Search results for "physical sciences"

showing 10 items of 20240 documents

Tin resonance-ionization schemes for atomic- And nuclear-structure studies

2020

This paper presents high-precision spectroscopic measurements of atomic tin using five different resonance-ionization schemes performed with the collinear resonance-ionization spectroscopy technique. Isotope shifts were measured for the stable tin isotopes from the $5{s}^{2}5{p}^{2}\phantom{\rule{0.28em}{0ex}}^{3}{P}_{0,1,2}$ and ${}^{1}{S}_{0}$ to the $5{s}^{2}5p6s\phantom{\rule{0.28em}{0ex}}^{1}{P}_{1},^{3}{P}_{1,2}$ and $5{s}^{2}5p7s{\phantom{\rule{0.28em}{0ex}}}^{1}{P}_{1}$ atomic levels. The magnetic dipole hyperfine constants ${A}_{\mathrm{hf}}$ have been extracted for six atomic levels with electron angular momentum $Jg0$ from the hyperfine structures of nuclear spin $I=1/2$ tin isot…

spektroskopiachemistry.chemical_elementPhysics Atomic Molecular & Chemical7. Clean energy01 natural sciences010305 fluids & plasmasatomifysiikkaAtomic theory0103 physical sciencesIsotopes of tinNuclear Physics - ExperimentPhysics::Atomic Physics010306 general physicsSpectroscopyHyperfine structurePhysicsisotoopitScience & TechnologyPhysicsNuclear structureCharge (physics)OpticsConfiguration interactionchemistryPhysical SciencestinaAtomic physicsTinPhysical Review A
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Spectroscopy of short-lived radioactive molecules

2020

Molecular spectroscopy offers opportunities for the exploration of the fundamental laws of nature and the search for new particle physics beyond the standard model1–4. Radioactive molecules—in which one or more of the atoms possesses a radioactive nucleus—can contain heavy and deformed nuclei, offering high sensitivity for investigating parity- and time-reversal-violation effects5,6. Radium monofluoride, RaF, is of particular interest because it is predicted to have an electronic structure appropriate for laser cooling6, thus paving the way for its use in high-precision spectroscopic studies. Furthermore, the effects of symmetry-violating nuclear moments are strongly enhanced5,7–9 in molecu…

spektroskopiacollinearnucl-ex01 natural sciences010305 fluids & plasmasRadiumchemistry.chemical_compoundIonizationExperimental nuclear physicsNuclear ExperimentPhysicsMultidisciplinaryLarge Hadron ColliderStable isotope rationew physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]hep-thmolekyylithep-phradiumelectron: electric momentNuclear Physics - Theoryradioactivitymany-body problemElectronic structure of atoms and moleculesAtomic physicsydinfysiikkaParticle Physics - Theoryexceptionalnucl-th[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]MonofluorideResearchInstitutes_Networks_Beacons/photon_science_institutechemistry.chemical_elementnucleus: structure functionElectronic structure[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Photon Science InstituteArticle0103 physical sciencesionizationMoleculeNuclear Physics - Experiment010306 general physicsSpectroscopyenhancementParticle Physics - Phenomenologystabilitysensitivitylaserchemistry[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Exotic atoms and moleculesnucleus: deformation
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Exotic Spin-Orbital Physics in Hybrid Oxides

2016

We compare the effective spin-orbital super\-exchange triggered by magnetic $3d$ impurities with $d^3$ and $d^2$ configurations and either no orbital degree of freedom (orbital dilution) or hole replacing a doublon (charge dilution) in a $4d^4$ Mott insulator with $S=1$ spins. Impurities causing orbital dilution act either as spin defects decoupled from the surrounding ions, or generate orbital polarons along $d^3$-$d^4$ hybrid bonds. The exchange on these bonds determines which orbital is occupied by a doublon on the host site. In case of charge dilution by $3d^2$ impurities additional $\propto T_i^+T_j^+$ terms arise which enhance orbital fluctuations. We show that such terms may radicall…

spin-orbital orderorbital fluctuationsFOS: Physical sciences02 engineering and technologyPolaron01 natural sciencesIonCondensed Matter - Strongly Correlated Electrons0103 physical sciences010306 general physicsSpin (physics)PhysicsCondensed Matter - Materials ScienceStrongly Correlated Electrons (cond-mat.str-el)Condensed matter physicsSpinsMott insulatorDopingMaterials Science (cond-mat.mtrl-sci)Charge (physics)021001 nanoscience & nanotechnologyCondensed Matter Physicsorbital/charge dilutionElectronic Optical and Magnetic MaterialsDoped Mott insulatorSuperexchangeCondensed Matter::Strongly Correlated ElectronsAstrophysics::Earth and Planetary Astrophysics0210 nano-technologyJournal of Superconductivity and Novel Magnetism
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Three-dimensional skyrmions in spin-2 Bose–Einstein condensates

