynamic and static structure factors, respectively, in soft matter. Usually, DLS and SANS measurements are performed separately, in different laboratories, on different samples, and at different times. However, this methodology has particular disadvantages for a large variety of soft materials, which exhibit a high sensitivity to small changes in fundamental parameters, such as waiting times, concentration, pH, and ionic strength. Here, we report on a new portable DLS-SANS apparatus that allows one to simultaneously measure both the microscopic dynamics (through DLS) and the static structure (through SANS) on the same sample. The apparatus has been constructed as a collaboration between two laboratories, each an expert in one of the scattering methods, and was commissioned on the LOQ and ZOOM SANS instruments at the ISIS Pulsed Neutron and Muon Source, U.K.

Could Vespa velutina nigrithorax be included in the World Organisation for Animal Health list of diseases, infections and infestations?

Vespa velutina nigrithorax is an invasive alien organism that has raised concerns in all beekeeping communities of invaded countries including the Republic of Korea, European countries and Japan. Known also as the yellow-legged hornet (or the 'Asian hornet'), it is native to northern India, eastern Nepal, Bhutan and the People's Republic of China. Given its climatic and biological characteristics and the effects of climate change, some coastal areas of North America, Argentina, South Africa, Australia and New Zealand are also susceptible to invasion. Vespa velutina nigrithorax notably affects managed honey-bee colonies by predation on foragers and causing a reduction in the collection of food resources. Being a generalist predator, the yellow-legged hornet also preys on other managed and wild pollinators, and therefore its impacts are not limited to the beekeeping sector but also represent a biodiversity concern. The purpose of this paper is to provide an assessment of V. v. nigrithorax against the four criteria established in Chapter 1.2. of the World Organisation for Animal Health (OIE) Terrestrial Animal Health Code for the inclusion of a disease, infection or infestation in the OIE list. The work was requested by the OIE Scientific Commission for Animal Diseases and presented to this Commission and to the OIE Terrestrial Animal Health Standards Commission in September 2017. Owing to the lack of effective measures to prevent its spread, the fact that its legal situation in some countries is under the mandate of environmental authorities rather than Veterinary Services, and because it is not considered a disease or parasite, V. v. nigrithorax is not currently being proposed for inclusion in the OIE list. At the end of the text, the statements from the two commissions are included and discussed.

Contributi scientifici in memoria di Antonio Fusco

Come si leggerà nell'Introduzione della sezione propriamente scientifica del Volume, il presente testo nasce dalla volontà e, soprattutto, dall'esigenza culturale di omaggiare il fu Prof. Antonio Fusco. Un debito scientifico ed umano che trova il suo locus naturale in questa prima parte del testo stesso, cui farà poi seguito la parte propriamente scientifica. In siffatta parentesi dovuta per le ragioni appena menzionate, il lettore, l'amico o l'allievo dell'opera del Prof. Fusco potranno trovare un suo sintetico Curriculum Vitae, correlato da una specifica ed accurata prosa, svolta dal già Magnifico Rettore Carlo Cipolli; il quale, oltre che evidenziare, ricordando, i meriti del collega oramai scomparso, aggiunge alsuo scritto un elemento che sarebbe imprescindibile a non trasformare lo stesso in una mera sequenza di parole: l'amicizia e l'affetto per un amico che, oramai, non c'è più. A fine lettura, evidente risuonerà il fatto che la vita di ognuno, se mossa dalla passione per ciò per cui si è predisposti cognitivamente e psicologicamente, può essere ricca di riconoscimenti, riconoscenze e soddisfazioni che, lungi dal divenire un cuscino di allori su cui adagiarsi, per una mente creativa come quella del Prof. Fusco hanno funto solo da motivazioni ad agire instancabilmente guardando sempre al futuro. Il lavoro di una vita che, materialmente, è sancito da un supporto poco più di cm 25x15: una targa. Una materialità evidente che, con grande commozione e riconoscenza, è stata affissa il 25 ottobre 2019 sull'aula fronte l'Aula Magna del Campus "La Folcara", a testimonianza che quello spirito creativo in continua evoluzione non si ferma; non si arresta neppure con la fine biologica di chi lo ha "posseduto". Rimangono le opere ed il pensiero del Prof. Fusco e restano gli affetti. A tal proposito, il lettore troverà una breve e sentita sezione su Testimonianze; coloro i quali hanno avuto modo, nell'arco della vita accademica ed umana, personale, di Fusco di conoscerlo. Ecco, allora, che i ricordi saranno i veri protagonisti di questa parentesi. Dopo di ciò, prima dei contributi prettamente scientifici dei lavori, tenutisi in occasione del Convegno Internazionale Psicologia, Arte, Letteratura. Antiche e Nuove Tendenze, seguiranno i saluti delle autorità che in quei due giorni si sono succedute a rappresentare non solo l'istituzione affiliata, ma anche la relazione di stima e di affetto che le legava al compianto Professore. Si passerà, infine, al volume tradizionalmente inteso.

