Search results for "Shock wave"

showing 10 items of 194 documents

Modeling particle acceleration and non-thermal emission in supernova remnants

2021

According to the most popular model for the origin of cosmic rays (CRs), supernova remnants (SNRs) are the site where CRs are accelerated. Observations across the electromagnetic spectrum support this picture through the detection of non-thermal emission that is compatible with being synchrotron or inverse Compton radiation from high energy electrons, or pion decay due to proton-proton interactions. These observations of growing quantity and quality promise to unveil many aspects of CRs acceleration and require more and more accurate tools for their interpretation. Here, we show how multi-dimensional MHD models of SNRs, including the effects on shock dynamics due to back-reaction of acceler…

Shock waveMagnetohydrodynamics (MHD)Radiation mechanisms: non-thermalElectromagnetic spectrumAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysicsElectronRadiation01 natural sciencesShock wavesAcceleration0103 physical sciencesCosmic rays010303 astronomy & astrophysicsInstrumentationAstrophysics::Galaxy AstrophysicsISM: supernova remnantsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstronomy and AstrophysicsParticle accelerationSupernovaSpace and Planetary SciencePhysics::Accelerator PhysicsAstrophysics - High Energy Astrophysical Phenomena
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Influence of custom-made and prefabricated insoles before and after an intense run

2017

[EN] Each time the foot contacts the ground during running there is a rapid deceleration that results in a shock wave that is transmitted from the foot to the head. The fatigue of the musculoskeletal system during running may decrease the ability of the body to absorb those shock waves and increase the risk of injury. Insoles are commonly prescribed to prevent injuries, and both custom-made and prefabricated insoles have been observed to reduce shock accelerations during running. However, no study to date has included a direct comparison of their behaviour measured over the same group of athletes, and therefore great controversy still exists regarding their effectiveness in reducing impact …

Shock waveMaleCritical Care and Emergency MedicinePhysiologylcsh:MedicineAccelerometerPathology and Laboratory MedicineMaterial FatigueRunning0302 clinical medicineMaterials PhysicsMedicine and Health SciencesTreadmillGroung Reaction Forcelcsh:ScienceMusculoskeletal SystemFatigueTrauma MedicineMultidisciplinaryPhysicsClassical MechanicsFoamShock (mechanics)Muscle FatiguePhysical SciencesLegsEngineering and TechnologyFemaleAnatomyShock AttenuationTraumatic InjuryResearch ArticleAdultmedicine.medical_specialtyMaterials by StructureMaterials ScienceSTRIDE03 medical and health sciencesAccelerationYoung AdultPhysical medicine and rehabilitationSigns and SymptomsDiagnostic MedicineTEORIA DE LA SEÑAL Y COMUNICACIONESmedicineHumansTibial Stress-FractureDamage Mechanicsbusiness.industryBiological Locomotionlcsh:RLimbs (Anatomy)Biology and Life Sciences030229 sport sciencesStride lengthShoesAthletesMusculoskeletal InjuryImpact loadingExercise Testlcsh:QFeet (Anatomy)ElectronicsAccelerometersbusiness030217 neurology & neurosurgery
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Diffusion of point defects in shocked molecular crystals

2005

The dynamic response of a molecular crystal containing defects to shock wave loading is modeled and the resulting diffusion of point defects is simulated. It is shown that diffusion proceeds not only via the stress assisted diffusion, which is point defect diffusion in a stress field, also known as the Gorsky effect, but also through defect diffusion in the field of inertial forces. The method for modeling diffusion of point defects in shocked solids is developed. It is shown that diffusion in the inertial field significantly exceeds the stress diffusion in organic molecular crystals. Interplay between stress-assisted and inertial diffusion leads to the separation of light particles from he…

Shock waveMaterials scienceField (physics)business.industryCondensed Matter PhysicsMolecular physicsCrystallographic defectElectronic Optical and Magnetic MaterialsCrystalStress (mechanics)Stress fieldOpticsDiffusion (business)businessExcitationPhysical Review B
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Experimental and Numerical Analysis of the Distribution of Residual Stresses Induced by Laser Shock Peening in a 2050-T8 Aluminium Alloy

2011

Laser shock peening (LSP) is an innovative surface treatment technique successfully applied to improving fatigue performance of metallic material. The specific characteristic of (LSP) is the generation of a low work-hardening and a deep compressive residual stresses mechanically produced by a laser-induced shock wave propagating in the material. The aim of this study is to analyse the residual stress distribution induced by laser peening in 2050-T8 aluminium alloy experimentally by the X-ray diffraction technique (method sin2Y) and numerically, by a finite element numerical modelling. A specific focus was put on the residual stress distribution along the surface of the impacted material.

Shock waveMaterials scienceMechanical EngineeringLaser peeningMetallurgyPeeningCondensed Matter PhysicsShot peeningFinite element methodShock (mechanics)Mechanics of MaterialsResidual stressvisual_artAluminium alloyvisual_art.visual_art_mediumGeneral Materials ScienceMaterials Science Forum
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Assessment of Fatigue Effects Induced by Fast Beam Transients in the IFMIF-DONES Li Target

2020

One of the crucial steps toward the commercial exploitation of fusion energy is the availability of a high-intensity neutron source able to test and qualify structural materials to be used in future fusion power reactors. The International Fusion Materials Irradiation Facility-DEMO Oriented NEutron Source (IFMIF-DONES) facility, which is currently being designed within the framework of the EUROfusion Consortium, represents the European effort to develop such a neutron source. It employs a liquid lithium target struck by an accelerated deuteron (D+) beam to produce fusion-like neutrons used to irradiate materials samples. So far, a detailed investigation of the thermomechanical behavior of t…

