Search results for "Ray"

showing 10 items of 8009 documents

Experimental study of 100Tc β decay with total absorption γ -ray spectroscopy

2017

The β decay of 100Tc has been studied by using the total absorption γ -ray spectroscopy technique at the Ion Guide Isotope Separator On-Line facility in Jyväskylä. In this work the new Decay Total Absorption γ -ray Spectrometer in coincidence with a cylindrical plastic β detector has been employed. The β intensity to the ground state obtained from the analysis is in good agreement with previous high-resolution measurements. However, differences in the feeding to the first-excited state as well as weak feeding to a new level at high excitation energy have been deduced from this experiment. Theoretical calculations performed in the quasiparticle random-phase approximation framework are also r…

total absorption gamma-ray spectroscopybeta decay
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r Process (n, γ) Rate Constraints from the γ Emission of Neutron Unbound States in β decay

2017

Total absorption gamma-ray spectroscopy is used to measure accurately the intensity of γγ emission from neutron-unbound states populated in the ββ-decay of delayed-neutron emitters. From the comparison of this intensity with the intensity of neutron emission a constraint on the (n, γγ) cross section for highly unstable neutron-rich nuclei can be deduced. A surprisingly large γγ branching was observed for a number of isotopes which might indicate the need to increase by a large factor the Hauser-Feshbach (n, γγ) cross-section estimates that impact on r process abundance calculations. peerReviewed

total absorption gamma-ray spectroscopybeta-delayed neutron emittersAstrophysics::High Energy Astrophysical Phenomenar-processutron-capture ratesNuclear Experiment
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Total absorption spectroscopy study of the β decay of 86Br and 91Rb

2017

The beta decays of 86Br and 91Rb have been studied using the total absorption spectroscopy technique. The radioactive nuclei were produced at the Ion Guide Isotope Separator On-Line facility in Jyväskylä and further purified using the JYFLTRAP. 86Br and 91Rb are considered to be major contributors to the decay heat in reactors. In addition, 91Rb was used as a normalization point in direct measurements of mean gamma energies released in the beta decay of fission products by Rudstam et al. assuming that this decay was well known from high-resolution measurements. Our results show that both decays were suffering from the Pandemonium effect and that the results of Rudstam et al. should be renor…

total absorption gamma-ray spectroscopyrubidiumneutron emissionHigh Energy Physics::Experimentbeta decaybromiNuclear Experiment
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Total absorption γ-ray spectroscopy of the β-delayed neutron emitters 87Br, 88Br, and 94Rb

2017

We investigate the decay of 87,88Br and 94Rb using total absorption γ -ray spectroscopy. These important fission products are β-delayed neutron emitters. Our data show considerable βγ intensity, so far unobserved in high-resolution γ -ray spectroscopy, from states at high excitation energy. We also find significant differences with the β intensity that can be deduced from existing measurements of the β spectrum. We evaluate the impact of the present data on reactor decay heat using summation calculations. Although the effect is relatively small it helps to reduce the discrepancy between calculations and integral measurements of the photon component for 235U fission at cooling times in the r…

total absorption gamma-ray spectroscopyrubidiumneutron emissionbeta decaybromiNuclear Experiment
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Haemolymphatic Parameters in Two Aquaculture Crustacean Species Cherax destructor (Clark, 1836) and Cherax quadricarinatus (Von Martens, 1868)

2022

In the last few years, there has been a notable development in the breeding of freshwater shrimp (astaciculture), which involved various species and in particular, the two Australian Parastacidae species, Cherax destructor and Cherax quadricarinatus. Information about the haemolymphatic parameters of these two species is fragmentary, and filling these gaps becomes important given their importance in aquaculture. Cellular and biochemical parameters were analyzed in both species to create a reference baseline for these parameters to identify the state of welfare or suffering of these animals. The results showed that the total haemocyte count, haemocyte subpopulations, enzymatic activities and…

total haemocytes countGeneral VeterinarycrayfishSettore BIO/10 - BiochimicaSettore BIO/05 - ZoologiaAnimal Science and Zoologytotal proteinaquaculture plantCherax spp.crayfish; <i>Cherax</i> spp.; total haemocytes count; total protein; aquaculture plantAnimals; Volume 12; Issue 5; Pages: 543
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Three-dimensional core-collapse supernovae with complex magnetic structures: I. Explosion dynamics