Evaluation of Crestal Bone Loss Around Straight and Tilted Implants in Patients Rehabilitated by Immediate-Loaded Full-Arch All-on-4 or All-on-6: A Prospective Study

The aim of this prospective study was to compare implant success rate and crestal bone loss around tilted and straight implants supporting immediate-loading full-arch rehabilitations. Twenty consecutive patients with edentulous jaws treated between June 2013 and July 2015 who satisfied all inclusion and exclusion criteria were included in the study. All patients were rehabilitated through a full-arch restoration supported by 4 or 6 immediately loaded implants. Clinical and radiographic examinations were scheduled every 12 months to evaluate implant success rates and crestal bone levels. Significant differences in crestal bone levels and success rates between straight and tilted implants were investigated by means of independent statistical analysis; differences were regarded as significant if P < .05. Seventy straight and 50 tilted implants were placed to rehabilitate 14 mandibles and 12 maxillae in 20 patients. After a follow-up of 12 to 36 months, survival rate was 97.1% for straight implants and 96.0% for tilted implants; while success rates were 94.3% and 94.0%, respectively. Success and survival rates were not significantly different (P > .05). Change in crestal bone level was 0.5 ± 0.4 mm for straight implants and 0.6 ± 0.4 mm for tilted implants (P > .05). Straight and tilted implants seemed to have similar behavior after immediate loading rehabilitations. After functional loading, straight and tilted implants did not differ significantly in clinical outcome.

Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914

On September 14, 2015, a gravitational wave signal from a coalescing black hole binary system was observed by the Advanced LIGO detectors. This paper describes the transient noise backgrounds used to determine the significance of the event (designated GW150914) and presents the results of investigations into potential correlated or uncorrelated sources of transient noise in the detectors around the time of the event. The detectors were operating nominally at the time of GW150914. We have ruled out environmental influences and non-Gaussian instrument noise at either LIGO detector as the cause of the observed gravitational wave signal.

Properties of the Binary Black Hole Merger GW150914

On September 14, 2015, the Laser Interferometer Gravitational-Wave Observatory (LIGO) detected a gravitational-wave transient (GW150914); we characterize the properties of the source and its parameters. The data around the time of the event were analyzed coherently across the LIGO network using a suite of accurate waveform models that describe gravitational waves from a compact binary system in general relativity. GW150914 was produced by a nearly equal mass binary black hole of masses 36_{-4}^{+5}M_{⊙} and 29_{-4}^{+4}M_{⊙}; for each parameter we report the median value and the range of the 90% credible interval. The dimensionless spin magnitude of the more massive black hole is bound to be <0.7 (at 90% probability). The luminosity distance to the source is 410_{-180}^{+160}  Mpc, corresponding to a redshift 0.09_{-0.04}^{+0.03} assuming standard cosmology. The source location is constrained to an annulus section of 610  deg^{2}, primarily in the southern hemisphere. The binary merges into a black hole of mass 62_{-4}^{+4}M_{⊙} and spin 0.67_{-0.07}^{+0.05}. This black hole is significantly more massive than any other inferred from electromagnetic observations in the stellar-mass regime.

GW150914: First results from the search for binary black hole coalescence with Advanced LIGO

On September 14, 2015 at 09:50:45 UTC the two detectors of the Laser Interferometer Gravitational-wave Observatory (LIGO) simultaneously observed the binary black hole merger GW150914. We report the results of a matched-filter search using relativistic models of compact-object binaries that recovered GW150914 as the most significant event during the coincident observations between the two LIGO detectors from September 12 to October 20, 2015. GW150914 was observed with a matched filter signal-to-noise ratio of 24 and a false alarm rate estimated to be less than 1 event per 203000 years, equivalent to a significance greater than 5.1 σ.

GW150914: First results from the search for binary black hole coalescence with Advanced LIGO

On September 14, 2015 at 09:50:45 UTC the two detectors of the Laser Interferometer Gravitational-wave Observatory (LIGO) simultaneously observed the binary black hole merger GW150914. We report the results of a matched-filter search using relativistic models of compact-object binaries that recovered GW150914 as the most significant event during the coincident observations between the two LIGO detectors from September 12 to October 20, 2015. GW150914 was observed with a matched filter signal-to-noise ratio of 24 and a false alarm rate estimated to be less than 1 event per 203000 years, equivalent to a significance greater than 5.1 σ.