Shock waveNuclear and High Energy PhysicsMaterials scienceNuclear engineeringchemistry.chemical_element7. Clean energy01 natural sciences010305 fluids & plasmasBeam trips0103 physical sciencesNeutronlithium targetSettore ING-IND/19 - Impianti NucleariStructural materialInternational Fusion Materials Irradiation Facility-DEMO Oriented NEutron Source (IFMIF-DONES)shock wavesFusion powerCondensed Matter Physics3. Good healthchemistry13. Climate actionNeutron sourceLithiumfatigueBeam (structure)Nominal power (photovoltaic)IEEE Transactions on Plasma Science
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Nuclear liquid-gas phase transition and supernovae evolution

2004

It is shown that the large density fluctuations appearing at the onset of the first order nuclear liquid-gas phase transition can play an important role in the supernovae evolution. Due to these fluctuations, the neutrino gas may be trapped inside a thin layer of matter near the proto-neutron star surface. The resulting increase of pressure may induce strong particle ejection a few hundred milliseconds after the bounce of the collapse, contributing to the revival of the shock wave. The Hartree-Fock+RPA scheme, with a finite-range nucleon-nucleon effective interaction, is employed to estimate the effects of the neutrino trapping due to the strong density fluctuations, and to discuss qualitat…

Shock waveNuclear and High Energy PhysicsPhase transition97.60.Bw; 26.50.+x; 25.30.Pt; 21.60.JzNuclear Theory[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]supernovaeAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryFOS: Physical sciencesTrappingAstrophysics7. Clean energy01 natural sciencesNuclear Theory (nucl-th)Nuclear physics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciences010306 general physicsPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsLiquid gasAstrophysics (astro-ph)FísicaneutrinosNuclear matterSupernovaphase transitionnuclear matterParticleNeutrino
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Observation of Optical Undular Bores in Multiple Four-Wave Mixing

2014

International audience; We demonstrate that wave-breaking dramatically affects the dynamics of nonlinear frequency conversion processes that operate in the regime of high efficiency (strong multiple four-wave mixing). In particular, by exploiting an all-optical-fiber platform, we show that input modulations propagating in standard telecom fibers in the regime of weak normal dispersion lead to the formation of undular bores (dispersive shock waves) that mimic the typical behavior of dispersive hydrodynamics exhibited, e.g., by gravity waves and tidal bores. Thanks to the nonpulsed nature of the beat signal employed in our experiment, we are able to clearly observe how the periodic nature of …

Shock waveOptical fiberQC1-999General Physics and AstronomyUndular boreTidal WavesFrequency conversionlaw.inventionNOFour-wave mixingOpticsFrequency conversionlawUndular bore Shock wave Optical fibre Frequency conversionNonlinear Sciences::Pattern Formation and SolitonsPhysics[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]business.industryPhysicsBreaking waveMechanicsWave phenomenonShock waveOptical fibrebusinessPhotonic-crystal fiber
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Application of High Energy Shock Waves to Single Cells

1989

Extracorporeal shock wave lithotripsy has been in clinical use since 1980 with several hundred thousand patients treated to date. Striking complications, like perirenal hematomas, are rare with a range of approximately 0.5%–1.5%. High dose applications in pigs and dogs have shown devastating effects on renal parenchyma with intrarenal hemorrhage and later fibrosis (Muschter et al. 1987). However, very little is known about shock wave effects on single cells like cellular blood components. Chaussy and coworkers (Chaussy 1982; Eisenberger et al. 1977) could show an increase of free hemoglobin after exposing canine erythrocytes to shock waves. Russo and associates (1986) found a profound influ…

Shock wavePathologymedicine.medical_specialtyDiagnostic ultrasoundbusiness.industryRenal parenchymamedicine.medical_treatmentHigh-Energy Shock WavesTumor cellsmedicine.diseaseExtracorporeal shock wave lithotripsyFibrosisFree hemoglobinMedicinebusiness
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Three-dimensional modeling from the onset of the SN to the full-fledged SNR. Role of an initial ejecta anisotropy on matter mixing

2020

Context. The manifold phases in the evolution of a core-collapse (CC) supernova (SN) play an important role in determining the physical properties and morphology of the resulting supernova remnant (SNR). Thus, the complex morphology of SNRs is expected to reflect possible asymmetries and structures developed during and soon after the SN explosion. Aims. The aim of this work is to bridge the gap between CC SNe and their remnants by investigating how post-explosion anisotropies in the ejecta influence the structure and chemical properties of the remnant at later times. Methods. We performed three-dimensional magneto-hydrodynamical simulations starting soon after the SN event and following the…

Shock wavePhysics010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaStratification (water)Instabilities ISM: supernova remnants Magnetohydrodynamics (MHD) Shock wavesAstronomy and AstrophysicsContext (language use)Astrophysics01 natural sciencesSupernovaSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary Science0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsRed supergiantAnisotropyEjectaSupernova remnant010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics
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A multidimensional hydrodynamic code for structure evolution in cosmology

1996

A cosmological multidimensional hydrodynamic code is described and tested. This code is based on modern high-resolution shock-capturing techniques. It can make use of a linear or a parabolic cell reconstruction as well as an approximate Riemann solver. The code has been specifically designed for cosmological applications. Two tests including shocks have been considered: the first one is a standard shock tube and the second test involves a spherically symmetric shock. Various additional cosmological tests are also presented. In this way, the performance of the code is proved. The usefulness of the code is discussed; in particular, this powerful tool is expected to be useful in order to study…

Shock wavePhysicsAstrophysics (astro-ph)Structure (category theory)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsCosmologyRiemann solverShock (mechanics)symbols.namesakeSpace and Planetary ScienceComponent (UML)symbolsCode (cryptography)Statistical physicsShock tube
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