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【硕导】赵先锋

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导师信息

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教师姓名:

赵先锋

 


 

说明: 地址图标

职称/职务:

教授

说明: 领英图标

学历/学位:

研究生/博士

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电子邮件:

zhaopioneer.student@sina.com

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研究领域:

核天体物理

光电智能检测与信息处理

 

 

物理测试技术及仪器

*  科研项目

1)国家自然科学基金项目(应急管理项目-理论物理专款),相对论平均场理论对大质量中子星的研究,114470032015.01-2017.12,主持,已结题

2)省级高校省级自然科学研究重点项目,大质量中子星PSR J0348+0432 的相对论平均场理论研究,KJ2014A1822014.1-2016.12,主持,已结题

3)省级自然科学基金面上项目,相对论平均场理论在中子星物质研究中的应用,1208085MA092012.07—2014.06,主持,已结题

4)省级高校省级自然科学研究项目,中子星PSR J1614-2230等致密天体的相对论平均场描述,KJ2012Z2972012.1-2012.12,主持,已结题

5)省级高校省级自然科学研究项目,慢旋转中子星转动惯量的研究,KJ2009B1062009.1-2010.09,主持,已结题

6)校级科学研究项目,奇异介子对慢旋转中子星转动惯量的影响,2008kj019B2009.01-2009.12,主持,已结题

*  论文专著

A 论文

[1] 赵先锋,洪时明,刘福生. 压力对碳氢氧超临界流体中碳的溶解度的影响[J]. 高压物理学报, 2003,17(2):101-105. EI

[2] 赵先锋. 相对运动的矢量图示解法 [J]. 数学.力学.物理学.高新技术研究进展, 2006,11:366-368.

[3] 赵先锋, 王顺金, 张华, 贾焕玉. 介子对中子星物质的影响 [J]. 高能物理与核物理,   2007, 31 (4): 345-349. SCI

[4] 赵先锋, 王顺金, 张华, 贾焕玉. 介子对有限温度中子星物质的影响 [J]. 高能物理与核物理,   2007, 31 (6): 532-537. SCI

[5] 赵先锋. 非平行平面薄膜反射光干涉公式的推导[J]. 滁州学院学报, 2009,11(1):53-54.

[6] 赵先锋, 王顺金, 张华, 贾焕玉. 介子对中子星转动惯量的影响 [J]. 四川大学学报 (自然科学版),   2009, 46 (3)5: 743-747.

[7] 赵先锋, 张华. 温度对前身中子星转动惯量的影响   [J]. 四川大学学报 (自然科学版), 2010, 47 (3)5 : 579-584.

[8] 赵先锋. 物理学史料在大学物理教学中的作用[J]. 滁州学院学报, 2010,12(2)4:102-103.

[9] Zhao Xian-Feng, Zhang Hua. Effect   of strange mesons on the moment of inertia of proto neutron star  [J]. Journal   of  Sichuan University ( Natural Science Edition), 2010, 47 (4)7:   825-830.

[10] 赵先锋, 张华. 自相互作用对超子星转变密度的影响 [J]   . 山东大学学报 (理学版), 2010, 45 (9)9: 96-100.

[11] Zhao Xian-Feng. The gravitational redshift of a proto   neutron star [J]. Chinese Physics Letters, 2010, 27 (9)9: 099701.SCI,   IF=0.731

[12] Zhao Xian-Feng. Zhang Hua, Jia Huan-Yu. On the   moment of inertia of a proto neutron star [J]. Chinese Physics C, 2010, 34 (10)10: 1587-1592. (SCI, IF=0.272

[13] Zhao Xian-Feng. Zhang Hua. Effect   of the mesons σ* and Φ and the variety of UΣ(N) on the transition density of hyperon stars [J]. Chinese Physics C, 2010, 34 (11)11: 1704-1708. (SCI, IF=0.272

[14] Zhao Xian-Feng. Constraining the gravitational redshift of a neutron star from   the Σ-meson well depth [J]. Astrophysics and Space Science, 2011, 332(1)3: 139–144.SCI,   IF=1.686

[15] Zhao Xian-Feng. Effects ofandmesons   on surface redshift of a neutron star [J]. Chinese Physics B, 2011, 20 (3)3:   039701. (SCI, IF=1.376)

[16] Zhao   Xian-Feng. Potential depth of Σ in nuclear matter and moment of inertia   of a proto neutron star [J]. 天文学报, 201152(2)3: 126-135.

