Search results for " shock waves"

showing 10 items of 37 documents

QPOs expected in rotating accretion flows around a supermassive black hole

2007

It is well known that rotating inviscid accretion flows with adequate injection parameters around black holes could form shock waves close to the black holes, after the flow passes through the outer sonic point and can be virtually stopped by the centrifugal force. We numerically examine such shock waves in 2D accretion flows with 10−5 to 106 Eddington critical accretion rates around a supermassive black hole with 106 M. As the results, the luminosities show QPO phenomena with modulations of a factor 2–3 and with quasi-periods of a few to several hours.

Accretion accretion disks – black hole physics – galaxies: active – hydrodynamics – radiation mechanisms: thermal – shock waves
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High-energy extracorporeal shock wave treatment of nonunions.

2001

Forty-three consecutive patients who did not have healing of tibial or femoral diaphyseal and metaphyseal fractures and osteotomies for at least 9 months after injury or surgery were examined prospectively for use of high-energy extracorporeal shock waves. Former treatment modalities (cast, external fixator, plate osteosynthesis, limitation of weightbearing) remained unchanged. In all cases a 99m Technetium dicarboxyphosphonate regional two-phase bone scintigraphy was performed before one treatment with 3000 impulses of an energy flux density of 0.6 mJ/mm 2 . Radiologic and clinical followups were done at 4-week intervals starting 8 weeks after shock wave treatment. The success criterion wa…

AdultMalemedicine.medical_specialtyAdolescentmedicine.medical_treatmentNonunionLong boneBone healingOsteotomyHigh-Energy Shock WavesmedicineHumansOrthopedics and Sports MedicineFemurProspective StudiesAgedOsteosynthesismedicine.diagnostic_testbusiness.industryGeneral MedicineMiddle Agedmedicine.diseaseSurgeryTibial FracturesPseudarthrosismedicine.anatomical_structureBone scintigraphyFractures UnunitedSurgeryFemalebusinessFemoral FracturesClinical orthopaedics and related research
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Shock wave therapy versus conventional surgery in the treatment of calcifying tendinitis of the shoulder.

2001

A prospective quasirandomized study was performed to compare the effects of surgical extirpation (Group I, 29 patients) with the outcome after high-energy extracorporeal shock wave therapy (Group II, 50 patients; 3,000 impulses of an energy flux density of 0.6 mJ/mm2) in patients with a chronic calcifying tendinitis in the supraspinatus tendon. Symptoms and demographic data of the two groups were comparable. According to the University of California Los Angeles Rating System, the mean score in Group I was 30 points with 75% good or excellent results after 12 months, and 32 points with 90% good or excellent results after 24 months. Radiologically, there was no calcific deposit in 85% of the …

AdultMalemedicine.medical_specialtymedicine.medical_treatmentRadiographyLithotripsylaw.inventionHigh-Energy Shock WavesTendonsRandomized controlled trialTendinitislawmedicineHumansOrthopedics and Sports MedicineProspective StudiesProspective cohort studyAgedbusiness.industryShoulder JointCalcinosisGeneral MedicineMiddle Agedmedicine.diseaseSurgeryClinical trialRadiographymedicine.anatomical_structureOrthopedic surgeryTendinopathyUpper limbSurgeryFemalebusinessClinical orthopaedics and related research
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Radiative accretion shocks along nonuniform stellar magnetic fields in classical T Tauri stars

2013

(abridged) AIMS. We investigate the dynamics and stability of post-shock plasma streaming along nonuniform stellar magnetic fields at the impact region of accretion columns. We study how the magnetic field configuration and strength determine the structure, geometry, and location of the shock-heated plasma. METHODS. We model the impact of an accretion stream onto the chromosphere of a CTTS by 2D axisymmetric magnetohydrodynamic simulations. Our model takes into account the gravity, the radiative cooling, and the magnetic-field-oriented thermal conduction. RESULTS. The structure, stability, and location of the shocked plasma strongly depend on the configuration and strength of the magnetic f…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesField strengthX-rays: starsAstrophysicsstars: pre-main sequence01 natural sciencesmagnetohydrodynamics (MHD)pre-main sequence X-rays: stars [accretion accretion disks instabilities magnetohydrodynamics (MHD) shock waves stars]010305 fluids & plasmasSettore FIS/05 - Astronomia E Astrofisicaaccretion0103 physical sciencesRadiative transferAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsChromosphereSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysicsaccretion disksAstronomy and AstrophysicsPlasmashock wavesAccretion (astrophysics)Magnetic fieldT Tauri starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceinstabilitiesPhysics::Space PhysicsOblique shockAstrophysics::Earth and Planetary Astrophysicsaccretion accretion disks instabilities magnetohydrodynamics (MHD) shock waves stars: pre-main sequence X-rays: stars[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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YSO accretion shocks: magnetic, chromospheric or stochastic flow effects can suppress fluctuations of X-ray emission