2021

Magnetic fields can play a major role in the dynamics of outstanding explosions associated to violent events such as GRBs and hypernovae, since they provide a natural mechanism to harness the rotational energy of the central proto-neutron star and power relativistic jets through the stellar progenitor. As the structure of such fields is quite uncertain, most numerical models of MHD-driven core-collapse supernovae consider an aligned dipole as initial magnetic field, while the field's morphology can actually be much more complex. We present three-dimensional simulations of core-collapse supernovae with more realistic magnetic structures, such as quadrupolar fields and, for the first time, an…

transients: supernovaeField (physics)MHDAstrophysics::High Energy Astrophysical Phenomenagamma-ray burst: generalFOS: Physical sciencesAstrophysics01 natural sciencesstars: magnetarsAstrophysical jet0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)relativistic processesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstronomy and AstrophysicsRotational energyMagnetic fieldDipoleAstrophysics - Solar and Stellar AstrophysicsinstabilitiesSpace and Planetary ScienceMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]HypernovaDynamo
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The impact of non-dipolar magnetic fields in core-collapse supernovae

2019

The magnetic field is believed to play an important role in at least some core-collapse supernovae if its magnitude reaches $10^{15}\,\rm{G}$, which is a typical value for a magnetar. In the presence of fast rotation, such a strong magnetic field can drive powerful jet-like explosions if it has the large-scale coherence of a dipole. The topology of the magnetic field is, however, probably much more complex with strong multipolar and small-scale components and the consequences for the explosion are so far unclear. We investigate the effects of the magnetic field topology on the dynamics of core-collapse supernovae and the properties of forming proto-neutron star (PNS) by comparing pre-collap…

transients: supernovaeMHDAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCompact starMagnetar01 natural sciencesstars: magnetars0103 physical sciences010303 astronomy & astrophysicsrelativistic processesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Toroid010308 nuclear & particles physicsgamma-ray burststurbulenceAstronomy and AstrophysicsRotational energyComputational physicsMagnetic fieldSupernovaDipoleSpace and Planetary ScienceMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Monthly Notices of the Royal Astronomical Society
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Clase social y acceso a la universidad

2021

La universidad es una institución que tiene más de ocho siglos de antigüedad. En la mayor parte de su historia, si no en toda, favoreció la desigualdad de género y de etnia, excluyendo durante siglos a las mujeres y a las minorías étnicas y relegándolas más recientemente a posiciones subalternas. Este artículo se centra en la desigualdad de clases sociales, que lógicamente intersecta con las otras.&#x0D; The university is an institution that is more than eight centuries old. For most of its history, if not all, it favored gender and ethnic inequality, excluding women and ethnic minorities for centuries and relegating them more recently to subordinate positions. This article focuses on the i…

trayectorias académicasClasses socialsincorporación a la universidadGeneral Medicine:PEDAGOGÍA [UNESCO]clases socialesUNESCO::PEDAGOGÍA
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Digital ulcer, Raynaud phenomenon and osteomyelitis of the fifth finger in patient with systemic sclerosis: personal experience

2012

ulcer raynaud phenomenon osteomyelitis scleroderma systemic
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Search for photons with energies above 1018 eV using the hybrid detector of the Pierre Auger Observatory

2017

A search for ultra-high energy photons with energies above 1 EeV is performed using nine years of data collected by the Pierre Auger Observatory in hybrid operation mode. An unprecedented separation power between photon and hadron primaries is achieved by combining measurements of the longitudinal air-shower development with the particle content at ground measured by the fluorescence and surface detectors, respectively. Only three photon candidates at energies 1-2 EeV are found, which is compatible with the expected hadron-induced background. Upper limits on the integral flux of ultra-high energy photons of 0.027, 0.009, 0.008, 0.008 and 0.007 km-2 sr-1 yr-1 are derived at 95% C.L. for ener…

ultra high energy cosmic rays cosmic ray experimentsPhoton[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]AstronomyHadronFluxultra high energy cosmic rays; cosmic ray experiments7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)energy: thresholdCosmic ray experiments[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsphoton: productionconstraint: energyCOSMIC-RAYSAugerobservatoryContent (measure theory)ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearfluorescenceAstrophysics - High Energy Astrophysical PhenomenalongitudinalAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesCosmic rayultra high energy cosmic raysdark matterUltra high energy cosmic rays Cosmic ray experiments Astronomy and Astrophysics.Nuclear physics[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesultra high energy cosmic rays; cosmic ray experiments; Astronomy and Astrophysicscosmic radiation: UHEHigh Energy PhysicsCiencias ExactasPierre Auger ObservatorySPECTRUMhybridbackgrounddetector: surface010308 nuclear & particles physicsFísicaUltra high energy cosmic raysAstronomy and AstrophysicsASTROFÍSICAULTRA-HIGH ENERGYfluxExperimental High Energy PhysicsHigh Energy Physics::Experimentcosmic ray experimentshadron[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)
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