Search results for "Expectation."

showing 10 items of 191 documents

Spin-restricted open-shell coupled-cluster theory

1997

Spin-restricted CC theory is suggested as a new approach for the treatment of high-spin open-shell systems in CC theory. Spin constraints are imposed on the wave function in the sense that the projected spin eigenvalue equations are fulfilled within the (truncated) excitation space. These constraints allow a reduction in the number of independent amplitudes, thus decreasing the computational cost when implemented efficiently. The approach ensures that the spin expectation value always corresponds to the exact value, though the wave function is (for truncated CC treatments) not rigorously spin-adapted. For the specific case of high-spin doublets, detailed equations are derived for amplitudes…

PhysicsGeneral Physics and AstronomyFunction (mathematics)Expectation valueSpace (mathematics)Coupled clusterQuantum mechanicsCondensed Matter::Strongly Correlated ElectronsStatistical physicsPhysical and Theoretical ChemistryWave functionOpen shellEigenvalues and eigenvectorsSpin-½The Journal of Chemical Physics
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Eternal hilltop inflation

2016

We consider eternal inflation in hilltop-type inflation models, favored by current data, in which the scalar field in inflation rolls off of a local maximum of the potential. Unlike chaotic or plateau-type inflation models, in hilltop inflation the region of field space which supports eternal inflation is finite, and the expansion rate $H_{EI}$ during eternal inflation is almost exactly the same as the expansion rate $H_*$ during slow roll inflation. Therefore, in any given Hubble volume, there is a finite and calculable expectation value for the lifetime of the "eternal" inflation phase, during which quantum flucutations dominate over classical field evolution. We show that despite this, i…

PhysicsInflationCosmology and Nongalactic Astrophysics (astro-ph.CO)Slow rollSpacetime010308 nuclear & particles physicsmedia_common.quotation_subjectSpace timeKeynesian economicsFOS: Physical sciencesAstronomy and AstrophysicsExpectation valueAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyHubble volume0103 physical sciences010306 general physicsEternal inflationScalar fieldmedia_commonAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Electromagnetic sum rules for light nuclei

2008

Electromagnetic sum rules describe gross features of the electromagnetic structure of nuclei 1). A well known example is the Thomas-Reiche-Kuhn (TRK) sum rule, which relates the integrated total El-absorption cross section to the ground state expectation value of the double commutator of the dipole operator D with the nuclear Hamiltonian. While the k inet ic energy gives a model independent contr ibut ion, i . e . , the classical sum rule ~cl = 60 NZ/A MeV mb, the nuclear twobody potential gives an additional contr ibution in the presence of exchange and/or momentum dependent (or nonlocal) forces. In this case, I

PhysicsLight nucleusDipolesymbols.namesakeQuantum mechanicsRule of sumsymbolsSum rule in quantum mechanicsExpectation valueGround stateHamiltonian (quantum mechanics)Ion
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Goodness-of-fit tests in many dimensions

2004

A method is presented to construct goodness-of-fit statistics in many dimensions for which the distribution of all possible test results in the limit of an infinite number of data becomes Gaussian if also the number of dimensions becomes infinite. Furthermore, an explicit example is presented, for which this distribution as good as only depends on the expectation value and the variance of the statistic for any dimension larger than one.

PhysicsNuclear and High Energy PhysicsGaussianFOS: Physical sciencesProbability and statisticsVariance (accounting)Expectation valuesymbols.namesakeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Goodness of fitPhysics - Data Analysis Statistics and ProbabilitysymbolsLimit (mathematics)Statistical physicsDimension (data warehouse)InstrumentationData Analysis Statistics and Probability (physics.data-an)Statistic
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Simplicial Quantum Gravity on a Randomly Triangulated Sphere

1999

We study 2D quantum gravity on spherical topologies employing the Regge calculus approach with the dl/l measure. Instead of the normally used fixed non-regular triangulation we study random triangulations which are generated by the standard Voronoi-Delaunay procedure. For each system size we average the results over four different realizations of the random lattices. We compare both types of triangulations quantitatively and investigate how the difference in the expectation value of the squared curvature, $R^2$, for fixed and random triangulations depends on the lattice size and the surface area A. We try to measure the string susceptibility exponents through finite-size scaling analyses of…

PhysicsNuclear and High Energy PhysicsHigh Energy Physics - Lattice (hep-lat)FOS: Physical sciencesAstronomy and AstrophysicsRegge calculusExpectation valueMeasure (mathematics)String (physics)Atomic and Molecular Physics and OpticsScaling limitHigh Energy Physics - LatticeExponentQuantum gravityStatistical physicsScaling
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Measure dependence of 2D simplicial quantum gravity

1995

We study pure 2D Euclidean quantum gravity with $R^2$ interaction on spherical lattices, employing Regge's formulation. We attempt to measure the string susceptibility exponent $\gamma_{\rm str}$ by using a finite-size scaling Ansatz in the expectation value of $R^2$. To check on effects of the path integral measure we investigate two scale invariant measures, the "computer" measure $dl/l$ and the Misner measure $dl/\sqrt A$.

