Search results for "Observable"

showing 10 items of 634 documents

Radiative muon capture on 12C and 16O

1979

Abstract We study exclusive radiative muon capture on 12 C(g.s.) leading to 12 B(g.s.), and on 16 O(g.s.) leading to 16 N(0 − , 120 keV). Our investigation, which is based on impulse approximation, puts special emphasis on elementary particle aspects of radiative capture, such as tests of magnitude and momentum transfer dependence of the induced pseudoscalar, and possible contributions of axial currents of second kind (weak electricity). We calculate several correlation observables which are sensitive to the nucleonic currents but depend very little on the structure of the nuclear initial and final states. In particular, it is shown that in capture on 12 C the polarization and alignment of …

Nuclear physicsPseudoscalarPhysicsNuclear and High Energy PhysicsParticle physicsPionNuclear TheoryMomentum transferRadiative transferPropagatorElementary particleObservableMuon captureNuclear Physics A
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Next-to-next-to-leading order corrections to three-jet observables in electron-positron annihilation.

2008

I report on a numerical program, which can be used to calculate any infrared safe three-jet observable in electron-positron annihilation to next-to-next-to-leading order in the strong coupling constant ${\ensuremath{\alpha}}_{s}$. The results are compared to a recent calculation by another group. Numerical differences in three color factors are discussed and explained.

Nuclear physicsQuantum chromodynamicsPhysicsRenormalizationParticle physicsColor modelAnnihilationElectron–positron annihilationGeneral Physics and AstronomyOrder (ring theory)ObservableJet (particle physics)Physical review letters
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The Astrophysicalr‐Process: A Comparison of Calculations following Adiabatic Expansion with Classical Calculations Based on Neutron Densities and Tem…

1999

The rapid neutron-capture process (r-process) encounters unstable nuclei far from β-stability. Therefore its observable features, like the abundances, witness (still uncertain) nuclear structure as well as the conditions in the appropriate astrophysical environment. With the remaining lack of a full understanding of its astrophysical origin, parameterized calculations are still needed. We consider two approaches: (1) the classical approach is based on (constant) neutron number densities nn and temperatures T over duration timescales τ; (2) recent investigations, motivated by the neutrino wind scenario from hot neutron stars after a supernova explosion, followed the expansion of matter with …

Nuclear reactionPhysicsNeutron starSupernovaSpace and Planetary ScienceNucleosynthesisr-processAstronomy and AstrophysicsNeutronObservableAstrophysicsNeutrinoThe Astrophysical Journal
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Sideward flow in Au + Au collisions at 400 A.MeV

1995

Abstract We present new experimental data obtained with the FOPI detector at SIS, for the Au + Au heavy-ion collisions at 400 A MeV incident energy. The sideward flow, determined from a method without reaction-plane reconstruction, and the nuclear stopping are studied as a function of the centrality of the collisions. In order to study the nuclear in-medium effects, which act on the NN cross sections and potential and hence on experimental observables like the nuclear-matter flow and stopping, these results are compared with the predictions of two different QMD versions. The first one offers a fully microscopic calculation of the cross sections and potential in the G-matrix formalism and na…

Nuclear reactionPhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsNuclear TheoryDetectorObservable01 natural sciences7. Clean energyNuclear physicsFormalism (philosophy of mathematics)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Incident energyNuclear Experiment010306 general physics
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Pathlength dependence of energy loss within in-medium showers

2010

Studying the pathlength dependence of high P_T hadron suppression in heavy-ion collisions by measuring the dependence of hard hadron production on the angle phi with the reaction plane in non-central collisions has so far been one of the most successful tools in constraining the microscopical picture of leading parton energy loss. With the imminent start of the LHC heavy-ion program and the possibility of full jet reconstruction, the focus has shifted to models which are capable of simulating full in-medium parton showers rather than tracing the leading parton only. Yet, on the level of single inclusive hadron observables, such shower models need to reproduce the findings of leading parton …

Nuclear reactionPhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron Colliderta114010308 nuclear & particles physicsPhysics::Instrumentation and DetectorsMonte Carlo methodHadronHigh Energy Physics::PhenomenologyFOS: Physical sciencesPartonObservableElementary particle01 natural sciencesNuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesProduction (computer science)High Energy Physics::Experiment010306 general physicsNuclear ExperimentPhysical Review C
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Jet quenching as a probe of the initial stages in heavy-ion collisions

2019

Jet quenching provides a very flexible variety of observables which are sensitive to different energy- and time-scales of the strongly interacting matter created in heavy-ion collisions. Exploiting this versatility would make jet quenching an excellent chronometer of the yoctosecond structure of the evolution process. Here we show, for the first time, that a combination of jet quenching observables is sensitive to the initial stages of heavy-ion collisions, when the approach to local thermal equilibrium is expected to happen. Specifically, we find that in order to reproduce at the same time the inclusive particle production suppression, $R_{AA}$, and the high-$p_T$ azimuthal asymmetries, $v…

