Search results for "dipole"

showing 10 items of 982 documents

The Ã 1Au state and the T2 potential surface of acetylene: Implications for triplet perturbations in the fluorescence spectra of the à state

1996

The cis–trans isomerization reaction on the T2 surface of acetylene and the lowest excited singlet state of acetylene, A 1Au, are investigated by ab initio electronic structure theory. We report optimized geometries, dipole moments, and harmonic vibrational frequencies of stationary points and adiabatic energy differences between them using basis sets as large as triple‐ζ plus double polarization with higher angular momentum functions, TZ(2df,2pd), and theoretical methods up to coupled‐cluster singles and doubles with a perturbative triples correction [CCSD(T)] and the equation‐of‐motion coupled‐cluster method (EOM‐CCSD). Our theoretical predictions should aid the interpretation of observat…

Angular momentumZeeman effectChemistryAb initioGeneral Physics and AstronomyElectronic structureQuantum chemistryPotential energyDipolesymbols.namesakechemistry.chemical_compoundAcetylenePhysics::Atomic and Molecular ClusterssymbolsPhysics::Chemical PhysicsPhysical and Theoretical ChemistryAtomic physicsThe Journal of Chemical Physics
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Entropy of transfer of n-nitroalkanes from n-octane to water at 25�C

1984

Entropy of transfer of nitromethane, nitroethane, 1-nitrobutane, 1-nitropentane, and 1-nitrohexane from n-octane to water at 25°C is calculated using an electrostatic model. The calculations indicate that the electrostatic transfer entropy depends primarily on the dipole moment and the size of the-C−NO2 group, showing a trend which is similar to that previously found for the transfer free energy of the same process.

Aqueous solutionNitromethaneBiophysicsThermodynamicsPhotochemistryBiochemistrychemistry.chemical_compoundDipoleEntropy (classical thermodynamics)chemistryNitroethaneTransfer entropyPhysical and Theoretical ChemistryAliphatic compoundMolecular BiologyOctaneJournal of Solution Chemistry
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Space charge and induced dipole relaxation in solid electrolytes

1996

The space charge relaxation and induced dipole relaxation in solid electrolytes is discussed. The di-electric responses of these relaxations gives a satisfactory fit to the universal conductivity behaviours in the frequency range from DC to infrared.

Arrhenius equationCondensed matter physicsChemistryInfraredGeneral ChemistryConductivityCondensed Matter PhysicsPolarization (waves)Space chargeDipolesymbols.namesakeElectrical resistivity and conductivityFast ion conductorsymbolsPhysical chemistryGeneral Materials Science
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Binary neutron star mergers: a jet engine for short gamma-ray bursts

2016

We perform magnetohydrodynamic simulations in full general relativity (GRMHD) of quasi-circular, equal-mass, binary neutron stars that undergo merger. The initial stars are irrotational, $n=1$ polytropes and are magnetized. We explore two types of magnetic-field geometries: one where each star is endowed with a dipole magnetic field extending from the interior into the exterior, as in a pulsar, and the other where the dipole field is initially confined to the interior. In both cases the adopted magnetic fields are initially dynamically unimportant. The merger outcome is a hypermassive neutron star that undergoes delayed collapse to a black hole (spin parameter $a/M_{\rm BH} \sim 0.74$) imme…

AstrofísicaAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyArticlePulsar0103 physical sciencesBinary starAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsBlack holeNeutron starStarsSpace and Planetary ScienceAstronomiaAstrophysics::Earth and Planetary AstrophysicsGamma-ray burstAstrophysics - High Energy Astrophysical PhenomenaMagnetic dipole
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Large-scale Cosmic-Ray Anisotropies above 4 EeV Measured by the Pierre Auger Observatory

