Search results for "mass [rho(770)]"

showing 10 items of 416 documents

Paramagnetic-diamagnetic interplay in quantum dots for non-zero temperatures

2000

In the usual Fock-and Darwin-formalism with parabolic potential characterized by the confining energy $\eps_o := \hbar\omega_o= 3.37$ meV, but including explicitly also the Zeeman coupling between spin and magnetic field, we study the combined orbital and spin magnetic properties of quantum dots in a two-dimensional electron gas with parameters for GaAs, for N =1 and N >> 1 electrons on the dot. For N=1 the magnetization M(T,B) consists of a paramagnetic spin contribution and a diamagnetic orbital contribution, which dominate in a non-trivial way at low temperature and fields rsp. high temperature and fields. For N >> 1, where orbital and spin effects are intrinsically coupled in a subtle w…

PhysicsZeeman effectCondensed matter physicsCondensed Matter - Mesoscale and Nanoscale PhysicsDemagnetizing fieldFOS: Physical sciencesElectronCondensed Matter PhysicsCondensed Matter::Mesoscopic Systems and Quantum Hall EffectMagnetic fieldsymbols.namesakeMagnetizationParamagnetismEffective mass (solid-state physics)Mesoscale and Nanoscale Physics (cond-mat.mes-hall)symbolsDiamagnetismGeneral Materials Science
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SATELLITES AROUND MASSIVE GALAXIES SINCE z ∼ 2: CONFRONTING THE MILLENNIUM SIMULATION WITH OBSERVATIONS

2012

Minor merging has been postulated as the most likely evolutionary path to produce the increase in size and mass observed in the massive galaxies since z$\sim$2. In this Letter, we test directly this hypothesis comparing the population of satellites around massive galaxies in cosmological simulations versus the observations. We use state-of-the-art, publically available, Millennium I and II simulations and the associated semi-analytical galaxy catalogues to explore the time evolution of the fraction of massive galaxies that have satellites, the number of satellites per galaxy, the projected distance at which the satellite locate from the host galaxy, and the mass ratio between the host galax…

Physicseducation.field_of_studyCosmology and Nongalactic Astrophysics (astro-ph.CO)Epoch (astronomy)media_common.quotation_subjectDark matterPopulationFOS: Physical sciencesAstronomyAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsMass ratioUniverseCosmologyGalaxySpace and Planetary ScienceSatelliteeducationAstrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysicsmedia_commonThe Astrophysical Journal
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Finite amplitude method applied to giant dipole resonance in heavy rare-earth nuclei

2015

Background: The quasiparticle random phase approximation (QRPA), within the framework of the nuclear density functional theory (DFT), has been a standard tool to access the collective excitations of the atomic nuclei. Recently, finite amplitude method (FAM) has been developed, in order to perform the QRPA calculations efficiently without any truncation on the two-quasiparticle model space. Purpose: We discuss the nuclear giant dipole resonance (GDR) in heavy rare-earth isotopes, for which the conventional matrix diagonalization of the QRPA is numerically demanding. A role of the Thomas-Reiche-Kuhn (TRK) sum rule enhancement factor, connected to the isovector effective mass, is also investig…

Physicsgiant dipole resonanceIsovectorta114Nuclear Theory010308 nuclear & particles physicsNuclear TheoryFOS: Physical sciences01 natural sciences3. Good healthNuclear physicsNuclear Theory (nucl-th)DipoleEffective mass (solid-state physics)0103 physical sciencesAtomic nucleusQuasiparticleheavy nucleiSum rule in quantum mechanics010306 general physicsRandom phase approximationNuclear ExperimentNuclear densityrare-earth elements
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Reply to “Comment to ‘Dynamics of supercooled confined water measured by deep inelastic neutron scattering’ by Y. Finkelstein and R. Moreh”

2019

We reply to the comment [Front. Phys. 14(5), 53605 (2019)] by Y. Finkelstein and R. Moreh on our article Front. Phys. 13(1), 138205 (2018). We agree with some of their criticisms about our calculation of the temperature effect on the kinetic energy of hydrogen atoms of supercooled confined water; we also agree with their statement that, in view of the current sensitivity of the technique, possible effects of the liquid-liquid water transition are hardly detected with deep inelastic neutron scattering (DINS). However, we disagree with their use of the translational mass ratio of a single water molecule and, in general, with their underestimation of collective effects.