PB-PB COLLISIONSNuclear and High Energy Physicsnucl-thNuclear TheoryFLOWInitial stagesFlow (psychology)PREDICTIONSFOS: Physical scienceshiukkasfysiikkanucl-ex114 Physical sciences01 natural sciencesENERGYNuclear Theory (nucl-th)Nuclear physicsHigh Energy Physics - Phenomenology (hep-ph)heavy-ionsTRANSVERSE-MOMENTUM DEPENDENCE0103 physical sciencesNuclear Physics - ExperimentROOT-S(NN)=2.76 TEVNuclear Experiment (nucl-ex)010306 general physicsJet quenchingNuclear ExperimentNuclear ExperimentParticle Physics - PhenomenologyHeavy-ionsPhysicsThermal equilibriumJet (fluid)ionit010308 nuclear & particles physicsElliptic flowLEAD COLLISIONShep-phObservablelcsh:QC1-999initial stagesJet quenchingjet quenchingHigh Energy Physics - PhenomenologyNuclear Physics - TheoryParticleHeavy ionlcsh:PhysicsPhysics Letters B
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Neutrino cosmology and Planck

2014

Relic neutrinos play an important role in the evolution of the Universe, modifying some of the cosmological observables. We summarize the main aspects of cosmological neutrinos and describe how the precision of present cosmological data can be used to learn about neutrino properties. In particular, we discuss how cosmology provides information on the absolute scale of neutrino masses, complementary to beta decay and neutrinoless double-beta decay experiments. We explain why the combination of Planck temperature data with measurements of the baryon acoustic oscillation angular scale provides a strong bound on the sum of neutrino masses, 0.23 eV at the 95% confidence level, while the lensing …

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)General Physics and AstronomyFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsCosmologydark matterHigh Energy Physics - Experimentsymbols.namesakeHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)PlanckAbsolute scaleParticle Physics - PhenomenologyPhysicsOscillationneutrino massesHigh Energy Physics::PhenomenologyFísicaObservablePlanck temperatureBaryonHigh Energy Physics - Phenomenology13. Climate action[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]symbolsHigh Energy Physics::ExperimentNeutrinocosmologyAstrophysics - Cosmology and Nongalactic Astrophysics
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How to relax the cosmological neutrino mass bound

2019

We study the impact of non-standard momentum distributions of cosmic neutrinos on the anisotropy spectrum of the cosmic microwave background and the matter power spectrum of the large scale structure. We show that the neutrino distribution has almost no unique observable imprint, as it is almost entirely degenerate with the effective number of neutrino flavours, $N_{\mathrm{eff}}$, and the neutrino mass, $m_{\nu}$. Performing a Markov chain Monte Carlo analysis with current cosmological data, we demonstrate that the neutrino mass bound heavily depends on the assumed momentum distribution of relic neutrinos. The message of this work is simple and has to our knowledge not been pointed out cle…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)cosmological neutrinosPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaCosmic microwave backgroundFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicscosmological parameters from LSS01 natural sciencesCosmologyMomentumsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)cosmological0103 physical sciencesPhysicsCOSMIC cancer database010308 nuclear & particles physicsMatter power spectrumHigh Energy Physics::Phenomenologycosmological parameters from CMBRAstronomy and AstrophysicsObservableMarkov chain Monte Carloneutrino masses from cosmologyHigh Energy Physics - Phenomenologyparameters from CMBRsymbolsHigh Energy Physics::ExperimentNeutrinoAstrophysics - Cosmology and Nongalactic Astrophysics
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Double Polarization Observables in Pentaquark Photoproduction

2019

We investigate the properties of the hidden charm pentaquark-like resonances first observed by LHCb in 2015, by measuring the polarization transfer KLL between the incident photon and the outgoing proton in the exclusive photoproduction of J/psi near threshold. We present a first estimate of the sensitivity of this observable to the pentaquark photocouplings and hadronic branching ratios, and extend our predictions to the case of initial state helicity correlation ALL, using a polarized target. These results serve as a benchmark for the SBS experiment at Jefferson Lab, which proposes to measure for the first time the helicity correlations ALL and KLL in J/psi exclusive photoproduction, in o…

Particle physicsFísica-Modelos matemáticosPhotonHadronpentaquarksFOS: Physical sciences01 natural sciencesexotic hadronsHigh Energy Physics - ExperimentPolarized targetHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesPhoton polarizationNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear ExperimentPhysicsexotic hadrons; pentaquarks; hadron spectroscopy010308 nuclear & particles physicshadron spectroscopyObservablePolarization (waves)HelicityPentaquarkHigh Energy Physics - PhenomenologyHigh Energy Physics::Experiment
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Flavour Les Houches Accord: Interfacing Flavour related Codes

2010

14 páginas, 2 tablas.-- arXiv:1008.0762v2.-- Mahmpudi, F. et al.

Particle physicsHigh Energy Physics::LatticeFlavourGeneral Physics and AstronomyFOS: Physical sciences01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsParticle Physics - PhenomenologyPhysics010308 nuclear & particles physics[PHYS.HLAT]Physics [physics]/High Energy Physics - Lattice [hep-lat]High Energy Physics - Lattice (hep-lat)High Energy Physics::PhenomenologyObservableSupersymmetryLes Houches AccordHigh Energy Physics - PhenomenologyStandard Model (mathematical formulation)Hardware and ArchitectureInterfacing[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::ExperimentFlavour physicsComput.Phys.Commun.
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