Search results for "Expansion"

showing 10 items of 630 documents

Comparative analysis of muon-capture and 0νββ -decay matrix elements

2020

Average matrix elements of ordinary muon capture (OMC) to the intermediate nuclei of neutrinoless double beta ($0\ensuremath{\nu}\ensuremath{\beta}\ensuremath{\beta}$) decays of current experimental interest are computed and compared with the corresponding energy and multipole decompositions of $0\ensuremath{\nu}\ensuremath{\beta}\ensuremath{\beta}$-decay nuclear matrix elements (NMEs). The present OMC computations are performed using the Morita-Fujii formalism by extending the original formalism beyond the leading order. The $0\ensuremath{\nu}\ensuremath{\beta}\ensuremath{\beta}$ NMEs include the appropriate short-range correlations, nuclear form factors, and higher-order nucleonic weak cu…

PhysicsFormalism (philosophy of mathematics)Particle physics010308 nuclear & particles physics0103 physical sciencesQuasiparticle010306 general physicsMultipole expansionWave function01 natural sciencesMuon capturePhysical Review C
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Entropy signature of the running cosmological constant

2007

Renormalization group (RG) improved cosmologies based upon a RG trajectory of Quantum Einstein Gravity (QEG) with realistic parameter values are investigated using a system of cosmological evolution equations which allows for an unrestricted energy exchange between the vacuum and the matter sector. It is demonstrated that the scale dependence of the gravitational parameters, the cosmological constant in particular, leads to an entropy production in the matter system. The picture emerges that the Universe started out from a state of vanishing entropy, and that the radiation entropy observed today is essentially due to the coarse graining (RG flow) in the quantum gravity sector which is relat…

PhysicsHigh Energy Physics - TheoryInitial singularityEntropy productionAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsCosmological constantGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsGeneral Relativity and Quantum CosmologyMetric expansion of spaceGravitationGeneral Relativity and Quantum CosmologyVacuum energyHigh Energy Physics - Theory (hep-th)Quantum gravityEntropy (arrow of time)Mathematical physics
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Distribution of electric multipole strengths in58Ni

1983

Inelastic electron scattering of 124 and 180 MeV electrons from58Ni has been measured for momentum transfers of 0.4 fm−1≤q≤1.2 fm−1 with an energy resolution of 110 keV. Using DWBA form factors with Tassie transition densities, we have extracted the electric multipole strength forL≤4 residing in 28 discrete states and in the inelastic continuum below 22.5 MeV of excitation.

PhysicsInelastic electron scatteringElectronAtomic physicsInelastic scatteringMultipole expansionExcitationIl Nuovo Cimento A
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Inflation, renormalization, and CMB anisotropies

2010

5 páginas.-- Trabajo presentado al Spanish Relativity Meeting (ERE 2009).-- El PDF es la versión pre-print (arXiv:1002.3914v1).

PhysicsInflation (cosmology)History010308 nuclear & particles physicsCosmic microwave backgroundScalar (mathematics)FOS: Physical sciencesObservableGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyComputer Science ApplicationsEducationMetric expansion of spaceRenormalizationRegularization (physics)0103 physical sciencesQuantum field theory010306 general physicsMathematical physics
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On the renormalization of ultraviolet divergences in the inflationary angular power spectrum

2015

We revise the role of ultraviolet divergences of cosmological observables and the corresponding renormalization from a space-time perspective. We employ the two-point function of primordial perturbations generated during inflation to derive an analytic expression for the multipole coefficients Cl in the Sachs-Wolfe regime. We analyzethe ultraviolet behaviorand stress the fact that the standard result in the literature is equivalent to a renormalization of the two-point function at zeroth adiabatic order. We also argue that renormalization at second adiabatic order seems to be more appropriate from a physical point of view. This may change significantly the predictions for Cl, while maintain…

PhysicsInflation (cosmology)HistoryObservableAstrophysics::Cosmology and Extragalactic AstrophysicsFunction (mathematics)Scale invarianceComputer Science ApplicationsEducationRenormalizationZeroth law of thermodynamicsQuantum electrodynamicsMultipole expansionAdiabatic processJournal of Physics: Conference Series
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Resummation of anisotropic quartic oscillator. Crossover from anisotropic to isotropic large-order behavior

