×
近期发现有不法分子冒充我刊与作者联系,借此进行欺诈等不法行为,请广大作者加以鉴别,如遇诈骗行为,请第一时间与我刊编辑部联系确认(《中国物理C》(英文)编辑部电话:010-88235947,010-88236950),并作报警处理。
本刊再次郑重声明:
(1)本刊官方网址为cpc.ihep.ac.cn和https://iopscience.iop.org/journal/1674-1137
(2)本刊采编系统作者中心是投稿的唯一路径,该系统为ScholarOne远程稿件采编系统,仅在本刊投稿网网址(https://mc03.manuscriptcentral.com/cpc)设有登录入口。本刊不接受其他方式的投稿,如打印稿投稿、E-mail信箱投稿等,若以此种方式接收投稿均为假冒。
(3)所有投稿均需经过严格的同行评议、编辑加工后方可发表,本刊不存在所谓的“编辑部内部征稿”。如果有人以“编辑部内部人员”名义帮助作者发稿,并收取发表费用,均为假冒。
                  
《中国物理C》(英文)编辑部
2024年10月30日

Symmetry energy from neutron-rich fragments in heavy-ion collisions, and its dependence on incident energy, and impact parameters

  • The yields of fragments produced in the 60Ni+12C reactions at 80 A and 140 A MeV, and with maximum impact parameters of 1.5, 2 and 7.3 fm at 80 A MeV are calculated by the statistical abrasion-ablation model. The yields of fragments are analyzed by the isobaric yield ratio (IYR) method to extract the coefficient of symmetry energy to temperature (asym/T). The incident energy is found to influence asym/T very little. It's found that asym/T of fragments with the same neutron-excess I=N-Z increases when A increases, while asym/T of isobars decreases when A increases. The asym/T of prefragments is rather smaller than that of the final fragments, and the asym/T of fragments in small impact parameters is smaller than that of the larger impact parameters, which both indicate that asym/T decreases when the temperature increases. The choice of the reference IYRs is found to have influence on the extracted asym/T of fragments, especially on the results of the more neutron-rich fragments. The surface-symmetry energy coefficient (bs/T) and the volume-symmetry energy coefficient (bv/T) are also extracted, and the bs/bv is found to coincide with the theoretical results.
      PCAS:
  • 加载中
  • [1] Danielewicz P, Lacey R, Lynch W G. Science, 2002, 298: 1592[2] Lattimer J M, Prakash M. Phys. Rep., 2000, 333: 121; Astrophys. J, 2001, 550: 426; Science, 2004, 304: 536[3] Baran V, Colonna M, Greco V et al. Phys. Rep., 2005, 410: 335.[4] Steiner A W, Prakash M, Lattimer J M et al. Phys. Rep., 2005, 411: 325[5] Fuchs C. J. Phys. G: Nucl. Part. Phys., 2008, 35: 014049[6] LI B A, CHEN L W, Ko C M et al. Phys. Rep., 2008, 464: 113[7] MA Y G, Natowitz J B, Wada R et al. Phys. Rev. C, 2005, 71: 054606[8] XU H S, Tsang M B, LIU T X et al. Phys. Rev. Lett., 2000, 85: 716[9] Henzlova D, Botvina A S, Schmidt K H et al. J. Phys. G: Nucl. Part. Phys., 2010, 37: 085010[10] Danagulyan A S, Balabekyan A R, Hovhannisyan G H. Phys. Atomic Nuclei, 2010, 73: 81[11] MA C W, FU Y, FANG D Q et al. Int. J. Mod. Phys. E, 2008, 17: 1669[12] ZHOU P, TIAN W D, MA Y G et al. Phys. Rev. C, 2011, 84: 037605[13] FANG D Q, MA Y G, ZHONG C et al. J. Phys. G: Nucl. Part. Phys., 2007, 34: 2173[14] HUANG M, CHEN Z, Kowalski S et al. Phys. Rev. C, 2010, 81: 044620[15] MA C W, WANG F, MA Y G et al. Phys. Rev. C, 2011, 83: 064620[16] MA C W, PU J, WANG S S, WEI H L. Chin. Phys. Lett., 2012, 29: 062101[17] Minich R W, Agarwal S, Bujak A et al. Phys. Lett. B, 1982, 458: 267c[18] Hirsch A S, Bujak A, Finn J E, Gutay L J, Minich R W, Porile N T, Scharenberg R P, Stringfellow B C, Turkot F. Phys. Rev. C, 1984, 29: 508[19] MA C W, WEI H L, LIU G J et al. J. Phys. G: Nucl. Part. Phys., 2010, 37: 015104[20] WEI H L, MA C W. Acta Phys. Sin., 2010, 59: 5364 (in Chinese)[21] MA C W, WANG S S. Chin. Phys. C (HEP NP), 2011, 35: 1017[22] FANG D Q, SHEN W Q, FENG J et al. Phys. Rev. C, 2000, 61: 044610[23] MA C W, WEI H L, FU Y et al. Phys. Rev. C, 2009, 79: 034606[24] von Weizscker C F. Z. Phys., 1935, 96: 431[25] Bethe H A. Rev. Mod. Phys., 1936, 8: 82[26] Green A E S, Edwards D F. Phys. Rev., 1953, 91: 46[27] Brohm T, Schmidt K H. Nucl. Phys. A, 1994, 569: 821[28] Gaimard J J, Schmidt K H. Nucl. Phys. A, 1991, 531: 709[29] MA C W, WEI H L, LI Y Q. Int. J. Mod. Phys. E, 2010, 19: 1545[30] MA C W, WEI H L, YU M. Phys. Rev. C, 2010, 82: 057602[31] MA C W, FU Y, FANG D Q et al. Chin. Phys. B, 2008, 17: 1216[32] FANG D Q, MA Y G, CAI X Z et al. Phys. Rev. C, 2010, 81: 047603[33] MA C W, WEI H L, WANG J Y et al. Chin. Phys. B, 2009, 18: 4781[34] CAI X Z, FENG J, SHEN W Q et al. Phys. Rev. C, 1998, 58: 572[35] DE J N, Samaddar S K. Phys. Rev. C, 2012, 85: 024310[36] WANG J, Wada R, Keutgen T et al. Phys. Rev. C, 2005, 72: 024603[37] Danielewicz P. Nucl. Phys. A, 2003, 727: 233[38] MEI H, HUANG Y, YAO J M, CHEN H. J. Phys. G: Nucl. Part. Phys., 2012, 39: 015107; and the reference therein
  • 加载中

