Search results for "Dewey"

showing 10 items of 102 documents

Search for Gravitational-wave Signals Associated with Gamma-Ray Bursts during the Second Observing Run of Advanced LIGO and Advanced Virgo

2019

We present the results of targeted searches for gravitational-wave transients associated with gamma-ray bursts during the second observing run of Advanced LIGO and Advanced Virgo, which took place from 2016 November to 2017 August. We have analyzed 98 gamma-ray bursts using an unmodeled search method that searches for generic transient gravitational waves and 42 with a modeled search method that targets compact-binary mergers as progenitors of short gamma-ray bursts. Both methods clearly detect the previously reported binary merger signal GW170817, with p-values of <9.38 10-6 (modeled) and 3.1 10-4 (unmodeled). We do not find any significant evidence for gravitational-wave signals associate…

Burst astrophysicAstrofísicaneutron star: binary010504 meteorology & atmospheric sciencesBinary numberAstrophysics01 natural sciencesLIGOQCSUPERNOVArelativistic jetsQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01counterpartGRBGravitational waves (678)Physical SciencesRELATIVISTIC JETSAstrophysics - High Energy Astrophysical PhenomenaGravitational waveGravitationstarsblack-holeAstrophysics::High Energy Astrophysical PhenomenaGeneral Relativity and Quantum Cosmology (gr-qc)precursor activityGravitational wavesSettore FIS/05 - Astronomia e AstrofisicasupernovaCORE-COLLAPSEGamma-ray burstGravitational wave sourcesScience & TechnologyVirgoRCUKAstronomy and AstrophysicsHigh energy astrophysics (739)RedshiftDewey Decimal Classification::500 | Naturwissenschaften::520 | Astronomie Kartographiedetector: sensitivityVIRGOSpace and Planetary Sciencegravitational radiation: emissionBLACK-HOLEddc:520Gravitational wave astronomyGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]STARSGravitacióAstronomySignalGeneral Relativity and Quantum CosmologyBurst astrophysicslocalizationemission010303 astronomy & astrophysicsPhysicsDetectorGamma-ray bursts (629)[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave sourcePRECURSOR ACTIVITYGamma-ray burstsLIGO (920)High energy astrophysicsdata analysis methodBurst astrophysics (187)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstAstronomy & AstrophysicsMASSgravitational radiation: direct detectionGravitational wave astronomy Gravitational wave sources LIGO; Gravitational waves Gamma-ray bursts Burst astrophysics High energy astrophysicsGravitational wave astronomy (675)electromagnetic field: production0103 physical sciencesnumerical calculationsGRB; gravitational waves; LIGO; VirgoSTFC0105 earth and related environmental sciencesgravitational wavesneutron starsGravitational waveCOUNTERPARTgravitational radiationLIGOcore-collapsegravitational radiation detectorGravitational wave sources (677)radiationNeutron starPhysics and AstronomymassRADIATIONEMISSIONGravitational wave astronomy; Gravitational wave sources; LIGO; Gravitational waves; Gamma-ray bursts; Burst astrophysics; High energy astrophysics
researchProduct

Improved limit on the directly measured antiproton lifetime

2017

Continuous monitoring of a cloud of antiprotons stored in a Penning trap for 405 days enables us to set an improved limit on the directly measured antiproton lifetime. From our measurements we extract a storage time of $3.15\times {10}^{8}$ equivalent antiproton-seconds, resulting in a lower lifetime limit of ${\tau }_{\bar{{\rm{p}}}}\gt 10.2\,{\rm{a}}$ with a confidence level of $68 \% $. This result improves the limit on charge-parity-time violation in antiproton decays based on direct observation by a factor of 7.

CPT symmetryPenning trapGeneral Physics and Astronomypenning traps01 natural sciencesLower limit010305 fluids & plasmasNuclear physicsContinuous monitoring0103 physical sciencesddc:530Limit (mathematics)Physics::Atomic Physics010306 general physicsNuclear ExperimentPhysicsCPT invariancePhysicsResearchContinuous monitoringDirect observationsDirect observationConfidence levelsPenning trapCharge parityAntiprotonlifetimesPhysics::Accelerator PhysicsCP violationHigh Energy Physics::ExperimentDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikPräzisionsexperimente - Abteilung BlaumantiprotonsParticle Physics - Experiment
researchProduct

Ultracold atomic Bose and Fermi spinor gases in optical lattices

2006

We investigate magnetic properties of Mott-insulating phases of ultracold Bose and Fermi spinor gases in optical lattices. We consider in particular the F=2 Bose gas, and the F=3/2 and F=5/2 Fermi gases. We derive effective spin Hamiltonians for one and two atoms per site and discuss the possibilities of manipulating the magnetic properties of the system using optical Feshbach resonances. We discuss low temperature quantum phases of a 87Rb gas in the F=2 hyperfine state, as well as possible realizations of high spin Fermi gases with either 6Li or 132Cs atoms in the F=3/2 state, and with 173Yb atoms in the F=5/2 state.