2018

We present a detailed study of the large-scale anisotropies of cosmic rays with energies above 4 EeV measured using the Pierre Auger Observatory. For the energy bins [4,8] EeV and $E\geq 8$ EeV, the most significant signal is a dipolar modulation in right ascension at energies above 8 EeV, as previously reported. In this paper we further scrutinize the highest-energy bin by splitting it into three energy ranges. We find that the amplitude of the dipole increases with energy above 4 EeV. The growth can be fitted with a power law with index $\beta=0.79\pm 0.19$. The directions of the dipoles are consistent with an extragalactic origin of these anisotropies at all the energies considered. Addi…

Astronomymagnetic fieldAstrophysicsAstrophysics01 natural sciencesAmplitudeastroparticle physics; cosmic raysAnisotropy010303 astronomy & astrophysicscosmic rayastroparticle physics cosmic raysRight ascensionHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HECOSMIC cancer databaseORIGINOBSERVATÓRIOSPhysicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsastroparticle physicAugerastroparticle physics; cosmic rays; Astronomy and Astrophysics; Space and Planetary ScienceobservatorymodulationAmplitudeastroparticle physicsCosmic cancer databaseAstrophysics - High Energy Astrophysical Phenomenalarge scale anysotropysplittingAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayContext (language use)cosmic radiation: anisotropycosmic rays0103 physical sciencesHigh Energy Physicscosmic radiation: UHEPierre auger observatoryPierre Auger Observatoryextragalactic origin010308 nuclear & particles physicsFísicaAstronomy and AstrophysicsContext (language use)Astronomy and AstrophysicCosmic rayDipoleSpace and Planetary ScienceExperimental High Energy PhysicsAnisotropyDipoleObservatoryAstroparticle physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Right ascensionlarge scale anysotropy extragalactic origindipole
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Indications of non-conservative mass-transfer in AMXPs

2019

Context. Since the discovery of the first Accreting Millisecond X-ray Pulsar SAX J1808.4-3658 in 1998, the family of these sources kept growing on. Currently, it counts 22 members. All AMXPs are transients with usually very long quiescence periods, implying that mass accretion rate in these systems is quite low and not constant. Moreover, for at least three sources, a non-conservative evolution was also proposed. Aims. Our purpose is to study the long term averaged mass-accretion rates in all the Accreting Millisecond X-ray Pulsars discovered so far, to investigate a non-conservative mass-transfer scenario. Methods. We calculated the expected mass-transfer rate under the hypothesis of a con…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)X-rays: starsAstrophysicsCompact star01 natural sciencesLuminositystars: neutronX-rays: binariesPulsarpulsars: general0103 physical sciencesX-rays: individuals: IGR J17498−2921X-rays: individuals: IGR J17498-2921010303 astronomy & astrophysicsX-rays: individuals: XTE J1814−338PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Accretion (meteorology)010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsX-rays: binarieX-rays: individuals: XTE J1814-338Radiation pressureSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Magnetic dipole
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Oceanic and atmospheric linkages with short rainfall season intraseasonal statistics over Equatorial Eastern Africa and their predictive potential

2014

Despite earlier studies over various parts of the world including equatorial Eastern Africa (EEA) showing that intraseasonal statistics of wet and dry spells have spatially coherent signals and thus greater predictability potential, no attempts have been made to identify the predictors for these intraseasonal statistics. This study therefore attempts to identify the predictors (with a 1-month lead time) for some of the subregional intraseasonal statistics of wet and dry spells (SRISS) which showed the greatest predictability potential during the short rainfall season over EEA. Correlation analysis between the SRISS and seasonal rainfall totals on one hand and the predefined predictors on th…

Atmospheric ScienceMagnitude (mathematics)Seasonalitymedicine.diseaseSea surface temperatureBayesian multivariate linear regressionClimatologyStatisticsmedicineEnvironmental sciencePrecipitationIndian Ocean DipolePredictabilityPartial correlationInternational Journal of Climatology
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Modification of the southern African rainfall variability/ENSO relationship since the late 1960s

