The effect of symmetry potential on the balance energy of light particles emitted from mass symmetric heavy-ion collisions with isotopes,isobars and isotones
Using the Ultrarelativistic Quantum Molecular Dynamics(UrQMD) model,the balance energies of free neutrons,free protons and Z=1 particles(including free protons,deuterons and tritons) from mass symmetric heavy-ion collisions with isotopes,isobars and isotones are studied.The influence of nuclear symm...
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| Published in | Science China. Physics, mechanics & astronomy Vol. 55; no. 12; pp. 2407 - 2413 |
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| Main Authors | , , , |
| Format | Journal Article |
| Language | English |
| Published |
Heidelberg
SP Science China Press
01.12.2012
Springer Nature B.V |
| Subjects | |
| Online Access | Get full text |
| ISSN | 1674-7348 1869-1927 1869-1927 |
| DOI | 10.1007/s11433-012-4922-3 |
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| Abstract | Using the Ultrarelativistic Quantum Molecular Dynamics(UrQMD) model,the balance energies of free neutrons,free protons and Z=1 particles(including free protons,deuterons and tritons) from mass symmetric heavy-ion collisions with isotopes,isobars and isotones are studied.The influence of nuclear symmetry potential energy on the balance energy is emphasized.It is found that the balance energy of free neutrons is sensitive to the nuclear symmetry energy,while that of free protons is not.Particularly,the initial neutron/proton ratio dependence of the balance energy of free neutrons from Sn isotopes can be taken as a useful probe to constrain the stiffness of the nuclear symmetry energy. |
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| AbstractList | Using the Ultrarelativistic Quantum Molecular Dynamics (UrQMD) model, the balance energies of free neutrons, free protons and Z=1 particles (including free protons, deuterons and tritons) from mass symmetric heavy-ion collisions with isotopes, isobars and isotones are studied. The influence of nuclear symmetry potential energy on the balance energy is emphasized. It is found that the balance energy of free neutrons is sensitive to the nuclear symmetry energy, while that of free protons is not. Particularly, the initial neutron/proton ratio dependence of the balance energy of free neutrons from Sn isotopes can be taken as a useful probe to constrain the stiffness of the nuclear symmetry energy. Using the Ultrarelativistic Quantum Molecular Dynamics(UrQMD) model,the balance energies of free neutrons,free protons and Z=1 particles(including free protons,deuterons and tritons) from mass symmetric heavy-ion collisions with isotopes,isobars and isotones are studied.The influence of nuclear symmetry potential energy on the balance energy is emphasized.It is found that the balance energy of free neutrons is sensitive to the nuclear symmetry energy,while that of free protons is not.Particularly,the initial neutron/proton ratio dependence of the balance energy of free neutrons from Sn isotopes can be taken as a useful probe to constrain the stiffness of the nuclear symmetry energy. Using the Ultrarelativistic Quantum Molecular Dynamics (UrQMD) model, the balance energies of free neutrons, free protons and Z =1 particles (including free protons, deuterons and tritons) from mass symmetric heavy-ion collisions with isotopes, isobars and isotones are studied. The influence of nuclear symmetry potential energy on the balance energy is emphasized. It is found that the balance energy of free neutrons is sensitive to the nuclear symmetry energy, while that of free protons is not. Particularly, the initial neutron/proton ratio dependence of the balance energy of free neutrons from Sn isotopes can be taken as a useful probe to constrain the stiffness of the nuclear symmetry energy. |
