Tian-Tian Ding·Chun-Wang Ma
An improved thermometer for intermediate-mass fragments
Tian-Tian Ding1·Chun-Wang Ma1
An improved thermometer(TIB)is proposed for intermediate-mass fragments via the difference between isobaric yield ratios.The residual free energy of three isobars is replaced by that of the binding energy.The measured fragments in the 140A MeV40,48Ca+9Be (181Ta)and58,64Ni+9Be(181Ta)reactions are analyzed to obtain TIBranging from 0.6 to 3.5 MeV.TIBis suggested to be a direct determination of temperature avoiding the fitting procedure.
Temperature.Intermediate-mass fragment. Isobaric ratio
The measured fragments in heavy-ion collisions have a lower temperature than the primary fragments which are formed in the hot source.The Albergo isotopic thermometer has been used to extract the temperature based on the yields of protons,neutrons,and some light isotopes[1]. Also,the isotopic thermometer has been used to extract the temperature of larger isotopes,such as the carbon isotopes [2,3]and intermediate-mass fragments(IMFs)[4,5]. Other methods employed to study this temperature in heavy-ion collisions include the thermal energy method [6],excitation energy method[7],momentum fluctuationmethod[8],the correlation of two-particle relative moment [9],and kinetic energy spectra of light particles[4]. Recently,the isobaric ratio method has been proposed to extract temperature for IMFs[10].
In the thermodynamic models,temperature is one part of the probes and cannot be separated easily.In the isobaric yield ratio method,the symmetry energy coefficient is studied by using its ratio to the temperature(asym/T)for neutron-rich nucleus[11].In this article,an improved thermometer is proposed to extract T of the IMFs which is based on the IYRs[12,13].
Here,the canonical ensemble theory is adopted.Based on the grand-canonical limitation,the cross section σ(A,I) of a fragment has the form of[14]

where C and τ are constants;T is the temperature, I=N-Z is the neutron excess;μn(μp)is the chemical potential of neutron(proton);and F(A,I)is the free energy of a fragment,which can be parameterized as the T-dependent mass formula[10,15-18].
The IYR is defined between the yield of isobars with I and I-2

where Δμ=μn-μp.Similarly,for isobars with I+2 and I,one has

Δμ/T for fragment changes very small,which has been shown in an isobaric ratio difference method[19-25], Thus,Δμ/T can be canceled out in the difference between isobaric yield ratios,

The residual free energy is defined as ΔF≡2 F(A, I)-F(A,I-2)-F(A,I+2).If ΔF is known,T can be obtained.It has been proven that within the finite temperature range,ΔF between two isobars can be replaced by that of the binding energy for the fragments[13].Following the assumption in Refs.[12,13],the residual free energy ΔF can be replaced by the residual binding energy ΔB=2B(A,I)-B(A,I-2)-B(A,I+2).From Eq.(4),the improved method to extract T based on the difference between IYRs(labeled as TIB)is

where ΔlnR=lnR(A,I+2,I)-lnR(A,I,I-2)is defined for simplification.The binding energy in the AME12 will be adopted in the analysis[26].
The fragments in the 140A MeV40,48Ca+9Be(181Ta) and58,64Ni+9Be(181Ta)reaction are adopted to verify the TIBmethod.They were measured by Mocko et al.[27] at the National Superconducting Cyclotron laboratory, Michigan State University.
ΔB and ΔlnR will be discussed separately,beginning with the distributions of ΔB for fragments in the 140A MeV40,48Ca+9Be and58,64Ni+9Be reactions (Fig.1).For the I=1 fragments,ΔB increases almost monotonically with A,while for fragments of I=3,5,7, ΔB staggers on the relative small A side.The staggering in ΔB becomes smaller for the A>33 fragments.ΔB for the I=9 fragments shows a small staggering,but the staggering is more evident for the A>47 fragments.
Secondly,ΔlnR for related isobars in the 140A MeV40,48Ca+9Be(181Ta)and58,64Ni+9Be(181Ta)reactions is plotted in Fig.2.For the I=1 fragments,ΔlnR almost keeps constant on the small A side,but increases with A at A>40,with some staggering at A>30.For the fragments of I=3,5,7,an obvious staggering appears in ΔlnR on the small A side,but it staggers little when A is relative large. The target(9Be and181Ta)shows very little influence on ΔlnR.In general,the distribution of ΔB and ΔlnR is similar in shape.

