Search results for "mirror nuclei"

showing 10 items of 24 documents

Isospin-breaking corrections to superallowed Fermi beta-decay in isospin- and angular momentum-projected nuclear Density Functional Theory

2012

Background: The superallowed beta-decay rates provide stringent constraints on physics beyond the Standard Model of particle physics. To extract crucial information about the electroweak force, small isospin-breaking corrections to the Fermi matrix element of superallowed transitions must be applied. Purpose: We perform systematic calculations of isospin-breaking corrections to superallowed beta-decays and estimate theoretical uncertainties related to the basis truncation, time-odd polarization effects related to the intrinsic symmetry of the underlying Slater determinants, and to the functional parametrization. Methods: We use the self-consistent isospin- and angular-momentum-projected nuc…

PhysicsNuclear and High Energy PhysicsParticle physicsUnitarityNuclear Theoryta114Physics beyond the Standard ModelHigh Energy Physics::PhenomenologyElectroweak interactionFOS: Physical sciencesNuclear Theory (nucl-th)IsospinSlater determinantMirror nucleiSymmetry breakingNuclear Experiment (nucl-ex)Nuclear ExperimentNuclear ExperimentNuclear densityPhysical review C
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Transition probabilities in 31P and 31S : A test for isospin symmetry

2021

International audience; Excited states in the mirror nuclei 31P and 31S were populated in the 1p and 1n exit channels of the reaction 20Ne + 12C, at a beam energy of 33 MeV. The 20Ne beam was delivered for the first time by the Piave-Alpi accelerator of the Laboratori Nazionali di Legnaro. Angular correlations of coincident γ-rays and Doppler-shift attenuation lifetime measurements were performed using the multi-detector array GASP in conjunction with the EUCLIDES charged particle detector. In the observed B(E1) strengths, the isoscalar component, amounting to 24% of the isovector one, provides strong evidence for breaking of the isospin symmetry in the A=31 mass region. Self-consistent bey…

Nuclear and High Energy PhysicsLifetime measurementIsoscalarQC1-999Lifetime measurementslifetime measurements[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesResonance (particle physics)Isospin symmetrytransition probabilitiesNuclear physicsMicroscopic multiphonon modelMirror nucleimirror nuclei0103 physical sciencesMirror nucleiIsospin symmetry; Lifetime measurements; Microscopic multiphonon model; Mirror nuclei; Transition probabilities010306 general physicsmirrorTransition probabilitiesPhysicsIsovector010308 nuclear & particles physicsPhysics31SCharge (physics)31PSymmetry (physics)Charged particleisospin symmetryIsospinmicroscopic multiphonon modelnucleiydinfysiikka
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Mirror decay of 75Sr

2003

The β-decay of 75Sr to its mirror nucleus 75Rb was studied at the ISOLDE PSB facility at CERN by means of β-delayed γ and proton spectroscopy. The decay Q-value and β-delayed γ intensity were measured for the first time. These results, 10.60±0.22 MeV and 4.5+1.9 -0.7%, together with accurate measurements of the β-decay half-life and β-delayed proton branching ratio yielded the Gamow-Teller strength 0.35±0.05 for the mirror transition. Implications of the results on studies of deformation effects and on the path of the rapid proton capture process are discussed.

Nuclear physicsPhysicsNuclear and High Energy PhysicsProtonBranching fractionQ valueMirror nucleiAtomic physicsProton emissionNucleonBeta decayRadioactive decayThe European Physical Journal A
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Reevaluation of theP30(p,γ)S31astrophysical reaction rate from a study of theT=1/2mirror nuclei,S31andP31

2006

The $^{30}\mathrm{P}$($p,\ensuremath{\gamma}$)$^{31}\mathrm{S}$ reaction rate is expected to be the principal determinant for the endpoint of nucleosynthesis in classical novae. To date, the reaction rate has only been estimated through Hauser-Feschbach calculations and is unmeasured experimentally. This paper aims to remedy this situation. Excited states in $^{31}\mathrm{S}$ and $^{31}\mathrm{P}$ were populated in the $^{12}\mathrm{C}$($^{20}\mathrm{Ne}$,$n$) and $^{12}\mathrm{C}$($^{20}\mathrm{Ne}$,$p$) reactions, respectively, at a beam energy of 32 MeV, and their resulting $\ensuremath{\gamma}$decay was detected with the Gammasphere array. Around half the relevant proton unbound states …

PhysicsNuclear and High Energy PhysicsProtonNucleosynthesisExcited stateCarbon-12GammaspherePhosphorus-31 NMR spectroscopyMirror nucleiAtomic physicsNuclear ExperimentMirror symmetryPhysical Review C
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Isospin symmetry in B(E2) values: Coulomb excitation study of Mg21

