Clustering and Medium Effects in Low Density Nuclear Matter

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In-Medium
BindingEffects
Energies
ClusteringCluster
and Medium
inin Low Density
and Mott Points
Low Density
Nuclear
Nuclear
MatterMatter
K. Hagel
SSNHIC 2014
Trento, Italy
8-Apr-2014
Outline
• Experimental Setup
• Clusterization and observables in low
density nuclear matter.
• Clusterization of alpha conjugate nuclei
• Summary
Beam Energy: 47 MeV/u
Reactions:40Ar + 112,124Sn
35 MeV/u
35 MeV/u
40Ca + 181Ta, Ca, C 28Si + 28Si
Cyclotron Institute, Texas A & M University
3
Beam Energy: 47 MeV/u
Reactions: 40Ar + 112,124Sn
35 MeV/u
35 MeV/u
40Ca + 181Ta, Ca, C 28Si + 28Si
NIMROD
•
•
•
•
14 Concentric Rings
3.6-167 degrees
Silicon Coverage
Neutron Ball
beam
S. Wuenschel et al., Nucl. Instrum. Methods. A604, 578–583 (2009).
4
Low Density Nuclear Matter
• Systems studied
– 47 MeV/u 40Ar + 112,124Sn
– 35 MeV/u 40Ca + 181Ta (preliminary
data)
• Use NIMROD as a violence filter
– Take 30% most violent collisions
• Use spectra from 40o ring
– Most of yield from intermediate
velocity source
• Coalescence analysis to extract
densities and temperatures
– Equilibrium constants
– Mott points
– Symmetry energy
Coalescence Parameters
π’…πŸ‘ 𝑡(𝒁, 𝑡)
π’…πŸ‘ 𝑡(𝟏, 𝟎)
𝑡
∝ 𝑹𝒏𝒑 𝒇(π‘·πŸŽ )
π’…π’‘πŸ‘
π’…π’‘πŸ‘
𝑨−𝟏
𝟏/𝟐
π’…πŸ‘ 𝑡(𝟏, 𝟎, 𝑬)
π’…π‘¬π’…πœ΄
𝑨
tavg, fm/c
πŸ’π… πŸ‘
𝑷
π’…πŸ‘ 𝑡(𝒁, 𝑡, 𝑬𝑨 )
𝑨−𝟏
πŸ‘ 𝟎
𝑡
= 𝑹𝒏𝒑
𝒅𝑬𝑨 π’…πœ΄
𝑡! 𝒁! πŸπ’ŽπŸ‘ 𝑬 − 𝑬𝒄
𝑨
vsurf, cm/ns
PRC 72 (2005) 024603
π’…πŸ‘ 𝑡(𝒁, 𝑡)
π‘¨πŸ‘ πŸπ’” + 𝟏 𝒆
𝑡
=
𝑹
𝒏𝒑
π’…π’‘πŸ‘
πŸπ‘¨
π‘¬πŸŽ /𝑻
π’‰πŸ‘
𝑽
𝑨−𝟏
π’…πŸ‘ 𝑡(𝟏, 𝟎)
π’…π’‘πŸ‘
3
𝑉=
𝑍! 𝑁! 𝐴
2𝐴
2𝑠 + 1 𝑒
𝐸0 /𝑇
1
𝐴−1
𝑨
3β„Ž3
4πœ‹π‘ƒ03
Temperatures and Densities
• Recall vsurf vs time calculation
• System starts hot
• As it cools, it expands
47 MeV/u 40Ar + 112Sn
Equilibrium constants from αparticles model predictions
𝐾𝑐 𝐴, 𝑍 =
•
•
•
•
•
•
𝜌(𝐴, 𝑍)
𝑍 (𝐴−𝑍)
πœŒπ‘ πœŒπ‘›
Many tests of EOS are done using
mass fractions and various
calculations include various different
competing species.
If any relevant species are not
included, mass fractions are not
accurate.
Equilibrium constants should be
independent of proton fraction and
choice of competing species.