2013

Context. Theoretical arguments and numerical simulations of radiative shocks produced by the impact of the accreting gas onto young stars predict quasi-periodic oscillations in the emitted radiation. However, observational data do not show evidence of such periodicity. Aims. We investigate whether physically plausible perturbations in the accretion column or in the chromosphere could disrupt the shock structure influencing the observability of the oscillatory behavior. Methods. We performed local 2D magneto-hydrodynamical simulations of an accretion shock impacting a chromosphere, taking optically thin radiation losses and thermal conduction into account. We investigated the effects of seve…

Astrophysics::High Energy Astrophysical Phenomenaaccretion accretion disks magnetohydrodynamics (MHD) radiative transfer shock waves instabilitiesFOS: Physical sciencesPerturbation (astronomy)Astrophysics01 natural sciencesmagnetohydrodynamics (MHD)Settore FIS/05 - Astronomia E Astrofisicaaccretion0103 physical sciencesRadiative transferAstrophysics::Solar and Stellar Astrophysics010306 general physics010303 astronomy & astrophysicsChromosphereSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysicsaccretion disksAstronomy and AstrophysicsObservablePlasmashock wavesThermal conductionMagnetic fieldAmplitudeAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary Scienceradiative transferinstabilities[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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On critical behaviour in generalized Kadomtsev-Petviashvili equations

2016

International audience; An asymptotic description of the formation of dispersive shock waves in solutions to the generalized Kadomtsev–Petviashvili (KP) equation is conjectured. The asymptotic description based on a multiscales expansion is given in terms of a special solution to an ordinary differential equation of the Painlevé I hierarchy. Several examples are discussed numerically to provide strong evidence for the validity of the conjecture. The numerical study of the long time behaviour of these examples indicates persistence of dispersive shock waves in solutions to the (subcritical) KP equations, while in the supercritical KP equations a blow-up occurs after the formation of the disp…

Differential equationsShock waveSpecial solutionBlow-upKadomtsev–Petviashvili equations[PHYS.MPHY]Physics [physics]/Mathematical Physics [math-ph]Mathematics::Analysis of PDEsFOS: Physical sciencesPainlevé equationsKadomtsev-Petviashvili equationsKadomtsev–Petviashvili equation01 natural sciences010305 fluids & plasmasShock wavesDispersive partial differential equationMathematics - Analysis of PDEs0103 physical sciencesFOS: MathematicsCritical behaviourLong-time behaviourSupercriticalDispersion (waves)0101 mathematicsKP equationSettore MAT/07 - Fisica MatematicaMathematical PhysicsMathematicsMathematical physicsKadomtsev-Petviashvili equationPainleve equationsConjectureNonlinear Sciences - Exactly Solvable and Integrable Systems010102 general mathematicsMathematical analysisDispersive shocks Kadomtsev–Petviashvili equations Painlevé equations Differential equations Dispersion (waves) Ordinary differential equations Shock waves Blow-up Critical behaviour Dispersive shocks Kadomtsev-Petviashvili equation KP equation Long-time behaviour Special solutions Supercritical Partial differential equationsStatistical and Nonlinear PhysicsMathematical Physics (math-ph)Condensed Matter PhysicsDispersive shocksPartial differential equationsNonlinear Sciences::Exactly Solvable and Integrable SystemsOrdinary differential equationSpecial solutions[ PHYS.MPHY ] Physics [physics]/Mathematical Physics [math-ph]Exactly Solvable and Integrable Systems (nlin.SI)Ordinary differential equationsAnalysis of PDEs (math.AP)
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Is it possible to change of the duration of consolidation period in the distraction osteogenesis with the repetition of extracorporeal shock waves?

2016

Background In this study we examined the effects of two different repeated Extracorporeal Shock Waves (ESW) on the consolidation period of the distraction osteogenesis (DO) of the rabbit mandible using stereological, radiological and immunohistochemical methods. Material and Methods DO was performed unilaterally in the mandible of 18 New Zealand rabbits (six months old, weighing between 2.5-3 kg). In the consolidation period, rabbits were divided into three groups randomly after the distraction period. The distraction zone of the mandible was received no treatment as controls (E0*2). Group 2 (E 500*2) received ESWT (twice 500 impulses at 14 kV and 0.19 mJ/mm2 energy) in the first and fourth…

