controlling the statistical decay of excited nuclei an crucial input for nucleosynthesis...
TRANSCRIPT
激发能相关的能级密度参数和重核衰变性质
叶 巍
(东南大学物理系 南京 )
内容
◆ 问题背景
◆ 理论模型
◆ 计算结果和结论
能级密度的重要性
● controlling the statistical decay of excited nuclei
● an crucial input for nucleosynthesis calculations (r-process), reactor science, etc.
Fermi-gas level-density expression
3/22
* *FG rot2
exp 2 aUa(E , J) 2J 1 , U E E (J)
2I 12 U
a
level-density parameter
It is employed in most statistical-model calculations
The level density parameter a is parametrized as:
d( ) [1 )) W / U]a U a (1-exp(-U/ E
d
U :W ::
a smoothed level-density parameter thermal energy
shell correction to the liquid-drop mass 18-20 MeV
E
1. Evaporation process: evaporation spectra
a
R.J.Charity, PRC82,014610(2010), and many other works
To fit energy spectra of evaporated particles, is large at low E* and small at higher E*, suggesting that must be dependent on E*
aa
2. Fission process: cross sections, particle yields
Critical factors that strongly influence the decay
mechanism of heavy nuclei at high energy
include:
A, E*, J, a(U) [af /an], , etc.
Experimental observation of enhanced emission of light particles prior to fission (with respect to predictions from standard statistical models) with increasing excitation energy in fusion-fission reactions. This is due to dissipation effects.
Theoretical Model
dq 1 dS(q,E*) T(t)
dt M dq M
The Langevin equation reads
q is the dimensionless fission coordinate and is definedas half of the distance between the center of mass of the future fission fragments divided by the radius of the compound nucleus. T is temperature, M is inertia parameter and is friction strength
(t) is a time-dependent stochastic variable which satisfies < (t) >=0 and < (t) (t’)> = 2δ(t-t’)
The driving force of the Langevin equation is calculated from the entropy:
E* is the total internal energy of the system, V(q) is potential energy.
deformation-dependent level density parameter
a(q) = a1A + a2 A2/3Bs(q)
where Bs(q) is the dimensionless surface area (for a sphereBs= 1). It is used to calculate af /an.
s(q,E*) 2 a(q)[E* V(q)]
● Evaporation residue cross section ER
Previous works on the role of the parameter af /an in the decay modes of thermal nuclei
B.Lott, et al. PRC 01, adjusting af /an to fit residue cross section data based on a statistical model
af /an changes with fissility
W.Ye, PRC81 (2010) 011603(R)
relativistic heavy-ion collisions vs. fusion reactions CN: (high E*,low L) vs. (low E*,high L)
W.Ye, PRC83 (2011) 044611
● spin distribution of evaporation residue
cross sections ER(L)
W.Ye, NPA853 (2011) 61
● prescission particle yields
role of spin: af /an (L)
Reactions systems
16O+181Ta 197Tl vs. 3,4He+197Au 200,201Tl
Scaling analysis of fission probability of systems 200Tl (right figure) and 201Tl (left figure) based on the standard statistical model
These figures are taken from L.G.Moretto et al., PRL75, 4186 (1995)and Th. Rubehn et al., PRC54, 3062 (1996)
16O+181Ta 197Tl
W.Ye, PRC84 (2011) 034617
Recent work on excitation-energy dependent af /an(E*) and its effects on the decay of hot nuclei
suggested probes: excitation energy at scission
E* = E*sc + V(q) + Ecoll + Eevap (tsc)
Ecoll is the kinetic energy of the collective degrees
of freedom, and Eevap(t) is the energy carried
away by all evaporated particles by the scission
time tsc
picture of fission process
Choose spallation reactions induced by
high energy protons
Models: QMD + SM, L.Ou, Z.X.Li, X.Z.Wu, etc.
BUU + SM, G.C.Yong, W.Zuo
INCL + SM , Belgium
main characteristics:
● the thermal excitation energy of the produced excited nuclei in spallation can reach 1 GeV
● significantly reduce side effects from compression, deformation and high spins. These distortions complicate the description of de-excitation process of excited nuclear systems
W.Ye, PRC85 (2012) 011601(R)
● The sensitivity of E*sc to nuclear friction depends on the af /an (E*).
● Experimentally, to probe information of af /an (E*), populating heavy systems with spallation reactions can significantly lower side effects associated with angular momentum, deformation, etc.
● Applications to spallation-induced reactions and the decay of superheavy nuclei.
Conclusions
Thanks for your attentions
W.Ye, High Energy Phys. Nucl. Phys. 26 (2000) 52
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