Search results for "Spin-flip"

showing 10 items of 23 documents

Accretion disks around binary black holes of unequal mass: General relativistic MHD simulations of postdecoupling and merger

2014

We report results from simulations in general relativity of magnetized disks accreting onto merging black hole binaries, starting from relaxed disk initial data. The simulations feature an effective, rapid radiative cooling scheme as a limiting case of future treatments with radiative transfer. Here we evolve the systems after binary-disk decoupling through inspiral and merger, and analyze the dependence on the binary mass ratio with $q\ensuremath{\equiv}{m}_{\text{bh}}/{M}_{\mathrm{BH}}=1,1/2$, and $1/4$. We find that the luminosity associated with local cooling is larger than the luminosity associated with matter kinetic outflows, while the electromagnetic (Poynting) luminosity associated…

AstrofísicaPhysicsNuclear and High Energy PhysicsActive galactic nucleusX-ray bursterAstrophysics::High Energy Astrophysical PhenomenaAstronomyAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsMass ratioBlack holeBinary black holeIntermediate-mass black holeAstronomiaStellar black holeSpin-flipAstrophysics::Galaxy AstrophysicsPhysical Review D
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Black hole lightning due to particle acceleration at subhorizon scales

2015

Supermassive black holes with masses of millions to billions of solar masses are commonly found in the centers of galaxies. Astronomers seek to image jet formation using radio interferometry, but still suffer from insufficient angular resolution. An alternative method to resolve small structures is to measure the time variability of their emission. Here, we report on gamma-ray observations of the radio galaxy IC 310 obtained with the MAGIC telescopes revealing variability with doubling time scales faster than 4.8 min. Causality constrains the size of the emission region to be smaller than 20\% of the gravitational radius of its central black hole. We suggest that the emission is associated …

Black HolesRadio galaxyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsVery High Energy Gamma AstronomyBlack Holes Very High Energy Gamma Astronomy Active Galactic NucleiX-shaped radio galaxysupermassive black hole ; jet formation ; IC 310 ; MAGIC telescopesAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HESupermassive black holeta115MultidisciplinaryPhysicsActive Galactic NucleiAstronomy and AstrophysicsGalaxyIntermediate-mass black holeStellar black holeElectrónicaFísica nuclearddc:500Spin-flipElectricidadAstrophysics - High Energy Astrophysical PhenomenaSchwarzschild radius
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Orbital-selective Mott transitions in two-band Hubbard models

2006

The anisotropic two-orbital Hubbard model is investigated at low temperatures using high-precision quantum Monte Carlo (QMC) simulations within dynamical mean-field theory (DMFT). We demonstrate that two distinct orbital-selective Mott transitions (OSMTs) occur for a bandwidth ratio of 2 even without spin-flip contributions to the Hund exchange, and we quantify numerical errors in earlier QMC data which had obscured the second transition. The limit of small inter-orbital coupling is introduced via a new generalized Hamiltonian and studied using QMC and Potthoff's self-energy functional method, yielding insight into the nature of the OSMTs and the non-Fermi-liquid OSM phase and opening the p…

Condensed Matter::Quantum GasesPhysicsQuantum phase transitionStrongly Correlated Electrons (cond-mat.str-el)Condensed matter physicsHubbard modelQuantum Monte CarloMonte Carlo methodFOS: Physical sciencesCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsMott transitionCondensed Matter - Strongly Correlated Electronssymbols.namesakeSelf-energysymbolsCondensed Matter::Strongly Correlated ElectronsSpin-flipHamiltonian (quantum mechanics)Journal of Magnetism and Magnetic Materials
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Structure and Electronic Properties of an Expanded Terpyridine Complex of Nickel(II) [Ni(ddpd)2](BF4)2

2018

Ligand field theory010405 organic chemistrychemistry.chemical_element010402 general chemistry01 natural sciences0104 chemical sciencesInorganic ChemistryNickelchemistry.chemical_compoundCrystallographychemistrySpin-flipTerpyridineElectronic propertiesZeitschrift für anorganische und allgemeine Chemie
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A Vanadium(III) Complex with Blue and NIR-II Spin-Flip Luminescence in Solution.