Extracorporeal Shockwave TherapyDistraction osteogenesisTime FactorsBone densitymedicine.medical_treatmentStereologyOsteogenesis DistractionStereologyRabbitMandibleNew Zealand rabbitsurgeryangiogenesisRandom Allocation0302 clinical medicinetime factorMedicineanimalconnective tissueBone mineralOrthodonticsFracture Healingbone density:CIENCIAS MÉDICAS [UNESCO]stereometry030220 oncology & carcinogenesisExtracorporeal shockwave therapyimmunohistochemistryUNESCO::CIENCIAS MÉDICASDistraction osteogenesisRabbitsmedicine.symptomOral Surgerymedicine.medical_specialtyshock waveLeporidaerabbitBone healingrandomizationExtracorporeal03 medical and health sciencesAnimalshumanproceduresGeneral Dentistrynonhumanbusiness.industryOssificationResearchcontrol group030206 dentistryhuman tissueextracorporeal shock wavesSurgeryossificationOtorhinolaryngologyExtracorporeal shock wavesshock wave therapystereologybusiness
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Extracorporeal Shock Waves Increase Markers of Cellular Proliferation in Bronchial Epithelium and in Primary Bronchial Fibroblasts of COPD Patients

2020

Chronic obstructive pulmonary disease (COPD) is due to structural changes and narrowing of small airways and parenchymal destruction (loss of the alveolar attachment as a result of pulmonary emphysema), which all lead to airflow limitation. Extracorporeal shock waves (ESW) increase cell proliferation and differentiation of connective tissue fibroblasts. To date no studies are available on ESW treatment of human bronchial fibroblasts and epithelial cells from COPD and control subjects. We obtained primary bronchial fibroblasts from bronchial biopsies of 3 patients with mild/moderate COPD and 3 control smokers with normal lung function. 16HBE cells were also studied. Cells were treated with a…

Extracorporeal Shockwave TherapyMalePathologyPulmonary Disease Chronic Obstructive0302 clinical medicineMedicine0303 health sciencesCOPDSmokersbiologyCell DifferentiationMiddle AgedProto-Oncogene Proteins c-kitmedicine.anatomical_structurepsychological phenomena and processesResearch ArticlePulmonary and Respiratory MedicineExtracorporeal Shock Waves COPDCell typemedicine.medical_specialtyArticle SubjectPrimary Cell CultureeducationConnective tissueBronchibehavioral disciplines and activitiesCollagen Type ICell LineTransforming Growth Factor beta1Diseases of the respiratory system03 medical and health sciencesProliferating Cell Nuclear AntigenParenchymaHumansCD90RNA MessengerAgedCell Proliferation030304 developmental biologyRC705-779business.industryCD117Cell growthTranscription Factor RelAEpithelial CellsFibroblastsmedicine.diseaserespiratory tract diseasesProliferating cell nuclear antigen030228 respiratory systemCase-Control Studiesbiology.proteinbusiness
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Assessment of a high-resolution central scheme for the solution of the relativistic hydrodynamics equations

2004

We assess the suitability of a recent high-resolution central scheme developed by Kurganov & Tadmor (2000) for the solution of the relativistic hydrodynamics equations. The novelty of this approach relies on the absence of Riemann solvers in the solution procedure. The computations we present are performed in one and two spatial dimensions in Minkowski spacetime. Standard numerical experiments such as shock tubes and the relativistic flat-faced step test are performed. As an astrophysical application the article includes two-dimensional simulations of the propagation of relativistic jets using both Cartesian and cylindrical coordinates. The simulations reported clearly show the capabili…

FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsNumerical methodAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAGeneral Relativity and Quantum Cosmologylaw.inventionHydrodynamics ; Numerical method ; Relativity ; Shock wavesRelativityShock wavessymbols.namesakeAstrophysical jetlawMinkowski spaceApplied mathematicsCartesian coordinate systemCylindrical coordinate systemPhysicsConservation lawAstrophysics (astro-ph)Astronomy and Astrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Riemann hypothesisRiemann problemExact solutions in general relativitySpace and Planetary ScienceHydrodynamicssymbolsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Astronomy & Astrophysics
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XMM-Newton Large Program on SN1006 - I: Methods and Initial Results of Spatially-Resolved Spectroscopy

2015

Based on our newly developed methods and the XMM-Newton large program of SN1006, we extract and analyze the spectra from 3596 tessellated regions of this SNR each with 0.3-8 keV counts $>10^4$. For the first time, we map out multiple physical parameters, such as the temperature ($kT$), electron density ($n_e$), ionization parameter ($n_et$), ionization age ($t_{ion}$), metal abundances, as well as the radio-to-X-ray slope ($\alpha$) and cutoff frequency ($\nu_{cutoff}$) of the synchrotron emission. We construct probability distribution functions of $kT$ and $n_et$, and model them with several Gaussians, in order to characterize the average thermal and ionization states of such an extended s…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsElectron densityAstrophysics::High Energy Astrophysical Phenomenadata analysis cosmic rays ISM: supernova remnants X-rays: ISM [acceleration of particles shock waves methods]FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsacceleration of particles shock waves methods: data analysis cosmic rays ISM: supernova remnants X-rays: ISMSpectral lineInterstellar mediumSupernovaSpace and Planetary ScienceIonizationAstrophysics::Solar and Stellar AstrophysicsSpectroscopySupernova remnantAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Equivalent widthAstrophysics::Galaxy Astrophysics
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