[17] 赵先锋. 相对论平均场理论中耦合常数g_ρ的确定与研究   [J]. 中山大学学报 (自然科学版), 2011, 50(2)3: 31-35.

[18] Zhao Xian-Feng.   Temprature effect of the gravitational redshist of a proto neutron star [J].   Chinese Journal of Physics, 2011, 49(2)4: 621-628. (SCI, IF=0.448)

[19] 赵先锋, 张华.    超子同位旋相互作用对中子星转动惯量的影响 [J]. 云南大学学报 (自然科学版)2011, 33(3)5: 303-307.

[20] 赵先锋, 张华. 超子同位旋相互作用能对超子星转变密度的影响 [J]. 吉林大学学报 (理学版), 2011, 49(3)5: 528-532.

[21] 赵先锋. 变重力加速度对自由落体落地速度的影响[J]. 滁州学院学报, 2011,13(2)4:120-122.

[22] Zhao Xian-feng. Potential depth of Σ-hyperons in   saturated nuclear matter and rotational inertia of proto neutron star [J].   Chinese Astronomy and Astrophysics, 2011, 35(7): 285-294.

[23] Zhao Xian-Feng. Constraining the surface   gravitational redshift of proto neutron stars with new nucleon coupling   constants [J]. International Journal of Theoretical Physics, 2011, 50(9)9: 2951-2960.SCI,   IF=0.845

[24] Zhao Xian-Feng. The   influence of the hyperon coupling constants on the gravitational redshift of   a proto neutron star [J]. Journal of Sichuan   University (Natural Science Edition), 2011, 48(4)7: 865-868.

[25] Zhao Xian-Feng. The potential well depth U^(N)_Σ constraints on the surface   gravitational redshift of a proto neutron star [J]. Journal of Astrophysics   and Astronomy. 2011, 32(3)9: 391-399. (SCI, IF=0.4)

[26] 赵先锋,方春阳,王大树,汪杰. 相对论平均场理论中的核子耦合参数分析[J]. 滁州学院学报,2011, 13(5)10: 45-47.

[27] Zhao Xian-Feng,   Jia Huan-Yu.   Mass of the neutron star PSR J1614-2230 [J]. Physical Review C,   2012, 85(6)6: 065806. (SCI, IF=3.308)

[28] Zhao Xian-Feng,   Dong Ai-Jun, Jia Huan-Yu. The mass calculations for the neutron star PSR   J1614-2230 [J]. Acta Physica Polonica B, 2012, 43(8)8: 1783-1789. (SCI,   IF=0.901)

[29] Zhao Xian-Feng,   Jia Huan-Yu. A set of new nucleon coupling constants and the proto neutron   star matter [J]. Chinese Physics B, 2012, 21(8)8: 089701. (SCI, IF=1.376)

[30] Zhao Xian-Feng,   Jia Huan-Yu. Constraints on the moment of inertia of a proto neutron star   from the hyperon coupling constants [J]. Journal of astrophysics and   astronomy, 2012, 33(3)9: 303-310. (SCI, IF=0.4)

[31]   Xian-Feng Zhao, Li Zhang. The Σ Well Depth and the Proto Neutron Star   Matter [J]. International Journal of Theoretical Physics, 2013, 52(2)2:   429-440.SCI, IF=0.845

[32] Zhao Xian-Feng,   Dong Ai-Jun, Jia Huan-Yu. Constraints on the transition density of a hyperon   star with a set of new nucleon coupling constants [J]. Chinese Journal of   Physics, 2013, 51(1)2:44-55. (SCI,   IF=0.448)

[33] Xian-Feng Zhao.   The surface gravitational redshift of the neutron star PSR J1614-2230 [J].  Acta Physica Polonica B, 2013,44(2)2:211-219. (SCI,   IF=0.901)

