Search results for "Quantum"

showing 10 items of 9714 documents

Intersystem crossing in Fe(II) coordination compounds

1994

Fe(II) spin-crossover systems can be quantitatively converted from the low-spin (LS) to the high-spin (HS) state well below the thermal transition temperature by irradiating either into the metal-ligand charge transfer or d-d absorption bands, and even in low-spin systems a transient population of the HS state can be achieved. This fact can be made use of to determine HS → LS relaxation rate constants for a wide variety of Fe(II) spin-crossover and low-spin systems. The HS → LS relaxation shows strong deviations from an Arrhenius behaviour, with nearly temperature-independent tunnelling below ∼70 K and a thermally activated process above ∼100 K. The range of more than 12 orders of magnitude…

Arrhenius equationNuclear and High Energy Physicseducation.field_of_studyChemistryPopulationCondensed Matter PhysicsInternal conversion (chemistry)PhotochemistryMolecular physicsAtomic and Molecular Physics and OpticsVibronic couplingsymbols.namesakeIntersystem crossingReaction rate constantsymbolsRelaxation (physics)Physical and Theoretical ChemistryeducationQuantum tunnellingHyperfine Interactions
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A theoreticalab initiostudy on the H2NO + O3reaction

2003

The deviation of the NH2 pseudo-first-order decay Arrhenius plots of the NH2 + O3 reaction at high ozone pressures measured by experimentalists, has been attributed to the regeneration of NH2 radicals due to the subsequent reactions of the products of this reaction with ozone. Although these products have not yet been characterized experimentally, the radical H2NO has been postulated, because it can regenerate NH2 radicals through the reactions: H2NO + O3 NH2 + O2 and H2NO + O3 HNO + OH + O2. With the purpose of providing a reasonable explanation from a theoretical point of view to the kinetic observed behaviour of the NH2 + O3 system, we have carried ab initio electronic structure calculat…

Arrhenius equationReaction mechanismChemistryRadicalAb initioGeneral ChemistryElectronic structureKinetic energyComputational Mathematicssymbols.namesakeAb initio quantum chemistry methodsComputational chemistryAtmospheric chemistrysymbolsJournal of Computational Chemistry
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A Contradiction between Pulsed and Steady-State Studies in the Recombination Kinetics of Close Frenkel Defects in KBr and KCl Crystals

1994

Theoretical study of the kinetics of the correlated annealing of pairs of close (geminate) F-H centers in KCl and KBr crystals controlled by their diffusion and elastic attraction shows that the multi-step (kink) decay in defect concentrations observed more than once in thermostimulated experiments takes place only for very close F-H center pairs which are no further than fourth nearest neighbors. On the other hand, it is demonstrated (both theoretically and experimentally) that such F-H center pairs should be destroyed by the tunneling recombination already at time ≤10 -4 s, i.e. much before beginning of the thermostimulated experiments. Possible explanations of this contradiction are sugg…

Arrhenius equationTunnel effectsymbols.namesakeMaterials scienceAnnealing (metallurgy)ExcitonKineticssymbolsGeneral Physics and AstronomyAtomic physicsCrystallographic defectQuantum tunnellingRecombinationJournal of the Physical Society of Japan
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MBE growth and properties of low-density InAs/GaAs quantum dot structures.

2011

We present the results of a comprehensive study carried out on morphological, structural and optical properties of InAs/GaAs quantum dot structures grown by Molecular Beam Epitaxy. InAs quantum dots were deposited at low growth rate and high growth temperature and were capped with InGaAs upper confining layers. Owing to these particular design and growth parameters, quantum dot densities are in the order of 4-5x109 cm-2 with emission wavelengths ranging from 1.20 to 1.33 µm at 10 K, features that make these structures interesting for single-photon operation at telecom wavelength. High resolution structural techniques show that In content and composition profiles in the structures depend on …

