導(dǎo)師信息

（1）國(guó)家自然科學(xué)基金項(xiàng)目（應(yīng)急管理項(xiàng)目-理論物理專(zhuān)款），相對(duì)論平均場(chǎng)理論對(duì)大質(zhì)量中子星的研究，11447003，2015.01-2017.12，主持，已結(jié)題

（2）省級(jí)高校省級(jí)自然科學(xué)研究重點(diǎn)項(xiàng)目，大質(zhì)量中子星PSR J0348+0432 的相對(duì)論平均場(chǎng)理論研究，KJ2014A182，2014.1-2016.12，主持，已結(jié)題

（3）省級(jí)自然科學(xué)基金面上項(xiàng)目，相對(duì)論平均場(chǎng)理論在中子星物質(zhì)研究中的應(yīng)用，1208085MA09，2012.07—2014.06，主持，已結(jié)題

（4）省級(jí)高校省級(jí)自然科學(xué)研究項(xiàng)目，中子星PSR J1614-2230等致密天體的相對(duì)論平均場(chǎng)描述，KJ2012Z297，2012.1-2012.12，主持，已結(jié)題

（5）省級(jí)高校省級(jí)自然科學(xué)研究項(xiàng)目，慢旋轉(zhuǎn)中子星轉(zhuǎn)動(dòng)慣量的研究，KJ2009B106，2009.1-2010.09，主持，已結(jié)題

（6）校級(jí)科學(xué)研究項(xiàng)目，奇異介子對(duì)慢旋轉(zhuǎn)中子星轉(zhuǎn)動(dòng)慣量的影響，2008kj019B，2009.01-2009.12，主持，已結(jié)題

A 論文

[1] 趙先鋒，洪時(shí)明，劉福生. 壓力對(duì)碳?xì)溲醭R界流體中碳的溶解度的影響[J]. 高壓物理學(xué)報(bào), 2003,17(2):101-105. （EI）

[2] 趙先鋒. 相對(duì)運(yùn)動(dòng)的矢量圖示解法 [J]. 數(shù)學(xué).力學(xué).物理學(xué).高新技術(shù)研究進(jìn)展, 2006,11:366-368.

[3] 趙先鋒, 王順金, 張華, 賈煥玉. 和介子對(duì)中子星物質(zhì)的影響 [J]. 高能物理與核物理,   2007, 31 (4): 345-349. （SCI）

[4] 趙先鋒, 王順金, 張華, 賈煥玉. 和介子對(duì)有限溫度中子星物質(zhì)的影響 [J]. 高能物理與核物理,   2007, 31 (6): 532-537. （SCI）

[5] 趙先鋒. 非平行平面薄膜反射光干涉公式的推導(dǎo)[J]. 滁州學(xué)院學(xué)報(bào), 2009,11(1):53-54.

[6] 趙先鋒, 王順金, 張華, 賈煥玉. 和介子對(duì)中子星轉(zhuǎn)動(dòng)慣量的影響 [J]. 四川大學(xué)學(xué)報(bào) (自然科學(xué)版),   2009, 46 (3)5: 743-747.

[7] 趙先鋒, 張華. 溫度對(duì)前身中子星轉(zhuǎn)動(dòng)慣量的影響   [J]. 四川大學(xué)學(xué)報(bào) (自然科學(xué)版), 2010, 47 (3)5 : 579-584.

[8] 趙先鋒. 物理學(xué)史料在大學(xué)物理教學(xué)中的作用[J]. 滁州學(xué)院學(xué)報(bào), 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] 趙先鋒, 張華. 自相互作用對(duì)超子星轉(zhuǎn)變密度的影響 [J]   . 山東大學(xué)學(xué)報(bào) (理學(xué)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 U_Σ^(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]. 天文學(xué)報(bào), 2011，52(2)3: 126-135.

[17] 趙先鋒. 相對(duì)論平均場(chǎng)理論中耦合常數(shù)g_ρ的確定與研究   [J]. 中山大學(xué)學(xué)報(bào) (自然科學(xué)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] 趙先鋒, 張華.    超子同位旋相互作用對(duì)中子星轉(zhuǎn)動(dòng)慣量的影響 [J]. 云南大學(xué)學(xué)報(bào) (自然科學(xué)版)，2011, 33(3)5: 303-307.

[20] 趙先鋒, 張華. 超子同位旋相互作用能對(duì)超子星轉(zhuǎn)變密度的影響 [J]. 吉林大學(xué)學(xué)報(bào) (理學(xué)版), 2011, 49(3)5: 528-532.

[21] 趙先鋒. 變重力加速度對(duì)自由落體落地速度的影響[J]. 滁州學(xué)院學(xué)報(bào), 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月): 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] 趙先鋒，方春陽(yáng)，王大樹(shù)，汪杰. 相對(duì)論平均場(chǎng)理論中的核子耦合參數(shù)分析[J]. 滁州學(xué)院學(xué)報(bào)，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, 66（1）：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 專(zhuān)著

1、趙先鋒，賈煥玉. 中子星的相對(duì)論平均場(chǎng)理論研究[M]. 成都：西南交通大學(xué)出版社，2012.11.  ISBN：978-7-5643-2052-2，p1-179.

2、趙先鋒. 大質(zhì)量中子星研究[M]. 成都：四川大學(xué)出版社，2017.08. ISBN：978-7-5690-1032-9，p1-208. 206千字。

C 教材

1、趙先鋒. 大學(xué)物理講義 上冊(cè)[M]. 成都：西南交通大學(xué)出版社，2015年12月.

2、趙先鋒. 大學(xué)物理講義 下冊(cè)[M]. 成都：西南交通大學(xué)出版社，2015年12月.

1、2009年，被學(xué)校評(píng)為“教學(xué)優(yōu)秀獎(jiǎng)”；

2、2008-2009年度，被學(xué)校評(píng)為“教書(shū)育人”先進(jìn)個(gè)人，2010-07；

3、2011年，被學(xué)校評(píng)為““五帶頭”優(yōu)秀共產(chǎn)黨員”，2011-07；

4、2010-2012年度，被學(xué)校評(píng)為“教書(shū)育人”先進(jìn)個(gè)人，2012-06；

5、2012年9月，被學(xué)校評(píng)為“雙能型”教師；

6、2012年，被學(xué)校評(píng)為“課堂教學(xué)優(yōu)秀獎(jiǎng)”，2013-12；

1、2014年12月，被學(xué)校評(píng)為“科技先進(jìn)工作者”。

1、大學(xué)物理（本科生）

2、近代物理選講（本科生）

3、理論力學(xué)（本科生）

4、熱力學(xué)統(tǒng)計(jì)物理學(xué)（本科生）

5、量子力學(xué)（本科生）

6、電動(dòng)力學(xué)（本科生）

7、自然辯證法（碩士研究生）