| Author | WANG YongJia GUO ChenChen LI QingFeng ZHANG HongFei |
| AuthorAffiliation | School of Science, Huzhou Teachers College, Huzhou 513000,China School of Nuclear Science and Technology, Lanzhou University Lanzhou 730000, China College of Nuclear Science and Technology, Beijing Normal University, Beijing 100875, China |
| Author_xml | – sequence: 1 givenname: YongJia surname: Wang fullname: Wang, YongJia organization: School of Science, Huzhou Teachers College, School of Nuclear Science and Technology, Lanzhou University – sequence: 2 givenname: ChenChen surname: Guo fullname: Guo, ChenChen organization: School of Science, Huzhou Teachers College, College of Nuclear Science and Technology, Beijing Normal University – sequence: 3 givenname: QingFeng surname: Li fullname: Li, QingFeng email: liqf@hutc.zj.cn organization: School of Science, Huzhou Teachers College – sequence: 4 givenname: HongFei surname: Zhang fullname: Zhang, HongFei organization: School of Nuclear Science and Technology, Lanzhou University |
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| CitedBy_id | crossref_primary_10_1140_epja_i2014_14038_5 crossref_primary_10_1007_s11433_017_9148_0 crossref_primary_10_1007_s41365_023_01269_1 crossref_primary_10_1103_PhysRevC_94_024608 crossref_primary_10_1007_s11433_015_5775_3 crossref_primary_10_1007_s11433_016_0120_3 crossref_primary_10_1103_PhysRevC_89_044603 crossref_primary_10_1103_PhysRevC_94_034608 crossref_primary_10_1007_s11433_016_0358_y crossref_primary_10_1007_s11467_020_0964_6 crossref_primary_10_1140_epja_i2015_15037_8 crossref_primary_10_1103_PhysRevC_90_054613 crossref_primary_10_1007_s11433_015_5673_8 crossref_primary_10_1016_j_ppnp_2018_01_002 crossref_primary_10_1103_PhysRevC_89_034606 crossref_primary_10_1103_PhysRevC_91_054615 |
| Cites_doi | 10.1103/PhysRevLett.78.1026 10.1103/PhysRevLett.71.1986 10.1103/PhysRevC.83.044617 10.1103/PhysRevC.69.054612 10.1103/PhysRevC.42.R10 10.1140/epja/i2006-10101-2 10.1016/j.physrep.2004.12.004 10.1016/j.physrep.2005.02.004 10.1016/j.physletb.2011.05.002 10.1103/PhysRevC.65.044604 10.1103/PhysRevLett.85.4221 10.1103/PhysRevC.82.014604 10.1103/PhysRevC.61.021602 10.1016/j.physletb.2011.02.033 10.1007/s11433-011-4616-2 10.1103/PhysRevC.82.024610 10.1016/j.nuclphysa.2011.12.006 10.1103/PhysRevC.80.024316 10.1103/PhysRevC.54.2457 10.1126/science.1078070 10.1007/s12043-010-0114-8 10.1088/0954-3899/37/8/085102 10.1103/PhysRevC.83.047604 10.1146/annurev.nucl.47.1.663 10.1103/PhysRevC.82.014603 10.1103/PhysRevC.58.3500 10.1103/PhysRevC.84.014611 10.1088/0954-3899/37/8/083101 10.1016/j.physletb.2004.05.053 10.1140/epja/i2006-10143-4 10.1103/PhysRevC.83.014603 10.1016/S0370-2693(99)00835-7 10.1016/j.physrep.2008.04.005 10.1007/s11433-011-4415-9 10.1103/PhysRevC.58.2283 |
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| Keywords | balance energy symmetry energy directed flow |