2017

We introduce topologically stable three-dimensional skyrmions in the cyclic and biaxial nematic phases of a spin-2 Bose-Einstein condensate. These skyrmions exhibit exceptionally high mapping degrees resulting from the versatile symmetries of the corresponding order parameters. We show how these structures can be created in existing experimental setups and study their temporal evolution and lifetime by numerically solving the three-dimensional Gross-Pitaevskii equations for realistic parameter values. Although the biaxial nematic and cyclic phases are observed to be unstable against transition towards the ferromagnetic phase, their lifetimes are long enough for the skyrmions to be imprinted…

spinor condensateSUPERFLUID HE-3Angular momentumSYMMETRYFOS: Physical sciencesGeneral Physics and AstronomyBose-Einstein condensation114 Physical sciences01 natural sciencesInstability010305 fluids & plasmaslaw.inventionPHASESKNOTSlaw0103 physical sciencesField theory (psychology)magnetismikvanttifysiikka010306 general physicsVORTICESSpin-½Condensed Matter::Quantum GasesPhysicsBose–Einstein condensationBiaxial nematicCondensed matter physicsSkyrmionMONOPOLESCondensed Matter::Mesoscopic Systems and Quantum Hall EffectFIELD-THEORYSymmetry (physics)skyrmionQuantum Gases (cond-mat.quant-gas)Condensed Matter - Quantum GasesBose–Einstein condensateNew Journal of Physics
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Design Scheme of New Tetragonal Heusler Compounds for Spin-Transfer Torque Applications and its Experimental Realization

2012

Band Jahn-Teller type structural instabilities of cubic Mn(2)YZ Heusler compounds causing tetragonal distortions can be predicted by ab initio band-structure calculations. This allows for identification of new Heusler materials with tunable magnetic and structural properties that can satisfy the demands for spintronic applications, such as in spin-transfer torque-based devices.

spintronics010302 applied physicsMaterials scienceCondensed matter physicsSpintronicsMechanical EngineeringAb initioSpin-transfer torqueNanotechnology02 engineering and technology021001 nanoscience & nanotechnology01 natural sciencesCommunicationsspin-transfer torquesCondensed Matter::Materials ScienceTetragonal crystal systemMechanics of Materials0103 physical sciencesTorqueCondensed Matter::Strongly Correlated ElectronsGeneral Materials Sciencemagnetic properties0210 nano-technologyHeusler compoundsRealization (systems)Advanced Materials
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Spin caloric transport from density-functional theory

2019

Spin caloric transport refers to the coupling of heat with spin transport. Its applications primarily concern the generation of spin currents and control of magnetisation by temperature gradients for information technology, known by the synonym spin caloritronics. Within the framework of ab initio theory, new tools are being developed to provide an additional understanding of these phenomena in realistic materials, accounting for the complexity of the electronic structure without adjustable parameters. Here, we review this progress, summarising the principles of the density-functional-based approaches in the field and presenting a number of application highlights. Our discussion includes th…

spintronicsMaterials scienceAcoustics and UltrasonicsSpintronicsCondensed matter physicsthermal spin torqueCaloric theory02 engineering and technologyPhysik (inkl. Astronomie)021001 nanoscience & nanotechnologyCondensed Matter Physics01 natural sciencesspin Nernst effectSurfaces Coatings and FilmsElectronic Optical and Magnetic Materialsspin Seebeck effectdensity functional calculations0103 physical sciencesspin caloritronicsDensity functional theoryCondensed Matter::Strongly Correlated Electronsmagneto-Seebeck effect010306 general physics0210 nano-technologySpin-½
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Pseudospectrum of Reissner-Nordström black holes: Quasinormal mode instability and universality