Tests of General Relativity with GW150914

The LIGO detection of GW150914 provides an unprecedented opportunity to study the two-body motion of a compact-object binary in the large-velocity, highly nonlinear regime, and to witness the final merger of the binary and the excitation of uniquely relativistic modes of the gravitational field. We carry out several investigations to determine whether GW150914 is consistent with a binary black-hole merger in general relativity. We find that the final remnant's mass and spin, as determined from the low-frequency (inspiral) and high-frequency (postinspiral) phases of the signal, are mutually consistent with the binary black-hole solution in general relativity. Furthermore, the data following the peak of GW150914 are consistent with the least-damped quasinormal mode inferred from the mass and spin of the remnant black hole. By using waveform models that allow for parametrized general-relativity violations during the inspiral and merger phases, we perform quantitative tests on the gravitational-wave phase in the dynamical regime and we determine the first empirical bounds on several high-order post-Newtonian coefficients. We constrain the graviton Compton wavelength, assuming that gravitons are dispersed in vacuum in the same way as particles with mass, obtaining a 90%-confidence lower bound of 10^{13}  km. In conclusion, within our statistical uncertainties, we find no evidence for violations of general relativity in the genuinely strong-field regime of gravity.

GW150914: Implications for the Stochastic Gravitational-Wave Background from Binary Black Holes

The LIGO detection of the gravitational wave transient GW150914, from the inspiral and merger of two black holes with masses ≳30M_{⊙}, suggests a population of binary black holes with relatively high mass. This observation implies that the stochastic gravitational-wave background from binary black holes, created from the incoherent superposition of all the merging binaries in the Universe, could be higher than previously expected. Using the properties of GW150914, we estimate the energy density of such a background from binary black holes. In the most sensitive part of the Advanced LIGO and Advanced Virgo band for stochastic backgrounds (near 25 Hz), we predict Ω_{GW}(f=25  Hz)=1.1_{-0.9}^{+2.7}×10^{-9} with 90% confidence. This prediction is robustly demonstrated for a variety of formation scenarios with different parameters. The differences between models are small compared to the statistical uncertainty arising from the currently poorly constrained local coalescence rate. We conclude that this background is potentially measurable by the Advanced LIGO and Advanced Virgo detectors operating at their projected final sensitivity.

GW150914: The Advanced LIGO Detectors in the Era of First Discoveries

Following a major upgrade, the two advanced detectors of the Laser Interferometer Gravitational-wave Observatory (LIGO) held their first observation run between September 2015 and January 2016. With a strain sensitivity of 10^{-23}/sqrt[Hz] at 100 Hz, the product of observable volume and measurement time exceeded that of all previous runs within the first 16 days of coincident observation. On September 14, 2015, the Advanced LIGO detectors observed a transient gravitational-wave signal determined to be the coalescence of two black holes [B. P. Abbott et al., Phys. Rev. Lett. 116, 061102 (2016)], launching the era of gravitational-wave astronomy. The event, GW150914, was observed with a combined signal-to-noise ratio of 24 in coincidence by the two detectors. Here, we present the main features of the detectors that enabled this observation. At full sensitivity, the Advanced LIGO detectors are designed to deliver another factor of 3 improvement in the signal-to-noise ratio for binary black hole systems similar in mass to GW150914.

Observation of Gravitational Waves from a Binary Black Hole Merger

On September 14, 2015 at 09:50:45 UTC the two detectors of the Laser Interferometer Gravitational-Wave Observatory simultaneously observed a transient gravitational-wave signal. The signal sweeps upwards in frequency from 35 to 250 Hz with a peak gravitational-wave strain of 1.0×10(-21). It matches the waveform predicted by general relativity for the inspiral and merger of a pair of black holes and the ringdown of the resulting single black hole. The signal was observed with a matched-filter signal-to-noise ratio of 24 and a false alarm rate estimated to be less than 1 event per 203,000 years, equivalent to a significance greater than 5.1σ. The source lies at a luminosity distance of 410(-180)(+160)  Mpc corresponding to a redshift z=0.09(-0.04)(+0.03). In the source frame, the initial black hole masses are 36(-4)(+5)M⊙ and 29(-4)(+4)M⊙, and the final black hole mass is 62(-4)(+4)M⊙, with 3.0(-0.5)(+0.5)M⊙c(2) radiated in gravitational waves. All uncertainties define 90% credible intervals. These observations demonstrate the existence of binary stellar-mass black hole systems. This is the first direct detection of gravitational waves and the first observation of a binary black hole merger.

Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO and Advanced Virgo

We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational-wave detectors over the next decade, with the intention of providing information to the astronomy community to facilitate planning for multi-messenger astronomy with gravitational waves. We determine the expected sensitivity of the network to transient gravitational-wave signals, and study the capability of the network to determine the sky location of the source. We report our findings for gravitational-wave transients, with particular focus on gravitational-wave signals from the inspiral of binary neutron-star systems, which are considered the most promising for multi-messenger astronomy. The ability to localize the sources of the detected signals depends on the geographical distribution of the detectors and their relative sensitivity, and 90% credible regions can be as large as thousands of square degrees when only two sensitive detectors are operational. Determining the sky position of a significant fraction of detected signals to areas of 5 deg2 to 20 deg2 will require at least three detectors of sensitivity within a factor of ∼ 2 of each other and with a broad frequency bandwidth. Should the third LIGO detector be relocated to India as expected, a significant fraction of gravitational-wave signals will be localized to a few square degrees by gravitational-wave observations alone.

Mental disorders and risk of suicide attempt: a national prospective study

Most mental disorders, when examined independently, are associated with an elevated risk for suicide attempt. However, mental disorders often co-occur, and that co-occurrence is well explained by models where specific mental disorders are understood as manifestations of latent dimensions of psychopathology. To date, it remains unclear whether the risk of suicide attempt is due to specific mental disorders, to specific dimensions of psychopathology (that is, internalizing and externalizing dimensions), to a general psychopathology factor or to a combination of these explanations. In a large nationally representative prospective survey, the National Epidemiologic Survey on Alcohol and Related Conditions (NESARC), we used structural equation modeling to examine the shared and specific effects of Axis I and Axis II disorders on the occurrence of suicide attempts in the general population and among individuals with a lifetime history of suicidal ideation. Effects of mental disorders on the risk of suicide attempt were exerted almost exclusively through a general psychopathology factor representing the shared effect across all mental disorders. Effects of remitted psychiatric disorders on the risk of suicide attempt were fully mediated by current mental disorders. Similar patterns of associations were found in individuals with suicidal ideation. These results held when using different approaches to modeling psychiatric comorbidity. Our findings underscore the importance of adopting dimensional approaches to comorbidity in the study of suicidal behavior. Because mental disorders increase the risk of suicide attempt through a general psychopathology liability, this dimension should be considered as an important therapeutic target to substantially advance suicide prevention.

Dye-sensitized-solar-cells based on calix[4]arene scaffolds

Calix[4]arene-based dyes open the possibility to prepare more D–π–A branched dyes for increasing light-current conversión efficiencies.

Improved upper limits on the stochastic gravitational-wave background from 2009-2010 LIGO and Virgo data

Gravitational waves from a variety of sources are predicted to superpose to create a stochastic background. This background is expected to contain unique information from throughout the history of the Universe that is unavailable through standard electromagnetic observations, making its study of fundamental importance to understanding the evolution of the Universe. We carry out a search for the stochastic background with the latest data from the LIGO and Virgo detectors. Consistent with predictions from most stochastic gravitational-wave background models, the data display no evidence of a stochastic gravitational-wave signal. Assuming a gravitational-wave spectrum of Ω_{GW}(f)=Ω_{α}(f/f_{ref})^{α}, we place 95% confidence level upper limits on the energy density of the background in each of four frequency bands spanning 41.5-1726 Hz. In the frequency band of 41.5-169.25 Hz for a spectral index of α=0, we constrain the energy density of the stochastic background to be Ω_{GW}(f)<5.6×10^{-6}. For the 600-1000 Hz band, Ω_{GW}(f)<0.14(f/900  Hz)^{3}, a factor of 2.5 lower than the best previously reported upper limits. We find Ω_{GW}(f)<1.8×10^{-4} using a spectral index of zero for 170-600 Hz and Ω_{GW}(f)<1.0(f/1300  Hz)^{3} for 1000-1726 Hz, bands in which no previous direct limits have been placed. The limits in these four bands are the lowest direct measurements to date on the stochastic background. We discuss the implications of these results in light of the recent claim by the BICEP2 experiment of the possible evidence for inflationary gravitational waves.

