(1)趙先鋒,洪時明,劉福生. 壓力對碳?xì)溲醭R界流體中碳的溶解度的影響[J]. 高壓物理學(xué)報, 2003,17(2):101-105. (EI) (2)趙先鋒. 相對運(yùn)動的矢量圖示解法 [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, 2009,11(1):53-54. (6)趙先鋒, 王順金, 張華, 賈煥玉. 和 介子對中子星轉(zhuǎn)動慣量的影響 [J]. 四川大學(xué)學(xué)報 (自然科學(xué)版), 2009, 46 (3): 743-747. (7)趙先鋒, 張華. 溫度對前身中子星轉(zhuǎn)動慣量的影響 [J]. 四川大學(xué)學(xué)報 (自然科學(xué)版), 2010, 47 (3) : 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, 2010,12(2):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): 825-830. (10)趙先鋒, 張華. 自相互作用對超子星轉(zhuǎn)變密度的影響 [J] . 山東大學(xué)學(xué)報 (理學(xué)版), 2010, 45 (9): 96-100. (11)Zhao Xian-Feng. The gravitational redshift of a proto neutron star [J]. Chinese Physics Letters, 2010, 27 (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): 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): 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): 139–144.(SCI, IF=1.686) (15)Zhao Xian-Feng. Effects of and mesons on surface redshift of a neutron star [J]. Chinese Physics B, 2011, 20 (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, 2011,52(2): 126-135. 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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): 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): 391-399. (SCI, IF=0.4) (26)趙先鋒,方春陽,王大樹,汪杰. 相對論平均場理論中的核子耦合參數(shù)分析[J]. 滁州學(xué)院學(xué)報,2011, 13(5): 45-47. (27)Zhao Xian-Feng, Jia Huan-Yu. Mass of the neutron star PSR J1614-2230 [J]. Physical Review C, 2012, 85(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): 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): 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): 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): 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):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):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): 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): 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):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): 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):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):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):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): 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): 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): 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): 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):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]: 1648-1655. (SCI, IF=0.514) (50)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) (51)Xian-Feng Zhao. Effect of the mesons on the baryons distribution in the massie NS PSR J0348+0432 [J]. Astrophysics and Space Science, 2019, 364: 38 (SCI, IF=1.622)
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