Search results for "Compact"

showing 10 items of 531 documents

Analytical approach for the mix design optimisation of bituminous mixtures with crumb rubber

2018

The present paper provides a basis for defining a mix design method specifically tailored to rubberised asphalt that takes into account the behaviour of crumb rubber. An analytical approach to quantifying the recovered deformation of crumb rubber in the post-compaction phase has been developed in order to adjust the number of gyrations proposed by the Superpave method for compacting specimens of hot mix asphalt using a Superpave gyratory compactor. The maximum allowable amount of rubber has been calculated. Finally, a step-by-step protocol has been proposed in order to fabricate and compact crumb rubber modified mixtures with the gyratory compactor.

Crumb rubber; Mix design; Rubberised asphalt; Superpave gyratory compactor; Civil and Structural Engineering; Building and Construction; Materials Science (all); Mechanics of MaterialsMaterials science0211 other engineering and technologies020101 civil engineeringMix design02 engineering and technologyMix designRubberised asphalt0201 civil engineeringNatural rubberAsphalt pavement021105 building & constructionSettore ICAR/04 - Strade Ferrovie Ed AeroportiGeneral Materials ScienceCrumb rubberComposite materialCivil and Structural EngineeringCrumb rubberBuilding and ConstructionStrength of materialsSuperpave gyratory compactorCrumb rubber Superpave gyratory compactor Mix design Rubberised asphaltAsphaltMechanics of Materialsvisual_artSolid mechanicsvisual_art.visual_art_mediumMaterials Science (all)Deformation (engineering)
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Increased Stability of Rubber-Modified Asphalt Mixtures to Swelling, Expansion and Rebound Effect during Post-Compaction

2017

The application of bituminous mixtures modified with rubber from scrap-tires require attention and care during mixing and compaction. Rubber modifies the properties because it reacts in the internal structure of bitumen at high temperatures changing the performance of the mixture (interaction process of solvents with binder-rubber aggregate). The main change is the increasing of the viscosity and elasticity of the binder due to the larger sizes of the rubber particles by dry process but, this positive effect is counteracted by short mixing times, compared to wet technology, and due to the transport processes, curing time and post-compaction of the mixtures. Therefore, negative effects as sw…

Crumb-rubber Gyratory Compactor Rebounding Effect Superpave Mix-Design Swelling Sub-ballast Railway.Settore ICAR/04 - Strade Ferrovie Ed Aeroporti
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Slow-roll corrections in multi-field inflation: a separate universes approach

2018

In view of cosmological parameters being measured to ever higher precision, theoretical predictions must also be computed to an equally high level of precision. In this work we investigate the impact on such predictions of relaxing some of the simplifying assumptions often used in these computations. In particular, we investigate the importance of slow-roll corrections in the computation of multi-field inflation observables, such as the amplitude of the scalar spectrum $P_\zeta$, its spectral tilt $n_s$, the tensor-to-scalar ratio $r$ and the non-Gaussianity parameter $f_{NL}$. To this end we use the separate universes approach and $\delta N$ formalism, which allows us to consider slow-roll…

DYNAMICSCosmology and Nongalactic Astrophysics (astro-ph.CO)ComputationFOS: Physical sciencesCMB01 natural sciences114 Physical sciences0103 physical sciencesStatistical physicsinflationMULTICOMPONENT INFLATON010303 astronomy & astrophysicsPhysicsSPECTRUMSlow roll010308 nuclear & particles physicsEquations of motionCONSTRAINTSAstronomy and AstrophysicsObservableCOSMOLOGICAL PERTURBATIONSEXPANSION115 Astronomy Space scienceAmplitudeHypersurfacecosmological perturbation theoryCompact formMulti field2ND-ORDERAPPROXIMATIONGENERATIONAstrophysics - Cosmology and Nongalactic Astrophysics
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Nigral influence on focal epilepsy.