Physicsliquid-liquid transitionPhysics and Astronomy (miscellaneous)HydrogenSettore FIS/07Front (oceanography)chemistry.chemical_elementvibrational density of statesMass ratioproton kinetic energyKinetic energy01 natural sciencesInelastic neutron scatteringSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)chemistry0103 physical sciencesLibrationlibrationAtomic physics010306 general physicsSupercoolingConfined waterdeep inelastic neutron scatteringsupercooled water
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Crypthecodinium cohnii Growth and Omega Fatty Acid Production in Mediums Supplemented with Extract from Recycled Biomass

2022

Crypthecodinium cohnii is a marine heterotrophic dinoflagellate that can accumulate high amounts of omega-3 polyunsaturated fatty acids (PUFAs), and thus has the potential to replace conventional PUFAs production with eco-friendlier technology. So far, C. cohnii cultivation has been mainly carried out with the use of yeast extract (YE) as a nitrogen source. In the present study, alternative carbon and nitrogen sources were studied: the extraction ethanol (EE), remaining after lipid extraction, as a carbon source, and dinoflagellate extract (DE) from recycled algae biomass C. cohnii as a source of carbon, nitrogen, and vitamins. In mediums with glucose and DE, the highest specific biomass gr…

QH301-705.5omega-3 fatty acidPharmaceutical Sciencefood and beveragesCrypthecodinium cohnii<i>Crypthecodinium cohnii</i>Article<i>Crypthecodinium cohnii</i>; omega-3 fatty acid; biomass recycling; dinoflagellate extract; FTIR spectroscopybiomass recyclingFTIR spectroscopyDrug Discoverydinoflagellate extractBiology (General)Pharmacology Toxicology and Pharmaceutics (miscellaneous)Marine Drugs
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Gluon mass and freezing of the QCD coupling

2007

Infrared finite solutions for the gluon propagator of pure QCD are obtained from the gauge-invariant non-linear Schwinger-Dyson equation formulated in the Feynman gauge of the background field method. These solutions may be fitted using a massive propagator, with the special characteristic that the effective mass employed drops asymptotically as the inverse square of the momentum transfer, in agreement with general operator-product expansion arguments. Due to the presence of the dynamical gluon mass the strong effective charge extracted from these solutions freezes at a finite value, giving rise to an infrared fixed point for QCD.

Quantum chromodynamicsPhysicsHistoryParticle physicsBackground field methodInfrared fixed pointHigh Energy Physics::LatticeMomentum transferHigh Energy Physics::PhenomenologyFísicaPropagatorFOS: Physical sciencesComputer Science ApplicationsEducationGluonsymbols.namesakeHigh Energy Physics - PhenomenologyEffective mass (solid-state physics)High Energy Physics - Phenomenology (hep-ph)Quantum electrodynamicssymbolsFeynman diagram
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Quasi-one-dimensional quantum spin liquid in the $\rm {Cu(C_4H_4N_2)(NO_3)_2}$ insulator

2015

We analyze measurements of the magnetization, differential susceptibility and specific heat of quasi-one dimensional insulator Cu(C$_4$H$_4$N$_2$)(NO$_3$)$_2$ (CuPzN) subjected to magnetic fields. We show that the thermodynamic properties are defined by quantum spin liquid formed with spinons, with the magnetic field tuning the insulator CuPzN towards quantum critical point related to fermion condensation quantum phase transition (FCQPT) at which the spinon effective mass diverges kinematically. We show that the FCQPT concept permits to reveal and explain the scaling behavior of thermodynamic characteristics. For the first time, we construct the schematic $T-H$ (temperature---magnetic field…