Arrhenius equationeducation.field_of_studystructural and optical characterizationPhotoluminescenceMaterials scienceCondensed matter physicslow-dimensional semiconductor systemsCondensed Matter::OtherPopulationmolecular-beam epitaxyGeneral ChemistryCondensed Matter PhysicsEpitaxyCondensed Matter::Mesoscopic Systems and Quantum Hall Effectlow-dimensional semiconductor systems molecular-beam epitaxy structural and optical characterizationsymbols.namesakeCondensed Matter::Materials ScienceQuantum dotQuantum dot lasersymbolsGeneral Materials ScienceeducationMolecular beam epitaxyWetting layer
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Statistical modeling, simulation, and experimental verification of wideband indoor mobile radio channel

2018

This paper focuses on the modeling, simulation, and experimental verification of wideband single-input single-output (SISO) mobile fading channels for indoor propagation environments. The indoor reference channel model is derived from a geometrical rectangle scattering model, which consists of an infinite number of scatterers. It is assumed that the scatterers are exponentially distributed over the two-dimensional (2D) horizontal plane of a rectangular room. Analytical expressions are derived for the probability density function (PDF) of the angle of arrival (AOA), the PDF of the propagation path length, the power delay profile (PDP), and the frequency correlation function (FCF). An efficie…

Article SubjectComputer Networks and CommunicationsComputer sciencelcsh:T020206 networking & telecommunications020302 automobile design & engineeringStatistical model02 engineering and technologyCorrelation function (quantum field theory)lcsh:Technologylcsh:Telecommunication0203 mechanical engineeringAngle of arrivallcsh:TK5101-67200202 electrical engineering electronic engineering information engineeringElectronic engineeringFadingElectrical and Electronic EngineeringWidebandPower delay profileInformation SystemsCommunication channelComputer Science::Information Theory
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A neural network-based approach to determine FDTD eigenfunctions in quantum devices

2009

This article combines a Neural Network (NN) algorithm with the Finite Difference Time Domain (FDTD) technique to estimate the eigenfunctions in quantum devices. A NN based on the Least Mean Squares (LMS) algorithm is combined with the FDTD technique to provide a first approach to the confined states in quantum wires. The proposed technique is in good agreement with analytical results and is more efficient than FDTD combined with the Fourier Transform. This technique is used to cal- culate a numerical approximation to the eigenfunctions associated to quan- tum wire potentials. The performance and convergence of the proposed technique are also presented in this article. © 2009 Wiley Periodica…

Artificial neural networkComputer scienceFinite-difference time-domain methodEigenfunctionCondensed Matter PhysicsAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsLeast mean squares filtersymbols.namesakeFourier transformConvergence (routing)symbolsElectronic engineeringApplied mathematicsElectrical and Electronic EngineeringQuantumMicrowaveMicrowave and Optical Technology Letters
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Minidisk dynamics in accreting, spinning black hole binaries: Simulations in full general relativity

2021

We perform magnetohydrodynamic simulations of accreting, equal-mass binary black holes in full general relativity focusing on the impact of black hole spin on the dynamical formation and evolution of minidisks. We find that during the late inspiral the sizes of minidisks are primarily determined by the interplay between the tidal field and the effective innermost stable orbit around each black hole. Our calculations support that a minidisk forms when the Hill sphere around each black hole is significantly larger than the black hole's effective innermost stable orbit. As the binary inspirals, the radius of the Hill sphere decreases, and minidisk sconsequently shrink in size. As a result, ele…

Astrofísica010504 meteorology & atmospheric sciencesGeneral relativityastro-ph.GAgr-qcAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyLuminosityGravitationGeneral Relativity and Quantum CosmologyBinary black hole0103 physical sciences010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Accretion (meteorology)Astronomy and AstrophysicsMass ratioAstrophysics - Astrophysics of Galaxies3. Good healthBlack holeSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Hill sphereAstronomiaAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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Astrophysics with the Laser Interferometer Space Antenna