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| Notes | 11-5000/N symmetry energy,directed flow,balance energy Using the Ultrarelativistic Quantum Molecular Dynamics(UrQMD) model,the balance energies of free neutrons,free protons and Z=1 particles(including free protons,deuterons and tritons) from mass symmetric heavy-ion collisions with isotopes,isobars and isotones are studied.The influence of nuclear symmetry potential energy on the balance energy is emphasized.It is found that the balance energy of free neutrons is sensitive to the nuclear symmetry energy,while that of free protons is not.Particularly,the initial neutron/proton ratio dependence of the balance energy of free neutrons from Sn isotopes can be taken as a useful probe to constrain the stiffness of the nuclear symmetry energy. ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 14 |
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| References | Li, Chen, Ko (CR4) 2008; 464 Cozma (CR9) 2011; 700 Di, Baran, Colonna (CR34) 2010; 37 Andronic, Łukasik, Reisdorf (CR27) 2006; 30 Gautam, Sood, Puri (CR22) 2011; 83 Steiner, Prakash, Lattimer (CR3) 2005; 411 Reisdorf, Leifels, Andronic (CR33) 2012; 876 Reisdorf, Ritter (CR6) 1997; 47 Shetty, Yennello (CR5) 2010; 75 (CR16) 2002; 65 Sood, Puri (CR24) 2004; 69 Chugh, Puri (CR20) 2010; 82 CR30 Gautam, Sood (CR18) 2010; 82 Li (CR8) 2000; 85 Sood, Puri (CR26) 2006; 30 Danielewicz, Lacey, Lynch (CR7) 2002; 298 Ogilvie, Bauer, Cebra (CR12) 1990; 42 Magestro, Bauer, Bjarki (CR11) 2000; 61 Li, Shen, Guo (CR32) 2011; 83 Pak, Li, Benenson (CR14) 1997; 78 Sood, Puri, Aichelin (CR25) 2004; 594 CR2 Russotto, Wu, Zoric (CR10) 2011; 697 Sood (CR17) 2011; 84 Baran, Colonna, Greco (CR35) 2005; 410 Westfall, Bauer, Craig (CR15) 1993; 71 Scalone, Colonna, Di (CR29) 1999; 461 Guo, Wang, Li (CR31) 2012; 55 Goyal (CR21) 2011; 83 Warda, Vinas, Roca-Maza (CR1) 2009; 80 Chen, Zhang, Jin (CR28) 1998; 58 Pak, Bjarki, Hannuschke (CR13) 1996; 54 Kumar, Rajni, Kumar (CR23) 2010; 82 Gautam, Chugh, Sood (CR19) 2010; 37 W. Reisdorf (4922_CR33) 2012; 876 V. Baran (4922_CR35) 2005; 410 S. Goyal (4922_CR21) 2011; 83 D. J. Magestro (4922_CR11) 2000; 61 R. Chugh (4922_CR20) 2010; 82 R. Pak (4922_CR14) 1997; 78 S. Kumar (4922_CR23) 2010; 82 P. Danielewicz (4922_CR7) 2002; 298 L. Scalone (4922_CR29) 1999; 461 4922_CR2 A. D. Sood (4922_CR17) 2011; 84 INDRA collaboration. (4922_CR16) 2002; 65 A. D. Sood (4922_CR24) 2004; 69 M. Warda (4922_CR1) 2009; 80 A. D. Sood (4922_CR26) 2006; 30 D. V. Shetty (4922_CR5) 2010; 75 Q. F. Li (4922_CR32) 2011; 83 A. W. Steiner (4922_CR3) 2005; 411 M. D. Cozma (4922_CR9) 2011; 700 P. Russotto (4922_CR10) 2011; 697 C. A. Ogilvie (4922_CR12) 1990; 42 S. Gautam (4922_CR22) 2011; 83 W. Reisdorf (4922_CR6) 1997; 47 R. Pak (4922_CR13) 1996; 54 B. A. Li (4922_CR4) 2008; 464 4922_CR30 B. A. Li (4922_CR8) 2000; 85 A. D. Sood (4922_CR25) 2004; 594 G. D. Westfall (4922_CR15) 1993; 71 T. M. Di (4922_CR34) 2010; 37 L. W. Chen (4922_CR28) 1998; 58 S. Gautam (4922_CR18) 2010; 82 S. Gautam (4922_CR19) 2010; 37 A. Andronic (4922_CR27) 2006; 30 C. C. Guo (4922_CR31) 2012; 55 |
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| SubjectTerms | Astronomy Classical and Continuum Physics Deuterons Heavy ions Ionic collisions Isotopes Molecular dynamics Neutrons Nuclear isobars Observations and Techniques Particle physics Physics Physics and Astronomy Potential energy Protons Symmetry Tritons 中子能量 同位素 对称势 相对论量子分子动力学模型 等压线 粒子 能量平衡 重离子碰撞 |
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| Title | The effect of symmetry potential on the balance energy of light particles emitted from mass symmetric heavy-ion collisions with isotopes,isobars and isotones |
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