Energy Dependence of the Isotopic Composition in Nuclear Fragmentation - PowerPoint PPT Presentation

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Energy Dependence of the Isotopic Composition in Nuclear Fragmentation

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Energy Dependence of the Isotopic Composition in Nuclear Fragmentation S. Yennello, D. Shetty, M. Veselsky, E. Martin, A. Keksis, G. Souliotis and D. Rowland – PowerPoint PPT presentation

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Title: Energy Dependence of the Isotopic Composition in Nuclear Fragmentation


1
Energy Dependence of the Isotopic Composition in
Nuclear Fragmentation
  • S. Yennello, D. Shetty, M. Veselsky, E. Martin,
    A. Keksis, G. Souliotis and D. Rowland
  • Texas AM University
  • Cyclotron Institute

2
Two component liquid
Single component liquid
Two component liquid
Free n/p ratio t/3He ratio N/Zfragments
Possible signatures
3
Neutron content as a function of fragment size
for N/Z 1.2 to 2 DLi 11.5 DSi 2.6
4
Veselsky, Phys. Rev. C 62, 064613 (2000).
5
Veselsky, Phys. Rev. C 62, 064613 (2000).
6
28Si 112,124Sn
Veselsky,Phys Lett B 497,1(2001)
7
Ratio of isotopic yields58Ni, 58Fe 58Ni, 58Fe
30 Mev/nuc
8
Scaling factor
9
Relative free neutron and proton densities
10
Scaling factor at 30,40,47 MeV/nuc
11
neutron and proton densities at 30,40,47 MeV/nuc
12
Energy dependence of the scaling parameter a
58Fe 58Fe / 58Ni 58Ni
30 MeV 40 MeV 47 MeV
a 0.372 0.269 0.23
b -0.395 -0.372 -0.32
.
13
Canonical model predictions (SMM-McGill)
Temperature (left panel) and density (right
panel) dependence of the scaling parameter a.
Tsang PRC64, 054615 (2002)
14
Botvina IsoscalingR21 C exp(aA b(N-Z)
a D(mn mp)/2T
b D(mn - mp)/2T
28Si 112,124Sn
30 MeV/nuc
50 MeV/nuc
b 0.2370.038
b 0.1860.017
15
Botvina IsoscalingR21 C exp(aA b(N-Z)
28Si 112,124Sn 50 MeV/nuc
E (MeV) b
3 0.31
4 0.20
5 0.19
6 0.18
7 0.17
16
Summary
  • The enhancement in free neutrons of neutron-rich
    systems is greater at lower energies.
  • Isoscaling in 58Ni, 58Fe 58Ni, 58Fe
  • 3H/3He in 28Si 112Sn, 124Sn
  • Isoscaling in 28Si 112Sn, 124Sn

17
Theory
Bao An Li PRL 2000
18
Summary
  • The enhancement in free neutrons of neutron-rich
    systems is greater at lower energies.
  • Isoscaling in 58Ni, 58Fe 58Ni, 58Fe
  • 3H/3He in 28Si 112Sn, 124Sn
  • Isoscaling in 28Si 112Sn, 124Sn
  • Theoretical comparisons are in progress.

This work was supported in part by the Department
of Energy and the Robert A Welch Foundation
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