更新时间：2023-04-29 11:14
张波，男，1957年3月出生，1980 年1月重庆师范学院物理系毕业， 1984 年 9 月考取河北师范大学物理系硕士研究生，1987年7月毕业。1987年开始在河北师范大学物理系任教。理论物理专业博士研究生导师，校学术带头人，一档教授，理论物理研究所所长。中科院国家天文台博士生导师，中国天文学会理事，国际天文联合会（IAU）会员，中国高等科技中心协联成员。
先后讲授过恒星物理，恒星大气物理，天体物理中的辐射机制、广义相对论、核天体物理、电动力学、电动力学（II）等多门课程。
张波教授现已招收16届全日制硕士研究生，已毕业32名，其中16名考取博士研究生。作为中科院国家天文台博士生导师，指导天文台博士生1名并已取得博士学位。作为理论物理专业博士生导师，指导博士生2名。
核天体物理是物理学与天体物理的重要交叉学科，其内容涉及天体物理学中恒星的演化、双星的演化、星系的化学演化、物理学中的原子物理学、原子核物理学等多个学科，研究手段包括理论计算和天文观测。事实上，宇宙中各种天体中的核合成是理论物理和原子核物理的天然实验场。自20世纪90年代以来，随着大口径望远镜的投入使用，使得人们对暗弱天体的观测成为可能，并积累了一批不同金属丰度和不同演化阶段的恒星的化学丰度资料，为恒星重元素核合成及中子俘获元素丰度的研究提供了必要的天文观测数据，也使得这方面的研究再次成为天体物理学的热点课题。张波教授主要研究核天体物理中与恒星演化相关的中子俘获元素的丰度和核合成问题，对它的研究既可了解自然界中各种原子核的来源，又可得到各种原子核性质方面的相关信息。其特色在于把基础理论研究和实验及观测数据的唯象分析相结合，重点研究核天体物理中的新现象新物理，在某些关键点上取得进展。研究内容主要包括四个方面：
（1）AGB星s-过程核合成；
（2）钡星系统轨道根数及s-过程元素丰度分布规律；
（3）恒星中子俘获元素丰度分布及星系化学演化；
（4）r-过程核合成场所及元素丰度分布规律。
1国家自然科学基金面上项目：贫金属环境中子俘获过程相关元素丰度分布特征及物理关联的整体研究
（批准号：10973006，2010-2012，主持人：张波，主研人：李冀、崔文元、张江、杨大卫；40万元）
2国家自然科学基金面上项目：铅星和s+r星的产生原因及形成机制探究
（批准号：10673002，2007-2009，主持人：张波，主研人：李冀、杨大卫；26万元）
3国家自然科学基金面上项目：AGB星s-过程核合成与中子辐照量分布函数
（批准号：10373005，2004-2006，主持人：张波，主研人：杨大卫；25万元）
4国家自然科学基金面上项目：中子俘获元素的丰度分布和星系化学演化
（批准号：19973002，2000-2002，主持人：张波，主研人：李冀、杨大卫；12万元）
5国家自然科学基金面上项目：矮造父变星周期的变化与变星内部核合成
（批准号：19673008，1997-1999，主持人：杨大卫，主研人：张波；4万元）
6国家自然科学基金天文联合基金面上项目：银盘恒星的化学丰度与运动学和年龄的关系
（批准号：10778616，2007-2009，主持人：李冀，主研人：张波、杨大卫；24万元）
[1] A model for calculating the abundances of neutron -capture elements in metal-poor stars
The Astrophysical Journal, 1999, 513: 910-918
Zhang Bo, Li Ji, Zhang Caixia, Liang Yanchun, Peng Qiuhe
[2] Neutron Capture Elements in the s- and r-Process-Rich Stars: Constraints on Neutron-Capture Nucleosynthesis Processes
The Astrophysical Journal，2006,642:1075-1081
Zhang Bo, Ma Kun, Zhou Guide
[3] Investigation for the Puzzling Abundance Pattern of the Neutron-Capture Elements in the Ultra Metal-Poor Star: CS 30322-023
The Astrophysical Journal, 2007, 657:1037-1041
Cui Wenyuan, Zhang Bo, Ma Kun, Zhang Lu
[4] Investigation for the Enrichment Pattern of the Elements Abundances in r+s Star HE 0338-3945: A Special r-II Star？
The Astrophysical Journal, 2010, 708: 51-57
Cui Wenyuan, Zhang Jiang, Zhu Zizhong, Zhang Bo
[5] The oxygen abundance calibrations and N/O abundance ratios of 40000 SDSS star-forming galaxies
The Astrophysical Journal, 2006, 652:257-269
Liang Yanchun, Yin Shaoying，F.Hammer, Deng Licai，H.Flores, Zhang Bo
[6] The heavy-element abundances of AGB Stars and the angular conservation model of wind accretion for barium stars
Astronomy and Astrophysics,2000，363: 555-567
Liang Yanchun, Zhao Gang, Zhang Bo
[7] Orbital elements of barium stars formed through a wind accretion scenario.
