Search results for "Particle physics"

showing 10 items of 6826 documents

Status of nuclear PDFs after the first LHC p–Pb run

2017

In this talk, I overview the recent progress on the global analysis of nuclear parton distribution functions (nuclear PDFs). After first introducing the contemporary fits, the analysis procedures are quickly recalled and the ambiguities in the use of experimental data outlined. Various nuclear-PDF parametrizations are compared and the main differences explained. The effects of nuclear PDFs in the LHC p-Pb hard-process observables are discussed and some future prospects sketched.

Nuclear and High Energy PhysicsParticle physicsNuclear TheoryNuclear TheoryFOS: Physical sciencesPartonhiukkasfysiikka01 natural sciences114 Physical scienceshigh-energy nuclear collisionsHigh Energy Physics - ExperimentNuclear physicsNuclear Theory (nucl-th)High Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNuclear ExperimentHigh-energy nuclear collisions nuclear parton distribution functionsNuclear theoryQuantum chromodynamicsPhysicsLarge Hadron Colliderta114010308 nuclear & particles physicsObservableHigh Energy Physics - Phenomenologynuclear parton distribution functionsDistribution functionParametrization
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Probing Novel Scalar and Tensor Interactions from (Ultra)Cold Neutrons to the LHC

2012

Scalar and tensor interactions were once competitors to the now well-established V-A structure of the Standard Model weak interactions. We revisit these interactions and survey constraints from low-energy probes (neutron, nuclear, and pion decays) as well as collider searches. Currently, the most stringent limit on scalar and tensor interactions arise from 0+ -> 0+ nuclear decays and the radiative pion decay pi -> e nu gamma, respectively. For the future, we find that upcoming neutron beta decay and LHC measurements will compete in setting the most stringent bounds. For neutron beta decay, we demonstrate the importance of lattice computations of the neutron-to-proton matrix elements t…

Nuclear and High Energy PhysicsParticle physicsNuclear TheoryNuclear TheoryLattice field theoryFOS: Physical sciences01 natural sciencesNuclear physicsNuclear Theory (nucl-th)PionHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Lattice0103 physical sciencesRadiative transferNeutronNuclear Experiment010306 general physicsCharged currentPhysicsLarge Hadron ColliderMissing energy010308 nuclear & particles physicsHigh Energy Physics - Lattice (hep-lat)Scalar (physics)High Energy Physics - PhenomenologyHigh Energy Physics::Experiment
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Rate Equation Network for Baryon Production in High Energy Nuclear Collisions

2003

We develop and solve a network of rate equations for the production of baryons and anti-baryons in high energy nuclear collisions. We include all members of the baryon octet and decuplet and allow for transformations among them. This network is solved during a relativistic 2+1 hydrodynamical expansion of the of the hot matter created in the collision. As an application we compare to the number of protons, lambdas, negative cascades, and omega baryons measured at mid-rapidity in central collisions of gold nuclei at 65 GeV per nucleon at the Relativistic Heavy Ion Collider (RHIC).

Nuclear and High Energy PhysicsParticle physicsNuclear TheoryOctetCritical phenomenaNuclear TheoryFOS: Physical sciences01 natural sciencesNuclear physicsNuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear ExperimentPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyRate equationOmega baryonBaryonHigh Energy Physics - PhenomenologyQuark–gluon plasmaNucleonRelativistic Heavy Ion Collider
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A road map to solar neutrino fluxes, neutrino oscillation parameters, and tests for new physics

2003

We analyze all available solar and related reactor neutrino experiments, as well as simulated future 7Be, p-p, pep, and ^8B solar neutrino experiments. We treat all solar neutrino fluxes as free parameters subject to the condition that the total luminosity represented by the neutrinos equals the observed solar luminosity (the `luminosity constraint'). Existing experiments show that the p-p solar neutrino flux is 1.02 +- 0.02 (1 sigma) times the flux predicted by the BP00 standard solar model; the 7Be neutrino flux is 0.93^{+0.25}_{-0.63} the predicted flux; and the ^8B flux is 1.01 +- 0.04 the predicted flux. The neutrino oscillation parameters are: Delta m^2 = 7.3^{+0.4}_{-0.6}\times 10^{-…