Quantum phase transitionPhysicsCondensed Matter::Quantum GasesPhysics and Astronomy (miscellaneous)Condensed matter physicsStrongly Correlated Electrons (cond-mat.str-el)FOS: Physical sciences01 natural sciencesSpinon010305 fluids & plasmasMagnetic fieldCondensed Matter - Strongly Correlated ElectronsMagnetizationEffective mass (solid-state physics)Quantum critical point0103 physical sciencesCondensed Matter::Strongly Correlated ElectronsQuantum spin liquid010306 general physicsPhase diagram
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Magnetic breakdown and charge density wave formation: a quantum oscillation study of the rare-earth tritellurides

2020

The rare-earth tritellurides ($R$Te$_3$, where $R$ = La, Ce, Pr, Nd, Sm, Gd, Tb, Dy, Ho, Er, Tm, Y) form a charge density wave state consisting of a single unidirectional charge density wave for lighter $R$, with a second unidirectional charge density wave, perpendicular and in addition to the first, also present at low temperatures for heavier $R$. We present a quantum oscillation study in magnetic fields up to 65T that compares the single charge density wave state with the double charge density wave state both above and below the magnetic breakdown field of the second charge density wave. In the double charge density wave state it is observed that there remain several small, light pockets…

Quantum phase transitionPhysicsCondensed matter physicsStrongly Correlated Electrons (cond-mat.str-el)Rare earthQuantum oscillationsFOS: Physical sciencesModel systemFermi surface02 engineering and technologyMagnetic breakdown021001 nanoscience & nanotechnology01 natural sciencesCondensed Matter - Strongly Correlated ElectronsEffective mass (solid-state physics)0103 physical sciences010306 general physics0210 nano-technologyCharge density wave
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Magnetic-field-induced reentrance of Fermi-liquid behavior and spin-lattice relaxation rates in

2009

Abstract A strong departure from Landau–Fermi liquid (LFL) behavior have been recently revealed in observed anomalies in both the magnetic susceptibility χ and the muon and 63Cu nuclear spin-lattice relaxation rates 1 / T 1 of YbCu 5 − x Au x ( x = 0.6 ). We show that the above anomalies along with magnetic-field-induced reentrance of LFL properties are indeed determined by the dependence of the quasiparticle effective mass M ∗ on magnetic field B and temperature T and demonstrate that violations of the Korringa law also come from M ∗ ( B , T ) dependence. We obtain this dependence theoretically utilizing our approach based on fermion condensation quantum phase transition (FCQPT) notion. Ou…

Quantum phase transitionPhysicsMagnetoresistanceCondensed matter physicsSpin–lattice relaxationGeneral Physics and Astronomy01 natural sciencesMagnetic susceptibility010305 fluids & plasmasEffective mass (solid-state physics)0103 physical sciencesQuasiparticleStrongly correlated materialFermi liquid theory010306 general physicsPhysics Letters A
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Energy scales and magnetoresistance at a quantum critical point

2009

The magnetoresistance (MR) of CeCoIn_5 is notably different from that in many conventional metals. We show that a pronounced crossover from negative to positive MR at elevated temperatures and fixed magnetic fields is determined by the scaling behavior of quasiparticle effective mass. At a quantum critical point (QCP) this dependence generates kinks (crossover points from fast to slow growth) in thermodynamic characteristics (like specific heat, magnetization etc) at some temperatures when a strongly correlated electron system transits from the magnetic field induced Landau Fermi liquid (LFL) regime to the non-Fermi liquid (NFL) one taking place at rising temperatures. We show that the abov…

Quantum phase transitionPhysicsMagnetoresistanceCondensed matter physicsStrongly Correlated Electrons (cond-mat.str-el)General Physics and AstronomyFOS: Physical sciences01 natural sciences010305 fluids & plasmasMagnetizationCondensed Matter - Strongly Correlated ElectronsEffective mass (solid-state physics)Quantum critical point0103 physical sciencesQuasiparticleStrongly correlated materialCondensed Matter::Strongly Correlated Electrons010306 general physicsScaling
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