个人简介

陈文聪，博士，河南省特聘教授，郑州大学硕士生导师，九三社员。安徽省太湖县人，2007年6月毕业于南京大学天文系天体物理专业，获理学博士学位。2011年12月北京大学核物理与核技术国家重点实验室物理学博士后出站。2016.01-2017.01 牛津大学物理系访问学者。 共发表SCI论文40余篇，其中在天体物理三大学术期刊Astrophysical Journal（IF：6.733)、Monthly Notices of the Royal Astronomical Society（IF：5.521）、Astronomy & Astrophysics（IF：5.084）发表论文27篇，被Nature等期刊引用300余次。主持完成国家自然科学基金面上项目2项、河南省科技创新人才（杰出青年）计划和河南省高校科技创新人才支持计划各1项，作为第一完成人获河南省高校科技成果一等奖1项，河南省自然科学学术奖优秀论文一等奖5项。目前主持国家自然科学基金重点项目子课题、国家自然科学基金面上项目和河南省高校科技创新团队支持计划各1项。

研究领域

脉冲星、X射线双星的时变特征及其演化规律。

主持科研项目 [1]《X射线双星的多波段研究》，国家自然科学基金重点项目子课题，11733009，分得经费80万元, 2018-2022 [2]《毫秒脉冲星双星形成和演化的研究》，国家自然科学基金面上项目，11573016，经费85+20万元, 2016-2019 [3]《星系X射线源的研究》，河南省高校科技创新团队支持计划，16IRTSTHN028，经费50+50万元, 2015-2017 [4]《致密星双星的前身星及其演化历史的研究》，国家自然科学基金面上项目，11173011，经费72+72万元, 2012-2015 [5]《毫秒脉冲星起源的研究》，河南省科技创新人才计划（杰出青年），114100510020, 经费30+30万元，2011-2013 [6]《脉冲星与含致密天体密近双星的演化》，国家自然科学基金面上项目，10873011，经费32+64万元, 2009-2011 [7]《致密天体与密近双星的研究》，河南省高校科技创新人才支持计划（第一层次），2009HASTIT011, 经费40万元, 2009-2010