2020

Luminescence from Earth-abundant metal ions in solution at room temperature is a very challenging objective due to the intrinsically weak ligand field splitting of first-row transition metal ions, which leads to efficient nonradiative deactivation via metal-centered states. Only a handful of 3d

Ligand field theoryChemistryMetal ions in aqueous solutionVanadiumchemistry.chemical_elementGeneral Chemistry010402 general chemistryPhotochemistry01 natural sciencesBiochemistryCatalysisTransition metal ions0104 chemical sciencesCondensed Matter::Materials ScienceColloid and Surface ChemistryPhysics::Plasma PhysicsSpin-flipLuminescenceJournal of the American Chemical Society
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Molecular Ruby under Pressure

2018

The intensely luminescent chromium(III) complexes [Cr(ddpd)2 ]3+ and [Cr(H2 tpda)2 ]3+ show surprising pressure-induced red shifts of up to -15 cm-1  kbar-1 for their sharp spin-flip emission bands (ddpd=N,N'-dimethyl-N,N'-dipyridine-2-yl-pyridine-2,6-diamine; H2 tpda=2,6-bis(2-pyridylamino)pyridine). These shifts surpass that of the established standard, ruby Al2 O3 :Cr3+ , by a factor of 20. Beyond the common application in the crystalline state, the very high quantum yield of [Cr(ddpd)2 ]3+ enables optical pressure sensing in aqueous and methanolic solution. These unique features of the molecular rubies [Cr(ddpd)2 ]3+ and [Cr(H2 tpda)2 ]3+ pave the way for highly sensitive optical pressu…

Materials scienceAqueous solution010405 organic chemistryAnalytical chemistryQuantum yieldchemistry.chemical_elementGeneral Chemistry010402 general chemistry01 natural sciencesCatalysis3. Good health0104 chemical sciencesChromiumchemistry.chemical_compoundchemistryExcited statePyridineMoleculeSpin-flipLuminescenceAngewandte Chemie International Edition
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Real-time observation of the intravalley spin-flip process in single-layer WS2

2019

We use helicity-resolved transient absorption spectroscopy to track intravalley scattering dynamics in monolayer WS2. We find that spin-polarized carriers scatter from upper to lower conduction band by reversing their spin orientation on a sub-ps timescale.

Materials scienceCondensed matter physicsScatteringPhysicsQC1-999MonolayerUltrafast laser spectroscopySettore FIS/01 - Fisica SperimentaleProcess (computing)ReversingSpin-flipSpectroscopySpin-½
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Equilibrating Glassy Systems with Parallel Tempering

2001

We discuss the efficiency of the so-called parallel tempering method to equilibrate glassy systems also at low temperatures. The main focus is on two structural glass models, SiO2 and a Lennard-Jones system, but we also investigate a fully connected 10 state Potts-glass. By calculating the mean squared displacement of a tagged particle and the spin-autocorrelation function, we find that for these three glass-formers the parallel tempering method is indeed able to generate, at low temperatures, new independent configurations at a rate which is O(100) times faster than more traditional algorithms, such as molecular dynamics and single spin flip Monte Carlo dynamics. In addition we find that t…

Mean squared displacementMolecular dynamicsMaterials scienceSpeedupFunction (mathematics)Statistical physicsParallel temperingSpin-flipFocus (optics)SupercoolingCondensed Matter::Disordered Systems and Neural Networks
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Spin-flip M1 giant resonance as a challenge for Skyrme forces

2010

Despite a great success of the Skyrme mean-field approach in exploration of nuclear dynamics, it seems to fail in description of the spin-flip M1 giant resonance. The results for different Skyrme parameterizations are contradictory and poorly agree with experiment. In particular, there is no parameterization which simultaneously describes the one-peak gross structure of M1 strength in doubly magic nuclei and two-peak structure in heavy deformed nuclei. The reason of this mismatch could lie in an unsatisfactory treatment of spin correlations and spin-orbit interaction. We discuss the present status of the problem and possible ways of its solution. In particular, we inspect i) the interplay o…

Nuclear Theory (nucl-th)PhysicsNuclear and High Energy PhysicsTheoretical physicsNuclear dynamicsIsovectorNuclear TheoryGiant resonanceNuclear TheoryFOS: Physical sciencesSpin-flip
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Diffusive thermal dynamics for the spin-S Ising ferromagnet

2008

We introduce an alternative thermal diffusive dynamics for the spin-S Ising ferromagnet realized by means of a random walker. The latter hops across the sites of the lattice and flips the relevant spins according to a probability depending on both the local magnetic arrangement and the temperature. The random walker, intended to model a diffusing excitation, interacts with the lattice so that it is biased towards those sites where it can achieve an energy gain. In order to adapt our algorithm to systems made up of arbitrary spins, some non trivial generalizations are implied. In particular, we will apply the new dynamics to two-dimensional spin-1/2 and spin-1 systems analyzing their relaxat…

PhysicsCondensed Matter - Materials ScienceStatistical Mechanics (cond-mat.stat-mech)Magnetic structureSpinsCritical phenomenaComplex systemMaterials Science (cond-mat.mtrl-sci)FOS: Physical sciencesRenormalization groupCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsRandom walker algorithmCondensed Matter::Strongly Correlated ElectronsIsing modelSpin-flipStatistical physicsCondensed Matter - Statistical MechanicsThe European Physical Journal B
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