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Opflow ◽  
2021 ◽  
Vol 47 (10) ◽  
pp. 10-15
Author(s):  
Bruce Macler ◽  
Samantha C. M. Bishop ◽  
David Smith
Keyword(s):  

2021 ◽  
Author(s):  
Georgios Krintiras ◽  
Keyword(s):  

Entropy ◽  
2021 ◽  
Vol 23 (10) ◽  
pp. 1325
Author(s):  
Ruijin Wang ◽  
Zhen Zhang ◽  
Long Li ◽  
Zefei Zhu

Calculation of the thermal conductivity of nanofluids by molecular dynamics (MD) is very common. Regrettably, general MD can only be employed to simulate small systems due to the huge computation workload. Instead, the computation workload can be considerably reduced due to the coarse-grained fluid when multiparticle collision dynamics (MPCD) is employed. Hence, such a method can be utilized to simulate a larger system. However, the selection of relevant parameters of MPCD noticeably influences the calculation results. To this end, parameterization investigations for various bin sizes, number densities, time-steps, rotation angles and temperatures are carried out, and the influence of these parameters on the calculation of thermal conductivity are analyzed. Finally, the calculations of thermal conductivity for liquid argon, water and Cu-water nanofluid are performed, and the errors compared to the theoretical values are 3.4%, 1.5% and 1.2%, respectively. This proves that the method proposed in the present work for calculating the thermal conductivity of nanofluids is applicable.


Solar RRL ◽  
2021 ◽  
pp. 2100518
Author(s):  
Davide Polverini ◽  
Ana Gracia Amillo ◽  
Nigel Taylor ◽  
Tony Sample ◽  
Elena Salis ◽  
...  

Author(s):  
Debasish Das

A strongly coupled Quark–Gluon Plasma (sQGP) is created in the high-energy heavy-ion collisions at Relativistic Heavy-Ion Collider (RHIC) and Large Hadron Collider (LHC). Our present understanding of sQGP as a very good liquid with astonishingly low viscosity is reviewed. With the arrival of the interesting results from LHC in high-energy [Formula: see text] and [Formula: see text], a new endeavor to characterize the transition from these small systems to heavy ions [Formula: see text] is now in place, since even the small systems showed prominent similarities to heavy ions in the rising multiplicity domains. An outlook of future possibilities for better measurements is also made at the end of this brief review.


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