近期论文

查看导师最新文章 （温馨提示：请注意重名现象，建议点开原文通过作者单位确认）

[1] L. Jiang, N. Wang*, W. C. Chen*, X. D. Li, W. M. Liu, Z. F. Gao, A strange star scenario for the formation of isolated millisecond pulsars, Astron Astrophys, 2020, 633, A45 [2] H. Shi, H. W. Hu, W. C. Chen*, Application of a two-dipole model to PSR J1640 –4631, a pulsar with an anomalous braking index, Publ. Astron. Soc. Japan, 2019, 71, L5 [3] W. C. Chen*, P. Podsiadlowski,Fast Orbital Shrinkage of Black Hole X-Ray Binaries Driven by Circumbinary Disks，Astrophys J Letters, 2019, 876, L11 [4] L. Jiang, W. C. Chen, X. D. Li, A strange dwarf scenario for the formation of the peculiar double white dwarf binary SDSS J125733.63+542850.5, Mon Not R Astron Soc，2018, 476, 109 [5] W. C. Chen*, Formation of Scorpius X-1 induced by anomalous magnetic braking of Ap/Bp stars, Astron Astrophys, 2017, 606, A60 [6] W. C. Chen*, P. Podsiadlowski, Rapid orbital decay in detached binaries: evidence for circumbinary disks, Astrophys J Letters, 2017, 837, L19 [7] L. Jiang, W. C. Chen, X. D. Li, A circumbinary disk scenario for the negative orbital-period derivative of the ultracompact X-Ray binary 4U 1820-303, Astrophys J, 2017, 837, 64 [8] W. C. Chen*, An evolutionary channel towards the accreting millisecond pulsar SAX J1808.4-3658, Mon Not R Astron Soc，2017,464, 4673 [9] W. C. Chen*, Constraining the dipolar magnetic field of M82 X-2 by the accretion model, Mon Not R Astron Soc，2017，465, L6 [10] W. C. Chen*, P. Podsiadlowski, Evolution of intermediate-mass X-ray binaries driven by magnetic braking of Ap/Bp stars. I. ultracompact X-ray binaries. Astrophys J, 2016, 830, 131 [11] W. C. Chen*, High braking index pulsar PSR J1640-4631: low-mass neutron star with a large inclination angle? Astron Astrophys, 2016, 593, L3 [12] W. C. Chen*, X. D. Li, Low braking index of PSR J1734−3333: an interaction between fall-back disc and magnetic field? Mon Not R Astron Soc，2016，455，L87-L90 [13] W. C. Chen*, X. D. Li, Orbital period decay of compact black hole X-ray binaries: the influence of circumbinary disks? Astron Astrophys, 2015, 583, A108 [14] W. M. Liu,W. C. Chen*, Magnetic braking of Ap/Bp stars: an alternative formation mechanism of compact intermediate-mass binary pulsars, Mon Not R Astron Soc, 2014，441, 3615 [15] W. C. Chen*, W. M. Liu, Evolution of neutron star + He star binaries: an alternative evolutionary channel to intermediate-mass binary pulsars，Mon Not R Astron Soc, 2013，432, L75 [16] W. M. Liu,W. C. Chen*, On the progenitors of millisecond pulsars by the recycl- ing evolutionary channel, Mon Not R Astron Soc, 2011, 416,2285 [17] W. C. Chen*, X. D. Li, R. X. Xu, He star evolutionary channel to intermediate-mass binary pulsar PSR J1802-2124, Astron Astrophys, 2011, 530, A104 [18] W. C. Chen*, J. A. Panei, The progenitor of binary millisecond radio pulsar PSR J1713+0747, Astron Astrophys, 2011, 527, A128 [19] W. C. Chen*, X. W. Liu, R. X. Xu, X. D. Li, Can eccentric binary millisecond pulsars form by accretion-induced collapse of white dwarfs? Mon Not R Astron Soc, 2011, 410, 1441 [20] Meng, X. C.*, Chen, W. C., Yang, W. M., Li, Z. M., The birth rate of subluminous and overluminous type Ia supernovae,Astron Astrophys. 2011, 525, A129 [21] W. M. Liu,W. C. Chen*, B. Wang, Z. W. Han, Helium-star evolutionary channel to super-Chandrasekhar mass type Ia supernovae, Astron Astrophys, 2010, 523, A3 [22] W. C. Chen*, X. D. Li, On the progenitors of super-Chandrasekhar mass type Ia supernovae, Astrophys J, 2009, 702, 686 [23] W. C. Chen*, Can angular momentum loss cause the period change of NN Ser? Astron Astrophys, 2009, 499, L1 [24]W. C. Chen*, X. D. Li, Evolving to Type Ia Supernovae with long delay times, Astrophys J, 2007, 658, L51 [25] W. C. Chen*, X. D. Li, Evolution of black-hole intermediate-mass X-ray binaries: the influence of a circumbinary disc, Mon Not R Astron Soc, 2006, 373，305 [26] W. C. Chen*, X. D. Li, and Qian S. B., Orbital Evolution of Algol Binaries with a Circumbinary Disk， Astrophys J, 2006, 649，973 [27] W. C. Chen*, X. D. Li, Why the braking indices of young pulsars are less than 3? Astron Astrophys, 2006, 450, L1 [28] W. C. Chen*, X. D. Li, Z. R. Wang，Low-Mass X-Ray Binary as the Progenitor of PSR J1713+0747, Publ Astron Soc Jpn，2006, 58，153

学术兼职

现为河南省学术技术带头人，国家自然科学基金通讯评审专家, 河南省优秀青年科技专家，河南省教学标兵, 河南省物理学会常务理事、河南省物理学专业教学指导委员会副主任。中国天文学会、中国物理学会会员