Condensed Matter::Quantum GasesPhysicseinstein condensationSpinorBose gasCondensed matter physicsFOS: Physical sciencesGeneral Physics and Astronomyresonant lightQuantum phasesState (functional analysis)quantum phasesCondensed Matter - Other Condensed Matterground-statesone bosonssystemsddc:530Condensed Matter::Strongly Correlated ElectronsantiferromagnetsDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikHyperfine structureOther Condensed Matter (cond-mat.other)Spin-½Fermi Gamma-ray Space TelescopeNew Journal of Physics
researchProduct

GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences

2018

The LIGO Scientific and Virgo Collaborations have announced the first detection of gravitational waves from the coalescence of two neutron stars. The merger rate of binary neutron stars estimated from this event suggests that distant, unresolvable binary neutron stars create a significant astrophysical stochastic gravitational-wave background. The binary neutron star background will add to the background from binary black holes, increasing the amplitude of the total astrophysical background relative to previous expectations. In the Advanced LIGO-Virgo frequency band most sensitive to stochastic backgrounds (near 25 Hz), we predict a total astrophysical background with amplitude $\Omega_{\rm…

Design sensitivityneutron star: binarygravitational radiation: stochasticAstronomyX-ray binaryGeneral Physics and AstronomyAstrophysicsAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologylocalizationGravitational wave backgroundGravitational Waves Neutron Stars Stochastic Background Virgo LIGOblack holeLIGOstochastic modelQCQBPhysicsGAMMA-RAY BURSTSSignal to noise ratioStochastic systemsBlack holesGravitational effectsarticleAstrophysics::Instrumentation and Methods for AstrophysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSING[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave sources Experimental studies of gravity Gravitational WavesGravitationBinary neutron starsX-ray bursterBinsAstrophysics::High Energy Astrophysical PhenomenaMERGERSFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsGravity wavesgravitational radiation: direct detectionBinary pulsarNeutron starsSTAR-FORMATIONPhysics and Astronomy (all)General Relativity and Quantum CosmologyBinary black holebinary: coalescence0103 physical sciencesFrequency bandsddc:530RATESINTERFEROMETERS010306 general physicsAstrophysics::Galaxy AstrophysicsNeutronsGravitational Waves010308 nuclear & particles physicsGravitational waveVirgogravitational radiation: backgroundgravitational radiationAstronomyNeutron Stars530 Physikbinary: compactsensitivityStarsLIGObackground: stochasticEVOLUTIONsignal noise ratioVIRGOPhysics and Astronomyblack hole: binarygravitational radiation: emissionStellar black holeStochastic BackgroundDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikHIGH-REDSHIFTneutron star: coalescencePhysical Review Letters
researchProduct

Klimt artwork: red-pigment material investigation by backscattering Fe-57 Mössbauer spectroscopy, SEM and p-XRF

2017

Material tests were performed on a rediscovered Klimt-artwork "Trompetender Putto". We performed studies on the red colored spots, mainly taken from non-restored parts. MIMOS II Fe-57 Mossbauer spectroscopy (novelty in art-pigment analysis) mainly reveals haematite and crystallized goethite in red colors. Electron microscopy can identify various layers of the original and overpainting of an artwork. The number of layers fluctuates between three and four chemically painted areas. The portable X-ray fluorescence analysis enables to reduce the pigment list to containing mercury (cinnabar), lead, zinc, iron and titanium. Infrared-light-irradiation visualizes the different age of the pigments.

