Search results for "Masses"

showing 8 items of 98 documents

Liturgie anlässlich der Staatsund Nationalfeierlichkeiten in Polen Geschichte, Probleme und Herausforderungen

2018

Historia, problemy i wyzwania. Historia Polski od przyjęcia chrztu w 966 r. pokazuje, jak pewne wydarzenia społeczne łączono z celebracjami liturgii. W artykule została podjęta próba pokazania nie tylko historii tego zjawiska, ale też problemów, jakie się z nim wiązały. Łączenie wątków religijnych ze świętowaniem wydarzeń narodowych miało miejsce wtedy, gdy pojawiało się zagrożenie wewnętrzne lub zewnętrzne. Przykładem są tzw. śluby lwowskie króla Jana Kazimierza, który 1 kwietnia 1656 r. uroczystym aktem religijno-państwowym oddał Rzeczpospolitą pod opiekę Matki Bożej, którą ogłosił Patronką oraz Królową Królestwa Polskiego i wszystkich jego ludów. Fakt ten przyczynił się zdecydowanie do t…

liturgia katolickaMasses for homelanduroczystości patriotyczno-narodowepatriotic-national celebrationsceremony of uniformed servicesmsze za Ojczyznęceremoniał służb mundurowychnarodowe sanktuariumCatholic liturgynational shrineStudia Teologiczno-Historyczne Śląska Opolskiego
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High-resolution, accurate multiple-reflection time-of-flight mass spectrometry for short-lived, exotic nuclei of a few events in their ground and low…

2019

Physical review / C covering nuclear physics 99(6), 064313 (2019). doi:10.1103/PhysRevC.99.064313

massaspektrometriaProtonResolution (mass spectrometry)FissionBinding energyMass spectrometrynucl-ex01 natural sciences530binding energy and massesnuclear bindingNuclear physics0103 physical sciencesNeutronddc:530NuclideNuclear Experiment010306 general physicsphysics.ins-detPhysicsbeam diagnostics010308 nuclear & particles physicsnuclear fragmentationlifetimes and widthsTime-of-flight mass spectrometryisomer decaysydinfysiikka
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Direct mass measurements on neutron-deficient xenon isotopes with the ISOLTRAP mass spectrometer

2002

The masses of Xe isotopes with 124 A 114 have been measured using the ISOLTRAP spectrometer at the on-line mass separator ISOLDE/CERN. A mass resolving power of 500000 was chosen resulting in an accuracy of m 12 keV for all isotopes investigated. Con icts with existing mass data of several standard deviations were found. peerReviewed

massaspektrometriaatomic massesXenon isotopesPhysics::Instrumentation and Detectorspenning trapNuclear Experimentradioactive ions
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Sonographische Charakteristika laterozervikaler Raumforderungen

2001

UNLABELLED Sonography of the head and neck mainly focuses on tumours of the lateral neck. Even though most of these masses are enlarged lymph nodes, other tumors have to be considered. AIM To determine whether different pathological cervical masses display a characteristic sonographic morphology. METHOD On the basis of 530 sonographical findings in the neck, typical ultrasound characteristics either in B-scan or in colour coded sonography were demonstrated. RESULTS Apart from enlarged lymph nodes, it was possible to differentiate other occurrences such as branchial cysts, abscesses, laryngoceles, lipomas, neurinomas, glomus tumours, paragangliomas and also fibromas by their specific ultraso…

medicine.medical_specialtybusiness.industryUltrasoundEarly detectionBranchial CystLateral neckCervical massesMedicineRadiology Nuclear Medicine and imagingLymphRadiologybusinessHead and neckPathologicalUltraschall in der Medizin
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Exotic properties of neutrinos using effective Lagrangians and specific models

2013

289 páginas. Tesis Doctoral del Departamento de Física Teórica, de la Universidad de Valencia, y del Instituto de Física Corpuscular (IFIC).

neutrino magnetic momentsneutrinoeffective field theorylepton number violationlepton flavor violationneutrino massesphenomenologycolliderneutrino astrophysicsbeyond standard modelneutrinoless double beta decayneutrino mixing
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GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

