理論研究室以天體物理學(xué)為主攻方向形成了較為合理的學(xué)術(shù)梯隊，共有科研人員4人，其中副研究員1名(碩士研究生導(dǎo)師)、助理研究員3名。研究領(lǐng)域涵蓋了行星物理、規(guī)范場理論、伽馬射線雙星、中子星物理等。主要開展太陽系以及行星系統(tǒng)形成與演化研究；新的規(guī)范方法模型研究；伽馬射線雙星高能輻射的產(chǎn)生機制研究；中子星物態(tài)與內(nèi)部結(jié)構(gòu)的研究。已發(fā)表SCI論文50余篇，EI及核心論文20余篇；主持國家和省部級項目10余項。
研究方向
1、行星物理
結(jié)合太陽系小天體物理性質(zhì)的觀測與統(tǒng)計分析結(jié)果，開展小天體碰撞演化基礎(chǔ)理論與數(shù)值模擬研究；同時開展行星形成與演化研究，重點開展行星系統(tǒng)形成與恒星環(huán)境關(guān)系等相關(guān)課題。
2、規(guī)范方法
開展新的規(guī)范方法模型研究，逐步推進(jìn)用于解決幾何化電磁力的難題，重點開展大統(tǒng)一理論的研究。
3、伽馬雙星演化
開展伽馬射線雙星高能輻射的產(chǎn)生機制研究，逐步推進(jìn)激波區(qū)域粒子的加速機制的研究。
4、中子星物理
開展中子星物態(tài)與內(nèi)部結(jié)構(gòu)的研究，逐步推進(jìn)中子星內(nèi)奇異物質(zhì)和星體熱演化性質(zhì)的研究；重點開展利用脈沖星、引力波等觀測數(shù)據(jù)限制中子星質(zhì)量、轉(zhuǎn)動慣量等宏觀性質(zhì)的研究。
主要設(shè)備
PowerEdge R730/R740 2U機架式服務(wù)器。
科研成果
[1] Cui Dou-Xing. “A Variant of the Hori-Lie Series Method”, Mech. Dynam. Astron. 35, 89, 1985.
[2] Cui Dou-Xing, Huang Tian-Yi. “A Numerical Method for Differential Equations of Second Order”, Mech. Dynam. Astron. 55, 405, 1993.
[3] Cui Dou-Xing. “Gravitational theory based on relativistic mechanics”, Int. J. Theor. Phys. 35, 1473, 1996.
[4] 崔斗星, 高階微商的一個恒等式, 大學(xué)數(shù)學(xué), 1998.
[5] Cui Dou-Xing, Zhao You, “The improvement of Changchun satellite laser ranging system”，Proceedings of SPIE, 3501, 453, 1998.
[6] 劉承志.長春人衛(wèi)站衛(wèi)星激光測距系統(tǒng)實現(xiàn)白天觀測所面臨的問題及解決方案.中國天文學(xué)會第一屆學(xué)術(shù)年會，1999.
[7] 劉承志， 崔斗星. 天文動力學(xué)方程數(shù)值積分中的一種有效變步法. 天文學(xué), 43, 387, 2002.
[8] Liu Cheng-Zhi, Zhao You, FanCun-Bo, Cui Dou-Xing, Han Xing-Wei and Yang Fu-Min. “Performance and observation summary of Changchun Satellite Laser Ranging Station”, Chin. Sci. Bull. 47, 1070, 2002.
[9] Liu Cheng-Zhi, ZhaoYou, Fan Cun-Bo, Han Xing-Wei, Zhang Xing-Hua, Shi Jian-Yong and Zhang Hai-Tao. “The Performance Of Changchun SLR Station, Proceeding of 14th International Workshop on Laser Ranging”. July 2004. Spain.
[10]LiuCheng-Zhi. “Atmospheric Refraction and Center-of-Mass Correction”.The 3rd ROK-PRC Optics Technology Workshop. March 2006. Korea.
[11]Liu Cheng-Zhi, Han Xing-Wei, Song Qing-Li, Fan Cun-Bo and Zhang Zi-Ang. “Progress in KHz SLR and Daylight tracking at Changchun Station”. Proceedings of 12.th International Workshop on Laser Ranging.