[34] Xian-Feng Zhao,   Huan-Yu Jia. Constraints the properties of neutron star matter from the mass   of neutron star PSR J1614-2230[J]. Astrophysics and Space Science, 2013,   346(1)7: 131-139. SCI, IF=1.686

[35] Xian-Feng Zhao.   The surface gravitational redshift of the neutron star 4U 1820-30[J]. Chinese   Journal of Physics, 2013, 51(5)10: 936-944. (SCI, IF=0.448)

[36] Xian-Feng Zhao,   Huan-Yu Jia. The surface gravitational redshift of the neutron star PSR   B2303+46 [J]. Bulletin of the Astronomical Society of India,   2013,41(4)12:291-298. (SCI, IF=0.31)

[37] Xian-Feng Zhao,   Huan-Yu Jia. The transition density of the large mass hyperon star [J].   Chinese Physics C, 2014, 38(1)1: 015101. (SCI,   IF=0.251)

[38] Xian-Feng Zhao,   Huan-Yu Jia. The surface gravitational redshift of the massive neutron star   PSR J0348+0432 [J]. Revista Mexicana de Astronomia y   Astrofisica, 2014,50(1)4:103-108 (SCI, IF=2.525)

[39] Xian-Feng Zhao,   Ai-Jun Dong, Huan-Yu Jia. The properties of the   neutron star PSR B2303+46[J]. Chinese Journal of Physics,   2014,52(2)4:679-690.  (SCI, IF=0.448)

[40] Xian-Feng Zhao.   Constraints the properties of the massive neutron star PSR J0348+0432 from   the mesons f0(975) and φ(1020)[J]. The European Physical Journal A,   2014,50(5)5:1-6. (SCI, IF=1.968)

[41] Xian-Feng Zhao.   The properties of the neutron star PSR J0348+0432[J]. International Journal   of Modern Physics D, 2015, 24(8)7: 1550058. (SCI, IF=1.963)

[42] Xian-Feng Zhao. Examination of the influence of the   f0(975) and φ(1020) mesons on the surface gravitational redshift of the   neutron star PSR J0348+0432 [J]. Physical Review C, 2015, 92(5)11: 055802. (SCI,   IF=3.146)

[43] Xian-Feng Zhao. The Hyperons in the Massive Neutron   Star PSR J0348+0432[J]. Chinese Journal of Physics, 2015, 53(6)11: 1-14. (SCI,   IF=0.464) 

[44] Xian-Feng Zhao.   On the moment of inertia of PSR J0348+0432 [J]. Chinese Journal of Physics,   2016, 54(5)10: 839-844. (SCI, IF=0.514)

[45] Xian-Feng Zhao,   Can the massive neutron star PSR J0348+0432 be hyperon star? [J].  Acta   Physica Polonica B, 2017, 48(2)2: 171-181. (SCI, IF=0.904)

[46] Xian-Feng Zhao, The moment of inertia of theneutron   star PSR J0348+0432 and its proto neutron star [J].  Astrophysics and   Space Science, 2017, 362(5)5:95. (SCI, IF=1.622)

[47] Xian-Feng Zhao,   Property difference between the neutron star PSR J0348+0432 and   its proto neutron star [J]. International Journal of Modern Physics D, 2017, 26(11)10: 1750133. (SCI, IF=1.963)

[48] Xian-Feng Zhao. Meson effect in the proto neutron star PSR J0348+0432 [J]. International Journal of Theoretical Physics, 2017, 56(10)10:3050–3060.    SCI, IF=0.845

[49] Xian-Feng Zhao.   Effect of entropy on properties of proto neutron star PSR J0348+0432 [J].   Chinese Journal of Physics, 2018, 56(7)8: 1648-1655. (SCI, IF=0.514)

[50] Xian-Feng Zhao. Effect   of the mesons on the baryons distribution in the massive NS PSR J0348+0432   [J]. Astrophysics and Space Science, 2019, 364(3)3: 38.(SCI, IF=1.622)

[51] Xian-Feng Zhao. The composition of baryon   in the proto neutron star PSR J0348+0432[J]. International Journal of   Theoretical Physics, 2019, 58(4)4, 1060-1070, SCI, IF=0.845

