Search results for "QC"

showing 10 items of 3477 documents

Magnetic fields and chiral asymmetry in the early hot universe

2016

In this paper, we study analytically the process of external generation and subsequent free evolution of the lepton chiral asymmetry and helical magnetic fields in the early hot universe. This process is known to be affected by the Abelian anomaly of the electroweak gauge interactions. As a consequence, chiral asymmetry in the fermion distribution generates magnetic fields of non-zero helicity, and vice versa. We take into account the presence of thermal bath, which serves as a seed for the development of instability in magnetic field in the presence of externally generated lepton chiral asymmetry. The developed helical magnetic field and lepton chiral asymmetry support each other, consider…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectHigh Energy Physics::LatticeFOS: Physical sciencesElectronGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciences7. Clean energyAsymmetryGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010303 astronomy & astrophysicsmedia_commonPhysics010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsHelicityUniverseMagnetic fieldHigh Energy Physics - PhenomenologyQuantum electrodynamicsAnomaly (physics)Astrophysics - Cosmology and Nongalactic AstrophysicsLepton
researchProduct

Impact of cosmic inhomogeneities on SNe observations

2009

We study the impact of cosmic inhomogeneities on the interpretation of SNe observations. We build an inhomogeneous universe model that can confront supernova data and yet is reasonably well compatible with the Copernican Principle. Our model combines a relatively small local void, that gives apparent acceleration at low redshifts, with a meatball model that gives sizeable lensing (dimming) at high redshifts. Together these two elements, which focus on different effects of voids on the data, allow the model to mimic the concordance model.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectgr-qcCosmic background radiationFOS: Physical sciencesAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences114 Physical sciencesGeneral Relativity and Quantum CosmologyCosmologysymbols.namesakeObservational cosmology0103 physical sciences010306 general physicsmedia_commonPhysicsCOSMIC cancer database010308 nuclear & particles physicsCopernican principleRedshiftUniverseLocal Voidsymbolsastro-ph.COAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

In the realm of the Hubble tension—a review of solutions

2021

The $\Lambda$CDM model provides a good fit to a large span of cosmological data but harbors areas of phenomenology. With the improvement of the number and the accuracy of observations, discrepancies among key cosmological parameters of the model have emerged. The most statistically significant tension is the $4-6\sigma$ disagreement between predictions of the Hubble constant $H_0$ by early time probes with $\Lambda$CDM model, and a number of late time, model-independent determinations of $H_0$ from local measurements of distances and redshifts. The high precision and consistency of the data at both ends present strong challenges to the possible solution space and demand a hypothesis with en…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)satellite: PlanckPhysics and Astronomy (miscellaneous)gravitation: modelPhysics beyond the Standard ModelCosmic microwave backgroundFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicsbaryon: oscillation: acoustic01 natural sciencesGeneral Relativity and Quantum CosmologyCosmologysymbols.namesakeTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)cosmological model: parameter space0103 physical sciencesstructurePlanckinflationcosmic background radiation: power spectrum010306 general physicsdark energyneutrino: interactionPhysicssupernova: Type IHubble constant010308 nuclear & particles physicsnew physicsmagnetic field: primordialtensionredshiftAstrophysics - Astrophysics of GalaxiesRedshiftrecombinationHigh Energy Physics - Phenomenology13. Climate actionAstrophysics of Galaxies (astro-ph.GA)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]relativisticsymbolsDark energy[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Phenomenology (particle physics)statisticalAstrophysics - Cosmology and Nongalactic AstrophysicsHubble's law
researchProduct

Dynamical formation and stability of fermion-boson stars

2020

Gravitationally bound structures composed by fermions and scalar particles known as fermion-boson stars are regular and static configurations obtained by solving the coupled Einstein-Klein-Gordon-Euler (EKGE) system. In this work, we discuss one possible scenario through which these fermion-boson stars may form by solving numerically the EKGE system under the simplifying assumption of spherical symmetry. Our initial configurations assume an already existing neutron star surrounded by an accreting cloud of a massive and complex scalar field. The results of our simulations show that once part of the initial scalar field is expelled via gravitational cooling the system gradually oscillates aro…

Coupling constantPhysicsCondensed Matter::Quantum Gases010308 nuclear & particles physicsScalar (mathematics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationTheoretical physicsNeutron starStars0103 physical sciencesCircular symmetry010306 general physicsScalar fieldAstrophysics::Galaxy AstrophysicsBoson
researchProduct

Polarizability of the neutron

1990

Abstract A first measurement of quasi-free Compton scattering by the neutron bound in the deuteron has yielded a value for the polarizability of the neutron of αn=(11.7 −11.7+4.3)×10 −4fm 3. This means that a finite value for the polarizability has been obtained, though the result is still consistent with zero. The π0 decay constant Fπ 0γγ and the pion nucleon coupling constant gNNπ have opposite signs.