1996

We present an approximative calculation of the ground-state energy for the anisotropic anharmonic oscillator Using an instanton solution of the isotropic action $\delta = 0$, we obtain the imaginary part of the ground-state energy for small negative $g$ as a series expansion in the anisotropy parameter $\delta$. From this, the large-order behavior of the $g$-expansions accompanying each power of $\delta$ are obtained by means of a dispersion relation in $g$. These $g$-expansions are summed by a Borel transformation, yielding an approximation to the ground-state energy for the region near the isotropic limit. This approximation is found to be excellent in a rather wide region of $\delta$ aro…

PhysicsInstantonQuantum PhysicsIsotropyFOS: Physical sciencesAtomic and Molecular Physics and OpticsQuartic functionDispersion relationQuantum electrodynamicsLimit (mathematics)ResummationAnisotropySeries expansionQuantum Physics (quant-ph)
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On quantum effects near the liquid-vapor transition in helium

2001

The liquid-vapor transition in He-3 and He-4 is investigated by means of path-integral molecular dynamics and the quantum virial expansion. Both methods are applied to the critical isobar and the critical isochore. While previous path-integral simulations have mainly considered the lambda transition and superfluid regime in He-4, we focus on the vicinity of the critical point and obtain good agreement with experimental results for the molar volume and the internal energy down to subcritical temperatures. We find that an effective classical potential that properly describes the two-particle radial distribution function exhibits a strong temperature dependence near the critical temperature. T…

PhysicsInternal energyCondensed matter physicsStatistical Mechanics (cond-mat.stat-mech)Lambda transitionGeneral Physics and Astronomychemistry.chemical_elementFOS: Physical sciencesCondensed Matter - Soft Condensed MatterRadial distribution functionSuperfluidityMolecular dynamicschemistryCritical point (thermodynamics)Virial expansionSoft Condensed Matter (cond-mat.soft)Physical and Theoretical ChemistryCondensed Matter - Statistical MechanicsHelium
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Angular Energy Distribution of Collapsar-Jets

2008

Collapsars are fast-spinning, massive stars, whose core collapse liberates an energy, that can be channeled in the form of ultrarelativistic jets. These jets transport the energy from the collapsed core to large distances, where it is dissipated in the form of long-duration gamma-ray bursts. In this paper we study the dynamics of ultrarelativistic jets produced in collapsars. Also we extrapolate our results to infer the angular energy distribution of the produced outflows in the afterglow phase. Our main focus is to look for global energetical properties which can be imprinted by the different structure of different progenitor stars. Thus, we employ a number of pre-supernova, stellar models…

PhysicsJet (fluid)Shock (fluid dynamics)Astrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsRotational energyAfterglowCore (optical fiber)StarsLorentz factorsymbols.namesakeSpace and Planetary SciencesymbolsFree expansionAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Galaxy Astrophysics
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Electromagnetic Multipole Moments and Transitions

2007

In the preceding chapter we constructed and discussed the simplest possible nuclear wave functions. This construction was done at the mean-field level. No account was taken of configuration mixing caused by the nuclear residual interaction. These simple wave functions produce degeneracies in energy spectra. This is contrary to experimental data, so improved wave functions are called for.

PhysicsMagnetic momentSimple (abstract algebra)Quantum electrodynamicsMultipole expansionResidualWave functionEnergy (signal processing)Mixing (physics)Spectral line
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Effects of damage on the response of Euler-Bernoulli beams traversed by a moving mass

2003

The perturbation induced by damage in the dynamic response of Euler-Bernoulli beams traversed by a moving mass is investigated. The structure is discretized into segments of constant bending stiffness, connected together by elastic hinges representing damaged sections. The beam-moving mass interaction force is modelled in the most accurate way by taking into account the effective structural mass distribution and the convective acceleration terms, often omitted in similar studies. The analytical response is obtained through a series expansion of the unknown deflection in a basis of the beam eigenfunctions. The results of experimental tests, performed on a small-scale model of a prototype bri…

PhysicsMass distributionbusiness.industryHingeMechanicsStructural engineeringsymbols.namesakeBernoulli's principleBending stiffnessEuler's formulasymbolsStructural health monitoringbusinessSeries expansionBeam (structure)
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