2000

Analysis of 149 raingauge series (1946–1988) shows a weak positive correlation between late summer rainfalls (January–March) in tropical southern Africa and the Southern Oscillation Index (SOI). The correlation coefficients have been unstable since World War II. They were close to zero before 1970 and significant thereafter. Before 1970, southern African late summer rainfalls were more specifically correlated with regional patterns of sea surface temperature (SST), mainly over the southwestern Indian Ocean. After 1970, teleconnections with near global SST anomaly patterns, i.e. over the central Pacific and Indian oceans, dominate the regional connections. The increase in the sensitivity of …

Atmospheric ScienceSea surface temperatureOceanographyRain gaugeSubtropical Indian Ocean DipoleEl NiñoAtmospheric circulationClimatologyExtratropical cycloneSubtropicsGeologyTeleconnectionClimate Dynamics
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Measurement of untruncated nuclear spin interactions via zero- to ultralow-field nuclear magnetic resonance

2015

Zero- to ultra-low-field nuclear magnetic resonance (ZULF NMR) provides a new regime for the measurement of nuclear spin-spin interactions free from effects of large magnetic fields, such as truncation of terms that do not commute with the Zeeman Hamiltonian. One such interaction, the magnetic dipole-dipole coupling, is a valuable source of spatial information in NMR, though many terms are unobservable in high-field NMR, and the coupling averages to zero under isotropic molecular tumbling. Under partial alignment, this information is retained in the form of so-called residual dipolar couplings. We report zero- to ultra-low-field NMR measurements of residual dipolar couplings in acetonitrile…

Atomic Physics (physics.atom-ph)Fluids & Plasmasphysics.chem-phFOS: Physical sciences010402 general chemistryJ-couplingphysics.atom-ph01 natural sciencesPhysics - Atomic Physicssymbols.namesakeEngineeringNuclear magnetic resonancequant-phPhysics - Chemical Physics0103 physical sciencesMagnetization transfer010306 general physicsChemical Physics (physics.chem-ph)PhysicsQuantum PhysicsZeeman effectCondensed matter physicsCondensed Matter Physics0104 chemical sciences3. Good healthElectronic Optical and Magnetic MaterialsMagnetic fieldSolid-state nuclear magnetic resonanceResidual dipolar couplingPhysical SciencesChemical SciencessymbolsQuantum Physics (quant-ph)Two-dimensional nuclear magnetic resonance spectroscopyMagnetic dipole–dipole interaction
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Optical Shielding of Destructive Chemical Reactions between Ultracold Ground-State NaRb Molecules

2020

Polar quantum gases represent promising platforms for studying many-body physics and strongly correlated systems with possible applications e.g. in quantum simulation or quantum computation. Due to their large permanent electric dipole moment polar molecules in electric field exhibit strong long-range anisotropic dipole-dipole interactions (DDIs). The creation and trapping of ultracold dipolar diatomic molecules of various species are feasible in many experimental groups nowadays. However long time trapping is still a challenge even in the case of the so called nonreactive molecules which are supposed to be immune against inelastic collisions in their absolute ground state [1] . Various hyp…

Atomic Physics (physics.atom-ph)Inelastic collisionGeneral Physics and AstronomyFOS: Physical sciencesQuantum simulator01 natural sciences7. Clean energyMolecular physicslaw.inventionPhysics - Atomic Physics[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]law0103 physical sciencesMoleculeSpontaneous emissionPhysics::Atomic Physics010306 general physicsComputingMilieux_MISCELLANEOUSPhysics[PHYS.PHYS.PHYS-ATOM-PH]Physics [physics]/Physics [physics]/Atomic Physics [physics.atom-ph]Rotational–vibrational spectroscopyLaserDiatomic moleculeDipoleElectric dipole momentQuantum Gases (cond-mat.quant-gas)Excited stateAtom optics[PHYS.PHYS.PHYS-CHEM-PH]Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]Atomic physicsCondensed Matter - Quantum GasesGround state
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