Astronomy and Astrophysics,2000，363: 660-666
Liu Junhong, Zhang Bo, Liang Yanchun, Peng Qiuhe
[8] Chemical compositions of four barium stars.
Astronomy and Astrophysics,2003，397: 257-265
Liang Yanchun, Zhao Gang ,Chen Yuqin, Qiu Hong-mei, Zhang Bo
[9] Empirical strong-line oxygen abundance calibrations from galaxies with electron-temperature measurements
Astronomy and Astrophysics,2007, 462: 535-546
Yin Shaoying, Liang Yanchun，F.Hammer,J.Brinchmann, Zhang Bo, Deng Licai，H.Flores
[10] The origin of the lead-rich stars in the Galactic Halo: investigation of the model parameters for the s-process .
Monthly Notices of the Royal Astronomical Society, 2006,368:305-309
Cui Wenyuan, Zhang Bo
[11] Investigation of the single neutron exposure model for the s-process: the primary nature of the neutron source.
Monthly Notices of the Royal Astronomical Society, 2007, 375:1418-1422
Ma Kun, Cui Wenyuan, Zhang Bo
[12] Study of Isotopic Fractions and Abundances of the Neutron-capture Elements in HD175305
Monthly Notices of the Royal Astronomical Society, 2009, in press
Zhang Jiang, Cui Wenyuan, Zhang Bo
[13] Evolution of the distribution of neutron exposures in the Galaxy disc: an analytical model
Journal of Astronomy and Astrophysics, 2007, 28:1-12
Cui Wenyuan, Zhang Weijuan，Zhang Bo
[14]Two r-process components in ultra-metal-poor stars:the neutron-capture element distribution of CS 22892-052.
Astrophysics and Space Science, 2002, 280:325-336.
Zhang Bo, Li Ji, Wang Yuexiang, Zhang Yanxia, Liu Junhong, Peng Qiuhe
[15] The yields of r- process elements and chemical evolution of the Galaxy.
Astrophysics and Space Science, 2006, 306:33-39
Chen Zhe，Zhang Jiang，Chen Yanping，Cui Wenyuan，Zhang Bo
[16] Orbital elements of the mild and strong barium stars formed through a wind accretion scenario
Astrophysics and Space Science, 2008, 314: 351-359
Cui Wenyuan，Zhang Bo, Quan Yamin, Zhou Guide, Chen Yanping
[17] Abundances of heavy elements in ultra-metal poor star CS22892-52
= 极贫金属星CS 22892-052的重元素丰度研究.
Science in China（A）,1999,42:401-406.=中国科学(A辑), 1998, 28:1102-1106.
