吳建宏 / 研究員

pi_image

連絡資訊

學歷

  • 美國明尼蘇達大學物理系博士

秘書

沈彩雲 / 886-2-2789-8386

研究興趣

粒子天文物理及宇宙論 ; 早期宇宙 ; 暴脹宇宙及量子起伏 ; 黑暗物質 ; 宇宙微波背景輻射 ;

經歷

  • 本所博士後研究、助研究員
  • 中央大學天文研究所兼任副教授
  • 中央研究院天文研究所合聘副研究員
  • 國家科學委員會研究獎勵
  • 中央研究院年輕研究人員著作獎

學術著作

期刊論文

  • [1]     Huitzu Tu, Kin-Wang Ng , 2016, “Effects of Goldstone Bosons on Gamma-Ray Bursts ”, JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 3, 037. (SCI) (IF: 5.634; SCI ranking: 14.5%,17.9%)

  • [2]     Shu-Lin Cheng, Wolung Lee, Kin-Wang Ng , 2016, “Numerical study of pseudoscalar inflation with an axion-gauge field coupling ”, PHYSICAL REVIEW D, 6, 063510. (SCI) (IF: 4.506; SCI ranking: 25.8%,28.6%)

  • [3]     Shu-Lin Cheng, Wolung Lee, Kin-Wang Ng, 2015, “Inflationary dilaton-axion magnetogenesis ”, CHINESE JOURNAL OF PHYSICS, 53(6), 110105-(1-14). (SCI) (IF: 0.464; SCI ranking: 89.9%)

  • [4]     Seokcheon Lee, Guo-Chin Liu, Kin-Wang Ng, 2015, “Cosmic Birefringence Fluctuations and Cosmic Microwave Background B-mode Polarization”, PHYSICS LETTERS B, 746, 406-409. (SCI) (IF: 4.787; SCI ranking: 25%,22.6%,19%)

  • [5]     Hing-Tong Cho, Kin-Wang Ng, I-Chin Wang, 2014, “Inflaton fluctuations in the presence of cosmological defects”, JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 11, 023. (SCI) (IF: 5.634; SCI ranking: 14.5%,17.9%)

  • [6]     G.-C. Liu, K.-W. Ng, I-C. Wang, 2014, “Naturally large tensor-to-scalar ratio in inflation”, PHYSICAL REVIEW D, 90(10), 103531. (SCI) (IF: 4.506; SCI ranking: 25.8%,28.6%)

  • [7]     Kin-Wang Ng, Huitzu Tu, Tzu-Chiang Yuan, 2014, “Supernova bounds on Weinberg’s Goldstone bosons”, PHYSICAL REVIEW D, 90, 075014. (SCI) (IF: 4.506; SCI ranking: 25.8%,28.6%)

  • [8]     Kin-Wang Ng, Huitzu Tu, Tzu-Chiang Yuan, 2014, “Dark photons as fractional cosmic neutrino masquerader”, Journal of Cosmology and Astroparticle Physics, 09, 035. (SCI) (IF: 5.634; SCI ranking: 14.5%,17.9%)

  • [9]     W. Lu, W. Lee, K.-W. Ng, 2014, “Teleparallel Poincar ́e cosmology and ΛCDM model”, INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 23 (6) 1450057. (SCI) (IF: 1.963; SCI ranking: 48.4%)

  • [10]     Seokcheon Lee, Guo-Chin Liu, Kin-Wang Ng, 2014, “Imprint of scalar dark energy on cosmic microwave background polarization”, PHYSICAL REVIEW D, 89, 063010. (SCI) (IF: 4.506; SCI ranking: 25.8%,28.6%)

  • [11]     C.-M. Lin, K.-W. Ng, 2013, “Primordial black holes from passive density fluctuations”, PHYSICS LETTERS B, 718(4-5), 1181-1185. (SCI) (IF: 4.787; SCI ranking: 25%,22.6%,19%)

  • [12]     K.-W. Ng, 2012, “Damping of tensor modes in inflation”, Phys. Rev. D, 86(10), 103510. (SCI) (IF: 4.506; SCI ranking: 25.8%,28.6%)

  • [13]     Seokcheon Lee, Kin-Wang Ng, 2012, “Growth Index with the Cosmological Constant”, CHINESE JOURNAL OF PHYSICS, 50(3), 367-374. (SCI) (IF: 0.464; SCI ranking: 89.9%)

  • [14]     C.-H. Wu, J.-T. Hsiang, L. Ford, K.-W. Ng, 2011, “Gravity waves from quantum stress tensor fluctuations in infaltion”, Phys. Rev. D, 84(10),103515. (SCI) (IF: 4.506; SCI ranking: 25.8%,28.6%)

  • [15]     D.-S. Lee, Y.-Y. Charng, K.-W. Ng, 2011, “Photon production from non-equilibrium disoriented chiral condensates in a longitudinal expansion: A theoretical framework”, PHYSICS LETTERS B, 705(5), 487-492. (SCI) (IF: 4.787; SCI ranking: 25%,22.6%,19%)