Coupling constantPhysicsNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryCompton scatteringlcsh:QC1-999Nuclear physicsPionDeuteriumPolarizabilityNeutronAstrophysics::Earth and Planetary AstrophysicsExponential decayAtomic physicsNuclear ExperimentNucleonlcsh:PhysicsPhysics Letters B
researchProduct

Mesonic enhancement of the weak axial charge and its effect on the half-lives and spectral shapes of first-forbidden J+↔J− decays

2018

The effects of the enhancement of the axial-charge matrix element γ5 were studied in medium heavy and heavy nuclei for first-forbidden J+↔J− decay transitions using the nuclear shell model. Noticeable dependence on the enhancement ϵMEC of the axial-charge matrix element, as well as on the value of the axial-vector coupling constant gA was found in the spectral shapes of $^{93}$Y, $^{95}$Sr, and $^{97}$Y. The importance of the spectrum of $^{138}$Cs in the determination of gA is discussed. Half-life analyses in the A≈95 and A≈135 regions were done, and consistent results gA≈0.90, 0.75, and 0.65, corresponding to the three enhancement scenarios ϵMEC=1.4, 1.7, and 2.0, were obtained. Connectio…

Coupling constantPhysicsNuclear and High Energy PhysicsSpectral shape analysista114010308 nuclear & particles physicsSpectrum (functional analysis)forbidden beta decaysNuclear shell modelCharge (physics)01 natural scienceslcsh:QC1-999nuclear medium effectsspectral shapemeson-exchange currents0103 physical sciencesweak interactionsMatrix elementAtomic physicsAnomaly (physics)ydinfysiikka010306 general physicslcsh:PhysicsPhysics Letters B
researchProduct

Unpolarized and polarized elementary kaon electroproduction cross sections measured at MAMI

2012

Present and future research into the electroproduction of kaons plays an im- portant role at Mainz Microtron MAMI. With the Kaos spectrometer employed for kaon detection in the multi-spectrometer facility, cross section measurements of the exclusive p(e;e 0 K + ); 0 reactions at low momentum transfers have been performed. Isobar and Regge-plus-resonance models were compared with the data. These measurements have clearly discriminated between e ective Lagrangian models for photo- and electroproduc- tion of strangeness. New experiments with polarized beam at low four-momentum transfer are addressing the imaginary part of the longitudinal-transverse response in this process, that can be separa…

Coupling constantPhysicsParticle physicsPhysicsQC1-999HadronNuclear TheoryStrangenessHelicityMomentumNuclear physicsIsobarHigh Energy Physics::ExperimentNuclear ExperimentMicrotronBeam (structure)EPJ Web of Conferences
researchProduct

Pentaquark decay width in QCD sum rules

2005

In a diquark-diquark-antiquark picture of the pentaquark we study the decay $\Theta \rightarrow K^{+} n$ within the framework of QCD sum rules. After evaluation of the relevant three-point function, we extract the coupling $g_{\Theta nK}$ which is directly related to the pentaquark width. Restricting the decay diagrams to those with color exchange between the meson-like and baryon-like clusters reduces the coupling constant by a factor of four. Whereas a small decay width might be possible for a positive parity pentaquark, it seems difficult to explain the measured width for a pentaquark with negative parity.

Coupling constantQuantum chromodynamicsPhysicsNuclear and High Energy PhysicsQCD sum rulesParticle physicsHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyHyperonFOS: Physical sciencesCoupling (probability)PentaquarkNuclear physicsHigh Energy Physics - PhenomenologyParticle decayColor modelHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics::ExperimentNuclear ExperimentPhysical Review D
researchProduct

Levels of 186Re populated in thermal neutron capture reaction

2015

Levels of 186 Re have been studied in the thermal neutron capture reaction with an enriched 185 Re target. Evaluation of spectrum measured with GAMS5 allowed to obtain energies and intensities of more than 500 γ -lines assigned to 186 Re. Most of the obtained transitions have been placed in the model-independent level scheme of the doubly odd 186 Re nucleus, taking into account the available data of earlier experiments as well as the results of recent 187 Re(p, d )186 Re reaction measurements. Structure of the 186 Re low-lying levels has been analysed in terms of the particle-plus-rotor coupling model.

CouplingNuclear physicsPhysicsPhysicsQC1-999Thermal neutron captureAtomic physicsEPJ Web of Conferences
researchProduct

Gamma(Z --> bb): A signature of hard mass terms for a heavy top

1988

Abstract We calculate analytically the weak radiative corrections to the weak neutral current gauge boson-bottom fermion vertex, keeping the mass mt of the internal fermion line for the relevant diagrams. We find, to order α, a hard mass-term dependence m t 2 M W 2 of the amplitude, for large mt values. Its origin comes from the unphysical charged Higgs coupling to fermions in the renormalizable gauge or, equivalently, from the longitudinal charged gauge boson couplings. The diagonal Z0 decay width to b-quarks decreases, due to these weak radiative corrections, by 0.6%–2.5% when the top mass mt varies from 45 to 200 GeV.

CouplingPhysicsNuclear and High Energy PhysicsGauge bosonParticle physicsNeutral currentHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyFísicaFermionlcsh:QC1-999Vertex (geometry)AmplitudeQuantum electrodynamicsRadiative transferHiggs bosonlcsh:Physics
researchProduct