[12]趙罡、趙有、孫明國、于歡歡. “利用LAGEOS數(shù)據(jù)評價衛(wèi)星激光測距站觀測水平”，第十六屆國際激光測距會議, 2008.
[13]Xu Yan, Liu Guang-Zhou, Wu Yao-Rui, Zhu Ming-Feng, Yu Zi, Wang Hong-Yan, Zhao En-Guang.“Direct Urca processes with hyperon in cooling neutron star”, Chin. Phys. Lett. 28, 079701, 2011.
[14]Xu Yan, Liu Guang-Zhou, Wu Yao-Rui, Wang Hong-Yan, Zhang Feng. “Influence of L hyperons 1S0superfluidity on the direct Urca processes with hyperons”, Commun. Theor. Phys. 56, 521, 2011.
[15]梁智鵬, 劉承志, 范存波, 孫明國.兩行根數(shù)輔助的SLR單站定軌, 天文學(xué)報, 53,137,2012.
[16]Liang Zhi-peng, Liu Cheng-zhi, Fan Cun-bo and Sun Ming-guo, “TLE-Aided Orbit Determination Using Single-station SLR Data”, Chin. Astron. Astrophys.36, 417, 2012.
[17]Zhang Xiao-Jun, Wang Hai-Hua, Liu Cheng-Zhi, Han Xing-Wei, Fan Cun-Bo, Wu Jin-Hui and Gao Jin-Yue. “Direct conversion of slow light into a stationary light pulse”, Phys. Rev. A 86, 023821, 2012.
[18]Xu Yan, Liu Guang-Zhou, Wu Yao-Rui, Zhu Ming-Feng, Yu Zi, Wang Hong-Yan and Zhao En-Guang.“The effect of delta meson on the neutron star cooling”, Plasma Sci.Technol. 14, 375, 2012.
[19]Xu Yan, Liu Guang-Zhou, Wang Hong-Yan, Ding Wen-Bo and Zhao En-Guang.“Influence of σ* and ？ Mesons on Λ Hyperon 1S0 Superfluidity in Neutron Star Matter”, Chin.Phys.Lett. 29, 059701, 2012.
[20]Zhang Xiao-Jun, Wang Hai-Hua, Wang Zeng-Bin，Dong Xue, Wang Lei, Han Li-Li, Xu Yan, Liu Cheng-Zhi, Fan Cun-Bo and Gao Jin-Yue “Tunable reflection based on electromagnetically induced transparency”, J. Opt. Soc. Am. B 30,1095 ,2013.
[21]Han Li-Li, Zhang Xiao-Jun, Liu Cheng-Zhi, Fan Cun-Bo, Han Xing-Wei, Wu Jin-Hui and Gao Jin-Yue, “Controlled Photonic Stop Bands in a Four-Level Atomic System of an Inhomogeneously Broadened Solid”, Chin. Phys. Lett. 30, 034203, 2013.
[22]Xu Yan, Liu Guang-Zhou, Liu Cheng-Zhi, Fan Cun-Bo, Han Xing-Wei,Zhu Ming-Feng Wang Hong-Yan and Zhang Xiao-Jun. “1S0 nucleon superfluidity in neutron star matter”, Chin.Phys.Lett. 30, 062101, 2013.
[23]Xu Yan, Liu Guang-Zhou, Liu Cheng-Zhi, Fan Cun-Bo, Wang Hong-Yan, Zhu Ming-Feng, ZhaoEn-Guang.“The Nucleon Direct Urca Processes in a Cooling Neutron Star”, Chin.Phys.Lett. 30, 129501, 2013.
[24]Wang Hong-Yan, Liu Guang-Zhou, Wu Yao-Rui, Xu Yan, Zhu Ming-Feng, BaoTmurbagan, Zhao En-Guang. “Bulk Properties of Hybrid Stars with the Color-Flavor Locked Quark Matter Core”, Chin. Phys. Lett. 30, 061201, 2013.
[25]Wang Hong-Yan, Liu Guang-Zhou, Wu Yao-Rui, Xu Yan, Zhu Ming-Feng, BaoTmurbagan. “The third family of compact stars with the color-flavor locked quark core”, Chin.Sci.Bull. 58, 3731, 2013.
