Search results for "Lamb"

showing 10 items of 745 documents

33S hyperfine interactions in H2S and SO2 and revision of the sulfur nuclear magnetic shielding scale

2014

Using the Lamb-dip technique, the hyperfine structure in the rotational spectra of H2(33)S and (33)SO2 has been resolved and the corresponding parameters--that is, the sulfur quadrupole-coupling and spin-rotation tensors--were determined. The experimental parameters are in good agreement with results from high-level coupled-cluster calculations, provided that up to quadruple excitations are considered in the cluster operator, sufficiently large basis sets are used, and vibrational corrections are accounted for. The (33)S spin-rotation tensor for H2S has been used to establish a new sulfur nuclear magnetic shielding scale, combining the paramagnetic part of the shielding as obtained from the…

H2(33)S and (33)SO2ChemistryOperator (physics)General Physics and AstronomySpectral linehigh-level coupled-cluster calculationParamagnetismElectromagnetic shieldingCluster (physics)hyperfine structure in the rotational spectraDiamagnetismTensorPhysical and Theoretical ChemistryAtomic physics33S spin-rotation tensorHyperfine structurenew sulfur nuclear magnetic shielding scaleLamb-dip technique
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Evidence for the decays of and *

2019

Abstract We study the hadronic decays of to the final states and , using an annihilation data sample of 567 pb-1 taken at a center-of-mass energy of 4.6 GeV with the BESIII detector at the BEPCII collider. We find evidence for the decays and with statistical significance of and , respectively. Normalizing to the reference decays and , we obtain the ratios of the branching fractions and to be and , respectively. The upper limits at the 90% confidence level are set to be and . Using BESIII measurements of the branching fractions of the reference decays, we determine % (<0.68%) and % (<1.9%). Here, the first uncertainties are statistical and the second systematic. The obtained branching …

Hadronic decayPhysicsNuclear and High Energy Physics010308 nuclear & particles physicsBranching fractionHadronAstronomy and AstrophysicsLambda01 natural sciencesOmegaCombinatorics0103 physical sciences010306 general physicsInstrumentationChinese Physics C
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Measurements of absolute hadronic branching fractions of the Λc+ baryon

2016

Kolcu, Onur Buğra (Arel Author) --- Makale 69 yazarlıdır.

Hadronic decayPhysicsParticle physicsBESIII детектор010308 nuclear & particles physicsBranching fractionElectron–positron annihilationадроныHigh Energy Physics::PhenomenologyHadronGeneral Physics and AstronomyBranching (polymer chemistry)Lambda01 natural sciencesNOdecayBaryonNuclear physicsPhysics and Astronomy (all)0103 physical sciencesбарионыHigh Energy Physics::Experiment010306 general physicsRadioactive decay
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Astrophysical constraints on extended gravity models

2015

We investigate the propagation of gravitational waves in the context of fourth order gravity nonminimally coupled to a massive scalar field. Using the damping of the orbital period of coalescing stellar binary systems, we impose constraints on the free parameters of extended gravity models. In particular, we find that the variation of the orbital period is a function of three mass scales which depend on the free parameters of the model under consideration; we can constrain these mass scales from current observational data.

High Energy Physics - TheoryCosmology and Nongalactic Astrophysics (astro-ph.CO)Wave propagationFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Cosmological constantGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyTheory of relativityPulsarBinary starRELATIVITYphysics of the early universemodified gravityCOSMOLOGICAL CONSTANTANISOTROPYPhysicsGravitational waveAstronomy and AstrophysicsSUPERNOVAEPULSARgravitational waves / theoryLAMBDASupernovaStarsDERIVATIVE QUANTUM-GRAVITY; COSMOLOGICAL CONSTANT; LAGRANGIANS; RELATIVITY; SUPERNOVAE; ANISOTROPY; LAMBDA; PULSARClassical mechanicsHigh Energy Physics - Theory (hep-th)LAGRANGIANSDERIVATIVE QUANTUM-GRAVITYAstrophysics - Cosmology and Nongalactic Astrophysics
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Effective interactions in Ricci-Based Gravity below the non-metricity scale

2020

We show how minimally-coupled matter fields of arbitrary spin, when coupled to Ricci-Based Gravity theories, develop non-trivial effective interactions that can be treated perturbatively only below a characteristic high-energy scale $\Lambda_Q$. Our results generalize to arbitrary matter fields those recently obtained for spin 1/2 fields in \cite{Latorre:2017uve}. We then use this interactions to set bounds on the high-energy scale $\Lambda_Q$ that controls departures of Ricci-Based Gravity theories from General Relativity. Particularly, for Eddington-inspired Born-Infeld gravity we obtain the strong bound $ |\kappa|<3.5 \times 10^{-14} \text{ m}^5 \text{kg}^{-1}\text{s}^{-2} $.

