[1] Ng Kin-Wang, Wu Yi-Peng, 2021, “Constant-rate inflation: primordial black holes from conformal weight transitions”, Journal of High Energy Physics, 2021(11), 1-25. (SCIE) (IF: 5.875; SCI ranking: 13.8%)
[2] Teng Yu-Ping, Lee Wolung, Ng Kin-Wang, 2021, “Constraining the dark-energy equation of state with cosmological data”, Physical Review D, 104(8), 1-7. (SCIE) (IF: 4.833; SCI ranking: 23.5%,20.7%)
[3] Chu Yu-Kuang, Liu Guo-Chin, Ng Kin-Wang, 2021, “Spherical harmonic analysis of anisotropies in polarized stochastic gravitational-wave background with interferometry experiments”, Physical Review D, 103(6), 1-16. (SCIE) (IF: 4.833; SCI ranking: 23.5%,20.7%)
[4] H.-T. Cho and K.-W. Ng, 2020, “Electromagnetic coupling effects in natural inflation”, Class. Quan- tum Grav., 37, 165011(1-20).
[5] P.-W. Chang, C.-W. Chiang, and K.-W. Ng, 2020, “Thermal loop effects on large-scale curvature perturbation in the Higgs inflation”, High Energy Phys., 04, 163(1-21).
[6] W.-C. Syu, D.-S. Lee, and K.-W. Ng, 2020, “Quantum loop effects to the power spectrum of primordial perturbations during ultra slow-roll inflation”, Phys. Rev. D, 101, 025013(1-13). (SCIE) (IF: 4.833; SCI ranking: 23.5%,20.7%)
[7] Huang Wei-Chih, Ng Kin-Wang, Yuan Tzu-Chiang, 2020, “Circularly polarized gamma rays in effective dark matter theory”, Physics Letters B, 800 135104. (SCIE) (IF: 4.384; SCI ranking: 26.5%,27.6%,21.1%)
[8] Lin Chia-Min, Ng Kin-Wang, Cheung Kingman, 2019, “Chaotic inflation on the brane and the swampland criteria”, Physical Review D, 100(2). (SCIE) (IF: 4.833; SCI ranking: 23.5%,20.7%)
[9] Cheng Shu-Lin, Lee Wolung, Ng Kin-Wang, 2019, “Superhorizon curvature perturbation in ultraslow-roll inflation”, Physical Review D, 99(6). (SCIE) (IF: 4.833; SCI ranking: 23.5%,20.7%)
[10] Levshakov S A, Ng K-W, Henkel C, Mookerjea B, Agafonova I I, Liu S-Y, Wang W-H, 2019, “Testing the weak equivalence principle by differential measurements of fundamental constants in the Magellanic Clouds”, Monthly Notices of the Royal Astronomical Society, 487(4) 5175-5187. (SCIE) (IF: 5.357; SCI ranking: 17.6%)
[11] Cheung Kingman, Kuo Jui-Lin, Ng Kin-Wang, Tsai Yue-Lin Sming, 2019, “The impact of EDGES 21-cm data on dark matter interactions”, Physics Letters B, 789 137-144. (SCIE) (IF: 4.384; SCI ranking: 26.5%,27.6%,21.1%)
[12] Chia-Chun Chang, Wolung Lee, Kin-Wang Ng, 2018, “Spherical collapse models with clustered dark energy”, PHYSICS OF THE DARK UNIVERSE, 19, 12-20. (SCIE) (IF: 4.473; SCI ranking: 25%)
[13] Huang Wei-Chih, Ng Kin-Wang, 2018, “Polarized gamma rays from dark matter annihilations”, Physics Letters B, 783 29-35. (SCIE) (IF: 4.384; SCI ranking: 26.5%,27.6%,21.1%)
[14] Cheng Shu-Lin, Lee Wolung, Ng Kin-Wang, 2018, “Primordial black holes and associated gravitational waves in axion monodromy inflation”, Journal of Cosmology and Astroparticle Physics, 2018(07) 001-001. (SCIE) (IF: 5.21; SCI ranking: 17.2%,19.1%)
[15] 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. (SCIE) (IF: 5.875; SCI ranking: 13.8%)
[16] 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. (SCIE) (IF: 5.357; SCI ranking: 17.6%)
[18] Guo-Chin Liu, Kin-Wang Ng, 2017, “Axion dark matter induced cosmic microwave background B-modes”, PHYSICS OF THE DARK UNIVERSE, 16, 22-25. (SCIE) (IF: 4.473; SCI ranking: 25%)
