Search results for "Particle radiation"

showing 10 items of 677 documents

Study on heat transfer coefficients during cooling of PET bottles for food beverages

2015

The heat transfer properties of different cooling systems dealing with Poly-Ethylene-Terephthalate (PET) bottles were investigated. The heat transfer coefficient (Ug) was measured in various fluid dynamic conditions. Cooling media were either air or water. It was shown that heat transfer coefficients are strongly affected by fluid dynamics conditions, and range from 10 W/m2 K to nearly 400 W/m2 K. PET bottle thickness effect on Ug was shown to become relevant under faster fluid dynamics regimes.

Fluid Flow and Transfer ProcessesRange (particle radiation)Natural convectionMaterials sciencebusiness.product_category020209 energyThermodynamics02 engineering and technologyHeat transfer coefficientCondensed Matter PhysicCondensed Matter PhysicsHeat transfer0202 electrical engineering electronic engineering information engineeringFluid dynamicsBottlebusiness
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Synthesis of complex organic molecules in soft x-ray irradiated ices

2019

We study the chemical evolution of H2O:CO:NH3 ice mixtures irradiated with soft X-rays, in the range 250-1250 eV. We identify many nitrogen-bearing molecules such as e.g., OCN-, NH4+ , HNCO, CH3CN, HCONH2, and NH2COCONH2. Several infrared features are compatible with glycine or its isomers. During the irradiation, we detected through mass spectroscopy many species desorbing the ice. Such findings support either the infrared identifications and reveal less abundant species with not clear infrared features. Among them, m/z = 57 has been ascribed to methyl isocyanate (CH3NCO), a molecule of prebiotic relevance, recently detected in protostellar environments. During the warm up after the irradi…

FormamidePhysicsRange (particle radiation)010504 meteorology & atmospheric sciencesInfraredAnalytical chemistryFOS: Physical sciencesAstronomy and AstrophysicsMass spectrometry01 natural sciencesAstrophysics - Astrophysics of GalaxiesStarschemistry.chemical_compoundchemistrySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)0103 physical sciencesMoleculeOrganic synthesisIrradiation010303 astronomy & astrophysics0105 earth and related environmental sciences
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Controlling laser assisted radiative recombination with few-cycle laser pulses

2006

We report on the radiative recombination of a free electron with a hydrogenic ion in the presence of a few-cycle pulses. It has been shown that the main features of the emission spectra may be described in the framework of a semiclassical model in which the recombination is viewed as a two-step process. The spectra width of the emitted photon energy is practically confined in a range of values in which the emission is classically allowed. Moreover, it has been found that spectra width can be controlled by varying the carrier envelope phase and/or the pulse peak intensity.

Free electron modelPhysicsRange (particle radiation)Physics and Astronomy (miscellaneous)Carrier-envelope phaseSemiclassical physicsPhoton energyLaserlaw.inventionlawSpontaneous emissionEmission spectrumAtomic physicsInstrumentationLaser Physics Letters
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Search for Neutrino‐induced Cascades from Gamma‐Ray Bursts with AMANDA

2007

Using the neutrino telescope AMANDA-II, we have conducted two analyses searching for neutrino-induced cascades from gamma-ray bursts. No evidence of astrophysical neutrinos was found, and limits are presented for several models. We also present neutrino effective areas which allow the calculation of limits for any neutrino production model. The first analysis looked for a statistical excess of events within a sliding window of 1 or 100 seconds (for short and long burst classes, respectively) during the years 2001-2003. The resulting upper limit on the diffuse flux normalization times E^2 for the Waxman-Bahcall model at 1 PeV is 1.6 x 10^-6 GeV cm^-2 s^-1 sr^-1 (a factor of 120 above the the…

