Search results for "Multiplet"

showing 5 items of 65 documents

First observation of excited states in 108Sb

1995

A spectroscopic study of Sb-108 has been carried out as a part of a larger experiment where in total twenty-nine different residual nuclei were identified. This study gives the first information on excited levels in this nucleus. A low-lying two-quasi-particle multiplet together with some of the higher lying levels are discussed within the framework of the nuclear shell model. A rotational, strongly coupled, band is identified as, most likely, being built on the deformed pig9/2(-1) nuh11/2 configuration in accordance with total routhian surface calculations. Tentative spins and parities are presented as well as B(M1)/B(E2) ratios for some of the transitions in the strongly coupled band.

Strongly coupledNuclear reactionPhysicsNuclear and High Energy PhysicsSpinsbusiness.industryRouthianNuclear shell modelOpticsmedicine.anatomical_structureExcited statemedicineAtomic physicsbusinessMultipletNucleusNuclear Physics A
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Search for magnetically-induced signatures in the arrival directions of ultra-high-energy cosmic rays measured at the Pierre Auger Observatory

2020

We search for signals of magnetically-induced effects in the arrival directions of ultra-high-energy cosmic rays detected at the Pierre Auger Observatory. We apply two different methods. One is a search for sets of events that show a correlation between their arrival direction and the inverse of their energy, which would be expected if they come from the same point-like source, they have the same electric charge and their deflection is relatively small and coherent. We refer to these sets of events as "multiplets". The second method, called "thrust", is a principal axis analysis aimed to detect the elongated patterns in a region of interest. We study the sensitivity of both methods using a …

electric [charge]AstronomydeflectionThrustmagnetic fieldAstrophysics01 natural sciencesmass spectrumhelium: nucleusbenchmarksurface [detector]Cosmic ray experimentsUltra-high-energy cosmic ray010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEAstrophysics::Instrumentation and Methods for AstrophysicsCosmic ray experiments; Ultra high energy cosmic raysAugerobservatoryacceleration [cosmic radiation]Astrophysics - High Energy Astrophysical PhenomenasignaturePrincipal axis theoremActive galactic nucleusCherenkov counter: waterAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]energy spectrumFOS: Physical sciencesnucleus [helium]Cosmic rayElectric chargeCosmic ray experimentGLASTdetector: fluorescence0103 physical sciencesddc:530thrustcosmic radiation: UHEHigh Energy Physicscosmic radiation: accelerationAGNAstrophysiquePierre Auger Observatoryfluorescence [detector]010308 nuclear & particles physicsdetector: surfacecharge: electricwater [Cherenkov counter]Astronomy and AstrophysicsUltra high energy cosmic raysAstronomiesensitivityGalaxycoherencefluxgamma raymultipletcorrelationExperimental High Energy Physicsgalaxy[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]RAIOS CÓSMICOS
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High-precision mass measurements for the isobaric multiplet mass equation atA= 52

2017

Masses of $^{52}$Co, $^{52}$Co$^m$, $^{52}$Fe, $^{52}$Fe$^m$, and $^{52}$Mn have been measured with the JYFLTRAP double Penning trap mass spectrometer. Of these, $^{52}$Co and $^{52}$Co$^m$ have been experimentally determined for the first time and found to be more bound than predicted by extrapolations. The isobaric multiplet mass equation for the $T=2$ quintet at $A=52$ has been studied employing the new mass values. No significant breakdown (beyond the $3\sigma$ level) of the quadratic form of the IMME was observed ($\chi^2/n=2.4$). The cubic coefficient was 6.0(32) keV ($\chi^2/n=1.1$). The excitation energies for the isomer and the $T=2$ isobaric analogue state in $^{52}$Co have been d…

massaspektrometriaNuclear and High Energy Physicsisobaric multipletProtonCo-52Proton decayastrofysiikkaPenning trapFOS: Physical scienceskupariQuadratic form (statistics)atomipainot114 Physical sciences01 natural sciences7. Clean energyPENNING TRAPS0103 physical sciencesNuclear Experiment (nucl-ex)Nuclear Experiment010306 general physicsNuclear ExperimentMultipletmass measurementPhysicsisotoopitSPECTROSCOPY010308 nuclear & particles physicsMIRROR NUCLEIRAMSEY METHODPenning trapMN-52Mass formulaANALOG STATESPROTON RADIOACTIVITYCOULOMB DISPLACEMENT ENERGIESIsobaric processBETA-RAYAtomic physicsydinfysiikkaDECAYExcitationJournal of Physics G: Nuclear and Particle Physics
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Mass of astrophysically relevant 31Cl and the breakdown of the isobaric multiplet mass equation

2015

The mass of $^{31}$Cl has been measured with the JYFLTRAP double Penning trap mass spectrometer at the Ion-Guide Isotope Separator On-Line (IGISOL) facility. The determined mass-excess value, -7034.7(34) keV, is 15 times more precise than in the Atomic Mass Evaluation 2012. The quadratic form of the isobaric multiplet mass equation for the T=3/2 quartet at A=31 fails ($\chi^2_n$=11.6) and a non-zero cubic term, d=-3.5(11) keV, is obtained when the new mass value is adopted. $^{31}$Cl has been found to be less proton-bound with a proton separation energy of $S_p$=265(4) keV. Energies for the excited states in $^{31}$Cl and the photodisintegration rate on $^{31}$Cl have been determined with s…

massaspektrometriaprotonitisotoopitklooriphotodisintegrationastrofysiikkaFOS: Physical sciencesNuclear Experiment (nucl-ex)Nuclear Experimentisobaric multiplet mass equationydinfysiikkaNuclear Experiment
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Crystal field and magnetism with Wannier functions: Rare-earth doped aluminum garnets

2015

Using the recently developed method we calculate the crystal field parameters in yttrium and lutetium aluminum garnets doped with seven trivalent Kramers rare-earth ions. We then insert calculated parameters into the atomic-like Hamiltonian taking into account the electron-electron, spin-orbit and Zeeman interactions and determine the multiplet splitting by the crystal field as well as magnetic $\hat{g}$ tensors. We compare calculated results with available experimental data.

rare earthsWannier functionZeeman effectStrongly Correlated Electrons (cond-mat.str-el)Condensed matter physicsMagnetismab initio calculationsFOS: Physical scienceschemistry.chemical_elementGeneral ChemistryYttriumLutetiumIongarnetssymbols.namesakeCondensed Matter::Materials ScienceCondensed Matter - Strongly Correlated ElectronschemistryGeochemistry and PetrologysymbolsCondensed Matter::Strongly Correlated ElectronsHamiltonian (quantum mechanics)crystal fieldMultiplet
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