1990

The substantia nigra (SN) has been proposed as a structure involved in epileptiform phenomena. Previous investigations demonstrated that SN is able to elicit hippocampal rhythmic slow activity (RSA) as well as to inhibit hippocampal interictal spikes induced by parenteral administration of penicillin. The present series of experiments was carried out in order to characterize the action of SN on a focal model of hippocampal epilepsy. Experiments were performed on encephale isole cats in which steady epileptiform activity was induced by locally applied penicillin. Electrical stimulation of SN pars reticulata (pr) caused a statistically significant decrease of hippocampal spike frequency and a…

Decerebrate StateChemistryPars compactaHippocampusStimulationSubstantia nigraGeneral MedicinePenicillinsHippocampal formationInhibitory postsynaptic potentialHippocampusElectric StimulationSubstantia NigraNeurologyPhysiology (medical)CatsAnimalsIctalNeurology (clinical)Epilepsies PartialPars reticulataNeuroscienceNeurophysiologie clinique = Clinical neurophysiology
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Second Generation of Freescoo Solar DEC Prototypes for Residential Applications

2015

Freescoo is an innovative all-in-one compact solar Desiccant Evaporative Cooling (DEC) air conditioner concept. Results of the first prototype developed were presented at SHC Conference last year. Now a second generation of freescoo prototypes for applications in residential and small office buildings have been installed in Italy at ENEA Casaccia and at UNIPA. The thermodynamic cycle is based on the use of fixed and cooled adsorption beds and advanced evaporative cooling concepts. The adsorption bed, which is a fin and tube heat exchanger packed with silica gel grains, allows simultaneous dehumidification and cooling of the process air. The indirect evaporative cooling process, operated dow…

Desiccantfreescoo compact Solar DEC Adsorption fixed and cooled bed stand-alone operationEngineeringSettore ING-IND/11 - Fisica Tecnica Ambientalebusiness.industryWet-bulb temperatureNuclear engineeringElectrical engineeringPlate heat exchangerstand-alone operationfreescooAdsorption fixed and cooled bedtand-alone operationstand-alone operation ;Energy(all)Air conditioningThermodynamic cycleThermalHeat exchangercompact Solar DECAdsorption fixed and cooled bed;freescoo;compact Solar DEC;stand-alone operationbusinessEvaporative coolerEnergy Procedia
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GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences

2018

The LIGO Scientific and Virgo Collaborations have announced the first detection of gravitational waves from the coalescence of two neutron stars. The merger rate of binary neutron stars estimated from this event suggests that distant, unresolvable binary neutron stars create a significant astrophysical stochastic gravitational-wave background. The binary neutron star background will add to the background from binary black holes, increasing the amplitude of the total astrophysical background relative to previous expectations. In the Advanced LIGO-Virgo frequency band most sensitive to stochastic backgrounds (near 25 Hz), we predict a total astrophysical background with amplitude $\Omega_{\rm…

Design sensitivityneutron star: binarygravitational radiation: stochasticAstronomyX-ray binaryGeneral Physics and AstronomyAstrophysicsAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologylocalizationGravitational wave backgroundGravitational Waves Neutron Stars Stochastic Background Virgo LIGOblack holeLIGOstochastic modelQCQBPhysicsGAMMA-RAY BURSTSSignal to noise ratioStochastic systemsBlack holesGravitational effectsarticleAstrophysics::Instrumentation and Methods for AstrophysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSING[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave sources Experimental studies of gravity Gravitational WavesGravitationBinary neutron starsX-ray bursterBinsAstrophysics::High Energy Astrophysical PhenomenaMERGERSFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsGravity wavesgravitational radiation: direct detectionBinary pulsarNeutron starsSTAR-FORMATIONPhysics and Astronomy (all)General Relativity and Quantum CosmologyBinary black holebinary: coalescence0103 physical sciencesFrequency bandsddc:530RATESINTERFEROMETERS010306 general physicsAstrophysics::Galaxy AstrophysicsNeutronsGravitational Waves010308 nuclear & particles physicsGravitational waveVirgogravitational radiation: backgroundgravitational radiationAstronomyNeutron Stars530 Physikbinary: compactsensitivityStarsLIGObackground: stochasticEVOLUTIONsignal noise ratioVIRGOPhysics and Astronomyblack hole: binarygravitational radiation: emissionStellar black holeStochastic BackgroundDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikHIGH-REDSHIFTneutron star: coalescencePhysical Review Letters
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Electrochemical detection of chloride ions using Ag-based electrodes obtained from compact disc

