SEMICLASSICAL DESCRIPTION OF SHELL EFFECTS IN FINITE FERMION SYSTEMS. M. Brack, University of Regensburg

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SEMICLASSICAL DESCRIPTION OF SHELL EFFECTS IN FINITE FERMION SYSTEMS M. Brack, University of Regensburg ( Nilsson model 50 years, Lund, 14. June 2005) 1. Semiclassics and POT: basics semiclassical quantization (WKB, EBK) Gutzwiller s trace formula Periodic Orbit Theory (POT) for shell effects 2. Applications to finite fermion systems nuclei (deformations, asymmetry of fission barrier) metal clusters (supershells, deformations) semiconductor nanostructures (conductance fluctuations) trapped dilute fermionic gases (supershells) 1) 1) omitted due to lack of time; see the talk of Magnus Ögren! For a general introduction to POT, see: M. Brack and R. K. Bhaduri: Semiclassical Physics (Westview Press, Boulder CO, USA 2003)

Semiclassical quantization Bohr-Sommerfeld quantization + WKB: (1-dim.) Quantization of action integral along periodic orbit: S(E) = p(x) dx = 2π (n+α) n = 0,1, 2,... quantized eneriges E n, become exact in limit n 1 (Bohr s correspondence principle!), i.e., for S (but works often well already for n = 0, 1, 2,...!) In (N>1) dimensions: torus (EBK) quantization, works only for integrable systems! Gutzwiller s trace formula: derived (1971) from the Feynman path-integral formulation of quantum mechanics in the limit S : works also for non-integrable and chaotic systems!

The Gutzwiller trace formula The quantum-mechanical density of states: g(e) = n δ(e E n) = g(e) + δg(e) Smooth part g(e): from extended Thomas-Fermi (ETF) model (or Weyl expansion) Oscillating part δg(e): semiclassical trace formula (to leading order in ) δg(e) po A po(e)cos [ 1 S po(e) π 2 σ ] po Sum over periodic orbits (po) of the classical system! S po = p dq = action integral along po po A po = amplitude (related to stability and degeneracy) σ po = Maslov index [M. Gutzwiller, J. Math. Phys. 12, 343 (1971)]

Trace formulae for finite fermion systems For N interacting fermions in a (self-consistent) mean field approximation (HF or DFT): { ˆT + V [φ]} φ n = E n φ n Total energy (using Strutinsky theorem): E = Ẽ + δe with N = Ñ + δn.1) Trace formulae from classical H(p, q) = T + V : [practically: using model potential V [φ] V (q)] δg(e) [ 1 A po (E) cos S po(e) π ] 2 σ po po ( ) 2 [ 1 A po(e F )cos ] δe po δn po T po ( T po S po(e F ) π 2 σ po ) [ 1 A po (E F ) sin S po(e F ) π ] 2 σ po E F (N) = Fermi energy 1) Average e E(N): from selfconsistent ETF (or liquid drop) model

Coarse graining and finite temperatures For finite resolution of energy spectrum: convolute level density over energy range γ g γ (E) = 1 πγ n e ( E E n γ ) 2 get exponential damping factor in trace formula: δg γ (E) [ A po (E)e (γt po/2 ) 2 1 cos S po(e) π ] 2 σ po po Only shortest orbits relevant for gross-shell effects! Similarly at finite temperatures T (for grand canonical ensemble): δg T (E) [ τ po 1 A po (E) Sinh(τ po po ) cos S po(e) π ] 2 σ po with τ po = k B TπT po / trace formula for free energy: δf = ( ) 2 [ A po (E F ) τ po 1 cos T po po Sinh(τ po ) S po(e F ) π ] 2 σ po

Bifurcations At a bifurcation (e.g., E = E bif ) of a periodic orbit, the amplitude A po (E bif ) diverges! Remedy: go beyond the second-order stationary phase approximation in the integral(s) used for the derivation of A po (E). This leads to Uniform approximations: local, near a bifurcation: see Ozorio de Almeida and Hannay, J. Phys. A 20, 5873 (1987) global, to recover also the asymptotic Gutzwiller amplitudes far from the bifurcation: see Sieber and H. Schomerus, J. Phys. A 31, 165 (1998) (and earlier work quoted therein) Attention: No physical meaning should be attached to the diverging amplitudes A po near bifurcations without doing appropriate uniform approximations!

