Search results for "LIGHT"

showing 10 items of 3575 documents

The frontiers of the virtual photons program at MAMI

2012

The most recent results and the future physics program of the high precision electron-scattering experiment at MAMI are briefly outlined. The A1 high-resolution spectrometers facility allows for a unique quality of virtual photon experiments. High precision form factor measurements, few-baryon systems highresolution structure studies and the innovative way in the search of dark photons illustrate the interplay between such diverse fields as precision atomic physics, nuclear astrophysics and astroparticle physics, where hadron physics plays a central and connecting role.

Astroparticle physicsPhysicsParticle physicsPhotonSpectrometerPhysicsQC1-999Form factor (quantum field theory)Virtual particleEngineering physicsHadron physicsNuclear astrophysicsvirtual photon; form factor measurements; dark photon; precision spectroscopy of light hypernucleiNuclear Experiment
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Study of the reflection spectrum of the LMXB 4U 1702-429

2016

The source 4U 1702-429 (Ara X-1) is a low-mass X-ray binary system hosting a neutron star. Albeit the source is quite bright ( $\sim10^{37}$ erg s$^{-1}$) its broadband spectrum has never been studied. Neither dips nor eclipses have been observed in the light curve suggesting that its inclination angle is smaller than 60$^{\circ}$.We analysed the broadband spectrum of 4U 1702-429 in the 0.3-60 keV energy range, using XMM-Newton and INTEGRAL data, to constrain its Compton reflection component if it is present. After excluding the three time intervals in which three type-I X-ray bursts occurred, we fitted the joint XMM-Newton and INTEGRAL spectra obtained from simultaneous observations. A bro…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSpectral lineAccretion accretion diskSettore FIS/05 - Astronomia E AstrofisicaIonization0103 physical sciencesStars: individual: 4U 1702-429Emission spectrum010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsindividual: 4U 1702-429; Stars: neutron; X-rays: binaries; Astronomy and Astrophysics; Space and Planetary Science [Accretion accretion disks; Stars]PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstronomy and AstrophysicsAstronomy and AstrophysicLight curveX-rays: binarieAccretion (astrophysics)Stars: neutronNeutron starAbsorption edgeSpace and Planetary ScienceElectron temperatureAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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Updating the orbital ephemeris of the dipping source XB 1254-690 and the distance to the source

2017

XB 1254-690 is a dipping low mass X-ray binary system hosting a neutron star and showing type I X-ray bursts. We aim at obtaining more accurate orbital ephemeris and at constraining the orbital period derivative of the system for the first time. In addition, we want to better constrain the distance to the source in order to locate the system in a well defined evolutive scenario. We apply for the first time an orbital timing technique to XB 1254-690, using the arrival times of the dips present in the light curves that have been collected during 26 years of X-ray pointed observations performed from different space missions. We estimate the dip arrival times using a statistical method that wei…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesLagrangian pointAstrophysicsStar (graph theory)Ephemeris01 natural sciencesstars: neutron0103 physical sciencesX-rays: star010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsstars: individual (XB 1254690)Astronomy and AstrophysicsQuadratic functionAstronomy and AstrophysicOrbital periodLight curveX-rays: binarieAstrometry and celestial mechanics: ephemerideNeutron starSpace and Planetary Scienceephemerides; stars: individual (XB 1254690); stars: neutron; X-rays: binaries; X-rays: stars; Astronomy and Astrophysics; Space and Planetary Science [Astrometry and celestial mechanics]Astrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaLow Mass
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Stability analysis of relativistic jets from collapsars and its implications on the short-term variability of gamma-ray bursts

2002

We consider the transverse structure and stability properties of relativistic jets formed in the course of the collapse of a massive progenitor. Our numerical simulations show the presence of a strong shear in the bulk velocity of such jets. This shear can be responsible for a very rapid shear--driven instability that arises for any velocity profile. This conclusion has been confirmed both by numerical simulations and theoretical analysis. The instability leads to rapid fluctuations of the main hydrodynamical parameters (density, pressure, Lorentz factor, etc.). However, the perturbations of the density are effectively decoupled from those of the pressure because the beam of the jet is radi…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesgalaxies jetsAstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAInstabilitysymbols.namesakeAstrophysical jetISM jets and outflowsPhysicsBurstsGamma ray theoryTurbulenceAstrophysics (astro-ph)Magnetohydradynamics (MHD) : Gamma rays ; Bursts ; Gamma ray theory ; ISM jets and outflows ; galaxies jetsAstronomy and AstrophysicsMechanicsLight curve:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Transverse planeLorentz factorSpace and Planetary SciencesymbolsGamma rays [Magnetohydradynamics (MHD)]OutflowUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaGamma-ray burst:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Discovery of a soft X-ray 8 mHz QPO from the accreting millisecond pulsar IGR J00291+5934

2016

In this paper, we report on the analysis of the peculiar X-ray variability displayed by the accreting millisecond X-ray pulsar IGR J00291+5934 in a 80 ks-long joint NuSTAR and XMM-Newton observation performed during the source outburst in 2015. The light curve of the source was characterized by a flaring-like behavior, with typical rise and decay time scales of ~120 s. The flares are accompanied by a remarkable spectral variability, with the X-ray emission being generally softer at the peak of the flares. A strong quasi periodic oscillation (QPO) is detected at ~8 mHz in the power spectrum of the source and clearly associated with the flaring-like behavior. This feature has the strongest po…

