吳建宏 / 研究員

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]     Chia-Chun Chang, Wolung Lee, Kin-Wang Ng, 2018, “Spherical collapse models with clustered dark energy”, PHYSICS OF THE DARK UNIVERSE, 19, 12-20. (SCI) (IF: 5.425; SCI ranking: 14.3%)
  
  
• [2]     Huitzu Tu, Kin-Wang Ng, 2017, “Supernovae and Weinberg’s Higgs portal dark radiation and dark matter”, JOURNAL OF HIGH ENERGY PHYSICS, 07(108), 1-21. (SCI) (IF: 6.063; SCI ranking: 10.3%)
  
  
• [3]     S.A. Levshakov, K. -W. Ng, C. Henkel, B. Mookerjea, 2017, “[CI], [CII] and CO emission lines as a probe for alpha variations at low and high redshifts”, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 471, 2143-2150. (SCI) (IF: 4.961; SCI ranking: 17.5%)
  
  
• [4]     Jen-Tsung Hsiang, L.H. Ford, Kin-Wang Ng, Chun-Hsien Wu, 2017, “Quantum stress tensor fluctuations and primordial gravity waves”, PHYSICAL REVIEW D, 95(6), 063524-1-063524-19. (SCI) (IF: 4.557; SCI ranking: 22.2%,27.6%)
  
  
• [5]     Guo-Chin Liu, Kin-Wang Ng, 2017, “Axion dark matter induced cosmic microwave background B-modes”, PHYSICS OF THE DARK UNIVERSE, 16, 22-25. (SCI) (IF: 5.425; SCI ranking: 14.3%)
  
  
• [6]     Shu-Lin Cheng, Wolung Lee, Kin-Wang Ng, 2017, “Production of high stellar-mass primordial black holes in trapped inflation”, JOURNAL OF HIGH ENERGY PHYSICS, 02(008), 1-11. (SCI) (IF: 6.063; SCI ranking: 10.3%)
  
  
• [7]     Seokcheon Lee, Guo-Chin Liu, Kin-Wang Ng, 2016, “Dark ultra-light scalars and cosmic parity violation”, Universe, 4, 29-44.
  
  
• [8]     Huitzu Tu, Kin-Wang Ng , 2016, “Effects of Goldstone Bosons on Gamma-Ray Bursts ”, JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 3, 037. (SCI) (IF: 4.734; SCI ranking: 24.1%,20.6%)
  
  
• [9]     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: 4.557; SCI ranking: 22.2%,27.6%)
  
  
• [10]     Shu-Lin Cheng, Wolung Lee, Kin-Wang Ng, 2015, “Inflationary dilaton-axion magnetogenesis ”, CHINESE JOURNAL OF PHYSICS, 53(6), 110105-(1-14). (SCI) (IF: 0.514; SCI ranking: 84.8%)
  
  
• [11]     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: 4.807; SCI ranking: 15%,19%,20.7%)
  
  
• [12]     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: 4.734; SCI ranking: 24.1%,20.6%)
  
  
• [13]     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: 4.557; SCI ranking: 22.2%,27.6%)
  
  
• [14]     Kin-Wang Ng, Huitzu Tu, Tzu-Chiang Yuan, 2014, “Supernova bounds on Weinberg’s Goldstone bosons”, PHYSICAL REVIEW D, 90, 075014. (SCI) (IF: 4.557; SCI ranking: 22.2%,27.6%)
  
  
• [15]     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: 4.734; SCI ranking: 24.1%,20.6%)
  
  
• [16]     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: 2.476; SCI ranking: 42.9%)
  
  
• [17]     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: 4.557; SCI ranking: 22.2%,27.6%)
  
  
• [18]     C.-M. Lin, K.-W. Ng, 2013, “Primordial black holes from passive density fluctuations”, PHYSICS LETTERS B, 718(4-5), 1181-1185. (SCI) (IF: 4.807; SCI ranking: 15%,19%,20.7%)
  
  
• [19]     K.-W. Ng, 2012, “Damping of tensor modes in inflation”, Phys. Rev. D, 86(10), 103510. (SCI) (IF: 4.557; SCI ranking: 22.2%,27.6%)
  
  
• [20]     Seokcheon Lee, Kin-Wang Ng, 2012, “Growth Index with the Cosmological Constant”, CHINESE JOURNAL OF PHYSICS, 50(3), 367-374. (SCI) (IF: 0.514; SCI ranking: 84.8%)
  
  
• [21]     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: 4.557; SCI ranking: 22.2%,27.6%)
  
  
• [22]     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: 4.807; SCI ranking: 15%,19%,20.7%)
  
  
• [23]     W. Lee, K.-W. Ng, I-C. Wang, C.-H. Wu, 2011, “Trapping effects on inflation”, Phys. Rev. D, 84(6),063527. (SCI) (IF: 4.557; SCI ranking: 22.2%,27.6%)
  
  
• [24]     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: 4.557; SCI ranking: 22.2%,27.6%)
  
  
• [25]     K.-W. Ng and S.-Y. Wang, 2011, “Collapse of vacuum bubbles in a vacuum”, Phys. Rev. D, 83, 043512. (SCI) (IF: 4.557; SCI ranking: 22.2%,27.6%)
  
  
• [26]     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: 3.119; SCI ranking: 15.2%,41.4%,31.7%)
  
  
• [27]     Lee S; Ng KW, 2010, “Spherical collapse model with non-clustering dark energy”, JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 10, 028. (SCI) (IF: 4.734; SCI ranking: 24.1%,20.6%)
  
  
• [28]     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: 4.557; SCI ranking: 22.2%,27.6%)
  
  
• [29]     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: 4.557; SCI ranking: 22.2%,27.6%)
  
  
• [30]     I-Chin Wang, Kin-Wang Ng, 2008, “Effects of a preinflation radiation-dominated epoch to CMB anisotropy”, Physical Review D, 77, 083501. (SCI) (IF: 4.557; SCI ranking: 22.2%,27.6%)
  
  
• [31]     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: 4.557; SCI ranking: 22.2%,27.6%)
  
  
• [32]     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: 4.734; SCI ranking: 24.1%,20.6%)
  
  
• [33]     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: 2.476; SCI ranking: 42.9%)
  
  
• [34]     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: 4.807; SCI ranking: 15%,19%,20.7%)
  
  
• [35]     Park CG and Ng KW, 2004, “E/B separation in cosmic microwave background interferometry”, ASTROPHYSICAL JOURNAL, 609((1): Part 1), 15-21. (SCI) (IF: 5.533; SCI ranking: 11.1%)
  
  
• [36]     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: 1.165; SCI ranking: 54.5%,86.2%,70%)
  
  
• [37]     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: 1.165; SCI ranking: 54.5%,86.2%,70%)
  
  
• [38]     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: 4.557; SCI ranking: 22.2%,27.6%)
  
  
• [39]     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: 5.533; SCI ranking: 11.1%)