Search results for "QUANTUM MECHANICS"

showing 10 items of 2468 documents

Analytic evaluation of the dipole Hessian matrix in coupled-cluster theory

2013

The general theory required for the calculation of analytic third energy derivatives at the coupled-cluster level of theory is presented and connected to preceding special formulations for hyperpolarizabilities and polarizability gradients. Based on our theory, we have implemented a scheme for calculating the dipole Hessian matrix in a fully analytical manner within the coupled-cluster singles and doubles approximation. The dipole Hessian matrix is the second geometrical derivative of the dipole moment and thus a third derivative of the energy. It plays a crucial role in IR spectroscopy when taking into account anharmonic effects and is also essential for computing vibrational corrections t…

Hessian matrixChemistryAnharmonicityGeneral Physics and AstronomyVDP::Mathematics and natural science: 400::Chemistry: 440::Theoretical chemistry quantum chemistry: 444Third derivativeMoment (mathematics)symbols.namesakeDipoleCoupled clusterClassical mechanicsPolarizabilityQuantum mechanicssymbolsNumerical differentiationPhysical and Theoretical ChemistryVDP::Matematikk og Naturvitenskap: 400::Kjemi: 440::Teoretisk kjemi kvantekjemi: 444
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A variational method for spectral functions

2016

The Generalized Eigenvalue Problem (GEVP) has been used extensively in the past in order to reliably extract energy levels from time-dependent Euclidean correlators calculated in Lattice QCD. We propose a formulation of the GEVP in frequency space. Our approach consists of applying the model-independent Backus-Gilbert method to a set of Euclidean two-point functions with common quantum numbers. A GEVP analysis in frequency space is then applied to a matrix of estimators that allows us, among other things, to obtain particular linear combinations of the initial set of operators that optimally overlap to different local regions in frequency. We apply this method to lattice data from NRQCD. Th…

High Energy Physics - LatticeVariational methodLattice (order)Quantum mechanicsHigh Energy Physics - Lattice (hep-lat)Euclidean geometryLattice field theoryFOS: Physical sciencesEstimatorApplied mathematicsLattice QCDLinear combinationEigendecomposition of a matrixProceedings of 34th annual International Symposium on Lattice Field Theory — PoS(LATTICE2016)
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N=2 topological gauge theory, the Euler characteristic of moduli spaces, and the Casson invariant

1991

We discuss gauge theory with a topological N=2 symmetry. This theory captures the de Rham complex and Riemannian geometry of some underlying moduli space $\cal M$ and the partition function equals the Euler number of $\cal M$. We explicitly deal with moduli spaces of instantons and of flat connections in two and three dimensions. To motivate our constructions we explain the relation between the Mathai-Quillen formalism and supersymmetric quantum mechanics and introduce a new kind of supersymmetric quantum mechanics based on the Gauss-Codazzi equations. We interpret the gauge theory actions from the Atiyah-Jeffrey point of view and relate them to supersymmetric quantum mechanics on spaces of…

High Energy Physics - Theory58Z05PhysicsInstantonFOS: Physical sciencesStatistical and Nonlinear PhysicsRiemannian geometry58D2958G26TopologyCasson invariant58D27Matrix modelModuli spaceHigh Energy Physics::Theorysymbols.namesakeHigh Energy Physics - Theory (hep-th)81Q60Euler characteristic57R20symbolsSupersymmetric quantum mechanicsGauge theoryMathematical PhysicsCommunications in Mathematical Physics
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EINSTEIN–PLANCK FORMULA, EQUIVALENCE PRINCIPLE, AND BLACK HOLE RADIANCE

2005

The presence of gravity implies corrections to the Einstein-Planck formula $E=h \nu$. This gives hope that the divergent blueshift in frequency, associated to the presence of a black hole horizon, could be smoothed out for the energy. Using simple arguments based on Einstein's equivalence principle we show that this is only possible if a black hole emits, in first approximation, not just a single particle, but thermal radiation.