Nuclear and High Energy PhysicsParticle physicsNuclear TheoryPhysics beyond the Standard ModelSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaSolar luminosityFOS: Physical sciencesAstrophysics7. Clean energy01 natural sciencesLuminosityHigh Energy Physics - ExperimentNuclear Theory (nucl-th)High Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNuclear fusionAstrophysics::Solar and Stellar AstrophysicsNuclear Experiment (nucl-ex)010306 general physicsNeutrino oscillationNuclear ExperimentParticle Physics - PhenomenologyPhysicsStandard solar model010308 nuclear & particles physicsAstrophysics (astro-ph)FísicaHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentAstrophysics::Earth and Planetary AstrophysicsNeutrino
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Solar Neutrinos Before and After Neutrino 2004

2004

We compare, using a three neutrino analysis, the allowed neutrino oscillation parameters and solar neutrino fluxes determined by the experimental data available Before and After Neutrino 2004. New data available after Neutrino2004 include refined KamLAND and gallium measurements. We use six different approaches to analyzing the KamLAND data. We present detailed results using all the available neutrino and anti-neutrino data for Delta m^2_{12}, tan^2 theta_{12}, sin^2 theta_{13}, and sin^2 eta (sterile fraction). Using the same complete data sets, we also present Before and After determinations of all the solar neutrino fluxes, which are treated as free parameters, an upper limit to the lumi…

Nuclear and High Energy PhysicsParticle physicsNuclear TheoryPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energyLuminosityNuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNuclear Experiment (nucl-ex)010306 general physicsNeutrino oscillationNuclear ExperimentPhysicsStandard solar model010308 nuclear & particles physicsScatteringOscillationAstrophysics (astro-ph)High Energy Physics::PhenomenologyFísicaSigmaHigh Energy Physics - Phenomenology13. Climate actionHigh Energy Physics::ExperimentNeutrino
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Eta and Etaprime Photoproduction on the Nucleon with the Isobar Model EtaMAID2018

2019

The isobar model EtaMAID has been updated with new and high precision data for eta and etaprime photoproduction on protons and neutrons from MAMI, ELSA, GRAAL and CLAS. The background is described in a recently developed Regge-cut model, and for the resonance part the whole list of nucleon resonances has been investigated with 21 N* states contributing to eta photoproduction and 12 N* states contributing to etaprime photoproduction. A new approach is discussed to avoid double counting in the overlap region of Regge and resonances. A comparison is done among four newly updated partial waves analyses for observables and partial waves. Finally, the possibility of a narrow resonance near W=1900…

Nuclear and High Energy PhysicsParticle physicsNuclear TheoryQC1-999HadronNuclear TheoryFOS: Physical sciences01 natural sciencesNuclear physicsNuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNuclear fusionNeutronNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear ExperimentPhysics010308 nuclear & particles physicsPhysicsResonanceObservableHigh Energy Physics - PhenomenologyIsobarAngular dependenceHigh Energy Physics::ExperimentNucleon
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Robust signatures of solar neutrino oscillation solutions

2001

With the goal of identifying signatures that select specific neutrino oscillation parameters, we test the robustness of global oscillation solutions that fit all the available solar and reactor experimental data. We use three global analysis strategies previously applied by different authors and also determine the sensitivity of the oscillation solutions to the critical nuclear fusion cross section, S_{17}(0), for the production of 8B. The favored solutions are LMA, LOW, and VAC in order of g.o.f. The neutral current to charged current ratio for SNO is predicted to be 3.5 +- 0.6 (1 sigma), which is separated from the no-oscillation value of 1.0 by much more than the expected experimental er…

Nuclear and High Energy PhysicsParticle physicsNuclear TheorySolar neutrinoFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energyHigh Energy Physics - ExperimentStandard ModelNuclear Theory (nucl-th)High Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNuclear Experiment (nucl-ex)010306 general physicsNeutrino oscillationNuclear ExperimentBorexinoCharged currentParticle Physics - PhenomenologyPhysicsStandard solar model010308 nuclear & particles physicsOscillationAstrophysics (astro-ph)FísicaHigh Energy Physics - Phenomenology13. Climate actionHigh Energy Physics::ExperimentNeutrino
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Photon emission in neutral-current interactions at intermediate energies

