Search results for "010308 nuclear & particles physics"

showing 10 items of 6362 documents

The Large Area Detector of LOFT: the Large Observatory for X-ray Timing

2014

LOFT (Large Observatory for X-ray Timing) is one of the five candidates that were considered by ESA as an M3 mission (with launch in 2022-2024) and has been studied during an extensive assessment phase. It is specifically designed to perform fast X-ray timing and probe the status of the matter near black holes and neutron stars. Its pointed instrument is the Large Area Detector (LAD), a 10 m 2 -class instrument operating in the 2-30keV range, which holds the capability to revolutionise studies of variability from X-ray sources on the millisecond time scales. The LAD instrument has now completed the assessment phase but was not down-selected for launch. However, during the assessment, most o…

[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Observatories ; Sensors ; X-rays ; Equipment and services ; X-ray sourcesComputer scienceObservatoriesFOS: Physical sciencesX-ray sources01 natural sciences7. Clean energyX-rayLoftObservatoryRange (aeronautics)0103 physical sciencesX-raysElectronicTimingOptical and Magnetic MaterialsElectrical and Electronic Engineering010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Compact Objects; Timing; X-ray; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringRemote sensingMillisecondEquipment and servicesCompact Objects010308 nuclear & particles physicsLarge area detectorSensorsApplied MathematicsComputer Science Applications1707 Computer Vision and Pattern RecognitionCondensed Matter Physics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Neutron starAstrophysics - Instrumentation and Methods for Astrophysicsastro-ph.IM
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LOFT: the Large Observatory For X-ray Timing

2012

The LOFT mission concept is one of four candidates selected by ESA for the M3 launch opportunity as Medium Size missions of the Cosmic Vision programme. The launch window is currently planned for between 2022 and 2024. LOFT is designed to exploit the diagnostics of rapid X-ray flux and spectral variability that directly probe the motion of matter down to distances very close to black holes and neutron stars, as well as the physical state of ultra-dense matter. These primary science goals will be addressed by a payload composed of a Large Area Detector (LAD) and a Wide Field Monitor (WFM). The LAD is a collimated (<1 degree field of view) experiment operating in the energy range 2-50 keV,…

[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]VisionX-ray timingAstronomySPIE ProceedingsObservatoriesX-ray timing X-ray spectroscopy X-ray imaging compact objectsSilicon Drift ChambersFOS: Physical sciencesddc:500.2X-ray missionsSpace (mathematics)Astrophysics01 natural sciences7. Clean energySettore FIS/05 - Astronomia E AstrofisicaX-rays0103 physical sciencesElectronicOptical and Magnetic MaterialsInstrumentation (computer programming)Electrical and Electronic EngineeringAerospace engineeringDiagnosticsCompact objects010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsSpatial resolutionsezeleSensors010308 nuclear & particles physicsbusiness.industryApplied MathematicsX-ray imagingSilicon Drift ChamberComputer Science Applications1707 Computer Vision and Pattern RecognitionCondensed Matter PhysicsCompact objects; X-ray imaging; X-ray spectroscopy; X-ray timing; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic Engineering[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]X-ray spectroscopySilicon Drift Chambers; X-ray missionsInstrumentation and Methods for AstrophysicsAstrophysics - Instrumentation and Methods for Astrophysicsbusiness
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A sum rule approach to total muon capture rates

1986

Abstract The total muon capture rate is expanded in terms of sum rules and the convergence of such an expansion is analyzed. It results that the energy-weighted and the inverse-energy-weighted sum rules provide an accurate estimate for the total rate in agreement with a complete RPA calculation through the response function. The static polarizability of the isovector dipole mode turns out to be the relevant quantity to determine the total muon capture rate, in light and medium nuclei.