High Energy Physics - TheoryAstrofísicaPhysicsGravitacióAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsEquivalence principle (geometric)General Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyBlueshiftBlack holeGeneral Relativity and Quantum Cosmologysymbols.namesakeHigh Energy Physics - Theory (hep-th)Space and Planetary ScienceThermal radiationQuantum mechanicsHorizon (general relativity)symbolsRadianceCamps Teoria quàntica dePlanckEinsteinMathematical PhysicsInternational Journal of Modern Physics D
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Mixing-induced spontaneous supersymmetry breaking

2010

It is conjectured that flavor mixing furnishes a universal mechanism for the spontaneous breaking of supersymmetry. The conjecture is proved explicitly for the mixing of two Wess--Zumino $\mathcal{N}=1$ supermultiplets and arguments for its general validity are given. The mechanism relies on the fact that, despite mixing treats fermions and bosons symmetrically, both the fermionic and the bosonic zero point energies are shifted by a positive amount and this kind of shift does not respect supersymmetry.

High Energy Physics - TheoryCondensed Matter::Quantum GasesPhysicsHigh Energy Physics::LatticeSpontaneous symmetry breakingHigh Energy Physics::PhenomenologyFOS: Physical sciencesGeneral Physics and AstronomySupersymmetrySupersymmetry breakingHigh Energy Physics - PhenomenologyHigh Energy Physics::TheoryExplicit symmetry breakingTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Quantum mechanicsSymmetry breakingQuantum field theoryChiral symmetry breakingMixing (physics)Physics Letters A
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The 1-loop effective potential for the Standard Model in curved spacetime

2018

The renormalisation group improved Standard Model effective potential in an arbitrary curved spacetime is computed to one loop order in perturbation theory. The loop corrections are computed in the ultraviolet limit, which makes them independent of the choice of the vacuum state and allows the derivation of the complete set of $\beta$-functions. The potential depends on the spacetime curvature through the direct non-minimal Higgs-curvature coupling, curvature contributions to the loop diagrams, and through the curvature dependence of the renormalisation scale. Together, these lead to significant curvature dependence, which needs to be taken into account in cosmological applications, which i…

High Energy Physics - TheoryDe Sitter spaceVacuum stateUNIVERSEfield theories in higher dimensionskosmologia01 natural sciencesGeneral Relativity and Quantum CosmologyPhysics Particles & FieldsHigh Energy Physics - Phenomenology (hep-ph)INFLATIONRADIATIVE-CORRECTIONSGauge theoryELECTROWEAK VACUUMMathematical physicsPhysics02 Physical SciencesPhysicshep-thhiukkasfysiikan standardimalliRENORMALIZATION-GROUP EQUATIONShep-phSPONTANEOUS SYMMETRY-BREAKINGNuclear & Particles PhysicsHigh Energy Physics - PhenomenologyHIGGS MASSPhysical SciencesGAUGE-THEORIESMathematics::Differential GeometryNuclear and High Energy Physicsgr-qcFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Curvatureclassical theories of gravityGeneral Relativity and Quantum Cosmology0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivityfield theories in lower dimensions010306 general physics01 Mathematical SciencesInflation (cosmology)Science & TechnologySpacetimeSTABILITYta114010308 nuclear & particles physicsgravitaatioLoop (topology)High Energy Physics - Theory (hep-th)INTERACTING SCALAR FIELDlcsh:QC770-798Perturbation theory (quantum mechanics)Journal of High Energy Physics
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The damped harmonic oscillator in deformation quantization

2005

We propose a new approach to the quantization of the damped harmonic oscillator in the framework of deformation quantization. The quantization is performed in the Schr\"{o}dinger picture by a star-product induced by a modified "Poisson bracket". We determine the eigenstates in the damped regime and compute the transition probability between states of the undamped harmonic oscillator after the system was submitted to dissipation.