Dewey Decimal Classification::500 | Naturwissenschaften::540 | ChemieArcheologyGoethiteMaterials scienceScanning electron microscopepigmentsAnalytical chemistryinfra-red-light investigationchemistry.chemical_elementZinc01 natural sciencesKlimt: “Trompetender Putto”PigmentMaterialcharakterisierung0103 physical sciencesMössbauer spectroscopy0601 history and archaeologyddc:750lcsh:CC1-960010306 general physics060102 archaeologyTrompetender PuttoMössbauer spectroscopy06 humanities and the artsDewey Decimal Classification::700 | Künste Bildende Kunst allgemein::750 | MalereiOverpaintingKlimt GustavDewey Decimal Classification::700 | Künste Bildende Kunst allgemeinCinnabarchemistryPigmentvisual_artddc:540visual_art.visual_art_mediumddc:660lcsh:ArchaeologyX-ray fluorescence analysisddc:700660 Technische Chemiescanning electron microscopyTitanium
researchProduct

High spatial resolution analysis of the iron oxidation state in silicate glasses using the electron probe

2018

The iron oxidation state in silicate melts is important for understanding their physical properties, although it is most often used to estimate the oxygen fugacity of magmatic systems. Often high spatial resolution analyses are required, yet the available techniques, such as μrXANES and μMössbauer, require synchrotron access. The flank method is an electron probe technique with the potential to measure Fe oxidation state at high spatial resolution but requires careful method development to reduce errors related to sample damage, especially for hydrous glasses. The intensity ratios derived from measurements on the flanks of FeLα and FeLβ X-rays (FeLβf/FeLαf) over a time interval (time-depend…

Dewey Decimal Classification::500 | Naturwissenschaften::540 | ChemieMaterials science010504 meteorology & atmospheric sciencesoxidationAnalytical chemistryreductionElectron010502 geochemistry & geophysics01 natural sciencesflank methodReduction (complexity)symbols.namesakeelectron beam damageGeochemistry and PetrologyOxidation stateElectron probe microanalysis (EPMA)High spatial resolutioniron (Fe) oxidation statesilicate glassSilicate glass0105 earth and related environmental sciencesGeophysicsddc:540Raman spectroscopysymbolsRaman spectroscopy
researchProduct

Volatile dilution during magma injections and implications for volcano explosivity

2016

Magma reservoirs underneath volcanoes grow through episodic emplacement of magma batches. These pulsed magma injections can substantially alter the physical state of the resident magma by changing its temperature, pressure, composition, and volatile content. Here we examine plagioclase phenocrysts in pumice from the 2014 Plinian eruption of Kelud (Indonesia) that record the progressive capture of small melt inclusions within concentric growth zones during crystallization inside a magma reservoir. High-spatial-resolution Raman spectroscopic measurements reveal the concentration of dissolved H2O within the melt inclusions, and provide insights into melt-volatile behavior at the single crystal…

Dewey Decimal Classification::500 | Naturwissenschaften::550 | GeowissenschaftenAsiaFar East010504 meteorology & atmospheric sciencesinclusionspyroclasticsMineralogyVolcanic explosivity indexengineering.material010502 geochemistry & geophysicsAnorthite01 natural sciencespumicePumiceddc:550PlagioclaseFluid inclusionsPetrology0105 earth and related environmental sciencesMelt inclusionsGeologyGeokemimagmasGeochemistryfluid inclusionsIndonesiaigneous rocksMagmaengineeringPhenocrystvolcanic rocksJavaGeology
researchProduct

A snapshot of the transition from monogenetic volcanoes to composite volcanoes: Case study on the Wulanhada Volcanic Field (northern China)

2022

The transition processes from monogenetic volcanoes to composite volcanoes are poorly understood. The Late Pleistocene to Holocene intraplate monogenetic Wulanhada Volcanic Field (WVF) in northern China provides a snapshot of such a transition. Here we present petrographic observations, mineral chemistry, bulk rock major and trace element data, thermobarometry, and a partial melting model for the WVF to evaluate the lithology and partial melting degree of the mantle source, the crystallization conditions, and pre-eruptive magmatic processes occurring within the magma plumbing system. The far-field effect of India–Eurasia collision resulted in a relatively high degree (10 %–20 %) of partial …

Dewey Decimal Classification::500 | Naturwissenschaften::550 | GeowissenschaftenDewey Decimal Classification::500 | Naturwissenschaften::540 | ChemieMagnesiaLithologyFeldsparddc:540ddc:550AlkalinityMelting
researchProduct

Combined proton NMR wideline and NMR relaxometry to study SOM-water interactions of cation-treated soils

