TING-WAI CHIU

Prof. Dr. TING-WAI CHIU

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Research Focus & Metrics

Academic Career Length

50Years (1977-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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8 January 2019 in Nature Astronomy
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KCKAGRA collaboration
KAGRA collaboration
TATomotada Akutsu
Tomotada Akutsu
MAM. Ando
M. Ando
KAK. Arai
K. Arai
YAY. Arai
Y. Arai
ZZZ.-H. Zhu
Z.-H. Zhu

15 November 1980 in Physical Review D
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Journal Article
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JBJames S. Ball
James S. Ball
TCTING-WAI CHIU
TING-WAI CHIU
The analytic properties of the vertex functions for massless scalar and massless and massive spinor electrodynamics are investigated. First, a general tensor form for the vertex consistent with the Ward identities and free of kinematic singularities is constructed. All of the scalar functions that appear are then calculated to one-loop order in perturbation theory. It is found that in both massive and massless theories the infrared singularities appear in the longitudinal parts of the vertex. The massless theories have additional photon mass-shell singularities which appear in the transverse terms. Complete expressions for each vertex are obtained which contain only one nonelementary function.

15 November 1980 in Physical Review D
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Journal Article
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JBJames S. Ball
James S. Ball
TCTING-WAI CHIU
TING-WAI CHIU
The analytic properties of the three-gluon vertex function for quantum chromodynamics in covariant gauges are investigated. First, a general tensor form for the vertex consistent with the Ward identity and free of kinematic singularities is constructed. The vertex is then calculated to one-loop order in the Feynman gauge. The complete expression for the off-shell one-loop vertex is expressed in terms of elementary functions plus one nonelementary function, the dilogarithm. Various kinematic limits of the vertex are considered. The most interesting results are the following. (1) Gluon mass-shell singularities occur in the transverse terms as well as the longitudinal terms. (2) The leading IR singularity is in the longitudinal part of the vertex, as is the case for QED; however, it is a pole singularity rather than the usual logarithmic singularity.

31 August 2009 in Physical Review D
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SAS. Aoki
S. Aoki
TCTING-WAI CHIU
TING-WAI CHIU
HFH. Fukaya
H. Fukaya
SHS. Hashimoto
S. Hashimoto
Tung-Han HsiehTung-Han Hsieh
Tung-Han Hsieh
NYN. Yamada
N. Yamada
We calculate pion vector and scalar form factors in two-flavor lattice QCD and study the chiral behavior of the vector and scalar radii ⟨r2⟩V,S. Numerical simulations are carried out on a 163×32 lattice at a lattice spacing of 0.12 fm with quark masses down to ∼ms/6, where ms is the physical strange quark mass. Chiral symmetry, which is essential for a direct comparison with chiral perturbation theory (ChPT), is exactly preserved in our calculation at finite lattice spacing by employing the overlap quark action. We utilize the so-called all-to-all quark propagator in order to calculate the scalar form factor including the contributions of disconnected diagrams and to improve statistical accuracy of the form factors. A detailed comparison with ChPT reveals that the next-to-next-to-leading-order contributions to the radii are essential to describe their chiral behavior in the region of quark mass from ms/6 to ms/2. Chiral extrapolation based on two-loop ChPT yields ⟨r2⟩V=0.409(23)(37)  fm2 and ⟨r2⟩S=0.617(79)(66)  fm2, which are consistent with phenomenological analysis. We also present our estimates of relevant low-energy constants.

23 July 2019 in Classical and Quantum Gravity
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Journal Article
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TATomotada Akutsu
Tomotada Akutsu
MAM Ando
M Ando
KAK Arai
K Arai
YAY Arai
Y Arai
SAS Araki
S Araki
ZZZong-Hong Zhu
Zong-Hong Zhu
KAGRA is a second-generation interferometric gravitational-wave detector with 3 km arms constructed at Kamioka, Gifu, Japan. It is now in its final installation phase, which we call bKAGRA (baseline KAGRA), with scientific observations expected to begin in late 2019. One of the advantages of KAGRA is its underground location of at least 200 m below the ground surface, which reduces seismic motion at low frequencies and increases the stability of the detector. Another advantage is that it cools down the sapphire test mass mirrors to cryogenic temperatures to reduce thermal noise. In April–May 2018, we operated a 3 km Michelson interferometer with a cryogenic test mass for 10 d, which was the first time that km-scale interferometer was operated at cryogenic temperatures. In this article, we report the results of this ‘bKAGRA Phase 1’ operation. We have demonstrated the feasibility of 3 km interferometer alignment and control with cryogenic mirrors.

1 July 2007 in Physics Letters B
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Journal Article
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TCTING-WAI CHIU
TING-WAI CHIU
Tung-Han HsiehTung-Han Hsieh
Tung-Han Hsieh
CHChao-Hsi Huang
Chao-Hsi Huang
KOKenji Ogawa
Kenji Ogawa