Nuclear Reactions. Shape, interaction, and excitation structures of nuclei. scattered particles. detector. solid angle. target. transmitted particles
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1 Nuclear Reactions Shape, interaction, and excitation structures of nuclei scattering expt. scattered particles detector solid angle projectile target transmitted particles K. Muto (TIT)
2 Nuclear fusion reactions two positive charges repel each other nuclear attractive intraction compound nucleus
3 Fusion reactions: compound nucleus formation Niels Bohr (1936) Neutron capture of nuclei compound nucleus N. Bohr, Nature 137 ( 36) 351 Wikipedia cf. Experiment of Enrico Fermi (1935) many very narrow (=long life-time) resonances (width ~ ev) M. Asghar et al., Nucl. Phys. 85 ( 66) 305
4 Fusion reactions: compound nucleus formation Niels Bohr (1936) Neutron capture of nuclei compound nucleus N. Bohr, Nature 137 ( 36) 351 Wikipedia forming a compound nucleus with heavy-ion reactions = H.I. fusion P T P+T compound nucleus
5 Fusion reactions: compound nucleus formation P T P+T compound nucleus cf. Bohr 36 energy production in stars (Bethe 39) nucleosynthesis superheavy elements Fusion and fission: large amplitude motions of quantum many-body systems with strong interaction microscopic understanding: an ultimate goal of nuclear physics
6 Fusion reactions: compound nucleus formation Evaporation P T P+T n,p,α emissions γ decay Evaporation + Fission A CN = A P + A T compound nucleus Fission cf. superheavy elements
7 Inter-nucleus potential Two interactions: 1. Coulomb force long range repulsion 2. Nuclear force short range attraction Above-barrier energies Sub-barrier energies (energies around the Coulomb barrier) Deep sub-barrier energies potential barrier due to a cancellation between the two (Coulomb barrier)
8 Why sub-barrier fusion? two obvious reasons: 30Zn fusion α decay 83Bi 113Nh 111Rg superheavy elements cf. 209 Bi ( 70 Zn,n) 278 Nh V B ~ 260 MeV E cm (exp) ~ 262 MeV
9 Why sub-barrier fusion? two obvious reasons: σ(e) resonance LOGARITMIC SCALE non-resonant direct measurements E 0 extrapolation needed! E coul Coulomb barrier figure: M. Aliotta nuclear astrophysics (nuclear fusion in stars) cf. extrapolation of data
10 Why sub-barrier fusion? two obvious reasons: superheavy elements other reasons: many-particle tunneling nuclear astrophysics reaction dynamics strong interplay between reaction and structure cf. high E reactions: much simpler reaction mechanisms E
11 Why sub-barrier fusion? two obvious reasons: superheavy elements other reasons: nuclear astrophysics reaction dynamics strong interplay between reaction and structure cf. high E reactions: much simpler reaction mechanisms many-particle tunneling many types of intrinsic degrees of freedom (several types of collective vibrations, deformation with several multipolarities) energy dependence of tunneling probability cf. alpha decay: fixed energy H.I. fusion reaction = an ideal playground to study quantum tunneling with many degrees of freedom
12 Quantum Tunneling Phenomena V(x) V 0 -a a x V(x) x Tunnel probability:
13 For a parabolic barrier V b x
14 Energy derivative of penetrability (note) Classical limit
15 cf. WKB approximation One dimensional Schrodinger equation: Assume
16 cf. WKB approximation Expand S as:
17 cf. WKB approximation this wave function breaks down at x which satisfies p(x) = 0. (a turning point) around x ~ b connect wave function from x > b to x < b (WKB connection formula) cf. solution for a linear potential : Airy function
18 cf. WKB approximation if applied to a tunneling problem:
19 for a Coulomb potential E R b -V 0
20 (note) for R 0 Sommerfeld parameter
21 The simplest approach to fusion: potential model Potential model: V(r) + absorption P l (E): barrier penetrability
22 Comparison with experimental data: large enhancement of σ fus Potential model: V(r) + absorption potential model
23 Comparison with experimental data: large enhancement of σ fus Potential model: V(r) + absorption potential model cf. seminal work: R.G. Stokstad et al., PRL41( 78) 465
24 154 Sm : a typical deformed nucleus 154 Sm (MeV) Sm
25 154 Sm : a typical deformed nucleus 154 Sm deformation of 154 Sm
26 Effects of nuclear deformation 154 Sm : a typical deformed nucleus 154 Sm θ 154 Sm 16 O
27 Effects of nuclear deformation 154 Sm : a typical deformed nucleus deformation θ 154 Sm 16 O Fusion: strong interplay between nuclear structure and reaction * Sub-barrier enhancement also for non-deformed targets: couplings to low-lying collective excitations coupling assisted tunneling
28 enhancement of fusion cross sections : a general phenomenon potential model strong correlation with nuclear spectrum coupling assisted tunneling
29 Enhancement of tunneling probability : a problem of two potential barriers barrier distribution due to couplings to excited states in projectile/target nuclei
30 Coupled-channels method: a quantal scattering theory with excitations many-body problem still very challenging two-body problem, but with excitations (coupled-channels approach) coupling
31 Coupled-channels method: a quantal scattering theory with excitations coupling if written down more explicitly: excitation energy excitation operator
32 Coupled-channels method: a quantal scattering theory with excitations entrance channel coupling excited channel excitation energy excitation operator full order treatment of excitation/de-excitation dynamics during reaction
33 Inputs for C.C. calculations i) Inter-nuclear potential a fit to experimental data at above barrier energies ii) Intrinsic degrees of freedom in most of cases, (macroscopic) collective model (rigid rotor / harmonic oscillator) simple harmonic oscillator 0 +,2 +, ε ε 0
34 C.C. approach: a standard tool for sub-barrier fusion reactions cf. CCFULL (K.H., N. Rowley, A.T. Kruppa, CPC123 ( 99) 143) Fusion barrier distribution (Rowley, Satchler, Stelson, PLB254( 91)) c.c. calculations K.H., N. Takigawa, PTP128 ( 12) 1061
35 K.H. and N. Takigawa, PTP128 ( 12) 1061
36 barrier distribution: a problem of two potential barriers
37 Fusion barrier distribution N. Rowley, G.R. Satchler, and P.H. Stelson, PLB254 ( 91) 25 J.X. Wei, J.R. Leigh et al., PRL67 ( 91) 3368 M. Dasgupta et al., Annu. Rev. Nucl. Part. Sci. 48 ( 98) 401 A.M. Stefanini et al., Phys. Rev. Lett. 74 ( 95) 864 sensitive to nuclear structure
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