[26]Xu Yan, Liu Guang-Zhou, Liu Cheng-Zhi, Fan Cun-Bo, Han Xing-Wei, Zhang Xiao-Jun, Wang Hong-Yan,Zhu Ming-Feng and Meng Yu. “Direct Urca processes involving hyperons in neutron star matter”, Chin.Sci.Bull. 59, 273, 2014.
[27]Sui Ning, Li Min, He Ping.“Statistical computation of Boltzmann entropy and estimation of the optimal probability density function from statistical sample”, Mon. Not. R. Astron. Soc. 445 , 4211, 2014.
[28][軟件著作權(quán)登記] 中國科學(xué)院國家天文臺長春人造衛(wèi)星觀測站,空間非合作目標(biāo)優(yōu)選預(yù)報程序V1.0,計算機軟件著作權(quán)登記證書,軟著登字第0910592號,登記號2015SR023510
[29]Zhang Xiao-Jun, Wang Hai-Hua, Liang Zhi-Peng, Xu Yan, Fan Cun-Bo, Liu Cheng-Zhi and Gao Jin-Yue. “Goos-Hanchen shift in a standing-wave-coupled electromagnetically-induced-transparency medium”, Phys.Rev. A 91, 033831, 2015.
[30]Li Min, Li Xiang “Masses of discs form from collapse of molecular cloud cores”,Mon. Not. R. Astron. Soc. 449, 2259, 2015.
[31]Xu Yan, Liu Cheng-Zhi, Fan Cun-Bo, Han Xing-Wei, Zhang Xiao-Jun, Zhu Ming-Feng, Wang Hong-Yan and Liu Guang-Zhou. “Singlet pairing gaps of neutrons and protons in hyperonic neutron Stars”, Research in Astron. Astrophy.15, 725, 2015.
[32]Zhang Xiao-Jun, Wang Hai-Hua, Wang Chun-Liang, Xu Yan, Liang Zhi-Peng, Fan Cun-Bao, Liu Cheng-Zhi and Gao Jin-Yue, “Goos–H？nchen shift of the reflected beam in a standing-wave coupled electromagnetically induced transparency system”, J. Opt. Soc. Am. B 32, 2281, 2015.
[33]Wang Xiao-Xiao, Li Ai-Jun, Sun Jia-Xiang, Sun Yuan-Hang, Chen Yi, Zhang Xiao-Jun, Wang Lei, Wang Hai-Hua, Gao Jin-Yue, "Preservation of transverse spatial coherencein the storage of double light pulses" , J. Opt. Soc. Am. B 32, 1318, 2015.
[34]Ma Yin-Zhe, Li Min, and He Ping, “Constraining cosmology with pairwise velocity estimator”, Astron. Astrophys. 582, 52, 2015.
[35]Huang Xiu-Lin, Wang Hai -Jun, Liu Guang- Zhou, Liu Cheng-Zhi, Xu Yan, “Effects of delta mesons on the baryonic direct Urca processes in neutron star matter”, Chin. Phys. C 39, 105102, 2015.
[36]Gao Zhi-Fu, Wang Na, Xu Yan, “The effects of superhigh magnetic fields on the equations of state of neutron stars, Astron. Nach. 336, 866, 2015.
[37]Li Min, Xiao Lin, “Lifetimes and Accretion Rates of Protoplanetary Disks”, Astro. Phys. J. 820, 36, 2016
[38]Li Xing-hu, Gao Zhi-Fu, Li Xiang-Dong, Wang Pei, Wang Na, Xu Yan, Peng Qiu-he, “Numerically fitting the electron Fermi energy and the electron fraction in a neutron star, In. J. Mon. Phys. D 25, 1650002, 2016.
[39]Huang Xiu-Lin, Liu Cheng-Zhi, Xu Yan, Liu Guang- Zhou, “Effects of tensor couplings of ω and ρ mesons on 1S0 nucleon superfluidity in neutron star matter”, In. J. Mon. Phys. D 25,1650059, 2016.
[40]Xiao Lin, Jin Li-Ping, Liu Cheng-Zhi, Fan Cun-Bo,“Gas giant planet formation in the photoevaporating I. Gap formation” , Astrophys. J., 826, 168, 2016.