Zhang Bo,Zhang Caixia, Li Ji, Liang Yanchun, Peng Qiuhe
[18] Correlativity of nucleosynthesis in low-mass AGB stars=
= 低质量 AGB 星核合成事件的相关性研究
Science in China（A）, 1996,39:1112-1120.=中国科学(A辑), 1996,26: 1050-1156.
Liu Yongxin，Zhang Bo,, Peng Qiuhe
[19] Inverse Correlation of abundances in AGB Stars.
Chinese Physics Letters, 1998, 15: 76-78.
Zhang Bo,Liu Junhong, Liang Yanchun, Peng Qiuhe
[20] Abundances of elements in metal-poor star HD 126238.
Chinese Physics Letters, 1999, 16.619-621.
Li Ji, Zhang Bo, Wei Guoqiang,Zhang Liping,, Peng Qiuhe
[21] Abundances distribution of slow-process main heavy elements in AGB stars.
Chinese Physics Letters 2003, 20.962-964.
Zhang Miaojing, Zhang Bo,Li Guanglie
[22] R-Process Nucleosynthesis and Galactic Chemical Evolution of the Ba Peak Elements.
Chinese Physics Letters, 2003,20：2084-2087.
Song Hanfeng, Zhang Bo, Zhang Jiang, Wu Haibin, Peng Qiuhe
[23] Neutron Capture Elements in the Double Enhenced Star HE1305-0007: a new s- and r-Process Paradigm.
Chinese Physics Letters, 2007,24：1417-1420.
Cui Wenyuan, Cui Dongnuan, Du Yunshuang, Zhang Bo
[24] Mass Fraction of C-Pocket in Metal-Poor AGB Stars and the Primary Nature of Neutron Source
Chinese Physics Letters, 2009,26：039701, 1-4
Cui Dongnuan, Geng Yuanyuan, Cui Wenyuan, Zhang Bo
[25] Galactic chemical evolution of the lighter neutron capture elements Sr,Y,Zr.
Chinese Journal of Astronomy and Astrophysics,2003,5:431-442.
Du Cui-hua，Zhang Bo, Song Hanfeng, Peng Qiuhe
[26]New variable stars discovered as by-product of the Beijing Astronomical Observatory Supernova survey
Chinese Journal of Astronomy and Astrophysics,2002,2:463-473.
Kong Minzhi，Qiu Yulei，Shen Chuanjian,Deng Jinsong,Zhang Bo
[27] A statistical model for predicting the average abundances patterns of the heavy elements in metal-poor-stars
Chinese Journal of Astronomy and Astrophysics,2002,2:429-440
Zhang Bo, Zhang Yan-xia,Li Ji, Peng Qiuhe
[28] The Distributions of Neutron Exposures in AGB stars and the Galaxy
Chinese Journal of Astronomy and Astrophysics,2007,7:224-233
Wen–YuanCui,Feng–HuaZhang,Wei–JuanZhang,LuZhang,BoZhang.
[29] Model of wind accretion in extrinsic AGB stars under conservation of total angular momentum
= 外赋AGB星星风吸积的角动量守恒模型.
Chinese Astronomy and Astrophysics,1999,23:189-194=天文学报,1998,39:424-429.
Zhang Bo, Liu Junhong, Liang Yanchun, Peng Qiuhe
[30] A methed of evaluating abundances of heavy elements in metal-poor stars
= 一种研究贫金属星重元素丰度分布的方法.
Chinese Astronomy and Astrophysics, 2000,24:88-94=天文学报,1999,40:256-262.
Zhang Bo,Li Ji, Zhang Caixia, Liang Yanchun, Peng Qiuhe
[31] The abundance distribution of Neutron-capture elements in metal Poor stars
= 贫金属星中子俘获元素丰度分布
Chinese Astronomy and Astrophysics, 2001,25:298-304=天文学报,2001,42:22-28.
Zhang Bo, Zhang Yanxia, Liu Junhong, Li Ji, Peng Qiuhe
[32] The nucleosynthesis of elements in low-mass AGB stars= 低质量 AGB 星重元素的核合成.