Get Citation
MA Chun-Wang, SONG Heng-Li, PU Jie, ZHANG Tong-Lin, ZHANG Sha, WANG Shan-Shan, ZHAO Xin-Li and CHEN Li. Symmetry energy from neutron-rich fragments in heavy-ion collisions, and its dependence on incident energy, and impact parameters[J]. Chinese Physics C, 2013, 37(2): 024102. doi: 10.1088/1674-1137/37/2/024102
MA Chun-Wang, SONG Heng-Li, PU Jie, ZHANG Tong-Lin, ZHANG Sha, WANG Shan-Shan, ZHAO Xin-Li and CHEN Li. Symmetry energy from neutron-rich fragments in heavy-ion collisions, and its dependence on incident energy, and impact parameters[J]. Chinese Physics C, 2013, 37(2): 024102.  doi: 10.1088/1674-1137/37/2/024102 shu
Milestone
Received: 2012-03-27
Revised: 1900-01-01
Article Metric

Article Views(2030)
PDF Downloads(405)
Cited by(0)
Policy on re-use
To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.
通讯作者: 陈斌, bchen63@163.com
  • 1. 

    沈阳化工大学材料科学与工程学院 沈阳 110142

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Email This Article

Title:
Email:

Symmetry energy from neutron-rich fragments in heavy-ion collisions, and its dependence on incident energy, and impact parameters

    Corresponding author: MA Chun-Wang,

Abstract: The yields of fragments produced in the 60Ni+12C reactions at 80 A and 140 A MeV, and with maximum impact parameters of 1.5, 2 and 7.3 fm at 80 A MeV are calculated by the statistical abrasion-ablation model. The yields of fragments are analyzed by the isobaric yield ratio (IYR) method to extract the coefficient of symmetry energy to temperature (asym/T). The incident energy is found to influence asym/T very little. It's found that asym/T of fragments with the same neutron-excess I=N-Z increases when A increases, while asym/T of isobars decreases when A increases. The asym/T of prefragments is rather smaller than that of the final fragments, and the asym/T of fragments in small impact parameters is smaller than that of the larger impact parameters, which both indicate that asym/T decreases when the temperature increases. The choice of the reference IYRs is found to have influence on the extracted asym/T of fragments, especially on the results of the more neutron-rich fragments. The surface-symmetry energy coefficient (bs/T) and the volume-symmetry energy coefficient (bv/T) are also extracted, and the bs/bv is found to coincide with the theoretical results.

    HTML

Reference (1)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return