In situ formation of highly controllable and stable Na3PS4 as a protective layer for Na metal anode

2019 ◽  
Vol 7 (8) ◽  
pp. 4119-4125 ◽  
Author(s):  
Yang Zhao ◽  
Jianwen Liang ◽  
Qian Sun ◽  
Lyudmila V. Goncharova ◽  
Jiwei Wang ◽  
...  

A facile and in situ solution-based method has been developed to synthesize an artificial protective layer of NaPS on the surface of Na metal with high stable performances.

2021 ◽  
pp. 129911
Author(s):  
Saisai Li ◽  
Yun Huang ◽  
Wenhao Ren ◽  
Xing Li ◽  
Mingshan Wang ◽  
...  

2021 ◽  
Vol 9 (12) ◽  
pp. 7667-7674
Author(s):  
Song Li ◽  
Xian-Shu Wang ◽  
Qi-Dong Li ◽  
Qi Liu ◽  
Pei-Ran Shi ◽  
...  

A multifunctional artificial protective layer is in situ fabricated on the surface of Li anode, which facilitates stable cycle of Li anode in carbonate electrolyte by forming a unique SEI and inducing homogeneous deposition of lithium ions.


2020 ◽  
Vol 4 (7) ◽  
pp. 3282-3287
Author(s):  
Hyunjin Kim ◽  
Youn Sang Kim ◽  
Jeeyoung Yoo

The artificial SEI layer that includes LiF can be fabricated simply through thermal curing of an F rich material on the surface of Li metal. The proposed artificial SEI layer design offers an alternative strategy for stabilizing the surface of Li metal.


ACS Omega ◽  
2020 ◽  
Vol 5 (14) ◽  
pp. 8299-8304 ◽  
Author(s):  
Shuaiguo Hao ◽  
Zhipeng Ma ◽  
Yao Zhao ◽  
Lina Kong ◽  
Haoyan He ◽  
...  

2020 ◽  
Vol 8 (3) ◽  
pp. 1247-1253 ◽  
Author(s):  
Lili Wang ◽  
Shiyang Fu ◽  
Teng Zhao ◽  
Ji Qian ◽  
Nan Chen ◽  
...  

Development of next-generation high-energy lithium (Li) metal batteries is hindered by uncontrollable growth of Li dendrites and the unstable Li/electrolyte interface during repeated Li plating/stripping.


Author(s):  
Yue Liu ◽  
Qintao Sun ◽  
Peiping Yu ◽  
Bingyun Ma ◽  
Hao Yang ◽  
...  

Developing advanced electrolytes has been considered as a promising approach to stabilize lithium (Li) metal anode via the formation of stable solid electrolyte interphase (SEI) that can protect Li anode...


2019 ◽  
Vol 491 (4) ◽  
pp. 5595-5620 ◽  
Author(s):  
Sanson T S Poon ◽  
Richard P Nelson ◽  
Seth A Jacobson ◽  
Alessandro Morbidelli

ABSTRACT The NASA’s Kepler mission discovered ∼700 planets in multiplanet systems containing three or more transiting bodies, many of which are super-Earths and mini-Neptunes in compact configurations. Using N-body simulations, we examine the in situ, final stage assembly of multiplanet systems via the collisional accretion of protoplanets. Our initial conditions are constructed using a subset of the Kepler five-planet systems as templates. Two different prescriptions for treating planetary collisions are adopted. The simulations address numerous questions: Do the results depend on the accretion prescription?; do the resulting systems resemble the Kepler systems, and do they reproduce the observed distribution of planetary multiplicities when synthetically observed?; do collisions lead to significant modification of protoplanet compositions, or to stripping of gaseous envelopes?; do the eccentricity distributions agree with those inferred for the Kepler planets? We find that the accretion prescription is unimportant in determining the outcomes. The final planetary systems look broadly similar to the Kepler templates adopted, but the observed distributions of planetary multiplicities or eccentricities are not reproduced, because scattering does not excite the systems sufficiently. In addition, we find that ∼1 per cent of our final systems contain a co-orbital planet pair in horseshoe or tadpole orbits. Post-processing the collision outcomes suggests that they would not significantly change the ice fractions of initially ice-rich protoplanets, but significant stripping of gaseous envelopes appears likely. Hence, it may be difficult to reconcile the observation that many low-mass Kepler planets have H/He envelopes with an in situ formation scenario that involves giant impacts after dispersal of the gas disc.


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