surface energy density
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Author(s):  
Lihong Wang ◽  
Liyuan Wang ◽  
Hongjun Han ◽  
Wei Han ◽  
Yu Wang

2020 ◽  
Vol 478 ◽  
pp. 228748
Author(s):  
Yuan Wang ◽  
Xiangjian Shen ◽  
Hamidreza Arandiyan ◽  
Yanting Yin ◽  
Fanfei Sun ◽  
...  

CrystEngComm ◽  
2020 ◽  
Vol 22 (15) ◽  
pp. 2601-2611
Author(s):  
Vyacheslav N. Gorshkov ◽  
Vladimir V. Tereshchuk ◽  
Pooya Sareh

The manifestation of anisotropy of surface energy density in the dynamics of 1D-nanostuctures, when annealed below melting temperature in different conditions, is studied on the basis of an analytical approach and Monte Carlo kinetic model.


2019 ◽  
Vol 25 (2) ◽  
pp. 337-347
Author(s):  
Liyuan Wang

The finite plane deformation of nanomaterial surrounding an elliptical hole subjected to remote loading is systematically investigated using a recently developed continuum theory. A complex variable formulation is utilized to obtain a closed-form solution for the hoop stress along the edge of the hole. The results show that when the size of the hole reduces to the same order as the ratio of the surface energy density to the applied remote stress, the influence of the surface energy density plays an even more significant role, and the shape of the hole coupled with surface energy density has a significant effect on the elastic state around the hole. Surprisingly, in the absence of any external loading, the hoop stress induced solely by surface effects is identical to that for a hole with surface energy in a linearly elastic solid derived by the Gurtin–Murdoch surface elasticity model. The results in this paper should be useful for the precise design of nanodevices and helpful for the reasonable assessment of test results of nano-instruments.


2017 ◽  
Vol 26 (14) ◽  
pp. 1750158 ◽  
Author(s):  
S. Habib Mazharimousavi ◽  
M. Halilsoy ◽  
S. N. Hamad Amen

We study spherically symmetric timelike thin-shells in [Formula: see text]-dimensional bulk spacetime with a variable equation-of-state for the fluid presented on the shell. In such a fluid, the angular pressure [Formula: see text] is a function of both surface energy density [Formula: see text] and the radius [Formula: see text] of the thin-shell. Explicit cases of the thin shells connecting two nonidentical cloud of strings spacetimes and a flat Minkowski spacetime to the Schwarzschild metric are investigated.


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