2022

Abstract In this work electrochemical sensors fabricated from compact disc material (waste or new) are used to quantify chloride ions in different types of samples. All three electrodes, working, counter, and pseudo-reference electrodes, were fabricated from the compact disc and directly used. Different parameters were studied in order to demonstrate the possibility of using this waste material for efficient and low-cost electrochemical sensors. Chloride sensing performance was evaluated using linear scan voltammetry as the detection technique. A sensitivity of 0.174 mA mM−1 cm−2 with a limit of detection of 20 μM and excellent selectivity against many interferents was observed. Selectivity…

Detection limitReproducibilityCompact DisksChemistryAnalytical chemistryReproducibility of ResultsElectrochemical TechniquesElectrochemistryBiochemistryChlorideAnalytical ChemistryElectrochemical gas sensorSettore ING-IND/23 - Chimica Fisica ApplicataChloridesChloride ions Compact disc Cystic fibrosis Disposable sensor Electrochemical sensor Real time monitoring Water quality Wearable sensorsElectrodeSettore ING-IND/17 - Impianti Industriali MeccanicimedicineEnvironmental ChemistrySelectivityVoltammetryElectrodesSpectroscopymedicine.drug
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Search for Subsolar Mass Ultracompact Binaries in Advanced LIGO's Second Observing Run

2019

We present a search for subsolar mass ultracompact objects in data obtained during Advanced LIGO’s second observing run. In contrast to a previous search of Advanced LIGO data from the first observing run, this search includes the effects of component spin on the gravitational waveform. We identify no viable gravitational-wave candidates consistent with subsolar mass ultracompact binaries with at least one component between \ud0.2\ud \ud \udM\ud⊙\ud–\ud1.0\ud \ud \udM\ud⊙\ud. We use the null result to constrain the binary merger rate of (\ud0.2\ud \ud \udM\ud⊙\ud, \ud0.2\ud \ud \udM\ud⊙\ud) binaries to be less than \ud3.7\ud×\ud10\ud5\ud \ud \udGpc\ud−\ud3\ud \udyr\ud−\ud1\udand the binary …

Dewey Decimal Classification::500 | Naturwissenschaften::550 | Geowissenschaftenbinary: massAstrofísicaGravitacióFormation modeldensity: fluctuationAstronomyGeneral Physics and Astronomydetector: networkspin01 natural sciencesGeneral Relativity and Quantum CosmologyLIMITSblack hole: formationddc:550black holeDark MatterAstrophysics::Solar and Stellar AstrophysicsLIGOQCQBnucleus: interactionSettore FIS/01astro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)gravitational wave; physics; astronomyPhysicsarticleDensity fluctuationgravitational wavesPhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]astro-ph.COAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomenablack hole: primordialGravitationAstrophysics - Cosmology and Nongalactic AstrophysicsMatter densitydensity: primordialCosmology and Nongalactic Astrophysics (astro-ph.CO)coolinggr-qcAstrophysics::High Energy Astrophysical PhenomenaPhysics MultidisciplinaryCooling mechanismPrimordial black holesFOS: Physical sciencesdark matter: densityGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsGravity wavesNuclear interactionGravitation and AstrophysicsMergingGeneral Relativity and Quantum Cosmologynull resultSettore FIS/05 - Astronomia e Astrofisicabinary: coalescence0103 physical sciencesddc:530010306 general physicsAstrophysics::Galaxy AstrophysicsSTFCScience & Technologymass: solarCosmologiaStellar evolutions010308 nuclear & particles physicsMatter fractionsgravitational radiationRCUKblack hole: massGalaxiesbinary: compactStarsgravitational radiation detectordetector: sensitivityVIRGOPhysics and Astronomygravitational radiation: emissionDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Gravitational waves Black holes (astronomy) Gravitational self forcePhysical Review Letters
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Search for Subsolar-Mass Ultracompact Binaries in Advanced LIGO's First Observing Run