Models converge at lowest densities,
but are significantly below data
Lattimer & Swesty with K=180, 220
show best agreement with data
QSM with p-dependent in-medium
binding energy shifts
PRL 108 (2012) 172701.
Density dependent binding energies
• From Albergo, recall that 𝑲𝒄(𝑨, 𝒁) = 𝐂 𝐓 𝒆
• Invert to calculate binding energies
𝑍
𝑁
• Entropy mixing term Δ𝐹 = 𝑇 𝑍𝑙𝑛
+ 𝑁𝑙𝑛
𝑩(𝑨,𝒁)
𝑻
𝐡
𝑍
𝑁
𝑙𝑛 𝐾𝑐 /𝐢(𝑇) = − 𝑍𝑙𝑛
− 𝑁𝑙𝑛( )
𝑇
𝐴
𝐴
𝐴
𝐴
PRL 108 (2012)
062702
Symmetry energy
S. Typel et al., Phys. Rev. C 81, 015803 (2010).
• Symmetry Free Energy
PRC 85, 064618 (2012).
– T is changing as ρ increases
– Isotherms of QS calculation that includes in-medium
modifications to cluster binding energies
• Entropy calculation (QS approach)
• Symmetry energy (Esym = Fsym + Tβˆ™Ssym)
– quasiparticle mean-field approach (RMF without clusters) does
not agree with the data
Alpha clustering in nuclei
• Ikeda diagram (K. Ikeda, N.
Takigawa, and H. Horiuchi,
Prog. Theor. Phys. Suppl. Extra
Number, 464, 1968.)
• Clusterization of low density
nuclear matter in collisions of
alpha conjugate nuclei
• Role of clusterization in
dynamics and disassembly.
Estimated limit N = 10α for selfconjugate nuclei(Yamada PRC 69, 024309)
Data Taken
40Ca
+
40Ca
28Si
+ 40Ca
40Ca
+
28Si
28Si
+ 28Si
40Ca
+
12C
28Si
+ 12C
+
180Ta
28Si
40Ca
+
180Ta
10, 25, 35 MeV/u
Alpha-like multiplicities
• Large number of
events with
significant alpha
conjugate mass for
all systems
Vparallel vs Amax
𝑀
𝐸∗ =
𝐾𝑐𝑝 𝑖 + 𝑀𝑛 𝐾𝑛 − 𝑄
𝑖=1
• Observe mostly PLF near beam velocity for low E*
• More neck (4-7 cm/ns) emission of α-like fragments
with increasing E*
Origin of alpha conjugate clusters
• Heavy partner is near
beam velocity
• alphas originate from
neck emission
Source Frame study of Origin of clusters
Origin of alpha conjugate clusters
(continued)
Source Frame Origin of clusters
(continued)
Summary
• Clusterization in low density nuclear
matter
– In medium effects important to describe data
– Equilibrium constants
• EOS Implications
– Density dependence of Mott points
– Symmetry Free energy -> Symmetry Energy
• Clusterization of alpha conjugate nuclei
– Large production of α-like nuclei
• Ca + Ca
• Ca + Ta
• Ca + C
– Neck emission of alphas important
Outlook and near future
• Low density nuclear matter
– We have a set of 35 MeV/u
28Si+181Ta
40Ca+181Ta
and
• Disassembly of alpha conjugate nuclei
– Analysis on presented systems continues
– Have Si + C, Si + Ta (almost calibrated) and
Ca + Si
Collaborators
J. B. Natowitz, K. Schmidt, K. Hagel, R. Wada,
S. Wuenschel, E. J. Kim, M. Barbui, G. Giuliani, L. Qin,
S. Shlomo, A. Bonasera, G. Röpke, S. Typel, Z. Chen,
M. Huang, J. Wang, H. Zheng, S. Kowalski,
M. R. D. Rodrigues, D. Fabris, M. Lunardon,
S. Moretto, G. Nebbia, S. Pesente, V. Rizzi, G. Viesti,
M. Cinausero, G. Prete, T. Keutgen, Y. El Masri,
Z. Majka, and Y. G. Ma
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