[41] Xu Yan，Huang Xiu-Lin, Liu Cheng-Zhi，Bao Tmurbagan， Liu Guang- Zhou， “Effects of tensor couplings on nucleonic direct Urca processes in neutron star matter”, Chin. Phys. Lett., 33, 099701, 2016.
[42]Sui Ning, Li Min, “The effects of different forms of viscosities on the formation of (pre-) transitional discs”, Mon. Not. R. Astron. Soc., 462, 323, 2016.
[43][軟件著作權(quán)登記] 中國科學(xué)院國家天文臺長春人造衛(wèi)星觀測站,梁智鵬*,董雪; 長春人衛(wèi)站衛(wèi)星激光測距軌道檢核程序V1.0；登記號2016SR235456；授權(quán)公告日2016.08.26.
[44]Zhang Xiao-Jun, Wang Hai-Hua, Liu Cheng-Zhi, Zhang Guo-Wan, Wang Lei,Wu Jin-Hui, “Controlling transverse shift of the reflected light via high refractive index with zero absorption”, Opt. Exp., 25,10335,2017.
[45]Xu Yan, Huang Xiu Lin, Zhang Xiao Jun, Yu Zi, Fan Cun Bo, Ding Wen Bo and Liu Cheng Zhi. “The influence of antikaon condensations on nucleon 1S0 superfluidity in neutron star matter”, Mon.Not.R.Astron.Soc.,474, 3576, 2018.
[46]Huang Xiu Lin, Xu Yan, Liu Cheng Zhi, “Gauge Method for a Special Spinor Field Transformation”. Can. J. Phys.,96,1309, 2018.
[47]Yu Zi, Xu Yan*, Zhang Gui Qing, Hu Tao Ping , “Effects of a weakly interacting light U boson on Protoneutron stars including the hyperon-hyperon interactions”, Commun. Theor. Phys., 69, 417,2018.
[48]Wang, Y.-B., Xu, Y., Fan, C.-B., Liu, C.-Z., Study on the spin states of asteroids using a simplistic shape model. Astronomische Nachrichten, Volume 339, Issue 6, 2018.
[49]Xu Yan*, Zhi Qi Jun, Wang Yi Bo, Huang Xiu Lin*, Ding Wen Bo, Yu Zi, and Liu Cheng Zhi*. Nucleonic 1S0 Superfluidity induced by a soft pion in neutron star matter with antikaon condensations, Chin.Phys.Lett., 36, 061301,2019.
[50]王夷博，劉承志，范存波，許妍，“Flora小行星族自轉(zhuǎn)特性研究”，天文學(xué)報，60，1，2019. Study on the Spin Characteristics of the Flora Asteroid Family, Chinese Astronomy and Astrophysics, 43, 375, 2019
[51]Wang Hong Yan, Xu Yan “CFL 色超導(dǎo)能隙對混合星性質(zhì)的影響”, 吉 林 大 學(xué) 學(xué) 報 (理 學(xué) 版), 57, 406, 2019.
[52]Xu Yan*, Ding Wen Bo, Liu Cheng Zhi, Han Jin Lin, Nucleonic Direct Urca Processes and Cooling of the Massive Neutron Star by Antikaon Condensations, Adv. Astron., Volume 2020, Article ID 6146913.
[53]Zhao Shi Yi, Liu Cheng Zhi, Huang Xiu Lin, Wang Yi Bo, Xu Yan*, Effects of the strong magnetic field on the moment of inertia and the surface gravitational redshift in neutron star, ActaPhys. Sin., 2021, 70, 222601.
[54]Xu Yan*, Huang Xiu Lin,Wang Yi Bo, Liu Cheng Zhi, Han Jin Lin, Baryon-Baryon interaction effects on neutrino emission from direct URCA processes of baryons and modified URCA processes of nucleons in neutron star matter, In. J. Mon. Phys. D, 2021, 30, 2150054.
[55]許妍，天文觀測對中子星內(nèi)部結(jié)構(gòu)的可能約束，天文學(xué)進(jìn)展，2022, 40, 193.
[56]Wang, Yi-Bo, Xu, Yan, Study on the asteroidal spin characteristics in the Hungaria region. Astronomische Nachrichten, Volume 342, Issue 914, 2021.