[PHYS.NUCL] Physics [physics]/Nuclear Theory [nucl-th]PhysicsNuclear and High Energy PhysicsIsovector[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]010308 nuclear & particles physicsNuclear TheoryFunction (mathematics)01 natural sciencesMuon captureNuclear physicsDipole modePolarizability0103 physical sciencesConvergence (routing)Rule of sumSum rule in quantum mechanicsAtomic physics010306 general physics
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Interférométrie et réflectométrie haute résolution en lumière incohérente : modélisation d'interférogrammes

1999

International audience; Nous présentons des résultats infrarouge de réflectométrie à basse cohérence dans des fibres optiques, des guides d'onde et des coupleurs afin de détecter les échos dûs aux défauts de propagation réflective et pour mesurer leurs propriétés optiques: pertes ou atténuation, dispersion. Cette technique est basée sur l'interférométrie et donne la plus haute résolution spatiale avec la plus faible puissance optique réfléchie. Nous balayons le bras de référence de notre interféromètre de Michelson autour de la position de la " frange en lumière blanche " et nous obtenons des interférogrammes dont les enveloppes et les franges contiennent l'information sur le spectre de la …

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics]Physics[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]010308 nuclear & particles physics020208 electrical & electronic engineeringGeneral Physics and Astronomy02 engineering and technology01 natural sciences[SPI.TRON] Engineering Sciences [physics]/Electronics[SPI.TRON]Engineering Sciences [physics]/Electronics[ SPI.TRON ] Engineering Sciences [physics]/Electronics010309 optics0103 physical sciences0202 electrical engineering electronic engineering information engineering010306 general physicsHumanities
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Coupled experiment/simulation approach for the design of radiation-hardened rare-earth doped optical fibers and amplifiers

2011

We developed an approach to design radiation-hardened rare earth -doped fibers and amplifiers. This methodology combines testing experiments on these devices with particle swarm optimization (PSO) calculations. The composition of Er/Yb-doped phosphosilicate fibers was improved by introducing Cerium inside their cores. Such composition strongly reduces the amplifier radiation sensitivity, limiting its degradation: we observed a gain decreasing from 19 dB to 18 dB after 50 krad whereas previous studies reported higher degradations up to 0°dB at such doses. PSO calculations, taking only into account the radiation effects on the absorption efficiency around the pump and emission wavelengths, co…

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics]YtterbiumOptical fiberMaterials scienceAstrophysics::High Energy Astrophysical PhenomenaRadiation effectschemistry.chemical_elementradiation effects optical fibers rare-earth ions amplifiers particle swarm optimization erbium ytterbiumRadiation7. Clean energy01 natural scienceslaw.invention010309 opticsErbiumOpticslaw0103 physical sciencesOptical fibersFiberIrradiationYtterbiumrare-earth ions[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]particle swarm optimization010308 nuclear & particles physicsbusiness.industryAmplifierAttenuationOptique / photoniquePhysics::Classical PhysicschemistryamplifiersbusinessErbium2011 12th European Conference on Radiation and Its Effects on Components and Systems
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Combined Temperature Radiation Effects and Influence of Drawing Conditions on Phosphorous‐Doped Optical Fibers

2018

International audience; This work focuses on the effects of high dose ionizing radiation, up to 10 MGy(SiO2), on P‐doped multimode optical fibers (OF) at different irradiation temperatures. The investigation is based on two complementary experimental techniques: radiation‐induced attenuation (RIA) measurements and electron paramagnetic resonance (EPR). The latter technique allows measuring the P1, P2, metastable‐POHC and stable‐POHC defects. Three OF samples are drawn from the same preform to evaluate the influence of changing their drawing conditions of the OFs on the radiation responses. This first study is performed under X‐rays at room temperature. The results are compared with the ones…

[PHYS]Physics [physics]Materials scienceOptical fiber010308 nuclear & particles physicsbusiness.industryDoping02 engineering and technologySurfaces and InterfacesRadiation021001 nanoscience & nanotechnologyCondensed Matter Physics01 natural sciencesSurfaces Coatings and FilmsElectronic Optical and Magnetic Materialslaw.invention[SPI]Engineering Sciences [physics]law0103 physical sciencesirradiation effects optical fibersMaterials ChemistryOptoelectronicsElectrical and Electronic Engineering0210 nano-technologybusinessphysica status solidi (a)
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Irradiation temperature influence on the in-situ measured radiation induced attenuation of Ge-doped fibers

2016

International audience; We report an experimental investigation on the radiation induced attenuation (RIA) in the ultraviolet-visible domain for Ge-doped optical fibers, during X-rays (10 keV) exposure at different temperatures. The objective is to characterize the impact of the irradiation temperature on the RIA levels and kinetics. Our data highlight that for dose exceeding 1 kGy(SiO2) the RIA spectrum changes with the irradiation temperature. In particular, for wavelengths below 470 nm the RIA depends both on the dose and on the irradiation temperature, whereas at higher wavelengths the RIA depends only on the dose. From the microscopic point of view the origin of this behavior is explai…