2018

We present the first Advanced LIGO and Advanced Virgo search for ultracompact binary systems with component masses between 0.2 $M_\odot$ - 1.0 $M_\odot$ using data taken between September 12, 2015 and January 19, 2016. We find no viable gravitational wave candidates. Our null result constrains the coalescence rate of monochromatic (delta function) distributions of non-spinning (0.2 $M_\odot$, 0.2 $M_\odot$) ultracompact binaries to be less than $1.0 \times 10^6 \text{Gpc}^{-3} \text{yr}^{-1}$ and the coalescence rate of a similar distribution of (1.0 $M_\odot$, 1.0 $M_\odot$) ultracompact binaries to be less than $1.9 \times 10^4 \text{Gpc}^{-3} \text{yr}^{-1}$ (at 90 percent confidence). N…

Dewey Decimal Classification::500 | Naturwissenschaften::550 | Geowissenschaftendensity: fluctuationMACHOAstronomyGeneral Physics and AstronomyPrimordial black holeAstrophysicsCoalescence01 natural sciencesGeneral Relativity and Quantum CosmologylocalizationLIMITSddc:550Massive compact halo objectLIGOneutron starQCQBPhysicseducation.field_of_studyPhysicsDensity fluctuationBinary systemsgravitational wavesPhysical SciencesSearch enginesastro-ph.COblack hole: primordialAstrophysics - Cosmology and Nongalactic AstrophysicsGravitationCosmology and Nongalactic Astrophysics (astro-ph.CO)gr-qcBinary formationAstrophysics::High Energy Astrophysical PhenomenaPopulationDark matterPhysics MultidisciplinaryEarly universeFOS: Physical sciencesPrimordial black holesGeneral Relativity and Quantum Cosmology (gr-qc)dark matter: densityAstrophysics::Cosmology and Extragalactic AstrophysicsGravity wavesCoalescence rateGravitation and AstrophysicsPhysics and Astronomy (all)General Relativity and Quantum Cosmologybinary: coalescence0103 physical sciencesddc:530Delta functions010306 general physicseducationSTFCAstrophysics::Galaxy AstrophysicsScience & Technologymass: solar010308 nuclear & particles physicsGravitational waveStellar evolutionsbinary: formationgravitational radiationRCUKblack hole: massGalaxiesStarsGalaxyLIGOBlack holeVIRGOPhysics and Astronomyblack hole: binarygravitational radiation: emissionDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikMicro-lensing[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Tests of General Relativity with GW170817

2019

The recent discovery by Advanced LIGO and Advanced Virgo of a gravitational wave signal from a binary neutron star inspiral has enabled tests of general relativity (GR) with this new type of source. This source, for the first time, permits tests of strong-field dynamics of compact binaries in presence of matter. In this paper, we place constraints on the dipole radiation and possible deviations from GR in the post-Newtonian coefficients that govern the inspiral regime. Bounds on modified dispersion of gravitational waves are obtained; in combination with information from the observed electromagnetic counterpart we can also constrain effects due to large extra dimensions. Finally, the polari…

Dewey Decimal Classification::500 | Naturwissenschaften::550 | Geowissenschaftenneutron star: binaryAstronomyTestingGravitational WaveGeneral Physics and AstronomyAstrophysics01 natural sciencesGeneral Relativity and Quantum Cosmologystrong fieldddc:550general relativityLIGOQCSettore FIS/01PhysicsPhysicsGravitational effectsarticlePolarization (waves)Gravitational-wave signalsExtra dimensionsgravitational wavesPhysical SciencesExtra dimensions[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Large extra dimensiondispersionBinary neutron starsgravitational radiation: polarizationGeneral RelativityGeneral relativitygr-qcPhysics MultidisciplinaryGRAVITATIONAL-WAVE OBSERVATIONSFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)gravitational wavesblack holesGravity wavesMASSgravitational radiation: direct detectionGravitation and Astrophysicselectromagnetic field: productionRelativityGeneral Relativity and Quantum CosmologyDipole radiationsGRAVITYTests of general relativitygravitation: weak field0103 physical sciencesddc:530High Energy Physicscapture010306 general physicsGravitational Wave; General RelativitySTFCradiation: dipolepolarizationScience & TechnologyStrong fieldGravitational wavegravitational radiationRCUKbinary: compactgravitational radiation detectorLIGONeutron starVIRGODewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikNewtonianshigher-dimensional
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