Search results for "Baryon"

showing 10 items of 759 documents

Cosmic microwave background constraints on secret interactions among sterile neutrinos

2017

Secret contact interactions among eV sterile neutrinos, mediated by a massive gauge boson $X$ (with $M_X \ll M_W$), and characterized by a gauge coupling $g_X$, have been proposed as a mean to reconcile cosmological observations and short-baseline laboratory anomalies. We constrain this scenario using the latest Planck data on Cosmic Microwave Background anisotropies, and measurements of baryon acoustic oscillations (BAO). We consistently include the effect of secret interactions on cosmological perturbations, namely the increased density and pressure fluctuations in the neutrino fluid, and still find a severe tension between the secret interaction framework and cosmology. In fact, taking i…

Sterile neutrinoParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)cosmological neutrinosDark matterCosmic microwave backgroundFOS: Physical sciencescosmological neutrinos; cosmological parameters from CMBR; neutrino masses from cosmology; neutrino properties; Astronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesNOsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesPlanck010303 astronomy & astrophysicsneutrino propertiesPhysicsGauge bosoncosmological neutrino010308 nuclear & particles physicsHigh Energy Physics::Phenomenologycosmological parameters from CMBRAstronomy and Astrophysicsneutrino masses from cosmologyCoupling (probability)3. Good healthHigh Energy Physics - Phenomenology13. Climate actionsymbolsHigh Energy Physics::ExperimentBaryon acoustic oscillationsNeutrinoAstrophysics - Cosmology and Nongalactic Astrophysics
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Revisiting cosmological bounds on sterile neutrinos

2014

We employ state-of-the art cosmological observables including supernova surveys and BAO information to provide constraints on the mass and mixing angle of a non-resonantly produced sterile neutrino species, showing that cosmology can effectively rule out sterile neutrinos which decay between BBN and the present day. The decoupling of an additional heavy neutrino species can modify the time dependence of the Universe's expansion between BBN and recombination and, in extreme cases, lead to an additional matter-dominated period; while this could naively lead to a younger Universe with a larger Hubble parameter, it could later be compensated by the extra radiation expected in the form of neutri…

Sterile neutrinoParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectCosmic microwave backgroundCosmic background radiationFOS: Physical sciencesNeutrino decouplingAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencessymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsmedia_commonPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaAstronomy and Astrophysicshep-phUniverseHigh Energy Physics - Phenomenology13. Climate actionsymbolsastro-ph.COHigh Energy Physics::ExperimentBaryon acoustic oscillationsNeutrinoHubble's lawAstrophysics - Cosmology and Nongalactic Astrophysics
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Measurement of the Cross Section for e+e−→Ξ−Ξ¯+ and Observation of an Excited Ξ Baryon

2020

Using a total of 11.0 fb−1 of e+e− collision data with center-of-mass energies between 4.009 and 4.6 GeV and collected with the BESIII detector at BEPCII, we measure fifteen exclusive cross sections and effective form factors for the process e+e−→Ξ−Ξ¯+ by means of a single baryon-tag method. After performing a fit to the dressed cross section of e+e−→Ξ−Ξ¯+, no significant ψ(4230) or ψ(4260) resonance is observed in the Ξ−Ξ¯+ final states, and upper limits at the 90% confidence level on ΓeeB for the processes ψ(4230)/ψ(4260)→Ξ−Ξ¯+ are determined. In addition, an excited Ξ baryon at 1820 MeV/c2 is observed with a statistical significance of 6.2–6.5σ by including the systematic uncertainty, an…

Systematic errorPhysicsParticle physicsForm factor (quantum field theory)General Physics and AstronomyState (functional analysis)01 natural sciencesResonance (particle physics)Measure (mathematics)BaryonCross section (physics)Excited state0103 physical sciences010306 general physicsPhysical Review Letters
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New results on the Roper resonance and the P_{11} partial wave