[19] 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. (SCIE) (IF: 5.875; SCI ranking: 13.8%)
[28] Kin-Wang Ng, Huitzu Tu, Tzu-Chiang Yuan, 2014, “Dark photons as fractional cosmic neutrino masquerader”, Journal of Cosmology and Astroparticle Physics, 09, 035. (SCIE) (IF: 5.21; SCI ranking: 17.2%,19.1%)
[29] W. Lu, W. Lee, K.-W. Ng, 2014, “Teleparallel Poincar ́e cosmology and ΛCDM model”, INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 23 (6) 1450057. (SCIE) (IF: 2.154; SCI ranking: 52.9%)
[30] Seokcheon Lee, Guo-Chin Liu, Kin-Wang Ng, 2014, “Imprint of scalar dark energy on cosmic microwave background polarization”, PHYSICAL REVIEW D, 89, 063010. (SCIE) (IF: 4.833; SCI ranking: 23.5%,20.7%)
[31] C.-M. Lin, K.-W. Ng, 2013, “Primordial black holes from passive density fluctuations”, PHYSICS LETTERS B, 718(4-5), 1181-1185. (SCIE) (IF: 4.384; SCI ranking: 26.5%,27.6%,21.1%)
[33] Seokcheon Lee, Kin-Wang Ng, 2012, “Growth Index with the Cosmological Constant”, CHINESE JOURNAL OF PHYSICS, 50(3), 367-374. (SCIE) (IF: 2.638; SCI ranking: 35.3%)
[34] 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. (SCIE) (IF: 4.833; SCI ranking: 23.5%,20.7%)
[35] 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. (SCIE) (IF: 4.384; SCI ranking: 26.5%,27.6%,21.1%)
[37] 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. (SCIE) (IF: 4.833; SCI ranking: 23.5%,20.7%)
[38] K.-W. Ng and S.-Y. Wang, 2011, “Collapse of vacuum bubbles in a vacuum”, Phys. Rev. D, 83, 043512. (SCIE) (IF: 4.833; SCI ranking: 23.5%,20.7%)
[39] Hing-Tong Cho, Kin-Wang Ng, I-Chin Wang, 2011, “Scalar field fluctuations in Schwarzschild–de Sitter spacetime”, CLASSICAL AND QUANTUM GRAVITY, 28, 055004. (SCIE) (IF: 3.071; SCI ranking: 28.2%,38.2%,41.2%,31%)
[40] Lee S; Ng KW, 2010, “Spherical collapse model with non-clustering dark energy”, JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 10, 028. (SCIE) (IF: 5.21; SCI ranking: 17.2%,19.1%)
[41] Lee S; Ng KW, 2010, “Properties of the exact analytic solution of the growth factor and its applications”, PHYSICAL REVIEW D, 82(4), 043004. (SCIE) (IF: 4.833; SCI ranking: 23.5%,20.7%)
[42] 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. (SCIE) (IF: 4.833; SCI ranking: 23.5%,20.7%)
[43] Lee S; Ng KW, 2010, “Growth index with the exact analytic solution of sub-horizon scale linear perturbation for dark energy models with constant equation of state”, Physics Letters B, 688(1), 1-3. (SCIE) (IF: 4.384; SCI ranking: 26.5%,27.6%,21.1%)
[44] Lee S; Liu GC; Ng KW, 2010, “Effects on the two-point correlation function from the coupling of quintessence to dark matter”, Physical Review D, 81(6), Art. No. 061302. (SCIE) (IF: 4.833; SCI ranking: 23.5%,20.7%)
[45] Ho PTP; Altamirano P; Chang CH; Chang SH; et al., 2009, “The Yuan-Tseh Lee Array for Microwave Background Anisotropy”, ASTROPHYSICAL JOURNAL, 694(2), 1610-1618. (SCIE) (IF: 5.746; SCI ranking: 14.7%)
[46] Ho PTP; Altimirano P;...; Chang S-W; Chang C-H; Chen MT; et al., 2008, “The Yuan Tseh Lee AMiBA Project”, MODERN PHYSICS LETTERS A, 23(20), 1243-1251. (SCIE) (IF: 1.391; SCI ranking: 72.1%,79.3%,73.7%,43.6%)
[47] I-Chin Wang, Kin-Wang Ng, 2008, “Effects of a preinflation radiation-dominated epoch to CMB anisotropy”, Physical Review D, 77, 083501. (SCIE) (IF: 4.833; SCI ranking: 23.5%,20.7%)