Astrophysics::High Energy Astrophysical PhenomenaPulsars: individual: IGR J00291+5934FOS: Physical sciencesAstrophysics01 natural sciencesPulsarMillisecond pulsar0103 physical sciences010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Millisecond010308 nuclear & particles physicsOscillationSpectral densityAstronomyAstronomy and AstrophysicsAstronomy and AstrophysicLight curveX-rays: binarieAstrophysics - Astrophysics of GalaxiesStars: neutronBlack holeNeutron starindividual: IGR J00291+5934; Stars: neutron; X-rays: binaries; Astronomy and Astrophysics; Space and Planetary Science [Pulsars]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics - High Energy Astrophysical Phenomena
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Neutron transmission measurements at nELBE

2020

International Conference on Nuclear Data for Science and Technology, ND 2019, Bejing, China, 19 May 2019 - 24 May 2019; The European physical journal / Web of Conferences 239, 01006 (2020). doi:10.1051/epjconf/202023901006

Astrophysics::High Energy Astrophysical PhenomenaQC1-999FluxNeutron transmission53001 natural sciences238UNuclear physicsXe0103 physical sciencesNeutronddc:530High pressure gas010306 general physicsPhysicsHe010308 nuclear & particles physicsNePhysicsOPtnELBE time of flight faciltiyneutron total cross sectionstransmission measurementNatBar (unit)
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TeV gamma-ray survey of the Northern sky using the ARGO-YBJ detector

2013

The ARGO-YBJ detector is an extensive air shower array that has been used to monitor the northern $\gamma$-ray sky at energies above 0.3 TeV from 2007 November to 2013 January. In this paper, we present the results of a sky survey in the declination band from $-10^{\circ}$ to $70^{\circ}$, using data recorded over the past five years. With an integrated sensitivity ranging from 0.24 to $\sim$1 Crab units depending on the declination, six sources have been detected with a statistical significance greater than 5 standard deviations. Several excesses are also reported as potential $\gamma$-ray emitters. The features of each source are presented and discussed. Additionally, $95\%$ confidence le…

Astrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectFOS: Physical sciencesFluxField of viewAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGamma rays: general – surveys01 natural sciencesDeclination0103 physical sciencesAbsorption (logic)010303 astronomy & astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsGamma rayAstronomy and Astrophysicsgeneral – su [gamma rays]Air showerExtragalactic background light13. Climate actionSpace and Planetary ScienceSkygeneral – surveys [Gamma rays]Astrophysics - High Energy Astrophysical Phenomena
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First Report of Southern Blight Caused by Sclerotium rolfsii on Hemp (Cannabis sativa) in Sicily and Southern Italy

2007

Hemp (Cannabis sativa L.), family Cannabaceae, is an annual herbaceous plant that is 1.5 to 4.0 m tall and native to the Caucasus Region, northern India, and Iran. It is cultivated in warm to temperate regions worldwide for its fiber, oil, and psychoactive substances. In Europe, commercial plantings have decreased from 52,872 ha in 1989 to 18,716 ha in 2005. Recently however, cultivation of hemp as a natural fiber species has been encouraged by European Union policy (2). During the summer of 2003, patches of dead plants were observed in test plots of 12 monoecious and dioecious hemp cultivars (Beniko, Epsylon 68, Felina 34, Ferimon, Fedora 17, Futura 75, Bialobrzeskie, Dioica 88, Fibranova…

Athelia rolfsiiSclerotiumbiologyPlant ScienceHerbaceous plantbiology.organism_classificationAgronomyBlightmedia_common.cataloged_instanceCultivarStem rotEuropean unionAgronomy and Crop ScienceMyceliummedia_common
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Blight of English Ivy (Hedera helix) caused by Sclerotium rolfsii in Sicily

2007

English ivy, Hedera helix L. (Araliaceae), an evergreen climbing vine is widely cultivated as an ornamental and foliage plant. In the summer of 2005, a severe blight of ivy plants trained as topiaries and grown in an open field was observed in a nursery near Giarre (eastern Sicily). Foliage of infected plants appeared lighter green and progressively turned bronze and withered. Eventually, the entire plant collapsed. Foliar symptoms were associated with basal stem and root rot. White, cottony mycelium and numerous sclerotia developed externally on the lower stem and on the soil around the affected plants. The disease was randomly distributed, affecting approximately 5% of plants in a stock …

Athelia rolfsiiVineSclerotiumbiologyHedera helixOrnamental plantBotanyRoot rotBlightPotato dextrose agarPlant Sciencebiology.organism_classificationAgronomy and Crop Science
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Atmosphere-Space Interactions Monitor (ASIM): State of the Art

2014

Atmosphere-Space Interactions Monitor (ASIM) mission is an ESA pay load which will be installed in the Columbus module of the International Space Station (ISS). ASIM is optimized to the observation and monitoring of luminescent phenomena in the upper atmosphere, the so called Transient Luminous Event (TLEs) and Terrestrial Gamma Ray Flashes(TGFs). Both TLEs and TGFs have been discovered recently (past two decades) and opened a new field of research in high energetic phenomena in the atmosphere. We will review the capabilities of ASIM and how it will help researchers to gain deeper knowledge of TGFs, TLEs, their inter-relationship and how they are linked to severe thunderstorms and the pheno…

AtmosphereEngineeringMeteorologybusiness.industrylcsh:TA1-2040International Space StationThunderstormGeneral Earth and Planetary Sciencesbusinesslcsh:Engineering (General). Civil engineering (General)LightningGeneral Environmental ScienceActa Polytechnica CTU Proceedings
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