2008

Properties of the Roper resonance, the first scalar excitation of the nucleon, are determined. Pole positions and residues of the $P_{11}$ partial wave are studied in a combined analysis of pion- and photo-induced reactions. We find the Roper pole at $\{(1371\pm7)-i(92\pm10)\}$ MeV and an elasticity of $0.61\pm 0.03$. The largest decay coupling is found for the $N\sigma$ ($\sigma=(\pi\pi)$-$S$-wave). The analysis is based on new data on $\gamma p\to p\pi^0\pi^0$ for photons in the energy range from the two-pion threshold to 820 MeV from TAPS at Mainz and from 0.4 to 1.3 GeV from Crystal Barrel at Bonn and includes further data from other experiments. The partial wave analysis excludes the p…

TAPSNuclear and High Energy PhysicsRoper resonancePhotonProtonPHOTON SPECTROMETERPartial wave analysisNuclear TheoryDalitz plotFOS: Physical sciencesPION-PHOTOPRODUCTIONPROTONTHRESHOLDNuclear physicsPionHigh Energy Physics - Phenomenology (hep-ph)Nuclear ExperimentPhysicsPI(0) PHOTOPRODUCTIONHigh Energy Physics - PhenomenologyRELATIVISTIC QUARK-MODELSTRANGE-BARYON SPECTRUMPOSITIVE-STRANGENESSFORCESNucleonExcitation
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Meson–meson and meson–baryon interactions in a chiral non-perturbative approach

1998

A qualitative account of the meson-meson and meson-baryon interactions using chiral Lagrangians and the inverse amplitude method in coupled channels is done. The method, imposing exact unitarity, proves to be a very useful tool to extend the information contained in the chiral Lagrangians at energies beyond the realm of applicability of chiral perturbation theory. Oset Baguena, Eulogio, Eulogio.Oset@ific.uv.es

UNESCO::FÍSICA::Física molecular:FÍSICA [UNESCO]:FÍSICA::Física molecular [UNESCO]Meson-meson ; Meson-Baryon ; Chiral Lagrangian ; Exact unitarityHigh Energy Physics::LatticeNuclear TheoryHigh Energy Physics::PhenomenologyUNESCO::FÍSICAExact unitarityMeson-BaryonNuclear ExperimentChiral LagrangianMeson-meson
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A model for the γN → ππN reaction

1996

We have studied the γN → ππN reaction using a model wich includes N, Δ(1232), N*(1440) and N*(1520) intermediate baryonic states and the ρ-meson as a intermediate ππ resonance. The model reproduces fairly well experimental cross sections below Eγ=800 MeV and invariant-mass distributions even at higher energies. One of the interesting findings of study is what the γN → N*(1520) → Δπ process is very important and interferes strongly with the dominant Δ-Kroll-Ruderman term to produce the experimental peak of the kross section. Oset Baguena, Eulogio, Eulogio.Oset@ific.uv.es

UNESCO::FÍSICA::NucleónicaInvariant-mass distributions:FÍSICA [UNESCO]intermediate baryonic statesUNESCO::FÍSICA:FÍSICA::Nucleónica [UNESCO]γN → ππN
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The Voyage of Metals in the Universe from Cosmological to Planetary Scales: the need for a Very High-Resolution, High Throughput Soft X-ray Spectrome…

2019

Metals form an essential part of the Universe at all scales. Without metals we would not exist, and the Cosmos would look completely different. Metals are primarily born through nuclear processes in stars. They leave their cradles through winds or explosions, and then start their journey through space. This can lead them in and out of astronomical objects on all scales, ranging from comets, planets, stars, entire galaxies, groups and clusters of galaxies to the largest structures of the Universe. Their wanderings are fundamental in determining how these objects, and the entire universe, evolve. In addition, their bare presence can be used to trace what these structures look like. The scope …