[PHYS]Physics [physics]Nuclear and High Energy PhysicsMaterials science010308 nuclear & particles physicsbusiness.industryAttenuationDopingAnalytical chemistry02 engineering and technology021001 nanoscience & nanotechnology01 natural sciencesTemperature measurementlaw.inventionWavelengthNuclear Energy and Engineeringlaw0103 physical sciencesOptoelectronicsFiberIrradiationElectrical and Electronic Engineering0210 nano-technologybusinessElectron paramagnetic resonanceLuminescenceIEEE Transactions on Nuclear Science
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Effect of irradiation temperature on the radiation induced attenuation of Ge-doped fibers

2016

International audience; The UV-visible radiation induced attenuation (RIA) was studied in Ge-doped optical fibers, during X-ray (10 keV) irradiations at different temperatures. By comparing the spectra recorded in dissimilarly irradiated samples we evidenced the impact of the irradiation temperature. In details, we highlighted that, from a certain dose, increasing the temperature the RIA decreases for wavelengths lower than 470 nm, whereas at higher wavelengths the RIA depends only on the dose. Such findings suggest that it is possible to distinguish the irradiation temperature by comparing the signal at two different wavelengths. From the microscopic point of view, it appears that the RIA …

[PHYS]Physics [physics]Optical fiberMaterials science010308 nuclear & particles physicsbusiness.industryAttenuationDopingAnalytical chemistry02 engineering and technology021001 nanoscience & nanotechnology01 natural sciencesTemperature measurementlaw.inventionWavelengthlaw0103 physical sciencesOptoelectronicsIrradiation0210 nano-technologybusinessAbsorption (electromagnetic radiation)Electron paramagnetic resonance
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New exclusion limits on scalar and pseudoscalar axionlike particles from light shining through a wall

2015

Physics beyond the Standard Model predicts the possible existence of new particles that can be searched at the low-energy frontier in the sub-eV range. The OSQAR photon regeneration experiment looks for ``light shining through a wall'' from the quantum oscillation of optical photons into ``weakly interacting sub-eV particles,'' such as axion or axionlike particles (ALPs) in a 9 T transverse magnetic field over a length of $2\ifmmode\times\else\texttimes\fi{}14.3\text{ }\text{ }\mathrm{m}$. In 2014, this experiment was run with an outstanding sensitivity, using an 18.5 W continuous wave laser emitting in the green at the single wavelength of 532 nm. No regenerated photons have been detected …

[PHYS]Physics [physics]PhysicsNuclear and High Energy PhysicsParticle physicsPhoton010308 nuclear & particles physicsPhysics beyond the Standard ModelScalar (mathematics)Scalar and Pseudoscalar Axion-like ParticlesPhoton RegenerationType (model theory)01 natural sciencesMassless particlePseudoscalarAxionQuantum mechanics0103 physical sciencesSensitivity (control systems)010306 general physicsAxionPhysical Review D
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ESPRESSO highlights the binary nature of the ultra-metal-poor giant HE 0107-5240

2020

Context. The vast majority of the known stars of ultra low metallicity ([Fe=H] >-4:5) are known to be enhanced in carbon, and belong to the 'low-carbon band' (A(C) = log(C=H) + 12 7:6). It is generally, although not universally, accepted that this peculiar chemical composition reflects the chemical composition of the gas cloud out of which these stars were formed. The first ultra-metalpoor star discovered, HE 0107-5240, is also enhanced in carbon and belongs to the 'low-carbon band'. It has recently been claimed to be a long-period binary, based on radial velocity measurements. It has also been claimed that this binarity may explain its peculiar composition as being due to mass transfer fro…

[PHYS]Physics [physics]Physics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsBinary numberabundances [Galaxy]Astronomy and AstrophysicsAstrophysics01 natural sciencesGalactic haloEspressospectroscopic [Binaries]Space and Planetary Scienceabundances [Stars]0103 physical scienceshalo [Galaxy]Astrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics
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