[48] Ng KW, 2007, “Some issues in CMB polarization observation”, MODERN PHYSICS LETTERS A, 22(25-28), 1901-1910. (SCIE) (IF: 1.391; SCI ranking: 72.1%,79.3%,73.7%,43.6%)
[49] Lee S; Ng KW, 2007, “Can strong gravitational lensing constrain dark energy?”, PHYSICAL REVIEW D, 76(4), 043518. (SCIE) (IF: 4.833; SCI ranking: 23.5%,20.7%)
[50] 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. (SCIE) (IF: 4.833; SCI ranking: 23.5%,20.7%)
[51] 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. (SCIE) (IF: 5.21; SCI ranking: 17.2%,19.1%)
[52] Liu G-C; Lee S; Ng K-W, 2006, “Effect on Cosmic Microwave Background Polarization of Coupling of Quintessence to Pseudoscalar Formed from the Electromagnetic Field and its Dual”, PHYSICAL REVIEW LETTERS, 97(16), 161303. (SCIE) (IF: 8.385; SCI ranking: 7.1%)
[53] Lee S; Liu GC; Ng KW, 2006, “Constraints on the coupled quintessence from cosmic microwave background anisotropy and matter power spectrum”, PHYSICAL REVIEW D, 73(8), 083516. (SCIE) (IF: 4.833; SCI ranking: 23.5%,20.7%)
[54] Ng KW, 2005, “Full-sky correlation functions for CMB experiments with asymmetric window functions”, PHYSICAL REVIEW D, 71(8), 083009. (SCIE) (IF: 4.833; SCI ranking: 23.5%,20.7%)
[55] 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. (SCIE) (IF: 2.154; SCI ranking: 52.9%)
[56] Chou C-H; Ng K-W, 2004, “Decaying Superheavy Dark Matter and Subgalactic Structure of the Universe”, PHYSICS LETTERS B, 594(1-2), 1-7. (SCIE) (IF: 4.384; SCI ranking: 26.5%,27.6%,21.1%)
[57] Chou CH and Ng KW, 2004, “Decaying superheavy dark matter and subgalactic structure of the Universe”, PHYSICS LETTERS B, 594(1-2), 1-7. (SCIE) (IF: 4.384; SCI ranking: 26.5%,27.6%,21.1%)
[58] Park CG and Ng KW, 2004, “E/B separation in cosmic microwave background interferometry”, ASTROPHYSICAL JOURNAL, 609((1): Part 1), 15-21. (SCIE) (IF: 5.746; SCI ranking: 14.7%)
[59] Park C-G; Ng K-W, 2004, “E/B Separation in Cosmic Microwave Background Interferometry”, ASTROPHYSICAL JOURNAL, 609(1), 15-21. (SCIE) (IF: 5.746; SCI ranking: 14.7%)
[60] 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. (SCIE) (IF: 1.391; SCI ranking: 72.1%,79.3%,73.7%,43.6%)
[61] 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. (SCIE) (IF: 1.391; SCI ranking: 72.1%,79.3%,73.7%,43.6%)
[62] Ho PTP; Chen M-T; ...; Chiueh T; Chu T-H; Jiang H; Koch P; Kubo D; Li C-T; ...; Lin K-Y; Liu G-C; Lo K-Y; Ma C-J; Martin RN; Ng K-W; Nishioka H; Patt F; ...; Wang H; Hwang Y-J; Umetsu K; et al., 2004, “The AMiBA Project”, MODERN PHYSICS LETTERS A, 19(13-16), 993-1000. (SCIE) (IF: 1.391; SCI ranking: 72.1%,79.3%,73.7%,43.6%)
[63] Cortiglioni S; Bernardi G; ...; Ng KW; et al, 2004, “The Sky Polarization Observatory (SPOrt)”, NEW ASTRONOMY, 9(4), 297-327. (SCIE) (IF: 1.058; SCI ranking: 82.4%)
[64] Lee W and Ng KW, 2003, “Constraining evolution of quintessence with CMB and SNIa data”, PHYSICAL REVIEW D, 67((10): Art. No. 107302). (SCIE) (IF: 4.833; SCI ranking: 23.5%,20.7%)
[65] Park CG; Ng KW; ...; Liu GC; Umetsu K, 2003, “Observational Strategies of Cosmic Microwave Background Temperature and Polarization Interferometry Experiments”, ASTROPHYSICAL JOURNAL, 589(1), 67-81. (SCIE) (IF: 5.746; SCI ranking: 14.7%)
[66] 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. (SCIE) (IF: 5.746; SCI ranking: 14.7%)