Very high resolutionAstronomical ObjectsCosmology and Nongalactic Astrophysics (astro-ph.CO)010504 meteorology & atmospheric sciencesGalaxy-ISM-CGM-IGM feedbackFOS: Physical sciencesSpace (mathematics)Cycle of baryons and metals7. Clean energy01 natural sciencesCycle of baryons and metals; Galaxy-ISM-CGM-IGM feedback; High-resolution X-ray spectrometer; X-ray gratingsSettore FIS/05 - Astronomia E Astrofisica0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]X-ray gratingsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsThroughput (business)0105 earth and related environmental sciencesCycle of baryons and metalHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSoft x rayCOSMIC cancer databaseSpectrometerSettore FIS/05AstronomyAstronomy and AstrophysicsHigh-resolution X-ray spectrometerAstrophysics - Astrophysics of GalaxiesStars13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysics
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Projected WIMP sensitivity of the XENONnT dark matter experiment

2020

XENONnT is a dark matter direct detection experiment, utilizing 5.9 t of instrumented liquid xenon, located at the INFN Laboratori Nazionali del Gran Sasso. In this work, we predict the experimental background and project the sensitivity of XENONnT to the detection of weakly interacting massive particles (WIMPs). The expected average differential background rate in the energy region of interest, corresponding to (1, 13) keV and (4, 50) keV for electronic and nuclear recoils, amounts to 12.3 ± 0.6 (keV t y)-1 and (2.2± 0.5)× 10−3 (keV t y)-1, respectively, in a 4 t fiducial mass. We compute unified confidence intervals using the profile construction method, in order to ensure proper coverage…

WIMP nucleon: scatteringdata analysis methodCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics - Instrumentation and DetectorsHadronDark matterFOS: Physical sciencesElementary particledark matter: direct detection01 natural sciencesWIMP: dark matterHigh Energy Physics - ExperimentNONuclear physicsHigh Energy Physics - Experiment (hep-ex)XENONPE2_2WIMPPE2_1electron: recoil0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutron[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsPE2_4Dark matter experimentComputingMilieux_MISCELLANEOUSactivity reportnucleus: recoilPhysicsxenon: liquid010308 nuclear & particles physicsbackgroundAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)Dark matter experiments dark matter simulationssensitivityBaryonDark matter experimentsDark matter simulationsWeakly interacting massive particlesDark matter experiments; Dark matter simulationsNucleon[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Short range correlations in the weak decay of Lambda hypernuclei.

1995

The differences found in the relativistic and nonrelativistic methods used in the literature to account for short range nuclear correlations in the decay of \ensuremath{\Lambda} hypernuclei are analyzed. By means of a schematic microscopic model for the origin of correlations, the appropriate method to include them in nuclear processes is derived and is found to be the same one used in the nonrelativistic approach. The differences do not stem from relativistic effects but from the improper implementation of the correlations in the relativistic approach, which leads to several pathologies as shown in the paper. General formulas are given to evaluate the nonmesonic decay width of finite hyper…

Weak interactions (Nuclear physics)PhysicsEstructura nuclearNuclear and High Energy PhysicsParticle physicsRange (particle radiation)Nuclear TheoryInteraccions febles (Física nuclear)Carbon-12HyperonsLambda baryonLambdaPionHiperonsNuclear structureNuclear ExperimentNucleonRelativistic quantum chemistryRadioactive decayPhysical review. C, Nuclear physics
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Multi-strange baryon production in p-Pb collisions at √sNN = 5.02 TeV

2016

The multi-strange baryon yields in Pb–Pb collisions have been shown to exhibit an enhancement relative to pp reactions. In this work, and production rates have been measured with the ALICE experiment as a function of transverse momentum, pT, in p–Pb collisions at a centre-of-mass energy of √sNN = 5.02 TeV. The results cover the kinematic ranges 0.6 GeV/c < pT < 7.2 GeV/c and 0.8 GeV/c < pT < 5 GeV/c, for and respectively, in the common rapidity interval −0.5 < yCMS < 0. Multi-strange baryons have been identified by reconstructing their weak decays into charged particles. The pT spectra are analysed as a function of event charged-particle multiplicity, which in p–Pb collisions ranges over on…

Xi baryonsp-Pb collisionsOmega baryonsHigh Energy Physics::ExperimentNuclear Experiment
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