PVDF-HFP/LiF Composite Interfacial Film to Enhance the Stability of Li-Metal Anodes

2020 ◽  
Vol 3 (7) ◽  
pp. 7191-7199
Author(s):  
Suogang Guo ◽  
Nan Piao ◽  
Li Wang ◽  
Hong Xu ◽  
Guangyu Tian ◽  
...  
Polymers ◽  
2021 ◽  
Vol 13 (7) ◽  
pp. 1127
Author(s):  
Yuejie Jin ◽  
Dingrong Liu ◽  
Jinhua Hu

Polyglycerol polyricinolate (PGPR) and polyglycerol-2 dioleate were selected as model surfactants to construct water-in-oil (W/O) emulsions, and the effect of interfacial rheological properties of surfactant film on the stability of emulsions were investigated based on the interfacial dilatational rheological method. The hydrophobicity chain of PGPR is polyricinic acid condensed from ricinic acid, and that of polyglycerol-2 dioleate is oleic acid. Their dynamic interfacial tensions in 15 cycles of interfacial compression-expansion were determined. The interfacial dilatational viscoelasticity was analyzed by amplitude scanning in the range of 1–28% amplitude and frequency sweep in the range of 5–45 mHz under 2% amplitude. It was found that PGPR could quickly reach adsorption equilibrium and form interfacial film with higher interfacial dilatational viscoelastic modulus to resist the deformation of interfacial film caused by emulsion coalescence, due to its branched chain structure and longer hydrophobic chain, and the emulsion thus presented good stability. However, polyglycerol-2 dioleate with a straight chain structure had lower interfacial tension, and it failed to resist the interfacial disturbance caused by coalescence because of its lower interfacial dilatational viscoelastic modulus, and thus the emulsion was unstable. This study reveals profound understanding of the influence of branched structure of PGPR hydrophobic chain on the interfacial film properties and the emulsion stability, providing experimental reference and theoretical guidance for future design or improvement of surfactant.


2020 ◽  
Vol 8 (18) ◽  
pp. 8979-8988 ◽  
Author(s):  
Qi Jin ◽  
Xitian Zhang ◽  
Hong Gao ◽  
Lu Li ◽  
Zhiguo Zhang

We propose an approach for Li metal anode protection by in situ growth of a LixSiSy/Nafion composite layer on the surface of the Li metal as an artificial SEI film to significantly enhance the stability of the Li metal anode.


Author(s):  
Hui Wang ◽  
Jaegeon Ryu ◽  
Scott A McClary ◽  
Daniel M Long ◽  
Mingxia Zhou ◽  
...  

Abstract Highly reversible Mg plating/stripping is key for rechargeable Mg batteries and has typically been successfully demonstrated using transient electrochemical techniques such as cyclic voltammetry measurements. However, little effort has been invested in studying the stability of the electrode/electrolyte interface over an extended time. We report here the development an in situ generated surface film for Mg anodes based on electrodeposited bismuth (E_Bi). This film improves the interfacial stability of Mg in contact with the electrolyte, particularly over an extended time, and possesses fast charge-transfer kinetics (< 30 Ω∙cm2) and low non-time-sensitive interfacial film resistance (ca. 5 Ω∙cm2) for active Mg species.


2016 ◽  
Vol 26 (18) ◽  
pp. 3059-3066 ◽  
Author(s):  
Ruiguo Cao ◽  
Junzheng Chen ◽  
Kee Sung Han ◽  
Wu Xu ◽  
Donghai Mei ◽  
...  

2021 ◽  
Vol 27 ◽  
pp. 102276
Author(s):  
Huan Zhang ◽  
Meiling Huang ◽  
Jie Song ◽  
Daming Sun ◽  
Yingjun Qiao ◽  
...  

2017 ◽  
Vol 5 (21) ◽  
pp. 10609-10621 ◽  
Author(s):  
Seongmin Ha ◽  
Youngjin Kim ◽  
Dongho Koo ◽  
Kwang-Ho Ha ◽  
Yuwon Park ◽  
...  

We clarified the failure mechanism of Li–O2batteries with a redox mediator.


2019 ◽  
Vol 7 (20) ◽  
pp. 12882-12892 ◽  
Author(s):  
Ji Young Kim ◽  
Guicheng Liu ◽  
Minh Xuan Tran ◽  
Ryanda Enggar Anugrah Ardhi ◽  
Hansung Kim ◽  
...  

This unique hierarchically structured 3D conducting scaffold could significantly improve the stability of Li metal anodes.


1982 ◽  
Vol 99 ◽  
pp. 605-613
Author(s):  
P. S. Conti

Conti: One of the main conclusions of the Wolf-Rayet symposium in Buenos Aires was that Wolf-Rayet stars are evolutionary products of massive objects. Some questions:–Do hot helium-rich stars, that are not Wolf-Rayet stars, exist?–What about the stability of helium rich stars of large mass? We know a helium rich star of ∼40 MO. Has the stability something to do with the wind?–Ring nebulae and bubbles : this seems to be a much more common phenomenon than we thought of some years age.–What is the origin of the subtypes? This is important to find a possible matching of scenarios to subtypes.


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