Effects of viscosity on viscous pressure bulging (VPB) of Al1060 sheet

2015 ◽  
Vol 86 (1-4) ◽  
pp. 215-225 ◽  
Author(s):  
Binxian Yuan ◽  
Wa Fang ◽  
Jiguang Li ◽  
Zhoude Qu ◽  
Yujun Cai ◽  
...  
2007 ◽  
Vol 21 (10) ◽  
pp. 1505-1511 ◽  
Author(s):  
Jianguang Liu ◽  
Qiucai Peng ◽  
Yan Liu ◽  
Zhongjin Wang

Universe ◽  
2021 ◽  
Vol 7 (5) ◽  
pp. 112
Author(s):  
Eman Abdel Hakk ◽  
Abdel Nasser Tawfik ◽  
Afaf Nada ◽  
Hayam Yassin

It is conjectured that in cosmological applications the particle current is not modified but finite heat or energy flow. Therefore, comoving Eckart frame is a suitable choice, as it merely ceases the charge and particle diffusion and conserves charges and particles. The cosmic evolution of viscous hadron and parton epochs in casual and non-casual Eckart frame is analyzed. By proposing equations of state deduced from recent lattice QCD simulations including pressure p, energy density ρ, and temperature T, the Friedmann equations are solved. We introduce expressions for the temporal evolution of the Hubble parameter H˙, the cosmic energy density ρ˙, and the share η˙ and the bulk viscous coefficient ζ˙. We also suggest how the bulk viscous pressure Π could be related to H. We conclude that the relativistic theory of fluids, the Eckart frame, and the finite viscous coefficients play essential roles in the cosmic evolution, especially in the hadron and parton epochs.


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