Search results for "Expectation value"

showing 10 items of 39 documents

From primordial $^4$He abundance to the Higgs field

2008

We constrain the possible time variation of the Higgs vacuum expectation value ($v$) by recent results on the primordial $^4$He abundance ($Y_P$). For that, we improve the analytic models of the key-processes in our previous analytic calculation of the primordial $^4$He abundance. Furthermore, the latest results on the neutron decay, the baryon to photon ratio based on 5-year WMAP observations and a new dependence of the deuteron binding energy on $v$ are incorporated. Finally, we approximate the weak freeze-out, the cross section of photo-disintegration of the deuteron, the mean lifetime of the free neutron, the mass difference of neutron and proton, the Fermi coupling constant, the mass o…

PhysicsCoupling constantProtonAstrophysics (astro-ph)Nuclear TheoryFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysicsDelta-v (physics)Nuclear physicsBaryonHiggs fieldSpace and Planetary ScienceHiggs bosonNeutronNuclear ExperimentVacuum expectation value
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Renormalization group approach to chaotic strings

2012

Coupled map lattices of weakly coupled Chebychev maps, so-called chaotic strings, may have a profound physical meaning in terms of dynamical models of vacuum fluctuations in stochastically quantized field theories. Here we present analytic results for the invariant density of chaotic strings, as well as for the coupling parameter dependence of given observables of the chaotic string such as the vacuum expectation value. A highly nontrivial and selfsimilar parameter dependence is found, produced by perturbative and nonperturbative effects, for which we develop a mathematical description in terms of suitable scaling functions. Our analytic results are in good agreement with numerical simulati…

PhysicsField (physics)General MathematicsApplied MathematicsChaoticGeneral Physics and AstronomyFOS: Physical sciencesStatistical and Nonlinear PhysicsObservableRenormalization groupNonlinear Sciences - Chaotic DynamicsString (physics)Nonlinear Sciences::Chaotic DynamicsClassical mechanicsCoupling parameterStatistical physicsChaotic Dynamics (nlin.CD)Quantum fluctuationVacuum expectation value
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Spin-orbit couplings within the equation-of-motion coupled-cluster framework: Theory, implementation, and benchmark calculations.

2015

We present a formalism and an implementation for calculating spin-orbit couplings (SOCs) within the EOM-CCSD (equation-of-motion coupled-cluster with single and double substitutions) approach. The following variants of EOM-CCSD are considered: EOM-CCSD for excitation energies (EOM-EE-CCSD), EOM-CCSD with spin-flip (EOM-SF-CCSD), EOM-CCSD for ionization potentials (EOM-IP-CCSD) and electron attachment (EOM-EA-CCSD). We employ a perturbative approach in which the SOCs are computed as matrix elements of the respective part of the Breit-Pauli Hamiltonian using zeroth-order non-relativistic wave functions. We follow the expectation-value approach rather than the response-theory formulation for p…

PhysicsGeneral Physics and AstronomyEquations of motionExpectation valuesymbols.namesakeCoupled clusterMean field theoryQuantum mechanicssymbolsStatistical physicsPerturbation theory (quantum mechanics)Physical and Theoretical ChemistryWave functionHamiltonian (quantum mechanics)Basis setThe Journal of chemical physics
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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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