Chinese Astronomy and Astrophysics,1997,21:59-69=天文学报,1996,37:243-253.
Wang Xinge, Zhang Bo, Peng Qiuhe
[33] Monte Carlo simulations of the orbital elements and abundances of Barium stars
= 钡星系统轨道根数及丰度分布的Monte-Carlo模拟计算.
Chinese Astronomy and Astrophysics,2003,27:292-302=天文学报，2003，44:116-125.
Shi Weibin, Niu Ping, Zhang Bo, Liu Junhong, Peng Qiuhe
[34] Evolution of the s-element abundances of 3M⊙ asymptotic giant branch stars
= 3 M⊙AGB 星表面重元素丰度的演化.
Chinese Astronomy and Astrophysics, 1998,22:49-55.=天文学报, 1997,38:232-238.
Zhang Bo, Chang Ruixiang, Peng Qiuhe
[35] A new formula for computing mean neutron exposure = 计算平均中子辐照量的新公式
Chinese Astronomy and Astrophysics, 2008, 32:369-379.=天文学报, 2008, 49: 133-143
Zhang Fenghua, Zhou Guide, Zhang Bo
[36] The color-magnitude relation of disk galaxies= 盘状星系的颜色星等关系
Chinese Astronomy and Astrophysics, 2007, 31:236-243 =天文学报, 2007, 48: 11-17
Wu Haibin, Liu Chengze, Zhang Bo, Chang Ruixiang
[37] The overbundance of s-process elements in Ba stars through wind accretion
= 星风吸积引起的钡星重元素超丰.
Chinese Astronomy and Astrophysics, 1997,21:453-460=天体物理学报,1997,17:284-290.
Chang Ruixiang, Zhang Bo, Peng Qiuhe
[38]The average abundance of heavy elements in metal poor stars in different metallicity ranges
=贫金属星中子俘获元素平均丰度的金属丰度分区研究.
Chinese Astronomy and Astrophysics, 2001,25:187-193=天体物理学报,2000,20:277-284.
Zhang Yanxia, Zhang Bo, Li Ji, Liu Junhong, Peng Qiuhe
[39] Period variation of x-ray pulsars and Kelvin-Helmholtz instability at the accretion disk boundary
= X-射线脉冲星周期的变化与吸积盘的K-H不稳定性.
Chinese Astronomy and Astrophysics,1989,13:366-372=天体物理学报,1989,9:244-250.
Zhang Bo, Ge Yunzao
[40] Nucleosynthesis of fluorine in low-mass AGB stars during the thermal pulse phase
= 小质量AGB星热脉冲阶段氟的核合成.
Chinese Astronomy and Astrophysics,1996,20:231-238=天体物理学报,1996,16:58-64
Liu Yongxing, Zhang Bo, Peng Qiuhe
[41] Ba星星风吸积机制的再研究. 天体物理学报,1999,19:213-219. 梁艳春, 张波，彭秋和
[42]贫金属星的表面元素丰度与慢中子俘获过程.高能物理与核物理,2003，27：304-308.张妙静,张波,厉光烈
[43]太阳系元素丰度与AGB星慢中子俘获元素.高能物理与核物理,2003，27：978-983。张妙静,张波,厉光烈
[44]贫金属星的中子俘获元素. 高能物理与核物理,2004，28：30-36.张妙静,张波,厉光烈
[45] AGB星演化过程中的核合成. 原子核物理评论,2002,13：321-328. 张妙静,张波,厉光烈
[46] AGB 星核合成理论的研究进展. 天文学进展,1996,14:275-285. 张波,常瑞香，彭秋和
[47]贫金属星中子俘获元素丰度. 天文学进展.2000,18:238-248. 张波，李冀，张彦霞，彭秋和
[48] AGB 星s-过程核合成相关问题的研究进展. 天文学进展 2006,24:54-61.张波，崔文元