0000000000089894

AUTHOR

P. Laurent

showing 5 related works from this author

Synchrotron x-ray transmission measurements and modeling of filters investigated for Athena

2020

International audience; Advanced Telescope for High-Energy Astrophysics is a large-class astrophysics space mission selected by the European Space Agency to study the theme "Hot and Energetic Universe." The mission essentially consists of a large effective area x-ray telescope and two detectors: the X-ray Integral Field Unit (X-IFU) and the Wide Field Imager (WFI). Both instruments require filters to shield from out-of-band radiation while providing high transparency to x-rays. The mission is presently in phase B; thus, to consolidate the preliminary design, investigated filter materials need to be properly characterized by experimental test campaigns. We report results from high-resolution…

synchrotron radiationComputer scienceAstrophysics::High Energy Astrophysical PhenomenaMechanical EngineeringAstrophysics::Instrumentation and Methods for AstrophysicsSynchrotron radiationtelescopesAstronomy and AstrophysicsElectronic Optical and Magnetic Materialslaw.inventionTelescopeFilter designSettore FIS/05 - Astronomia E AstrofisicaTransmission (telecommunications)Space and Planetary ScienceControl and Systems EngineeringlawFilter (video)[SDU]Sciences of the Universe [physics]CalibrationOptical filterInstrumentationDigital filterastrophysics space mission Athena optical and thermal filters Wide Field Imager X-ray Integral Field Unit x-ray transmissionRemote sensing
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Axion search with BabyIAXO in view of IAXO

2020

Axions are a natural consequence of the Peccei-Quinn mechanism, the most compelling solution to the strong-CP problem. Similar axion-like particles (ALPs) also appear in a number of possible extensions of the Standard Model, notably in string theories. Both axions and ALPs are very well motivated candidates for Dark Matter, and in addition, they would be copiously produced at the sun's core. A relevant effort during the last decade has been the CAST experiment at CERN, the most sensitive axion helioscope to-date. The International Axion Observatory (IAXO) is a large-scale 4th generation helioscope. As its primary physics goal, IAXO will look for solar axions or ALPs with a signal to backgro…

Particle physicsPhysics - Instrumentation and Detectorssolar axion[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]experimental methodsDark matterFOS: Physical sciences7. Clean energyString (physics)Standard Modelaxion helioscopedesign [detector]International Axion Observatory (IAXO)ObservatoryPeccei-Quinn mechanismDark Matterdetector design[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Detectors and Experimental TechniquesAxionsun-tracking systemsphysics.ins-detactivity reportdetector: designPhysicsinstrumentationHelioscopeLarge Hadron Colliderdetectorsolar [axion]DESYInstrumentation and Detectors (physics.ins-det)[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]IAXOmagnetopticsaxion: solar
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A deep study of the high–energy transient sky

2021

This is an open access article. This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds t…

Electromagnetic spectrumESA voyage 2050; High-energy transient sky; Multi-messenger astrophysics; Space mission concept; X–/γ–ray polarimetry; X–/γ–ray telescopes01 natural sciences7. Clean energylaw.inventionSettore FIS/05 - Astronomia E AstrofisicalawNuclear astrophysicsoptical010303 astronomy & astrophysicsmedia_commonPhysicsdensityStrong gravityAstrophysics::Instrumentation and Methods for AstrophysicsnucleosynthesisimagingParticle accelerationHigh-energy transient skyNeutrinoburstparticlelensmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenainterferometerSpace mission conceptTelescope0103 physical sciencesTeVequation of statepolarization010308 nuclear & particles physicsGravitational wavenucleusgravitational radiationAmbientaleAstronomyAstronomy and AstrophysicsaccelerationsensitivityMulti-messenger astrophysicsUniversemonitoringelectromagneticX–/γ–ray telescopesangular resolution[SDU]Sciences of the Universe [physics]13. Climate actionSpace and Planetary Sciencegamma raygravitationX–/γ–ray polarimetry[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]ESA voyage 2050
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Next Generation Search for Axion and ALP Dark Matter with the International Axion Observatory

2018

International audience; More than 80 years after the postulation of dark matter, its nature remains one of the fundamental questions in cosmology. Axions are currently one of the leading candidates for the hypothetical, non-baryonic dark matter that is expected to account for about 25% of the energy density of the Universe. Especially in the light of the Large Hadron Collider at CERN slowly closing in on Weakly-Interacting Massive Particle (WIMP) searches, axions and axion-like particles (ALPs) provide a viable alternative approach to solving the dark matter problem. The fact that makes them particularly appealing is that they were initially introduced to solve a long-standing problem in qu…

Particle physicsCERN LabPhysics::Instrumentation and DetectorsDark matterObservatoriesaxion: detector7. Clean energy01 natural sciencesCosmologyHigh Energy Physics::TheoryPrimakoff effectSensitivityWIMP0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsAxionPrimakoff effectactivity reportPhysicsHelioscopeLarge Hadron Collider010308 nuclear & particles physicsPhysicsHigh Energy Physics::PhenomenologyToroidal magnetic fieldsDetectorsobservatory13. Climate actionCouplingsaxion-like particlesproposed experimentCERN Axion Solar Telescopeaxion: solarTelescopes
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Elaboration de systèmes de culture adaptés à la préservation de la qualité de l'eau. Programme Bretagne eau pure II

1999

33 ref. *INRA Unité Sol et Agronomie Rennes-Quimper 65 Rue de Saint-Brieuc 35042 Rennes Cedex (FRA) Diffusion du document : INRA Unité Sol et Agronomie Rennes-Quimper 65 Rue de Saint-Brieuc 35042 Rennes Cedex (FRA); National audience

[SDV] Life Sciences [q-bio][SDE] Environmental Sciences[SDV]Life Sciences [q-bio]LIXIVIATION[SDE]Environmental SciencesAGRONOMIE[INFO]Computer Science [cs][INFO] Computer Science [cs]COLZA
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