Search for gravitational waves associated with γ-ray bursts detected by the interplanetary network

We present the results of a search for gravitational waves associated with 223 γ-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, second, and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality gravitational wave data are available, we place lower bounds on the distance to the source in accordance with an optimistic assumption of gravitational wave emission energy of 10(-2)M⊙c(2) at 150 Hz, and find a median of 13 Mpc. For the 27 short-hard GRBs we place 90% confidence exclusion distances to two source models: a binary neutron star coalescence, with a median distance of 12 Mpc, or the coalescence of a neutron star and black hole, with a median distance of 22 Mpc. Finally, we combine this search with previously published results to provide a population statement for GRB searches in first-generation LIGO and Virgo gravitational wave detectors and a resulting examination of prospects for the advanced gravitational wave detectors.

Search for gravitational waves associated with γ-ray bursts detected by the interplanetary network

We present the results of a search for gravitational waves associated with 223 γ-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, second, and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality gravitational wave data are available, we place lower bounds on the distance to the source in accordance with an optimistic assumption of gravitational wave emission energy of 10(-2)M⊙c(2) at 150 Hz, and find a median of 13 Mpc. For the 27 short-hard GRBs we place 90% confidence exclusion distances to two source models: a binary neutron star coalescence, with a median distance of 12 Mpc, or the coalescence of a neutron star and black hole, with a median distance of 22 Mpc. Finally, we combine this search with previously published results to provide a population statement for GRB searches in first-generation LIGO and Virgo gravitational wave detectors and a resulting examination of prospects for the advanced gravitational wave detectors.

Hepatitis C virus NS3/4A quasispecies diversity in acute hepatitis C infection in HIV-1 co-infected patients

The growing number of cases of acute hepatitis C (AHC) infections among human immunodeficiency virus type 1 (HIV-1)-positive men who have sex with men (MSM) in the last 10 years has promoted the search for predictors of AHC clearance as well as for epidemiological networks of viral transmission. We characterized the diversity and catalytic efficiency of HCV NS3/4A protease quasispecies in AHC patients coinfected with HIV-1. Plasma samples obtained at HCV diagnosis from 18 MSM HIV-coinfected patients with AHC were studied. Five HCV monoinfected patient samples with AHC were also investigated. An average of 39 clones from each sample was analysed. The catalytic efficiency of the dominant quasispecies (i.e. the most abundant) from each quasispecies was also assayed for mitochondrial antiviral signalling protein (MAVS) cleavage. Phylogenetic analysis identified two clusters of patients with highly related viruses, suggesting a common source of HCV infection. None of the 18 MSM HIV-coinfected patients spontaneously cleared HCV, although 78% of the treated patients achieved a sustained virological response after early treatment with pegylated interferon (pegIFN) plus ribavirin (RBV). The synonymous-nonsynonymous (ds/dn) mutation ratio, a marker of selective pressure, was higher in AHC compared to 26 HIV-1-infected men with genotype 1a chronic hepatitis C (CHC) (P < 0.0001). NS3/4A proteases from AHC patients also exhibited higher catalytic efficiency compared to CHC patients (P < 0.0001). No differences were found when ds/dn mutation ratios and NS3/4A protease catalytic efficiencies from AHC HIV-coinfected patients were compared with AHC monoinfected patients. The presence of epidemiological networks of HCV transmission was confirmed among HIV-1-positive MSM. In addition, substantial genetic diversity was demonstrated in AHC. NS3/4A protease efficiency cleaving MAVS may be associated with virus transmission and response to pegIFN/RBV treatment.

Constraints on cosmic strings from the LIGO-Virgo gravitational-wave detectors

Cosmic strings can give rise to a large variety of interesting astrophysical phenomena. Among them, powerful bursts of gravitational waves (GWs) produced by cusps are a promising observational signature. In this Letter we present a search for GWs from cosmic string cusps in data collected by the LIGO and Virgo gravitational wave detectors between 2005 and 2010, with over 625 days of live time. We find no evidence of GW signals from cosmic strings. From this result, we derive new constraints on cosmic string parameters, which complement and improve existing limits from previous searches for a stochastic background of GWs from cosmic microwave background measurements and pulsar timing data. In particular, if the size of loops is given by the gravitational backreaction scale, we place upper limits on the string tension Gμ below 10(-8) in some regions of the cosmic string parameter space.