Fig.1(Color online)ΔB for the fragments in the 140A MeV 40,48Ca+9Be(181Ta)and58,64Ni+9Be(181Ta)reactions
Finally,we use ΔB and ΔlnR in 140A MeV40,48Ca+9Be (181Ta)and58,64Ni+9Be(181Ta)reactions to calculate TIB(Fig.3).TIBfor the I=1 fragments is almost constant at 1.5 MeV.TIBfor I=3 staggers for small A fragments,but becomes small and constant at A>35.TIBfor I=5 staggers,too,in a small manner though.But the staggering becomes larger again for I=7 and I=9 fragments.For most of the I>3 fragments,the TIBvalues range from 0.6 to 3.5 MeV,which agrees with the temperatures extracted by the IYR method[12,13].Only for some fragments of very rich neutrons,the TIBvalues are large.This agrees with the results in the canonical ensemble theory to estimate the mass of neutron-rich copper isotopes at T=2.2 MeV[14].Great difference can be seen between the TIBvalues for the reactions using9Be and181Ta targets when I is large(I=7 and 9),showing obvious target effect.
An improved isobaric ratio thermometer(TIB)for intermediate-mass fragments has been proposed based on the difference between IYRs,in which the residual free energy is replaced by the residual binding energy among these isobars.In contrast to the IYR thermometer,TIBis directly obtained from the yields of fragments and avoids the fitting procedure,which serve as a direct probe of temperature.TIBof the odd I fragments in the 140 MeV40,48Ca+9Be(181Ta)and58,64Ni+9Be(181Ta)reactions has been obtained.The values of TIBfor most considered IMFs are low.There is some inference that for similar reactions with different asymmetries,TIBcan be assumedas the same,so the assumption is reasonable that the temperatures in two similar reactions are similar.

Fig.2(Color online)ΔlnR for the fragments in the 140A MeV 40,48Ca+9Be(181Ta)and58,64Ni+9Be(181Ta)reactions