2017

On August 17, 2017 at 12-41:04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral. The signal, GW170817, was detected with a combined signal-to-noise ratio of 32.4 and a false-alarm-rate estimate of less than one per 8.0×104 years. We infer the component masses of the binary to be between 0.86 and 2.26 M, in agreement with masses of known neutron stars. Restricting the component spins to the range inferred in binary neutron stars, we find the component masses to be in the range 1.17-1.60 M, with the total mass of the system 2.74-0.01+0.04M. The source was localized within a sky region of 28 deg2 (90% probabili…

neutron star: binary[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]X-ray binaryADVANCED LIGOAstrophysicsKilonovagravitational waves; LIGO; binary neutron star inspiralspin01 natural sciencesLIGOGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)QCQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Electromagnetic observationsGravitational-wave signals3100 General Physics and AstronomyPoint MassesAstrophysics - High Energy Astrophysical PhenomenaBlack-Hole MergersBinary neutron starsBlack HolesX-ray bursterCoalescing BinariesAstrophysics::High Energy Astrophysical Phenomena10192 Physics InstituteGeneral Relativity and Quantum Cosmology (gr-qc)Gravity wavesGravitational wavesNeutron starsPhysics and Astronomy (all)ddc:530Electromagnetic spectraNeutrons010308 nuclear & particles physicsVirgoGamma raysAstronomyRCUKVIRGOelectromagneticgravitational radiation: emissionStellar black holeGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Compact Binariesbinary: masscosmological modelAstronomyGeneral Physics and AstronomyAstrophysicsneutron starsGamma ray burstsGeneral Relativity and Quantum CosmologyGravitational wave detectorsUniverseDENSE MATTER010303 astronomy & astrophysicsastro-ph.HEPhysicsSignal to noise ratioSettore FIS/01 - Fisica SperimentaleGravitational effectsFalse alarm rateEQUATION-OF-STATEMergers and acquisitionsgravitational waves[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]530 PhysicsMERGERSGeneral Relativity and Quantum Cosmology; General Relativity and Quantum Cosmology; astro-ph.HEFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstgravitational radiation: direct detectionMerging[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]GAMMA-RAY BURSTLIGO (Observatory)binary: coalescenceGravitational waves neutron stars gamma-ray burst LIGO Virgo0103 physical sciencesGW151226MASSESSTFCAstrophysics::Galaxy AstrophysicsPhysiqueGravitational wavegravitational radiationPULSARgravitational radiation detectorNeutron starPhysics and AstronomygravitationRADIATIONDewey Decimal Classification::500 | Naturwissenschaften::530 | Physikbinary neutron star inspiralSignal detectionPHYS REV LETT PHYSICAL REVIEW LETTERS
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Gaia-ESO Survey: Cha I members

2017

Investigating the physical mechanisms driving the dynamical evolution of young star clusters is fundamental to our understanding of the star formation process and the properties of the Galactic field stars. The young (~2Myr) and partially embedded cluster Chamaeleon I is one of the closest laboratories to study the early stages of star cluster dynamics in a low-density environment. The aim of this work is to study the structural and kinematical properties of this cluster combining parameters from the high-resolution spectroscopic observations of the Gaia-ESO Survey with data from the literature. Our main result is the evidence of a large discrepancy between the velocity dispersion ({sigma}_…

observational astronomyOpen star clustersEffective temperatureAstrophysics and AstronomyRadial velocityExoplanet AstronomyStellar AstronomyPhysicsAstrophysics::Solar and Stellar AstrophysicsStellar massesAstrophysics::Cosmology and Extragalactic AstrophysicsNatural SciencesAstrophysics::Galaxy Astrophysics
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Valeur de l’IRM de diffusion pour caractériser les petites masses rénales (< 3cm)

2012

Objectifs: Décrire l’aspect des masses rénales (< 3cm) en imagerie de diffusion et déterminer le rôle de l’ADC pour la différentiation entre lésion maligne et bénigne. Matériels et méthodes: 47 tumeurs rénales < 3cm (23 malignes, 24 bénignes) furent explorées en IRM 3T incluant en sus du protocole habituel une séquence de diffusion (b1000). Une analyse rétrospective qualitative et quantitative (ADC) fut réalisée avec corrélation anatomopathologique et tests statistiques pour déterminer l’efficacité de la valeur d’ADC pour caractériser la lésion. Résultats: En diffusion, toutes les masses étaient hyperintenses au parenchyme sain. L’ADC moyen des CC RCC était supérieur à celui des angiomyolip…

petites masses rénalesdiffusionIRM
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