2019

The Tz=−32 nucleus 21Mg has been studied by Coulomb excitation on 196Pt and 110Pd targets. A 205.6(1)-keV γ-ray transition resulting from the Coulomb excitation of the 52+ ground state to the first excited 12+ state in 21Mg was observed for the first time. Coulomb excitation cross-section measurements with both targets and a measurement of the half-life of the 12+ state yield an adopted value of B(E2;52+→12+)=13.3(4) W.u. A new excited state at 1672(1) keV with tentative 92+ assignment was also identified in 21Mg. This work demonstrates a large difference in the B(E2;52+→12+) value between T=32, A=21 mirror nuclei. The difference is investigated in the shell-model framework employing both i…

Physics010308 nuclear & particles physicsNuclear structureAb initioCoulomb excitation01 natural sciencesSymmetry (physics)Excited stateIsospin0103 physical sciencesMirror nucleiAtomic physics010306 general physicsGround statePhysical Review C
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Nuclear moments of neon isotopes in the range fromNe17at the proton drip line to neutron-richNe25

2005

Nuclear moments of odd-A neon isotopes in the range 17 ≤ A ≤ 25 have been determined from optical hyperfine structures measured by collinear fast-beam laser spectroscopy. The magnetic dipole moments of 17 Ne, 23 Ne and 25 Ne, as well as the electric quadrupole moment of 23 Ne are either reported for the first time or improved considerably. The measurements also decide for a 1/2 + ground state of 25 Ne. The behavior of the magnetic moments of the proton drip-line nucleus 17 Ne and its mirror partner 17 N suggests isospin symmetry. Thus, no clear indication of an anomalous nuclear structure is found for 17 Ne. The magnetic moments of the investigated nuclei are discussed in a shell-model appr…

PhysicsNuclear and High Energy PhysicsProtonMagnetic momentNuclear TheoryIsotopes of neonQuadrupoleNeutronPhysics::Atomic PhysicsMirror nucleiAtomic physicsNuclear ExperimentHyperfine structureMagnetic dipolePhysical Review C
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Asymptotic normalization coefficients and continuum coupling in mirror nuclei

2012

Background: An asymptotic normalization coefficient (ANC) characterizes the asymptotic form of a one-nucleon overlap integral required for description of nucleon-removal reactions. Purpose: We investigate the impact of the particle continuum on proton and neutron ANCs for mirror systems from $p$- and $sd$-shell regions. Method: We use the real-energy and complex-energy continuum shell model approaches. Results: We studied the general structure of the single-particle ANCs as a function of the binding energy and orbital angular momentum. We computed ANCs in mirror nuclei for different physical situations, including capture reactions to weakly-bound and unbound states. Conclusions: We demonstr…

Normalization (statistics)Nuclear and High Energy PhysicsAngular momentumNuclear Theory[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Nuclear TheoryMany-body theoryBinding energyFOS: Physical sciencesOrbital overlap[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesNuclear Theory (nucl-th)Quantum mechanics0103 physical sciencesNeutronMirror nucleiNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear ExperimentSolar and Stellar Astrophysics (astro-ph.SR)Physicsta114010308 nuclear & particles physics[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR][PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Asymptotic formAstrophysics - Solar and Stellar AstrophysicsAtomic physics
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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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Gamow-Teller Transitions Starting from T[sub z] = +3∕2 Nucleus [sup 47]Ti

2011

Gamow‐Teller (GT) transitions are mediated by the στ operator. Owing to its simplicity and also its spin‐isospin nature, GT transitions play key roles in the studies of nuclear structure as well as astro‐nuclear processes. In violent neutrino‐induced reactions at the core‐collapse stage of type II supernovae, Gamow‐Teller (GT) transitions starting from stable as well as unstable pf‐shell nuclei play important roles. We study GT transitions starting from 47Ti in a high‐resolution (3He,t) charge‐exchange reactions at 0° and at an intermediate incident energy of 140 MeV/nucleon at Research Center for Nuclear Physics (RCNP), Osaka. Individual GT transitions up to high excitations were observed.…

Nuclear physicsPhysicsNuclear reactionIsospinNuclear TheoryHadronNuclear structureMirror nucleiAtomic physicsNuclear ExperimentNucleonSpin (physics)Resonance (particle physics)AIP Conference Proceedings
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Symmetries in mirror nuclei $^{31}$S and $^{31}$P

2018

Excited states in mirror nuclei 31S and 31P were populated in the 1n and 1p exit channels, respectively, of the reaction 20Ne + 12C. The beam of 20Ne, with an energy of 33 MeV, was delivered for the first time by the Piave-Alpi accelerator of the Laboratori Nazionali di Legnaro. Angular correlations of coincident pairs and Doppler-shift attenuation lifetime measurements in 31S and 31P were performed using the multidetector array GASP in conjunction with the EUCLIDES charged particle detector. A comparison of the determined B(E1) strengths of the analog mirror 7/2- → 5/2+ transitions indicates the presence of a violation of isospin symmetry.

Physicsta114010308 nuclear & particles physicsAttenuationPhysicsQC1-999[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesCharged particleSymmetry (physics)Nuclear physicsPhysics and Astronomy (all)Coincidentnuclear physicsIsospinExcited state0103 physical sciencesMirror nuclei010306 general physicsydinfysiikkaBeam (structure)
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