Search results for "actin"

showing 10 items of 1375 documents

Chemical studies of elements with Z≥ 104 in liquid phase

2015

Abstract Recent studies of the chemical separation and characterization experiments of the first three transactinide elements, rutherfordium (Rf), dubnium (Db), and seaborgium (Sg), conducted atom-at-a-time in liquid phases, are reviewed. A short description on experimental techniques based on partition methods, specifically automated rapid chemical separation systems, is also given. A newly developed experimental approach to investigate single atoms of the heaviest elements with an electrochemical method is introduced. Perspectives for liquid-phase chemistry experiments on heavier elements are briefly discussed.

PhysicsDubniumNuclear and High Energy PhysicsCountercurrent chromatographyChemical substancechemistrySeaborgiumRutherfordiumAnalytical chemistryLiquid phaseTransactinide elementchemistry.chemical_elementScience technology and societyNuclear Physics A
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Frontiers of Heavy - Ion Physics and Superheavy Elements

2003

This contribution will focus on three topics of GSI nuclear structure research: super heavy elements, direct mass measurements in the storage ring, and the measurement of spallation cross section in reversed kinematics. The GSI project for an extended synchrotron facility will be outlined.

PhysicsFocus (computing)Nuclear and High Energy PhysicsFissionNuclear structureTransactinide elementSuperheavy ElementsSynchrotronlaw.inventionNuclear physicsCross section (physics)Nuclear Energy and EngineeringlawHeavy ionSpallationStorage ringJournal of Nuclear Science and Technology
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Isomeric states in Rf256

2021

The question of the number and origin of isomeric states in $^{256}\mathrm{Rf}$ arose from two independent experiments but remained unanswered for a decade. To shed light on this puzzle, we studied isomeric decay in $^{256}\mathrm{Rf}$ by measuring conversion electrons with fast fully digital electronics. $^{256}\mathrm{Rf}$ was produced in the fusion-evaporation reactions of $^{50}\mathrm{Ti}+^{207}\mathrm{Pb}$ and $^{50}\mathrm{Ti}+^{208}\mathrm{Pb}$ at the gas-filled recoil separator TransActinide Separator and Chemistry Apparatus. Among a total of 120 decays of $^{256}\mathrm{Rf}$, we detected 22 and 12 decays proceeding through one and two isomeric states. Half-lives of the low- and hi…

PhysicsGood quantum numbereducation.field_of_studyPopulationTransactinide elementProduction (computer science)ElectronAtomic physicseducationRecoil separatorPhysical Review C
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Constraints on black-hole charges with the 2017 EHT observations of M87*

2021

Full list of authors: Kocherlakota, Prashant; Rezzolla, Luciano; Falcke, Heino; Fromm, Christian M.; Kramer, Michael; Mizuno, Yosuke; Nathanail, Antonios; Olivares, Héctor; Younsi, Ziri; Akiyama, Kazunori; Alberdi, Antxon; Alef, Walter; Algaba, Juan Carlos; Anantua, Richard; Asada, Keiichi; Azulay, Rebecca; Baczko, Anne-Kathrin; Ball, David; Baloković, Mislav; Barrett, John; Benson, Bradford A.; Bintley, Dan; Blackburn, Lindy; Blundell, Raymond; Boland, Wilfred; Bouman, Katherine L.; Bower, Geoffrey C.; Boyce, Hope; Bremer, Michael; Brinkerink, Christiaan D.; Brissenden, Roger; Britzen, Silke; Broderick, Avery E.; Broguiere, Dominique; Bronzwaer, Thomas; Byun, Do-Young; Carlstrom, John E.; …

PhysicsGravitació010308 nuclear & particles physicsAstronomyKinoAstrophysics::High Energy Astrophysical Phenomenagr-qcChatterjeeFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Creative commons01 natural sciencesGeneral Relativity and Quantum Cosmology0103 physical sciencesAstronomiaFish <Actinopterygii>010306 general physicsGeneral relativity and quantum cosmologyHumanitiesPhysical Review D. Particles and Fields
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Search for dark matter in the Sun with the ANTARES neutrino telescope in the CMSSM and mUED frameworks

2012

ANTARES is the first neutrino telescope in the sea. It consists of a three-dimensional array of 885 photomultipliers to collect the Cherenkov light induced by relativistic muons produced in CC interactions of high energy neutrinos. One of the main scientific goals of the experiment is the search for dark matter. We present here the analysis of data taken during 2007 and 2008 to look for a WIMP signal in the Sun. WIMPs are one of the most popular scenarios to explain the dark matter content of the Universe. They would accumulate in massive objects like the Sun or the Galactic Center and their self-annihilation would produce (directly or indirectly) high energy neutrinos detectable by neutrin…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Nuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaDark matterAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSolar neutrino problemHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Neutrino detectorWeakly interacting massive particlesHigh Energy Physics::ExperimentFísica nuclearNeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical PhenomenaInstrumentationLight dark matter
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Fuzzy Dark Matter and Non-Standard Neutrino Interactions