[52] Xian-Feng Zhao.   Effect of hyperon coupling constants on the properties of the massive neutron   star PSR J0348+0432 [J]. International Journal of Modern   Physics D, 2019, 28(11)11: 1950144. (SCI, IF=1.963)

[53] Xian-Feng Zhao.   The hyperon coupling constants and the surface gravitational redshift of   massive neutron stars [J]. Chinese Journal of Physics, 2020, 63:240-247. (SCI,   IF=0.514)

[54] Xian-Feng Zhao,   Rui Huang, Jian-Li Huo, Effect of nucleon coupling constants on properties of   proto neutron star PSR J0740+6620[J]. 2022, International Journal of Modern Physics D, 31(8)6, 2250062. (SCI, IF=1.963)

[55]   Zhao, Xian-Feng, Liu, Ting-Ping, Effect of hyperon interaction on   properties of proto neutron star PSR J0740+6620[J], 2022, European Physical Journal C, 82(8)8, 682. (SCI, IF=4.607)

[56] Xian-Feng Zhao,   Bin Tang, The Moment of Inertia of Proto Neutron Star PSR J0737-3039A[J].   2022, Brazilian   Journal Of Physics, 52(5)10, 149. (SCI, IF=1.018)

[57] Xian-Feng Zhao,   Zhen-Hai Wu, The Moment of Inertia of Proto-Neutron Star PSR J0740+6620[J].   2022, Acta Physica Polonica B, 53(8), 8-A1. (SCI,   IF=0.669)

[58] Xian-Feng Zhao,   The interaction between hyperons and the surface gravitational redshift of proto neutron star PSR J0740+6620[J]. 2022,   Contrib. Astron. Obs. Skalnaté Pleso, 52(2), 58-71. (SCI,   IF=0.595).

[59] Xian-Feng Zhao,   Shui-Rong Zhong, Jian-Li Huo, Properties of proto neutron star PSR   J0737-3039A[J]. 2022, Chinese Physics C, 46(10)10, 105102. (SCI, IF=2.145)

[60] Xian-Feng   Zhao, The role of hyperonic interactions in proto neutron stars[J].   2022, Int J Mod Phys E, 31(12)12, 2250101. (SCI,   IF=1.199)

[61]   Xian-Feng Zhao, Effect of the interaction between hyperons on the   moment of inertia of the proto neutron stars[J]. 2023, Astrophysics, 661):84-97. (SCI, IF=0.556)

[62]   Zhao, Xian-Feng, Huo, Jian-Li, Chen, Jian-Yong, Effect of nucleon   coupling constants on the mass radius ratio of proto neutron star PSR   J0737-3039A[J]. 2023, Modern Physics Letters A,  38(1)4: 2350004. (SCI, IF=1.594)

B 专著

1、赵先锋,贾焕玉. 中子星的相对论平均场理论研究[M]. 成都:西南交通大学出版社,2012.11.  ISBN978-7-5643-2052-2p1-179.

2、赵先锋. 大质量中子星研究[M]. 成都:四川大学出版社,2017.08. ISBN978-7-5690-1032-9p1-208. 206千字。

C 教材

1、赵先锋. 大学物理讲义 上册[M]. 成都:西南交通大学出版社,201512.

2、赵先锋. 大学物理讲义 下册[M]. 成都:西南交通大学出版社,201512.

*  获奖情况

12009年,被学校评为教学优秀奖

22008-2009年度,被学校评为教书育人先进个人,2010-07

32011年,被学校评为““五带头优秀共产党员2011-07

42010-2012年度,被学校评为教书育人先进个人,2012-06

520129月,被学校评为双能型教师;

62012年,被学校评为课堂教学优秀奖2013-12

 *  荣誉称号

1201412月,被学校评为“科技先进工作者”。

 *  讲授课程

1、大学物理(本科生)

2、近代物理选讲(本科生)

3、理论力学(本科生)

4、热力学统计物理学(本科生)

5、量子力学(本科生)

6、电动力学(本科生)

7、自然辩证法(硕士研究生)

 

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