2013

Neutral current photon emission reactions with nucleons and nuclei are studied. These processes are important backgrounds for nu_mu to nu_e (bar(nu)_mu to bar(nu)_e) appearance oscillation experiments where electromagnetic showers instigated by electrons (positrons) and photons are not distinguishable. At intermediate energies, these reactions are dominated by the weak excitation of the Delta(1232) resonance and its subsequent decay into Ngamma There are also non-resonant contributions that, close to threshold, are fully determined by the effective chiral Lagrangian of strong interactions. In addition, we have also included mechanisms mediated by nucleon excitations (N*) from the second res…

Nuclear and High Energy PhysicsParticle physicsNuclear TheoryStrong interactionNuclear TheoryFOS: Physical sciencesElectron01 natural sciencesResonance (particle physics)High Energy Physics - ExperimentNuclear Theory (nucl-th)symbols.namesakeHigh Energy Physics - Experiment (hep-ex)Pauli exclusion principleHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationNuclear ExperimentPhysicsNeutral current010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaHigh Energy Physics - Phenomenology13. Climate actionsymbolsHigh Energy Physics::ExperimentNeutrinoAtomic physicsNucleon
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Quark-model based study of the triton binding energy

2001

The three-nucleon bound state problem is studied employing a nucleon-nucleon potential obtained from a basic quark-quark interaction in a five-channel Faddeev calculation. The obtained triton binding energy is comparable to those predicted by conventional models of the $NN$ force.

Nuclear and High Energy PhysicsParticle physicsNuclear Theorycoupled channel [partial wave analysis]Nuclear TheoryBinding energyFOS: Physical scienceselastic scattering [nucleon nucleon]Few-body systemsinteraction [quark quark]Nuclear Theory (nucl-th)Nuclear physicsHigh Energy Physics - Phenomenology (hep-ph)Bound stateddc:530numerical calculationsNuclear ExperimentNuclear theoryPhysicsQuark modelbinding energy [tritium]Three-body problemHigh Energy Physics - Phenomenologynonrelativistic [quark]three-body problempotential [nucleon nucleon]Physical Review C
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Observation of charmonium pairs produced exclusively in $pp$ collisions

2014

A search is performed for the central exclusive production of pairs of charmonia produced in proton-proton collisions. Using data corresponding to an integrated luminosity of $3{\rm\ fb}^{-1}$ collected at centre-of-mass energies of 7 and 8 TeV, $J/\psi J/\psi$ and $J/\psi\psi(2S)$ pairs are observed, which have been produced in the absence of any other activity inside the LHCb acceptance that is sensitive to charged particles in the pseudorapidity ranges $(-3.5,-1.5)$ and $(1.5,5.0)$. Searches are also performed for pairs of P-wave charmonia and limits are set on their production. The cross-sections for these processes, where the dimeson system has a rapidity between 2.0 and 4.5, are measu…

Nuclear and High Energy PhysicsParticle physicsNuclear TheorydiffractionFOS: Physical sciencesLHCb - Abteilung HofmannHEAVY-ION COLLISIONSQCD diffraction charmoniaNOHigh Energy Physics - ExperimentLuminosityHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Quantum chromodynamiccharmonia; diffraction; QCDcharmonia; diffraction; QCD; Nuclear and High Energy PhysicsRapiditySDG 7 - Affordable and Clean EnergyNuclear ExperimentQCPhysics/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyhep-ex12.38.-tParticle physicsHadron-induced high- and super-high-energy interactions (energy > 10 GeV): Inclusive production with identified hadronHEAVY-ION COLLISIONS; 450 GEV/C; DIFFRACTION; LHCQCDCromodinàmica quànticaLHCbDifracció450 GEV/CPseudorapidityPhysics::Accelerator PhysicscharmoniaFísica nuclearHigh Energy Physics::ExperimentProduction (computer science)LHCHEAVYFísica de partículesExperiments13.85.NiDiffractionQuantum chromodynamicsParticle Physics - ExperimentJournal of Physics G: Nuclear and Particle Physics
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