Nuclear deformations Neutron shell-correction energy δe n (η, N) versus deformation (axis ratio) η and neutron number N: Contours: quantum-mechanics with spheroidal Woods- Saxon potential (including spin-orbit interaction) Bars: semiclassical valleys of minima: δs po = 0 for actions of shortest periodic orbits in ellipsoidal cavity (no spin-orbit; Fermi energy adjusted to reproduce correct magic numbers!) [V. M. Strutinsky, A. G. Magner, S. R. Ofengenden and T. Døssing, Z. Phys. A 283, 269 (1977)]

The double-humped fission barrier Deformation energy of a typical actinide nucleus (schematic, projected onto one-dimensional deformation variable): Difference from smooth (classical) liquid drop model (LDM) behaviour: quantum shell effects ( shell-correction energy) Lowest outer barrier for left-right asymmetric shapes Leads to mass asymmetry of the fragment distribution (Classical LDM would give symmetric distribution)

A short Lund history of the fission asymmetry: 1962: S. A. E. Johansson [Nucl. Phys. 22, 529 (1962)] studies octopole deformations in the single-particle model, finds instability at LDM fission barrier of heavy nuclei. 1970: P. Möller and S. G. Nilsson [Phys. Lett. 31 B, 283 (1970)] obtain instability of outer fission barrier with respect to suitable combinations of ɛ 3 and ɛ 5 deformations in the Nilsson model using Strutinsky s shell-correction method. 1971: C. Gustafsson, P. Möller and S. G. Nilsson [Phys. Lett. 34 B, 349 (1971)] explained the quantum-mechanical mechanism of this instability by certain pairs of diabatic single-particle states whose energy levels are particularly sensitive to the ɛ 3 -ɛ 5 deformations. 2001: S. M. Reimann contributes to a semiclassical interpretation of this instability as due to periodic orbits, along which the wavefunctions of the same type of single-particle states have their maxima, and whose local EBK quantization gives the correct single-particle energies of the diabatic states. [M. Brack, M. Sieber and S. M. Reimann, Physica Scripta T90, 146 (2001)].

A simple semiclassical model for fission: Axially symmetric shapes from LDM model: c: elongation parameter h: neck parameter α 0: left-right asymmetry parameter Replace nuclear mean field by 3d cavity with the same shapes (c,h, α) Find the shortest periodic orbits and calculate shellcorrection energy δe(c, h, α) using the semiclassical trace formula!

Semiclassical fission barrier Fission barrier of 240 Pu nucleus versus elongation c and asymmetry α: A 0 A symm. asymm. B 0.1 B C 10 0 δe C α 0.2 1.3 1.5 c -10 1.7 h = - 0.075 h = 0.0 Comparison with quantum-mechanical results: 0.0 0.1 α 0.2 0.0 0.1 α 0.2 1.3 1.5 c 1.7 A B C 1.3 1.5 c 1.7 Valley of minimal energy (A-B-C): classical action of dominant orbits is constant! δs po = 0 Left: quantum-mechanical δe (Strutinsky) (1971) Right: semiclassical δe with only 2 orbits in equator plane(s) [M. Brack, S. Reimann, M. Sieber, PRL 79, 1817 (1997)]

Poincaré surface of section (not area conserving!) at symmetric barrier (c=1.53, h=0, α=0): Shortest periodic orbits lie in same planes as the wavefunction extrema of the diabatic single-particle states! [M. Brack, M. Sieber and S. M. Reimann, Physica Scripta T90, 146 (2001)]

Poincaré surface of section (not area conserving!) at asymmetric saddle (point B: c=1.53, h=0, α=0.13): A tiny regular island in the middle of a sea of chaos causes the onset of the mass asymmetry!

Quantization of small regular island Approximate EBK quantization of the linearized motion near the shortest periodic orbits 1) : 12 (2,3) (1,3) 10 k R 8 (2,2) (1,2) 6 4 (2,1) (1,1) 0.0 0.05 0.1 0.15 0.2 Coloured dashed lines: EBK levels (n z, n ρ ), approximate the diabatic quantum states! Black lines: exact quantum-mechanical levels 1) as if in ellipsoid with same curvatures at turning points