Local excision with adjuvant imatinib therapy for anorectal gastrointestinal stromal tumors

Rectal gastrointestinal stromal tumors (GISTs) are uncommon, and the role of local excision versus a more extensive resection after the advent of effective targeted chemotherapy with imatinib is not known. Our aim is to present two cases of large anorectal GIST treated with local excision through a new anterolateral trans-sphincteric approach followed by adjuvant therapy with imatinib. Two patients (both males, 68 and 63 years old) presented at our institution with anorectal GIST in the period October-November 2010. Their medical records, pathology results, and imaging studies were retrospectively reviewed. Both patients presented with an anterior perianal mass. Imaging studies were characteristic of GIST originating in the lower rectum, circumscribed by a pseudocapsule, and protruding into the ischiorectal fossa. Both patients underwent local excision via an anterolateral trans-sphincteric approach. Both tumors were removed intact, with microscopically negative margins. The maximum tumor diameter was 8 and 9 cm, and the diagnosis of GIST was confirmed by positive CD117 and CD34 staining in both cases. Both tumors had a high (>5/50HPF) mitotic index. The patients had an uneventful postoperative course and were discharged on days 5 and 6. Both patients were started on imatinib 400 mg bid postoperatively. Postoperative magnetic resonance imaging and positron emission tomography computed tomography were carried out at 12 months and did not reveal any signs of recurrence. The patients are currently disease-free at 24 and 23 months of follow-up. In selected cases, complete excision of rectal GIST with negative margins is feasible via a trans-sphincteric approach. With the use of adjuvant therapy, which is currently advocated in all high-risk cases, it is possible that local excision with its reduced morbidity may become a viable alternative, especially in patients who would otherwise require abdominoperineal excision such as the two presented here. Prospective studies with longer follow-up are needed to confirm adequate oncologic results.

Natural prevalence of HCV minority variants that are highly resistant to NS3/4A protease inhibitors

Minority drug-resistant hepatitis C virus (HCV) variants may go undetected yet be clinically important. NS3/4A protease resistance substitutions V36A and A156S/T/V were selected in patients treated with protease inhibitors. The aim of this study was to investigate whether these substitutions pre-existed in HCV infected patients. An allele-specific PCR protocol that detected the NS3/4A protease resistance substitutions V36A and A156S/T/V was used to determine the prevalence of naturally occurring variants in 45 patients. All patient samples were infected with HCV of genotype 1b and were naïve for pegIFNα/ribavirin treatment. Thirty samples (67%) had at least one HCV PI-resistant variant. A156T (23, 51%) was detected more frequently than A156V (13, 29%) or A156S (1, 2%). V36A was detected in 12 samples (27%). These results demonstrate the high prevalence of minority drug-resistant NS3/4 protease resistance substitutions. Our results also demonstrate that allele-specific PCR can be used to detect minor HCV NS3 protease resistant variants in pretreatment samples and to study in detail the evolution of mutant viruses during targeted antiviral therapy.

An Evaluation of the Safety and Efficacy of Lapatinib Plus Trastuzumab Plus Paclitaxel in First-Line HER2+ Metastatic Breast Cancer

Background: Trastuzumab given concomitantly with paclitaxel is an established first-line metastatic breast cancer (MBC) treatment; however, approximately 30% to 40% of patients show no response as defined by RECIST to this combination. Lapatinib is an oral dual tyrosine kinase inhibitor of EGFR and HER2 and approved, in combination with capecitabine, after trastuzumab-based therapy for HER2+ MBC. The differing mechanisms of action may allow synergy between lapatinib and trastuzumab when given concurrently with paclitaxel for MBC.Methods: This is an open-label phase I safety study. The primary objective of the study was to assess the safety and tolerability of lapatinib when administered with concurrent paclitaxel and trastuzumab. Patients were enrolled into 1 of 3 cohorts. Cohort 1 received lapatinib (1000 mg/d), paclitaxel (80 mg/m2 weekly for 3 weeks of a 4-week cycle), and the standard weekly dose of trastuzumab. Cohort 2 received lapatinib (1000 mg/d), paclitaxel (70 mg/m2), and trastuzumab. Cohort 3 received lapatinib (750 mg/d), paclitaxel (80 mg/m2), and trastuzumab. Patients: were 3+ by IHC or FISH amplified for HER2; had not received prior treatment in the metastatic setting; and had an ECOG performance status of 0 or 1. Safety was assessed weekly and tumor response per RECIST every 8 weeks. Treatment continued until disease progression or toxicity. All patients received prophylactic loperamide per protocol amendment.Results: Open-label safety enrollment is complete and preliminary safety data are available for all 63 patients. The most frequently reported AEs for all cohorts were diarrhea (81%), fatigue (71%), rash (68%), nausea (59%), alopecia (56%), and vomiting (37%). Dehydration was the most frequently reported serious AE (SAE) (n=6; 10%) and most were in cohort 1 (5 patients). Diarrhea of any grade was reported for 97% of patients in cohort 1, 93% of patients in cohort 2, and 50% of patients in cohort 3. No grade 4 or 5 diarrhea events were reported. The proportion of patients with a maximum toxicity of grade 3 diarrhea was 62% in cohort 1, 43% in cohort 2, and 20% in cohort 3. Two patients (both in cohort 1) reported diarrhea as a serious AE and a total of 4 patients (6%) had lapatinib withdrawn due to diarrhea (none in cohort 3).Conclusions: Preliminary safety results show a high incidence of grade 3 diarrhea when lapatinib was given at a dose of 1000 mg/d concurrently with paclitaxel and trastuzumab. This incidence was significantly reduced with a lapatinib dose of 750 mg/d in combination with paclitaxel and trastuzumab when given with loperamide. Final safety and efficacy data, including overall response and progression-free survival, from this open-label safety study will be presented.

