Bing-Bing Liu

Bing-Bing Liu


Research Focus & Metrics

Academic Career Length

28Years (1999-Present)

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

Representative Publications

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24 November 2021 in Nature
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YSYuchen Shang
Yuchen Shang
ZLZhaodong Liu
Zhaodong Liu
JDJiajun Dong
Jiajun Dong
MYMingguang Yao
Mingguang Yao
ZYZhenxing Yang
Zhenxing Yang
BLBing-Bing Liu
Bing-Bing Liu

14 July 2006 in Advanced Materials
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Journal Article
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LWL. Wang
L. Wang
BLBing-Bing Liu
Bing-Bing Liu
DLD. Liu
D. Liu
MYM. Yao
M. Yao
YHY. Hou
Y. Hou
BSB. Sundqvist
B. Sundqvist

21 March 2023 in Advanced Materials
Verified
Journal Article
Closed access
PSPengfei Shen
Pengfei Shen
PYPei Yin
Pei Yin
YZYongtao Zou
Yongtao Zou
MLMu Li
Mu Li
NZNanqiu Zhang
Nanqiu Zhang
BLBing-Bing Liu
Bing-Bing Liu

15 June 2017 in Physical Review Letters
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XYXigui Yang
Xigui Yang
MYMingguang Yao
Mingguang Yao
XWXiangying Wu
Xiangying Wu
SLShijie Liu
Shijie Liu
SCShuanglong Chen
Shuanglong Chen
BLBing-Bing Liu
Bing-Bing Liu
Design and synthesis of new carbon allotropes have always been important topics in condensed matter physics and materials science. Here we report a new carbon allotrope, formed from cold-compressed C70 peapods, which most likely can be identified with a fully sp3-bonded monoclinic structure, here named V carbon, predicted from our simulation. The simulated x-ray diffraction pattern, near K-edge spectroscopy, and phonon spectrum agree well with our experimental data. Theoretical calculations reveal that V carbon has a Vickers hardness of 90 GPa and a bulk modulus ∼400  GPa, which well explains the “ring crack” left on the diamond anvils by the transformed phase in our experiments. The V carbon is thermodynamically stable over a wide pressure range up to 100 GPa, suggesting that once V carbon forms, it is stable and can be recovered to ambient conditions. A transition pathway from peapod to V carbon has also been suggested. These findings suggest a new strategy for creating new sp3-hybridized carbon structures by using fullerene@nanotubes carbon precursor containing odd-numbered rings in the structures.

2 July 2021 in Nature Communications
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CZChunguang Zhai
Chunguang Zhai
XYXiu Yin
Xiu Yin
SNShifeng Niu
Shifeng Niu
MYMingguang Yao
Mingguang Yao
SHShuhe Hu
Shuhe Hu
BLBing-Bing Liu
Bing-Bing Liu
Developing a universal strategy to design piezochromic luminescent materials with desirable properties remains challenging. Here, we report that insertion of a non-emissive molecule into a donor (perylene) and acceptor (1,2,4,5-tetracyanobezene) binary cocrystal can realize fine manipulation of intermolecular interactions between perylene and 1,2,4,5-tetracyanobezene (TCNB) for desirable piezochromic luminescent properties. A continuous pressure-induced emission enhancement up to 3 GPa and a blue shift from 655 to 619 nm have been observed in perylene-TCNB cocrystals upon THF insertion, in contrast to the red-shifted and quenched emission observed when compressing perylene-TCNB cocrystals and other cocrystals reported earlier. By combining experiment with theory, it is further revealed that the inserted non-emissive THF forms blue-shifting hydrogen bonds with neighboring TCNB molecules and promote a conformation change of perylene molecules upon compression, causing the blue-shifted and enhanced emission. This strategy remains valid when inserting other molecules as non-emissive component into perylene-TCNB cocrystals for abnormal piezochromic luminescent behaviors.

10 November 2008 in Physical Review B
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MYMingguang Yao
Mingguang Yao
ZWZhigang Wang
Zhigang Wang
BLBing-Bing Liu
Bing-Bing Liu
YZYonggang Zou
Yonggang Zou
SYShidan Yu
Shidan Yu
BSB. Sundqvist
B. Sundqvist
Raman spectra of single-walled carbon nanotubes (SWNTs) with diameters of 0.6–1.3 nm have been studied under high pressure. A “plateau” in the pressure dependence of the G-band frequencies was observed in all experiments, both with and without pressure transmission medium. Near the onset of the G-band plateau, the corresponding radial breathing mode (RBM) lines become very weak. A strong broadening of the full width at half maximum of the RBMs just before the onset of the G-band plateau suggests that a structural transition starts in the SWNTs. Raman spectra from SWNTs released from different pressures also indicate that a significant structural transition occurs during the G-band plateau process. Simulations of the structural changes and the corresponding Raman modes of a nanotube under compression show a behavior similar to the experimental observations. Based on the experimental results and the theoretical simulation, a detailed model is suggested for the structural transition of SWNTs, corresponding to the experimentally obtained Raman results in the high-pressure domain.