Gamma rays: burstsNormalization (statistics)PhysicsRange (particle radiation)MuonAstrophysics::High Energy Astrophysical PhenomenaGamma rays: bursts; Neutrinos; TelescopesAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysicsCoincidenceSpace and Planetary ScienceCascadeAstronomiaDiffuse fluxHigh Energy Physics::ExperimentNeutrinosNeutrinoGamma-ray burstTelescopesThe Astrophysical Journal
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First search for dyons with the full MoEDAL trapping detector in 13 TeV pp collisions

2021

The MoEDAL trapping detector, consists of approximately 800 kg of aluminium volumes. It was exposed during Run-2 of the LHC program to 6.46 fb^-1 of 13 TeV proton-proton collisions at the LHCb interaction point. Evidence for dyons (particles with electric and magnetic charge) captured in the trapping detector was sought by passing the aluminium volumes comprising the detector through a SQUID magnetometer. The presence of a trapped dyon would be signalled by a persistent current induced in the SQUID magnetometer. On the basis of a Drell-Yan production model, we exclude dyons with a magnetic charge ranging up to 5 Dirac charges, and an electric charge up to 200 times the fundamental electric …

General PhysicsMoEDAL electric and magnetic charge dyonPhysics MultidisciplinaryMagnetic monopoleFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciences7. Clean energyElectric charge114 Physical sciencesMoEDAL Collaboration09 Engineeringlaw.inventionHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)MAGNETIC MONOPOLESSTOPPING-POWERlaw0103 physical sciencesPARTICLES010306 general physics01 Mathematical SciencesParticle Physics - PhenomenologyPhysicsRange (particle radiation)Large Hadron ColliderScience & Technology02 Physical Scienceshep-exPhysicsDetectorPersistent currenthep-phSQUIDHigh Energy Physics - PhenomenologyDyonPhysical SciencesHigh Energy Physics::ExperimentParticle Physics - Experiment
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Main Sequence Stars with Asymmetric Dark Matter

2012

We study the effects of feebly or non-annihilating weakly interacting Dark Matter (DM) particles on stars that live in DM environments denser than that of our Sun. We find that the energy transport mechanism induced by DM particles can produce unusual conditions in the core of Main Sequence stars, with effects which can potentially be used to probe DM properties. We find that solar mass stars placed in DM densities of rhochi>= e2 GeV/cm3 are sensitive to Spin-Dependent scattering cross-section sigmsd >= e-37 cm2 and a DM particle mass as low as mchi=5 GeV, accessing a parameter range weakly constrained by current direct detection experiments.

General Physicsastro-ph.SRPhysics MultidisciplinaryDark matterFOS: Physical sciencesGeneral Physics and AstronomyAstrophysics01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010303 astronomy & astrophysicsLight dark matterSolar and Stellar Astrophysics (astro-ph.SR)PhysicsSolar massRange (particle radiation)Science & Technology02 Physical Sciences010308 nuclear & particles physicsPhysicsHot dark matter1ST STARShep-phHigh Energy Physics - PhenomenologyStarsAstrophysics - Solar and Stellar AstrophysicsSTELLAR EVOLUTION13. Climate actionPhysical SciencesMixed dark matterAstrophysics::Earth and Planetary AstrophysicsMain sequencePhysical Review Letters
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Defects in glasses

1995

Abstract The absence of long range order in the glass structure allows to define only point defects in these materials. They are: 1) intrinsic defects—atomic size local deviation from short range order; 2) impurity defects—isolated impurity atoms or ions in the glass network; 3) intrinsic impurity defects—complexes consisting of the impurity atoms chemically bonded to one of the intrinsic defect atoms. The latter defects are characteristic for the doped glasses. Presence of point defects in glasses introduces new spectroscopic properties of these solid materials. Defect generation, interaction and recombination reactions resulting from the external influence causes the glass spectroscopic p…

Glass structureNuclear and High Energy PhysicsRange (particle radiation)RadiationMaterials scienceAbsorption spectroscopyCondensed matter physicsbusiness.industryDopingCondensed Matter PhysicsCondensed Matter::Disordered Systems and Neural NetworksCrystallographic defectIonOpticsImpurityGeneral Materials SciencebusinessRecombinationRadiation Effects and Defects in Solids
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Highlights from the ARGO-YBJ Experiment