PhysicsNuclear and High Energy PhysicsHigh Energy Physics - Lattice (hep-lat)Measure (physics)FOS: Physical sciencesExpectation valueScale invarianceEuclidean quantum gravityString (physics)Atomic and Molecular Physics and OpticsGeneral Relativity and Quantum CosmologyHigh Energy Physics - LatticePath integral formulationQuantum gravityAnsatzMathematical physics
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Left-right symmetry and Neutrino Stability

1995

We consider a left-right symmetric model in which neutrinos acquire mass due to the spontaneous violation of both the gauged $B-L$ and a global $U(1)$ symmetry broken by the vacuum expectation value (VEV) of a gauge singlet scalar boson $\VEV{\sigma}$. For suitable choices of $\VEV{\sigma}$ consistent with all laboratory and astrophysical observations neutrinos will be unstable against majoron emission. All neutrino masses in the keV to MeV range are possible, since the expected neutrino decay lifetimes can be short enough to dilute their relic density below the cosmologically required level. A wide variety of possible new phenomena, associated to the presence of left-right symmetry and/or …

PhysicsNuclear and High Energy PhysicsParticle physicsHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaScalar bosonGlobal symmetrySymmetry (physics)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Higgs bosonHigh Energy Physics::ExperimentNeutrinoMajoronVacuum expectation valueBoson
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Phenomenology of supersymmetry with broken R-parity

1985

Abstract In some phenomenological supersymmetric models R -parity (+1 for particles, −1 for sparticles) is spontaneously broken along with tau-lepton number L τ by a vacuum expectation value υ τ of the tau sneutrino ν τ . To avoid excess stellar energy loss through majorons, there should also be explicit L τ violation through right-handed neutrinos. To have a sufficiently light ν τ , either υ τ is very small which is unnatural and boring, and/or the Higgs mixing parameter ϵ is very small. We find that in the limit ϵ → 0: -both the forward-backward asymmetry in e + e − → τ + τ − and the τ lifetime are unchanged, -Z 0 → ggν⊥ decays are possible where ν τ is an extra neutrino, -squarks and glu…

PhysicsNuclear and High Energy PhysicsParticle physicsHigh Energy Physics::PhenomenologySuperpartnerFísicaSupersymmetryNuclear physicsR-parityHiggs bosonHigh Energy Physics::ExperimentNeutrinoPhotinoVacuum expectation valueLeptonParticle Physics - Phenomenology
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Tau lepton mixing with charginos and its effects on chargino searches at e+e− colliders

1998

In bilinear R-Parity violating models where a term \epsilon_3L_3H_2 is introduced in the superpotential, the tau lepton can mix with charginos. We show that this mixing is fully compatible with LEP1 precision measurements of the Z\tau\tau and W\tau\nu_\tau couplings even for large values of \epsilon_3 and of the induced vacuum expectation value v_3 of the tau-sneutrino. The single production of charginos at e+e- colliders is possible in this case and we present numerical values of the cross-section at LEP1, LEP2 and an NLC. We find maximum values of 10 pb at LEP1 and 1 fb at NLC, while the corresponding values at LEP2 are too small to observe.

PhysicsNuclear and High Energy PhysicsParticle physicsHigh Energy Physics::PhenomenologySuperpotentialFOS: Physical sciencesFísicaHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)CharginoHigh Energy Physics::ExperimentProduction (computer science)Mixing (physics)LeptonVacuum expectation valuePhysics Letters B
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A Unified Approach to High Density: Pion Fluctuations in Skyrmion Matter

2003

As the first in a series of systematic work on dense hadronic matter, we study the properties of the pion in dense medium using Skyrme's effective Lagrangian as a unified theory of the hadronic interactions applicable in the large $N_c$ limit. Dense baryonic matter is described as the ground state of a skyrmion matter which appears in two differentiated phases as a function of matter density: i) at high densities as a stable cubic-centered (CC) half-skyrmion crystal; ii) at low densities as an unstable face-centered cubic (FCC) skyrmion crystal. We substitute the latter by a stable inhomogeneous phase of lumps of dense matter, which represents a naive Maxwell construction of the phase trans…

PhysicsNuclear and High Energy PhysicsPhase transitionParticle physicsField (physics)Nuclear TheorySkyrmionMaxwell constructionHigh Energy Physics::PhenomenologyNuclear TheoryFOS: Physical sciencesFísicaExpectation valueNuclear Theory (nucl-th)High Energy Physics - PhenomenologyPionHigh Energy Physics - Phenomenology (hep-ph)Ground stateUnified field theory
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