High Energy Physics - TheoryGravity (chemistry)Physics and Astronomy (miscellaneous)General relativityFOS: Physical sciencesScale (descriptive set theory)lcsh:AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Lambda01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationHigh Energy Physics - Phenomenology (hep-ph)Born–Infeld model0103 physical scienceslcsh:QB460-466lcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsEngineering (miscellaneous)Spin-½Mathematical physicsPhysics010308 nuclear & particles physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)lcsh:QC770-798
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Differential Regularization of a Non-relativistic Anyon Model

1994

Differential regularization is applied to a field theory of a non-relativistic charged boson field $\phi$ with $\lambda (\phi {}^{*} \phi)^2$ self-interaction and coupling to a statistics-changing $U(1)$ Chern-Simons gauge field. Renormalized configuration-space amplitudes for all diagrams contributing to the $\phi {}^{*} \phi {}^{*} \phi \phi$ 4-point function, which is the only primitively divergent Green's function, are obtained up to 3-loop order. The renormalization group equations are explicitly checked, and the scheme dependence of the $\beta$-function is investigated. If the renormalization scheme is fixed to agree with a previous 1-loop calculation, the 2- and 3-loop contributions …

High Energy Physics - TheoryPhysicsFOS: Physical sciencesLie groupFísicaRenormalization groupSymmetry groupLambdaRenormalizationHigh Energy Physics - Theory (hep-th)Quantum mechanicsRegularization (physics)Gauge theoryBoson
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Dark energy cosmologies for codimension-two branes

2005

A six-dimensional universe with two branes in the "football-shaped" geometry leads to an almost realistic cosmology. We describe a family of exact solutions with time dependent characteristic size of internal space. After a short inflationary period the late cosmology is either of quintessence type or turns to a radiation dominated Friedmann universe where the cosmological constant appears as a free integration constant of the solution. The radiation dominated universe with relativistic fermions is analyzed in detail, including its dimensional reduction.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsBig RipFOS: Physical sciencesNon-standard cosmologyLambda-CDM modelCosmological constantAstrophysics::Cosmology and Extragalactic AstrophysicsMetric expansion of spaceTheoretical physicsGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)De Sitter universeQuantum cosmologyScale factor (cosmology)
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Gravitational waves in the presence of a cosmological constant

2011

We derive the effects of a non-zero cosmological constant $\Lambda$ on gravitational wave propagation in the linearized approximation of general relativity. In this approximation we consider the situation where the metric can be written as $g_{\mu\nu}= \eta_{\mu\nu}+ h_{\mu\nu}^\Lambda + h_{\mu\nu}^W$, $h_{\mu\nu}^{\Lambda,W}<< 1$, where $h_{\mu\nu}^{\Lambda}$ is the background perturbation and $h_{\mu\nu}^{W}$ is a modification interpretable as a gravitational wave. For $\Lambda \neq 0$ this linearization of Einstein equations is self-consistent only in certain coordinate systems. The cosmological Friedmann-Robertson-Walker coordinates do not belong to this class and the derived linearized…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsCosmologiaGravitational waveGeneral relativityPlane waveFísicaFOS: Physical sciencesCosmological constantGeneral Relativity and Quantum Cosmology (gr-qc)LambdaGeneral Relativity and Quantum CosmologyGravitational wavesCosmologySupernovaGeneral Relativity and Quantum CosmologyAmplitudeHigh Energy Physics - Theory (hep-th)Ones gravitacionalsQuantum mechanicsMinkowski space
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Limits on the parameters of the equation of state for interacting dark energy

2010

Under the assumption that cold dark matter and dark energy interact with each other through a small coupling term, $Q$, we constrain the parameter space of the equation of state $w$ of those dark energy fields whose variation of the field since last scattering do not exceed Planck's mass. We use three parameterizations of $w$ and two different expressions for $Q$. Our work extends previous ones.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsParticle physicsEquation of stateCosmology and Nongalactic Astrophysics (astro-ph.CO)Hot dark matterScalar field dark matterFOS: Physical sciencesLambda-CDM modelAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyThermodynamics of the universeHigh Energy Physics - Theory (hep-th)Quantum mechanicsQuantum electrodynamicsMixed dark matterWarm dark matterDark energyLight dark matterDark fluidAstrophysics - Cosmology and Nongalactic Astrophysics
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p−p, p−Λ, and Λ−Λ correlations studied via femtoscopy in pp reactions at √s = 7 TeV

2019

We report on the first femtoscopic measurement of baryon pairs, such as p−p, p−Λ, and Λ−Λ, measured by ALICE at the Large Hadron Collider (LHC) in proton-proton collisions at √s=7 TeV. This study demonstrates the feasibility of such measurements in pp collisions at ultrarelativistic energies. The femtoscopy method is employed to constrain the hyperon-nucleon and hyperon-hyperon interactions, which are still rather poorly understood. A new method to evaluate the influence of residual correlations induced by the decays of resonances and experimental impurities is hereby presented. The p−p, p−Λ, and Λ−Λ correlation functions were fitted simultaneously with the help of a new tool developed spec…

High Energy Physics::Experimentproton-proton collisionslambda baryonshiukkasfysiikkaNuclear Experiment
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