2021

Black hole spectroscopy is a powerful tool to probe the Kerr nature of astrophysical compact objects and their environment. The observation of multiple ringdown modes in gravitational waveforms could soon lead to high-precision gravitational spectroscopy, so it is critical to understand if the quasinormal mode spectrum is stable against perturbations. It was recently shown that the pseudospectrum can shed light on the spectral stability of black hole quasinormal modes. We study the pseudospectrum of Reissner-Nordstr\"om spacetimes and we find a spectral instability of scalar and gravitoelectric quasinormal modes in subextremal and extremal black holes, extending similar findings for the Sch…

star: compactspace-time: Schwarzschildblack hole: Reissner-NordstroemScalar (mathematics)[PHYS.MPHY]Physics [physics]/Mathematical Physics [math-ph]01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationGeneral Relativity and Quantum Cosmology0103 physical sciencesQuasinormal mode010306 general physicsperturbation: gravitationMathematical PhysicsMathematical physicsPseudospectrumPhysicsSpacetime010308 nuclear & particles physicsHorizonquasinormal modegravitational radiationblack hole: stabilityMathematics::Spectral Theorystabilityblack hole: quasinormal modequasinormal mode: spectrumBlack holeperturbation: scalarwave: model[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Schwarzschild radius
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The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST)

2007

(abridged:) The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST) surveys the most populated ~5 square degrees of the Taurus star formation region, using the XMM-Newton X-ray observatory to study the thermal structure, variability, and long-term evolution of hot plasma, to investigate the magnetic dynamo, and to search for new potential members of the association. Many targets are also studied in the optical, and high-resolution X-ray grating spectroscopy has been obtained for selected bright sources. The X-ray spectra have been coherently analyzed with two different thermal models (2-component thermal model, and a continuous emission measure distribution model). We present ov…

stars : pre-main sequence010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaBrown dwarfFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesLuminosity[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Observatory0103 physical sciencesProtostarAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsstars : formationStar formationMolecular cloudAstrophysics (astro-ph)Astronomy and AstrophysicsAccretion (astrophysics)Starsgravitational waves13. Climate actionSpace and Planetary ScienceX-rays : star
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Spectral properties of X-ray bright variable sources in the Taurus Molecular Cloud

2006

We analyze 19 bright variable X-ray sources detected in the XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST), in order to characterize the variations with time of their coronal properties and to derive informations on the X-ray emitting structures. We performed time-resolved spectroscopy of the EPIC PN and MOS spectra of the XEST sources, using a model with one or two thermal components, and we used the time evolution of the temperatures and emission measures during the decay phase of flares to derive the size of the flaring loops. The light curves of the selected sources show different types of variability: flares, long-lasting decay or rise through the whole observation, sl…

stars : pre-main sequence010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaX-rays : starsFOS: Physical sciencesFluxAstrophysicsAstrophysics01 natural sciences7. Clean energySpectral linelaw.inventionlaw0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsSpectroscopy010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsMolecular cloudAstrophysics (astro-ph)Astronomy and Astrophysicsstars : late-typeRadiusPlasmaLight curve13. Climate actionSpace and Planetary Sciencestars : coronaeFlare
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Stochastic gravito-inertial modes discovered by CoRoT in the hot Be star HD 51452

2012

International audience; Context. Be stars are rapidly rotating stars with a circumstellar decretion disk. They usually undergo pressure and/or gravity pulsation modes excited by the κ-mechanism, i.e. an effect of the opacity of iron-peak elements in the envelope of the star. In the Milky Way, p-modes are observed in stars that are hotter than or equal to the B3 spectral type, while g-modes are observed at the B2 spectral type and cooler. Aims. We observed a B0IVe star, HD 51452, with the high-precision, high-cadence photometric CoRoT satellite and high-resolution, ground-based HARPS and SOPHIE spectrographs to study its pulsations in great detail. We also used the lower resolution spectra a…

starsBe -stars010504 meteorology & atmospheric sciencesBe starK-type main-sequence staroscillations -starsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsrotation01 natural sciences0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsStellar structureindividual010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciences[PHYS]Physics [physics]PhysicsASTROFÍSICA ESTELARStellar rotationFlare starAstronomyAstronomy and AstrophysicsLight curveESPECTROSCOPIAHD 51452 -starsStarsT Tauri star13. Climate actionSpace and Planetary ScienceAstrophysics::Earth and Planetary Astrophysicsemission-line[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astronomy & Astrophysics
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