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Proton-neutron interactions. The key to structural evolution. Paradigm Benchmark 700 333 100 0 Rotor J(J + 1). Amplifies structural differences Centrifugal stretching Deviations. 6 + 690. 4 + 330. 2 + 100. 0 + 0. J E (keV).
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Proton-neutron interactions The key to structural evolution
Paradigm Benchmark 700 333 100 0 Rotor J(J + 1) Amplifies structural differences Centrifugal stretching Deviations 6+690 4+330 2+100 0+0 JE (keV) Identify additional degrees of freedom Detour before starting ? Without rotor paradigm
Microscopic perspective Valence Proton-Neutron Interaction Development of configuration mixing, collectivity and deformation – competition with pairing Changes in single particle energies and magic numbers Partial history: Goldhaber and de Shalit (1953); Talmi (1962); Federman and Pittel ( late 1970’s); Casten et al (1981); Heyde et al (1980’s); Nazarewicz, Dobacewski et al (1980’s); Otsuka et al( 2000’s) and many others.
Sn – Magic: no valence p-n interactions Both valence protons and neutrons Two effects Configuration mixing, collectivity Changes in single particle energies and shell structure
Microscopic mechanism of first order phase transition (Federman-Pittel, Heyde) Gap obliteration (N ~ 90 ) 1-space 2-space Monopole shift of proton s.p.e. as function of neutron number Can we see this experimentally?
A simple signature of phase transitions MEDIATEDby sub-shell changesBubbles and Crossing patterns
Seeing structural evolution Different perspectives can yield different insights Mid-sh. magic Onset of deformation as a phase transition mediated by a change in shell structure Onset of deformation “Crossing” and “Bubble” plots as indicators of phase transitional regions mediated by sub-shell changes
R4/2 Observable E2 Nucleon number, Z or N Sudden changes in R4/2 signify changes in structure, usually from spherical to deformed structure Def. 1/E2 Sph. Onset of deformation
Often, esp. in exotic nuclei, R4/2 is not available. A easier-to-obtain observable, E(21+), in the form of 1/ E(21+), can substitute equally well
Masses and Nucleonic Interactions Masses: • Shell structure: ~ 1 MeV • Quantum phase transitions: ~ 100s keV • Collective effects ~ 100 keV • Interaction filters ~ 10-15 keV Total mass/binding energy:Sum of all interactions Mass differences:Separation energies shell structure, phase transitions Double differences of masses:Interaction filters Macro Micro
Measurements of p-n Interaction Strengths dVpn Average p-n interaction between last protons and last neutrons Double Difference of Binding Energies Vpn (Z,N) = ¼ [ {B(Z,N) - B(Z, N-2)} - {B(Z-2, N) - B(Z-2, N-2)} ] Ref: J.-y. Zhang and J. D. Garrett
Valence p-n interaction: Can we measure it? Vpn (Z,N) = ¼[ {B(Z,N) - B(Z, N-2)} - {B(Z-2, N) - B(Z-2, N-2)} ] - - - p n p n p n p n - Int. of last two n with Z protons, N-2 neutrons and with each other Int. of last two n with Z-2 protons, N-2 neutrons and with each other Empirical average interaction of last two neutrons with last two protons
82 50 82 126 Orbit dependence of p-n interactions Low j, high n High j, low n
Z 82 , N < 126 3 1 2 3 2 1 82 50 82 126 Z > 82 , N < 126 Z > 82 , N > 126 Behavior of p-n interactions
126 82 LOW j, HIGH n HIGH j, LOW n 50 82 In terms of proton and neutron orbit filling, p-n interaction p-n interaction is short range similar orbits give largest p-n interaction Largest p-n interactions if proton and neutron shells are filling similar orbits
82 50 82 126 Empirical p-n interaction strengths indeed strongest along diagonal. Low j, high n High j, low n Neidherr et al, preliminary First direct correlation of observed growth rates of collectivity with empirical p-n interaction strengths
W. Nazarewicz, M. Stoitsov, W. Satula Realistic Calculations Microscopic Density Functional Calculations with Skyrme forces and different treatments of pairing
Density Functional Theory My understanding of DFT: Would you like to see it again? OK. So, I hope all this is clear. Anyway, Nazarewicz, Stoitsov and Satula calculated masses for over 1000 nuclei across the nuclear chart with several interactions, and, from these masses, computed the p-n interactions using the same double difference expression. Lots of results. A few examples:
Principal Collaborators • Burcu Cakirli (Istanbul) dVpn, Bubbles, Masses • Klaus Blaum (MPI – Heidelberg) Masses • Magda Kowalska (CERN – ISOLDE) Masses • And the GSI Schottky and CERN-ISOLDE mass groups for their measurements of Hg, Rn and Xe masses