  • [16]     W. Lee, K.-W. Ng, I-C. Wang, C.-H. Wu, 2011, “Trapping effects on inflation”, Phys. Rev. D, 84(6),063527. (SCI) (IF: 4.506; SCI ranking: 25.8%,28.6%)

  • [17]     G.-C. Liu, K.-W. Ng, and U.-L. Pen, 2011, “Improved dark energy detection through the polarization-assisted WMAP-NVSS ISW correlation”, Phys. Rev. D, 83, 063001. (SCI) (IF: 4.506; SCI ranking: 25.8%,28.6%)

  • [18]     K.-W. Ng and S.-Y. Wang, 2011, “Collapse of vacuum bubbles in a vacuum”, Phys. Rev. D, 83, 043512. (SCI) (IF: 4.506; SCI ranking: 25.8%,28.6%)

  • [19]     Hing-Tong Cho, Kin-Wang Ng, I-Chin Wang, 2011, “Scalar field fluctuations in Schwarzschild–de Sitter spacetime”, CLASSICAL AND QUANTUM GRAVITY, 28, 055004. (SCI) (IF: 2.837; SCI ranking: 38.7%,42.9%,17.7%)

  • [20]     Lee S; Ng KW, 2010, “Spherical collapse model with non-clustering dark energy”, JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 10, 028. (SCI) (IF: 5.634; SCI ranking: 14.5%,17.9%)

  • [21]     Lee S; Ng KW, 2010, “Properties of the exact analytic solution of the growth factor and its applications”, PHYSICAL REVIEW D, 82(4), 043004. (SCI) (IF: 4.506; SCI ranking: 25.8%,28.6%)

  • [22]     L. H. Ford, S.-P. Miao, K.-W. Ng, R. P. Woodard, and C.-H. Wu, 2010, “uantum stress tensor fluctuations of a conformal field and inflationary cosmology”, Phys. Rev. D, 82, 043501. (SCI) (IF: 4.506; SCI ranking: 25.8%,28.6%)

  • [23]     I-Chin Wang, Kin-Wang Ng, 2008, “Effects of a preinflation radiation-dominated epoch to CMB anisotropy”, Physical Review D, 77, 083501. (SCI) (IF: 4.506; SCI ranking: 25.8%,28.6%)

  • [24]     Chun-Hsien Wu, Kin-Wang Ng, L. H. Ford, 2007, “Possible constraints on the duration of inflationary expansion from quantum stress tensor fluctuations”, Physical Review D, 75, 103502. (SCI) (IF: 4.506; SCI ranking: 25.8%,28.6%)

  • [25]     Chun-Hsien Wu, Kin-Wang Ng , Wolung Lee , Da-Shin Lee , Yeo-Yie Charng, 2007, “Quantum noise and a low cosmic microwave background quadrupole”, JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 006. (SCI) (IF: 5.634; SCI ranking: 14.5%,17.9%)

  • [26]     Lee DS, Lee W and Ng KW, 2005, “Bound on the time variation of the fine structure constant driven by quintessence”, INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 14(2), 335-343. (SCI) (IF: 1.963; SCI ranking: 48.4%)

  • [27]     Chou CH and Ng KW, 2004, “Decaying superheavy dark matter and subgalactic structure of the Universe”, PHYSICS LETTERS B, 594(1-2), 1-7. (SCI) (IF: 4.787; SCI ranking: 25%,22.6%,19%)

  • [28]     Park CG and Ng KW, 2004, “E/B separation in cosmic microwave background interferometry”, ASTROPHYSICAL JOURNAL, 609((1): Part 1), 15-21. (SCI) (IF: 5.909; SCI ranking: 12.9%)

  • [29]     Chou CH and Ng KW, 2004, “Decaying superheavy dark matter and the cusp halo problem”, MODERN PHYSICS LETTERS A, 19((13-16): Sp. Iss. SI), 1227-1230. (SCI) (IF: 1.116; SCI ranking: 81%,89.3%,52.8%)

  • [30]     Lee WL, Ng KW and Lee DS, 2004, “Limit on the time variation of the fine structure constant driven by quintessence”, MODERN PHYSICS LETTERS A, 19((13-16): Sp. Iss. SI), 1089-1092. (SCI) (IF: 1.116; SCI ranking: 81%,89.3%,52.8%)

  • [31]     Lee W and Ng KW, 2003, “Constraining evolution of quintessence with CMB and SNIa data”, PHYSICAL REVIEW D, 67((10): Art. No. 107302). (SCI) (IF: 4.506; SCI ranking: 25.8%,28.6%)

  • [32]     Park CG, Ng KW and Park C et al., 2003, “Observational strategies of cosmic microwave background temperature and polarization interferometry experiments”, ASTROPHYSICAL JOURNAL, 589((1): Part 1), 67-81. (SCI) (IF: 5.909; SCI ranking: 12.9%)

學術會議(研討會)論文

專書

專書著作

主編之專書

專書內之論文

技術報告

其他論文

獎項及殊榮

發現與突破

個人資料維護 | 著作目錄維護同步更新 | 最後更新日期 : 2017-09-11
2
Back To Top