2012

""The ARGO-YBJ experiment at YangBaJing in Tibet (4300m a.s.l.) has been taking data with its full layout since October 2007. Here we present a few significant results obtained in gamma-ray astronomy and cosmic-ray physics. Emphasis is placed on the analysis of gamma-ray emission from point-like sources (Crab Nebula, MRK 421), on the preliminary limit on the antiproton\\\/proton flux ratio, on the large-scale cosmic-ray anisotropy and on the proton-air cross-section. The performance of the detector is also discussed, and the perspectives of the experiment are outlined.""

HistoryAstronomyFluxAstrophysicsProton flux01 natural sciencesArgo-YbjGamma-ray emissionSettore FIS/05 - Astronomia E AstrofisicaCosmic-ray physicsResistive Plate ChambersInstrumentation010303 astronomy & astrophysicsArgoPhysicsRange (particle radiation)DetectorSettore FIS/01 - Fisica SperimentaleCrab nebulaAstrophysics::Instrumentation and Methods for AstrophysicsGamma rayCrab nebula Extensive air showers Flux ratio Gamma-ray astronomy Gamma-ray emission Ground based Resistive plate chambers; Astronomy Cosmic rays Cosmology Experiments; Gamma raysFlux ratioCosmologyComputer Science ApplicationsResistive plate chambersNuclear and High Energy PhysicsX- and γ-ray instrumentGround-based gamma-ray astronomyAstrophysics::High Energy Astrophysical PhenomenaExtensive air showerCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsCosmic RayEducationResistive Plate Chambers Extensive air showers Ground-based g ray astronomy Cosmic-ray physicsGround-based γ-ray astronomy0103 physical sciencesExtensive air showersCosmic raysExtensive air showers X- and γ-ray instruments Pulsars. Quasars active or peculiar galaxies objects and systemsAstrophysics::Galaxy AstrophysicsGamma-ray astronomy010308 nuclear & particles physicsGamma raysAstronomyResistive Plate ChamberGround basedCrab NebulaAntiprotonResistive Plate Chambers; Extensive air showers; Ground-based γ-ray astronomy; Cosmic-ray physicsSatelliteGamma-ray burstExperimentsJournal of Physics: Conference Series
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Thermo-optical studies of NaNbO3thin films

2007

Thermo-optical studies of sodium niobate NaNbO3 (NN) thin films, deposited by the pulsed laser ablation technique on Si/SrRuO3 substrates, were performed by spectroscopic ellipsometry in the temperature range 300-550°C. Optical constants at the room temperature were measured in the spectral range 250-1000 nm. Substantial changes in the refractive index temperature behaviour (taken at λ = 300 nm) were found at temperatures 370, 445, 503, 520, and 532°C, where the first and the last temperatures are the phase transitions P → R and S → T1, respectively. Other temperatures (445, 503, and 520°C) are suggested as the points of some local structural changes in the NN film.

HistoryPhase transitionRange (particle radiation)Materials scienceSodium niobateAnalytical chemistrySpectroscopic ellipsometryThin filmAtmospheric temperature rangeRefractive indexComputer Science ApplicationsEducationPulsed laser ablationJournal of Physics: Conference Series
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Anomalous behaviour of periodic domain structure in Gd-doped LiNbO3single crystals

2007

Atomic force microscopy studies of etching patterns, stability of regular domain structure, and anomalies of electrical characteristics in the 300 - 385 K range of a series of Gddoped lithium niobate single crystals grown under equal conditions are reported.

HistoryRange (particle radiation)Materials scienceCondensed matter physicsAtomic force microscopyLithium niobateDopingStructure (category theory)Computer Science ApplicationsEducationchemistry.chemical_compoundCrystallographychemistryEtching (microfabrication)Domain (ring theory)Journal of Physics: Conference Series
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