Citation Information: Cancer Res 2009;69(24 Suppl):Abstract nr 5085.

Cardiac Safety of Lapatinib Given Concurrently with Paclitaxel and Trastuzumab as Part of Adjuvant Therapy for Patients with HER2+ Breast Cancer: Pilot Data from the Mayo Clinic Cancer Research Consortium Trial RC0639

Background: Despite the impressive results of the trastuzumab adjuvant therapy trials, 15% of patients (pts) with HER2 overexpressing or amplified breast cancer developed tumor relapse at 4 years. Lapatinib is a reversible tyrosine kinase inhibitor against ErbB1 and ErbB2. The current study was developed to assess the cardiac safety and feasibility of adding lapatinib to paclitaxel and trastuzumab following doxorubicin and cyclophosphamide as part of adjuvant therapy.Methods: A single-arm phase II study of doxorubicin (A, 60 mg/m2 day 1) and cyclophosphamide (C, 600 mg/m2 day 1) [q2w or q3w for 4 cycles]; followed by PTL: paclitaxel (P, 80 mg/m2 weekly), trastuzumab (T, 4 mg/kg loading dose then 2 mg/kg weekly), and lapatinib (L, 1000 mg PO daily which was later amended to 750 mg) [total of 12 weeks of treatment]; followed by T (6 mg/kg day 1, every 3 weeks) and L (1000 mg PO daily) [total of 40 weeks of treatment] was conducted. The primary endpoint was severe symptomatic congestive heart failure (CHF: New York Heart Association Class III or IV with a drop in left ventricular ejection fraction [LVEF] of at least 10 percentage points to below 50% confirmed by cardiologist) with secondary endpoints of cardiac death and grade 3+ cardiac adverse events (AEs).Results: From April 2007 to October 2008, 109 evaluable pts were enrolled and initiated study treatment. Median age was 51 (range 28-72). Median follow-up is 10.2 months. No pts experienced CHF or cardiac death while on active treatment. One pt had CHF and 1 pt died due to myocardial infarction (MI) after they went off study treatment. The pt with CHF refused further treatment after completing 2 cycles of PTL and had CHF 1.8 months post PTL discontinuation with LVEF of 45% and dyspnea on exertion. The pt with MI went off study treatment due to non-cardiac AEs after completing 2 cycles of PTL and died 2.9 months post PTL discontinuation. Mean LVEF at baseline was 63.6% (N=109, SD=5.7); end of AC was 63.3% (N=104, SD=6.4); end of PTL was 59.9% (N=89, SD=8.3); and cycle 12 was 59.7% (N=66, SD=7.1). Grade 3+ non-hematologic AEs with incidence &gt;5% include diarrhea (N=42, 39% & included both 1000mg & later amended 750mg dosing), fatigue (N=15, 14%), nausea (N=7, 6%), vomiting (N=7, 6%), acne (N=6, 6%), and hypokalemia (N=6, 6%). Pre-treatment cardiac marker data (troponin-T, troponin-I, brain natriuretic peptide, creatine kinase MB isoenzyme) will also be presented.Conclusions: Preliminary data suggest that the inclusion of L does not add to the cardiac profile of T. Data from ALTTO and long-term follow data are needed to confirm the cardiac safety of this regimen. Cardiac marker data are being analyzed in the context of changes in LVEF. We gratefully acknowledge support from the Breast Cancer Research Foundation and GlaxoSmthKline for this study.

Citation Information: Cancer Res 2009;69(24 Suppl):Abstract nr 3086.