Multipole deformations of metal clusters Deformations ɛ 2, ɛ 3, ɛ 4 of axial 3d cavities with N particles (minimizing E tot = E LDM + δe): 0.2 0.1 2 0.0-0.1 100 120 140 160 180 200 0.1 qm sc 3 0.05 0.0 100 120 140 160 180 200 0.1 4 0.0-0.1 100 120 140 160 180 200 N Solid lines: quantum-mechanical δe with Strutinsky method Dashed lines: semiclassical δe with perturbative trace formula [V. V. Pashkevich, P. Meier, M. Brack and A. V. Unzhakova, Phys. Lett. A 294, 314 (2002)]

Supershells in metal clusters Abundance of Na clusters with N atoms (most stable for magic numbers N i ) [J. Pedersen et al., Nature 353, 733 (1991)]. Semiclassically: interference of triangle and square orbits in spherical cavity [R. Balian and C. Bloch, Ann. Phys. 69, 76 (1972)] or Woods-Saxon potential [H. Nishioka, K. Hansen and B. R. Mottelson, Phys. Rev. B 42, 9377 (1990)]. Quantum-mechanically: DFT (Kohn-Sham eqs.) in jellium model [H. Genzken and M. Brack, Phys. Rev. Lett. 67, 3286 (1991)].

Experimental magic radii of Na clusters: plot of R i = r 0 N 1/3 i (dots) against shell number i: ignore this look here! Experiment: Slope of red line (also for other metals: Li, Ga): s exp = 0.61 ± 0.01 Semiclassics: From the mean length of triangular (3,1) and square (4,1) orbits in the Balian-Bloch sphere one gets: s POT = 0.603 Quantum-mechanics: (Jellium + LDA-Kohn-Sham): s = 0.61

Magnetoconductance in a quantum dot Experimental conductance of a circular quantum dot with 1500 electrons (NBI/Chalmers, 1995); gray-scale plot of δg: Semicl. trace formula (circular billard); gray-scale plot of δg(e F ): period ( ) R average length of shortest orbit(s)! period ( ) B average area of shortest orbit(s)!

Effect of a (homogeneous) magnetic field B: Canonical momentum: p p e c A Action: S po S po e c po A dq = S po e c BF po = S po e c Φ po shift of phase by magnetic flux Φ po of periodic orbit; analogous to Aharonov-Bohm (AB) effect! In weak homogeneous magnetic field B (perturbation theory!): δg(e F, B) ( 1 A po cos S po π ) e ) 2 σ po cos( c BF po po First factor: B = 0 case shell oscillations versus energy E or radius R Last factor: AB oscillations versus B [S. M. Reimann, M. Persson, P. E. Lindelof, M. Brack, Z. Phys. B 101, 377 (1996)]

Magnetoconductance oscillations in a mesoscopic channel with antidots The device (A. Sachraida et al., Ottawa): Gate Gate Gate 0.2µm 1.0µm Gate 0 E F E Conductance (Aharonov-Bohm) oscillations δg xx : δg xx [arb.u.] 0.15 0.20 0.25 B[T] solid line: experimental, dashed line: semiclassical results. [J. Blaschke, PhD Thesis (Regensburg, 1999); J. Blaschke and M. Brack, Europhys. Lett. 50, 294 (2000)]

Observable footprints of periodic orbit bifurcations Plots of oscillation maxima of δg xx versus magnetic field B (vertical) and gate voltage V g or antidot radius s d (horizontal): (a) 0.28 B[T] (b) 0.24 0.2-1.4-1.2 V g [V] 0.16 2.2 (c) 2.1 2.0 1.9 s d (a) experimental results (b) semiclassical theory: shaded lines mark bifurcation loci of leading periodic orbits (c) local comparison experiment semiclassical theory dislocations are signatures of orbit bifurcations!

Thanks 1. To my postdocs and students at Regensburg: M. Seidl, O. Zaisev H. Genzken, P. Meier, J. Blaschke Ch. Amann, J. Kaidel, M. Pletyukhov 2. To my visitors and external collaborators: R. K. Bhaduri (McMaster, Canada) M. V. N. Murthy (I.M.Sc. Madras, India) S. Creagh (Nottingham, UK) M. Sieber (Bristol, UK) V. Pashkevich (JINR Dubna, Russia) A. Sugita (Tokio, Japan) S. Reimann, M. Ögren (LTH, Lund) 3. To my sponsors: Deutsche Forschungsgemeinschaft SFSR and Swedish Research Council NSERC (Canada) 4. To a patient audience!