Fig.3(Color online)TIBfor the fragments in the 140A MeV 40,48Ca+9Be(181Ta)and58,64Ni+9Be(181Ta)reactions
1.S.Albergo et al.,Temperature and free-nucleon densities of nuclear matter exploding into light clusters in heavy-ion collisions.Nuovo Cimento A 89,1(1985).doi:10.1007/BF02773614
2.H.F.Xi et al.,Dynamical emission and isotope thermometry. Phys.Rev.C 58,R2636(1998).doi:10.1103/PhysRevC.58. R2636
3.W.Trautmann,ALADIN Collaboration et al.,Thermal and chemical freeze-out in spectator fragmentation.Phys.Rev.C 76, 064606(2007).doi:10.1103/PhysRevC.76.064606
4.T.Odeh et al.,Fragment kinetic energies and modes of fragment formation.Phys.Rev.Lett.84,4557(2000).doi:10.1103/Phys RevLett.84.4557
5.C.W.Ma et al.,Temperature of heavy fragments in heavy-ion collisions.Commun.Theor.Phys.59,95 (2013).http:// iopscience.iop.org/0253-6102/59/1/17
6.H.Zheng,A.Bonasera,Density and temperature of fermions from quantum fluctuations.Phys.Lett.B 696,178(2011).doi:10. 1016/j.physletb.2010.12.019
7.P.Zhou,W.D.Tian et al.,Influence of statistical sequential decay on isoscaling and symmetry energy coefficient in a gemini simulation.Phys.Rev.C 84,037605(2011).doi:10.1103/Phys RevC.84.037605
8.S.Wuenschel et al.,Measuring the temperature of hot nuclear fragments.Nucl.Phys.A 843,1(2010).doi:10.1016/j.nuclphysa. 2010.04.013
9.V.Serfling et al.,Temperatures of exploding nuclei.Phys.Rev. Lett.80,3928(1998).doi:10.1103/PhysRevLett.80.3928
10.C.W.Ma et al.,Temperature of intermediate mass fragments in simulated40Ca+40Ca reactions around the Fermi energies by AMD model.Nucl.Sci.Tech.27,111(2016).doi:10.1007/ s41365-016-0112-8
11.M.Huang et al.,Isobaric yield ratios and the symmetry energy in heavy-ion reactions near the Fermi energy.Phys.Rev.C 81, 044620(2010).doi:10.1103/PhysRevC.81.044620
12.C.W.Ma,J.Pu,Y.G.Ma,S.S.Wang et al.,Temperature determined by isobaric yield ratios in heavy-ion collisions.Phys.Rev. C 86,054611(2012).doi:10.1103/PhysRevC.86.054611
13.C.W.Ma et al.,Temperature determined by isobaric yield ratios in a grand-canonical ensemble theory.Phys.Rev.C 88,014609 (2013).doi:10.1103/PhysRevC.88.014609
14.M.B.Tsang et al.,Fragmentation cross sections and binding energies of neutron-rich nuclei. Phys. Rev. C 76, 041302(R)(2007).doi:10.1103/PhysRevC.76.041302
15.S.J.Lee,A.Z.Mekjian,Symmetry and surface symmetry energies in finite nuclei.Phys.Rev.C 82,064319(2010).doi:10.1103/ PhysRevC.82.064319
16.C.W.Ma,F.Wang,Y.G.Ma et al.,Isobaric yield ratios in heavyion reactions,and symmetry energy of neutron-rich nuclei at intermediate energies.Phys.Rev.C 83,064620(2011).doi:10. 1103/PhysRevC.83.064620
17.C.W.Ma et al.,Symmetry energy extracted from fragments in relativistic energy heavy-ion collisions induced by124,136Xe.Eur. Phys.J.A 48,78(2012).doi:10.1140/epja/i2012-12078-5
18.C.W.Ma et al.,The symmetry energy from the neutron-rich nucleus produced in the intermediate-energy40,48Ca and58,64Ni projectile fragmentation.Chin.Phys.Lett.29,062101(2012). doi:10.1088/0256-307X/29/6/062101
19.C.W.Ma,H.L.Wei et al.,Neutron-skin effects in isobaric yield ratios for mirror nuclei in a statistical abrasion-ablation model. Phys.Rev.C 88,044612(2013).doi:10.1103/PhysRevC.88. 044612
20.C.W.Ma,S.S.Wang,Y.L.Zhang et al.,Isobaric yield ratio difference in heavy-ion collisions,and comparison to isoscaling. Phys.Rev.C 87,034618(2013).doi:10.1103/PhysRevC.87. 034618
21.C.W.Ma,S.S.Wang,Y.L.Zhang et al.,Chemical properties of colliding sources in124,136Xe and112,124Sn induced collisions in isobaric yield ratio difference and isoscaling methods.J.Phys. G Nucl.Part.Phys.40,125106(2013).doi:10.1088/0954-3899/ 40/12/125106
22.C.W.Ma,J.Yu,X.M.Bai et al.,Isobaric yield ratio difference and neutron density difference in calcium isotopes.Phys.Rev.C 89,057602(2014).doi:10.1103/PhysRevC.89.057602
23.C.W.Ma,X.M.Bai,J.Yu et al.,Neutron density distributions of neutron-rich nuclei studied with the isobaric yield ratio difference.Eur.Phys.J.A 50,139(2014).doi:10.1140/epja/i2014-14139-1
24.C.W.Ma,Y.-L.Zhang,C.-Y.Qiao et al.,Target effects in isobaric yield ratio differences between projectile fragmentation reactions.Phys.Rev.C 91,014615(2015).doi:10.1103/Phys RevC.91.014615
25.C.Y.Qiao et al.,Isobaric yield ratio difference between the 140A MeV58Ni+9Be and64Ni+9Be reactions studied by the antisymmetric molecular dynamics model.Phys.Rev.C 92, 014612(2015).doi:10.1103/PhysRevC.92.014612
26.M.Wang et al.,The Ame 2012 atomic mass evaluation.Chin. Phys.C 36,1603(2012).doi:10.1088/1674-1137/36/12/003
27.M.Mocko et al.,Projectile fragmentation of40Ca,48Ca,58Ni,and64Ni at 140 MeV/nucleon.Phys.Rev.C 74,054612(2006). doi:10.1103/PhysRevC.74.054612
28 August 2016/Revised:28 August 2016/Accepted:15 September 2016
©Shanghai Institute of Applied Physics,Chinese Academy of Sciences,Chinese Nuclear Society,Science Press China and Springer Science+Business Media Singapore 2016
✉ Chun-Wang Ma
machunwang@126.com
1Institute of Particle and Nuclear Physics,Henan Normal University,Xinxiang 453007,China
Nuclear Science and Techniques
2016年6期