Circulating tumor cell and endothelial cell data from a phase II evaluation of lapatinib and bevacizumab in HER2-overexpressing metastatic breast cancer

Abstract #3154

Background: Overexpression of both HER2 and VEGF is associated with worse outcome than overexpression of either receptor alone. In preclinical models, combination anti-HER2 and anti-VEGF therapy has been shown to be more effective than either treatment alone. Bevacizumab (B) plus trastuzumab and lapatinib (L) plus pazopanib have shown activity in patients (pts) with HER2+ MBC. We evaluated the combination of L+B in a phase 2 trial in HER2+ MBC pts. To explore new biomarkers of treatment effect, we measured circulating tumor cells (CTCs) with two different methods of CTC enumeration: CellSearch (Veridex LLC), and immunomagnetic enrichment followed by flow cytometry (IE/FC), as well as circulating endothelial cells (CECs) in pts receiving study treatment.&#x2028; Methods: This study evaluated L (1500 mg PO daily) plus B (10 mg/kg IV q2wk) in 50 HER2+ MBC pts. The primary endpoint is crude progression-free survival (PFS) at 12 wks. Serial evaluation of CTC and CEC was performed. Blood was obtained from consenting pts at baseline, weeks 2, 6 then every 12 weeks until end of study. CellSearch assay was performed as previously described using 7.5 cc blood in a CellSave tube and the CellSpotter analyzer. For IE/FC, 20 ml of blood was subjected to IE using anti-EpCAM ferrofluid, followed by FC for EpCAM, CD45, and nucleic acid content. CTC data were correlated with assay method and with best response. CECs were defined as CD34/31+, CD45-, or CD34/146+, CD45-, and were assayed by FC.&#x2028; Results: Enrollment to this study ended in March 2008 (n=52). Clinical data is presented at this meeting (Dickler et al). 47 patients have evaluable CTC and CEC data at baseline and/or first follow-up; 32 patients have response data. CTC determined by CellSearch or IE/FC showed significant correlation at baseline (R=0.58; P=0.012). CTC by CellSearch at first followup correlated with treatment response (P=0.01) with levels above 5 CTC/sample associated with progression; there was no correlation with baseline values. There were too few positive IE/FC values to evaluate correlation with outcome. The change in CEC/CD146 from baseline to first followup for is of borderline significance in this preliminary analysis (P=0.07) between PR (N=2, Mean Change Score/MCS=-4.345) and SD/PD (N=18, MCS=0.8); a decrease of CEC/CD146 from baseline to first followup suggests greater likelihood of response.&#x2028; Conclusions: L+B is an active regimen in pts with MBC. CTC measurements correlated between two separate methodologies, and for the CellSearch assay predicted response to therapy. A decrease in CEC from baseline to first followup correlated with response to this combined targeted therapy, consistent with our previous results with other B-based therapy. PFS and response correlations for the full study cohort will be presented.

Citation Information: Cancer Res 2009;69(2 Suppl):Abstract nr 3154.

The influence of early counselling on weaning from a bottle

OBJECTIVES

To evaluate the effectiveness of intensive counselling on bottle weaning.

METHODS

A randomised prospective controlled study was conducted. Parents of 4-month-old babies who attended an inner-city clinic affiliated with the Department of Paediatrics, University of Louisville, Louisville, Kentucky with predominately African-American, indigent population were invited to participate. The parent/infant pairs were randomized to either intervention or control groups. Demographic information was recorded and both groups were surveyed on the parent's beliefs and knowledge of weaning from the bottle. The intervention group parents received scripted counselling, including use of feeding cups, and were shown pictures of severe early childhood caries and a dental model of early childhood caries at four, six, nine, and 12 month visits. Two paediatricians who are on the clinic staff used the same script when talking to parents while showing the same photos and dental model to assure symmetry. The control group parents received brief counselling on the use of a feeding cup at 6 month and bottle weaning at nine and 12 months with no photographs or dental models shown. Two dentists, blinded to the group assignment, examined all of the children between the ages of 12 months and 24 months.

RESULTS

One hundred eighty-five parent/infant pairs were enrolled and 132 pairs (65 control and 67 intervention) remained at the end of the study. Demographic variables, socioeconomic status and race were similar for both groups. When surveyed, more of the control mothers believed that children should be weaned by 12 months (p = 0.049). Yet, only 17% of their infants were weaned by 12 months, compared to 27% of the intervention infants (p = 0.168).

CONCLUSION

This small study demonstrated no change in parental behaviour after intense counselling.