2018

We discuss novel ways in which neutrino oscillation experiments can probe dark matter. In particular, we focus on interactions between neutrinos and ultra-light ("fuzzy") dark matter particles with masses of order $10^{-22}$ eV. It has been shown previously that such dark matter candidates are phenomenologically successful and might help ameliorate the tension between predicted and observed small scale structures in the Universe. We argue that coherent forward scattering of neutrinos on fuzzy dark matter particles can significantly alter neutrino oscillation probabilities. These effects could be observable in current and future experiments. We set new limits on fuzzy dark matter interacting…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Particle physicsSterile neutrino010308 nuclear & particles physicsSolar neutrinoDark matterScalar field dark matterFOS: Physical sciencesSolar neutrino problem7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Weakly interacting massive particles0103 physical sciencesNeutrinoAstrophysics - High Energy Astrophysical Phenomena010306 general physicsDark fluid
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Single Particle Levels and ββ-Decay Matrix Elements in The Interacting Boson Model

2018

Recently a new method to calculate the occupancies of single particle levels in atomic nuclei was developed in the context of the microscopic interacting boson model, in which neutron and proton degrees of freedom are treated explicitly (IBM-2). The energies of the single particle levels constitute a very important input for the calculation of the occupancies in this method, and further they play important role in the calculation of double beta decay nuclear matrix elements. Here we discuss how the 0νββ, 0νhββ, and 2νββ-decay nuclear matrix elements (NMEs) are affected when the energies of single particle levels are changed. peerReviewed

PhysicsHistoryProtonNuclear TheoryDegrees of freedom (physics and chemistry)double beta decayContext (language use)nuclear matrix elementsComputer Science ApplicationsEducationNuclear physicsMatrix (mathematics)Double beta decayAtomic nucleusNeutronInteracting boson modelNuclear Experimentydinfysiikka
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The star formation activity in cosmic voids

2014

Using a sample of cosmic voids identified in the Sloan Digital Sky Survey Data Release 7, we study the star formation activity of void galaxies. The properties of galaxies living in voids are compared with those of galaxies living in the void shells and with a control sample, representing the general galaxy population. Void galaxies appear to form stars more efficiently than shell galaxies and the control sample. This result can not be interpreted as a consequence of the bias towards low masses in underdense regions, as void galaxy subsamples with the same mass distribution as the control sample also show statistically different specific star formation rates. This highlights the fact that g…

PhysicsIntergalactic starFOS: Physical sciencesAstronomyAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGalaxy mergerAstrophysics - Astrophysics of GalaxiesVoid galaxyPeculiar galaxySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Elliptical galaxyGalaxy formation and evolutionInteracting galaxyLenticular galaxyAstrophysics::Galaxy Astrophysics
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ACTINIDE AND ULTRA-HEAVY ABUNDANCES IN THE LOCAL GALACTIC COSMIC RAYS: AN ANALYSIS OF THE RESULTS FROM THELDEFULTRA-HEAVY COSMIC-RAY EXPERIMENT

2012

The LDEF Ultra-Heavy Cosmic-Ray Experiment (UHCRE) detected Galactic cosmic rays (GCRs) of charge Z ≥ 70 in Earth orbit with an exposure factor of 170 m2 sr yr, much larger than any other experiment. The major results include the first statistically significant uniform sample of GCR actinides with 35 events passing quality cuts, evidence for the existence of transuranic nuclei in the GCR with one 96Cm candidate event, and a low 82Pb/78Pt ratio consistent with other experiments. The probability of the existence of a transuranic component is estimated as 96%, while the most likely 92U/90Th ratio is found to be 0.4 within a wide 70% confidence interval ranging from 0 to 0.96. Overall, the resu…

PhysicsInterstellar mediumEarth's orbitSpace and Planetary ScienceSource materialAstronomyAstronomy and AstrophysicsSmall sampleCosmic rayAstrophysicsActinideEvent (particle physics)Confidence intervalThe Astrophysical Journal
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Investigation of nuclear collectivity in the neutron mid-shell nucleusPb186

2007

For the first time, non-yrast structures of the neutron mid-shell nucleus $^{186}\mathrm{Pb}$ have been identified in an in-beam \ensuremath{\gamma}-ray spectroscopy measurement using the recoil-decay tagging technique. The yrast band has been tentatively extended up to ${I}^{\ensuremath{\pi}}=20{}^{+},$ revealing a similar backbend to that observed in the Pt and Hg isotones. Three new bands and several other transitions have been observed. Calculations carried out in the framework of the interacting boson model together with mean-field studies using the generator coordinate method provide arguments for the association of one of the new bands with an oblate shape. The present data also show…

PhysicsMass numberNuclear and High Energy PhysicsGenerator (category theory)YrastNuclear TheoryNuclear physicsMean field theoryNeutronGamma spectroscopyInteracting boson modelAtomic physicsNuclear ExperimentSpectroscopyPhysical Review C
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