2013

Abstract Focusing on the idea that multivalent cations affect SOM matrix and surface, we treated peat and soil samples by solutions of NaCl, CaCl2 or AlCl3. Water binding was characterized with low field 1H-NMR-relaxometry (20 MHz) and 1H wideline NMR spectroscopy (400 MHz) and compared to contact angles. From 1H wideline, we distinguished mobile water and water involved in water molecule bridges (WaMB). Large part of cation bridges (CaB) between SOM functional groups are associated with WaMB. Unexpectedly, 1H NMRrelaxometry relaxation rates suggest that cross-linking in the Al-containing peat is not stronger than that by Ca. The relation between percentage of mobile water and WaMB water in…

Dewey Decimal Classification::500 | Naturwissenschaften::550 | GeowissenschaftenDewey Decimal Classification::500 | Naturwissenschaften::570 | Biowissenschaften BiologieDewey Decimal Classification::600 | Technik::630 | Landwirtschaft VeterinärmedizinAnalytical chemistrySoil organic matter (SOM); Low field 1H NMR relaxometry; 1H wideline NMR spectroscopy; Contact angle; Cation bridges; Water molecule bridges.TA Engineering (General). Civil engineering (General)soil organic matter (som)Low field H-1 NMR relaxometrystateContact angleNuclear magnetic resonancewater molecule bridgesddc:550ddc:630natural organic-mattercontact angleWater Science and TechnologyFluid Flow and Transfer Processeschemistry.chemical_classificationhumic substancesWater molecule bridges.Nuclear magnetic resonance spectroscopycation bridgesCation bridgemultiexponential decay datanuclear-magnetic-resonanceH-1 wideline NMR spectroscopyProton NMRWater bindingTC1-978Relaxometryuniform-penalty inversionlow field 1h nmr relaxometrySettore AGR/13 - Chimica AgrariaContext (language use)1h wideline nmr spectroscopyforest soilsCation bridgesddc:570sandy soilOrganic mattercontact-angleContact angleSoil organic matter (SOM)repellencyMechanical EngineeringHydraulic engineeringchemistrySoil waterWater molecule bridgesJournal of Hydrology and Hydromechanics
researchProduct

Search for Subsolar Mass Ultracompact Binaries in Advanced LIGO's Second Observing Run

2019

We present a search for subsolar mass ultracompact objects in data obtained during Advanced LIGO’s second observing run. In contrast to a previous search of Advanced LIGO data from the first observing run, this search includes the effects of component spin on the gravitational waveform. We identify no viable gravitational-wave candidates consistent with subsolar mass ultracompact binaries with at least one component between \ud0.2\ud \ud \udM\ud⊙\ud–\ud1.0\ud \ud \udM\ud⊙\ud. We use the null result to constrain the binary merger rate of (\ud0.2\ud \ud \udM\ud⊙\ud, \ud0.2\ud \ud \udM\ud⊙\ud) binaries to be less than \ud3.7\ud×\ud10\ud5\ud \ud \udGpc\ud−\ud3\ud \udyr\ud−\ud1\udand the binary …

Dewey Decimal Classification::500 | Naturwissenschaften::550 | Geowissenschaftenbinary: massAstrofísicaGravitacióFormation modeldensity: fluctuationAstronomyGeneral Physics and Astronomydetector: networkspin01 natural sciencesGeneral Relativity and Quantum CosmologyLIMITSblack hole: formationddc:550black holeDark MatterAstrophysics::Solar and Stellar AstrophysicsLIGOQCQBnucleus: interactionSettore FIS/01astro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)gravitational wave; physics; astronomyPhysicsarticleDensity fluctuationgravitational wavesPhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]astro-ph.COAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomenablack hole: primordialGravitationAstrophysics - Cosmology and Nongalactic AstrophysicsMatter densitydensity: primordialCosmology and Nongalactic Astrophysics (astro-ph.CO)coolinggr-qcAstrophysics::High Energy Astrophysical PhenomenaPhysics MultidisciplinaryCooling mechanismPrimordial black holesFOS: Physical sciencesdark matter: densityGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsGravity wavesNuclear interactionGravitation and AstrophysicsMergingGeneral Relativity and Quantum Cosmologynull resultSettore FIS/05 - Astronomia e Astrofisicabinary: coalescence0103 physical sciencesddc:530010306 general physicsAstrophysics::Galaxy AstrophysicsSTFCScience & Technologymass: solarCosmologiaStellar evolutions010308 nuclear & particles physicsMatter fractionsgravitational radiationRCUKblack hole: massGalaxiesbinary: compactStarsgravitational radiation detectordetector: sensitivityVIRGOPhysics and Astronomygravitational radiation: emissionDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Gravitational waves Black holes (astronomy) Gravitational self forcePhysical Review Letters
researchProduct