2023

Full list of authors: Amaro-Seoane, Pau; Andrews, Jeff; Sedda, Manuel Arca; Askar, Abbas.; Baghi, Quentin; Balasov, Razvan; Bartos, Imre; Bavera, Simone S.; Bellovary, Jillian; Berry, Christopher P. L.; Berti, Emanuele; Bianchi, Stefano; Blecha, Laura; Blondin, Stephane; Bogdanovic, Tamara; Boissier, Samuel; Bonetti, Matteo; Bonoli, Silvia; Bortolas, Elisa; Breivik, Katelyn; Capelo, Pedro R.; Caramete, Laurentiu; Cattorini, Federico; Charisi, Maria; Chaty, Sylvain; Chen, Xian; Chruslinska, Martyna; Chua, Alvin J. K.; Church, Ross; Colpi, Monica; D'Orazio, Daniel; Danielski, Camilla; Davies, Melvyn B.; Dayal, Pratika; De Rosa, Alessandra; Derdzinski, Andrea; Destounis, Kyriakos; Dotti, Massi…

AstrofísicaACTIVE GALACTIC NUCLEICosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)Black holeAstronomyStellar remnantFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)TIDAL DISRUPTION EVENTSGeneral Relativity and Quantum CosmologyGravitational wavesMOCCA-SURVEY DATABASESettore FIS/05 - Astronomia e AstrofisicaStellar remnantsSoftware ScienceMulti-messengerGRAVITATIONAL-WAVE SOURCESInstrumentation and Methods for Astrophysics (astro-ph.IM)Extreme mass ratio in-spiralsSolar and Stellar Astrophysics (astro-ph.SR)High Energy Astrophysical Phenomena (astro-ph.HE)Black holes; Extreme mass ratio in-spirals; Gravitational waves; Multi-messenger; Stellar remnantsBlack holesData ScienceAstrophysics::Instrumentation and Methods for AstrophysicsExtreme mass ratio in-spiralAM-CVN STARSAstrophysics - Astrophysics of GalaxiesWHITE-DWARF BINARIESDOUBLE NEUTRON-STARSAstrophysics - Solar and Stellar Astrophysics[SDU]Sciences of the Universe [physics]Astrophysics of Galaxies (astro-ph.GA)AstronomiaMASSIVE BLACK-HOLEAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsX-RAY BINARIESCOMMON-ENVELOPE EVOLUTIONGravitational waveAstrophysics - Cosmology and Nongalactic Astrophysics
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Relativistic simulations of black hole-neutron star coalescence: the jet emerges

2014

We perform magnetohydrodynamic simulations in full general relativity (GRMHD) of a binary black hole-neutron star on a quasicircular orbit that undergoes merger. The binary mass ratio is 3:1, the black hole initial spin parameter $a/m=0.75$ ($m$ is the black hole Christodoulou mass) aligned with the orbital angular momentum, and the neutron star is an irrotational $\Gamma=2$ polytrope. About two orbits prior to merger (at time $t=t_B$), we seed the neutron star with a dynamically weak interior dipole magnetic field that extends into the stellar exterior. At $t=t_B$ the exterior has a low-density atmosphere with constant plasma parameter $\beta\equiv P_{\rm gas}/P_{\rm mag}$. Varying $\beta$…

AstrofísicaAngular momentumGeneral relativityAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmology0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsMass ratioPolytropeBlack holeNeutron starSpace and Planetary ScienceAstronomiaAstrophysics::Earth and Planetary AstrophysicsGamma-ray burstAstrophysics - High Energy Astrophysical Phenomena
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Dark coupling and gauge invariance

2010

We study a coupled dark energy–dark matter model in which the energymomentum exchange is proportional to the Hubble expansion rate. The inclusion of its perturbation is required by gauge invariance. We derive the linear perturbation equations for the gauge invariant energy density contrast and velocity of the coupled fluids, and we determine the initial conditions. The latter turn out to be adiabatic for dark energy, when assuming adiabatic initial conditions for all the standard fluids. We perform a full Monte Carlo Markov Chain likelihood analysis of the model, using WMAP 7-year data.

AstrofísicaAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)Monte Carlo methodFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesCosmologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesCosmological perturbation theoryGauge theoryAdiabatic process010303 astronomy & astrophysicsPhysics010308 nuclear & particles physicsFísicaAstronomy and AstrophysicsMarkov chain Monte CarloHigh Energy Physics - PhenomenologyQuantum electrodynamicssymbolsDark energyHubble's lawAstrophysics - Cosmology and Nongalactic Astrophysics
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