High Energy Physics - TheoryDeformation quantization[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]Canonical quantizationGeneral Physics and AstronomyFOS: Physical sciences01 natural sciences[ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th]Poisson bracket[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]Quantum mechanics0103 physical sciencesdissipative systems010306 general physicsNonlinear Sciences::Pattern Formation and Solitonsquantum mechanics.Harmonic oscillatorEigenvalues and eigenvectorsPhysicsQuantum Physics010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Quantization (signal processing)quantum mechanicsPACS numbers: 03.50.-z 03.50.De 11.10.-z 03.65.DbLandau quantization16. Peace & justiceSecond quantizationClassical mechanicsHigh Energy Physics - Theory (hep-th)Schrödinger pictureQuantum Physics (quant-ph)
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Hierarchies of geometric entanglement

2007

We introduce a class of generalized geometric measures of entanglement. For pure quantum states of $N$ elementary subsystems, they are defined as the distances from the sets of $K$-separable states ($K=2,...,N$). The entire set of generalized geometric measures provides a quantification and hierarchical ordering of the different bipartite and multipartite components of the global geometric entanglement, and allows to discriminate among the different contributions. The extended measures are applied to the study of entanglement in different classes of $N$-qubit pure states. These classes include $W$ and $GHZ$ states, and their symmetric superpositions; symmetric multi-magnon states; cluster s…

High Energy Physics - TheoryFOS: Physical sciencesMONOTONESQuantum entanglementSquashed entanglementMultipartite entanglementCombinatoricsSYSTEMSQuantum mechanicsMathematical PhysicsPhysicsQuantum PhysicsQUANTUM-MECHANICSCluster stateCURRENT SITUATIONQUANTUM-MECHANICS CURRENT SITUATION STATES SYSTEMS MONOTONESMathematical Physics (math-ph)Quantum PhysicsAtomic and Molecular Physics and OpticsCondensed Matter - Other Condensed MatterMultipartiteHigh Energy Physics - Theory (hep-th)STATESQubitBipartite graphW stateQuantum Physics (quant-ph)Other Condensed Matter (cond-mat.other)Physical Review A
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Strong monogamy of bipartite and genuine multipartite entanglement: The Gaussian case

2007

We demonstrate the existence of general constraints on distributed quantum correlations, which impose a trade-off on bipartite and multipartite entanglement at once. For all N-mode Gaussian states under permutation invariance, we establish exactly a monogamy inequality, stronger than the traditional one, that by recursion defines a proper measure of genuine N-partite entanglement. Strong monogamy holds as well for subsystems of arbitrary size, and the emerging multipartite entanglement measure is found to be scale invariant. We unveil its operational connection with the optimal fidelity of continuous variable teleportation networks.

High Energy Physics - TheoryINFORMATIONGaussianGeneral Physics and AstronomyFOS: Physical sciencesQuantum entanglementSquashed entanglementTeleportationMultipartite entanglementMeasure (mathematics)symbols.namesakeQuantum mechanicsCondensed Matter - Statistical MechanicsMathematical PhysicsMathematicsDiscrete mathematicsQuantum PhysicsStatistical Mechanics (cond-mat.stat-mech)Mathematical Physics (math-ph)Quantum PhysicsHigh Energy Physics - Theory (hep-th)symbolsBipartite graphCONTINUOUS-VARIABLE SYSTEMSW stateQuantum Physics (quant-ph)
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Hawking radiation of massive modes and undulations

2012

We compute the analogue Hawking radiation for modes which posses a small wave vector perpendicular to the horizon. For low frequencies, the resulting mass term induces a total reflection. This generates an extra mode mixing that occurs in the supersonic region, which cancels out the infrared divergence of the near horizon spectrum. As a result, the amplitude of the undulation (0-frequency wave with macroscopic amplitude) emitted in white hole flows now saturates at the linear level, unlike what was recently found in the massless case. In addition, we point out that the mass introduces a new type of undulation which is produced in black hole flows, and which is well described in the hydrodyn…

High Energy Physics - TheoryNuclear and High Energy PhysicsHAWKING RADIATIONWhite holeFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyMicro black holeGeneral Relativity and Quantum CosmologyQuantum mechanics0103 physical sciencesExtremal black holeWave vectormassive modes010306 general physicsPhysics010308 nuclear & particles physicsBlack holeInfrared divergenceHigh Energy Physics - Theory (hep-th)Quantum Gases (cond-mat.quant-gas)Quantum electrodynamicsReflection (physics)[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Condensed Matter - Quantum GasesHawking radiation
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