Search results for "MIRROR NUCLEI"

showing 10 items of 24 documents

The β-decay approach for studying 12C

2008

6 pags., 3 figs. -- 9th International Conference on Clustering Aspects of Nuclear Structure and Dynamics (CLUSTERS'07) 3–7 September 2007, Stratford upon Avon, UK

HistoryChemistryDetectorCoincidenceComputer Science ApplicationsEducationNuclear physicsmedicine.anatomical_structuremedicineMirror nucleiAtomic physicsSpin (physics)NucleusEnergy (signal processing)Journal of Physics: Conference Series
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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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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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Isospin mixing and the continuum coupling in weakly bound nuclei

2009

The isospin breaking effects due to the Coulomb interaction in weakly-bound nuclei are studied using the Gamow Shell Model, a complex-energy configuration interaction approach which simultaneously takes into account many-body correlations between valence nucleons and continuum effects. We investigate the near-threshold behavior of one-nucleon spectroscopic factors and the structure of wave functions along an isomultiplet. Illustrative calculations are carried out for the T=1 isobaric triplet. By using a shell-model Hamiltonian consisting of an isoscalar nuclear interaction and the Coulomb term, we demonstrate that for weakly bound or unbound systems the structure of isobaric analog states v…

Nuclear and High Energy PhysicsNuclear Theory[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]IsoscalarNuclear TheoryFOS: Physical sciences01 natural sciencesNuclear Theory (nucl-th)symbols.namesakeQuantum mechanics0103 physical sciencesCoulombSymmetry breakingMirror nucleiNuclear Experiment010306 general physicsWave functionPhysics010308 nuclear & particles physics3. Good healthIsospinsymbols21.10.Sf 21.60.Cs 24.10.Cn 21.10.JxAtomic physicsHamiltonian (quantum mechanics)Nucleon
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Single-particle shell strengths near the doubly magic nucleus 56Ni and the 56Ni(p,γ)57Cu reaction rate in explosive astrophysical burning

2019

Angle-integrated cross-section measurements of the $^{56}$Ni(d,n) and (d,p) stripping reactions have been performed to determine the single-particle strengths of low-lying excited states in the mirror nuclei pair $^{57}$Cu-$^{57}$Ni situated adjacent to the doubly magic nucleus $^{56}$Ni. The reactions were studied in inverse kinematics utilizing a beam of radioactive $^{56}$Ni ions in conjunction with the GRETINA $\gamma$-array. Spectroscopic factors are compared with new shell-model calculations using a full $pf$ model space with the GPFX1A Hamiltonian for the isospin-conserving strong interaction plus Coulomb and charge-dependent Hamiltonians. These results were used to set new constrain…

Nuclear and High Energy Physicsastro-ph.SRNuclear TheoryExplosive materialnucl-thStrong interactionnucl-ex01 natural sciencesIonReaction ratesymbols.namesake0103 physical sciencesCoulombMirror nuclei010306 general physicsNuclear ExperimentNuclear ExperimentPhysicsradioactive beams010308 nuclear & particles physicsshell modellcsh:QC1-999Astrophysics - Solar and Stellar AstrophysicsExcited statesymbolsX-ray burststransfer reactionsAtomic physicsHamiltonian (quantum mechanics)ydinfysiikkalcsh:PhysicsPhysics Letters B
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Mirror energy differences above the 0f7/2 shell: First γ-ray spectroscopy of the Tz = −2 nucleus 56Zn

2021

5 pags., 4 figs.

Nuclear and High Energy Physicssinkki (metallit)QC1-999Nuclear Theory01 natural sciencesnucleon removalmirror nuclei0103 physical sciencesSubatomic Physicsmedicine010306 general physicsSpectroscopyradioactive ion beamsNuclear ExperimentNucleonsPhysics[PHYS]Physics [physics]isotoopitValence (chemistry)Isovector010308 nuclear & particles physicsYrastPhysicsFísicaSymmetry Breakingmedicine.anatomical_structureisospin symmetryshell-model calculationsExcited stateEnergy DifferenceAtomic physicsMultipole expansionydinfysiikkaNucleusBeam (structure)
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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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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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The $T_{z} = \pm 1 \to 0$ and $\pm 2 \to \pm 1$ Mirror Gamow--Teller Transitions in $pf$-shell Nuclei

2016

Gamow–Teller (GT) transitions are the most common weak-interaction processes in the Universe. They play important roles in various processes of nucleosynthesis, for example, in the rapid proton-capture process (rp-process). In the pf-shell region, the rp-process runs through neutron-deficient nuclei with Tz = −2, −1, and 0 mainly by means of GT and Fermi transitions, where Tz is the z component of isospin T defined by Tz = (N − Z)∕2. Under the assumption of isospin symmetry, mirror nuclei with reversed Z and N numbers, and thus with opposite signs of Tz, have the same structure. Therefore, symmetry is also expected for the GT transitions starting from and ending up in mirror nuclei. We have…

Physics010308 nuclear & particles physicsHadronShell (structure)General Physics and Astronomy01 natural sciencesSymmetry (physics)Nuclear physicsNucleosynthesisIsospin0103 physical sciencesMirror nuclei010306 general physicsFermi Gamma-ray Space TelescopeActa Physica Polonica B
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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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