scholarly journals Equilibrium and Non-equilibrium Studies of Protein G using High-Resolution Optical Trapping Unveil Heterogeneous Unfolding Pathways

2018 ◽  
Vol 114 (3) ◽  
pp. 577a
Author(s):  
Yujie Chen ◽  
Dena Izadi ◽  
Miles L. Whitmore ◽  
Joseph D. Slivka ◽  
Lisa J. Lapidus ◽  
...  
2015 ◽  
Vol 449 (1) ◽  
pp. 243-267 ◽  
Author(s):  
Giovanni Natale ◽  
Cristina C. Popescu ◽  
Richard. J. Tuffs ◽  
Victor P. Debattista ◽  
Jörg Fischera ◽  
...  

2018 ◽  
Vol 122 (49) ◽  
pp. 11155-11165 ◽  
Author(s):  
Dena Izadi ◽  
Yujie Chen ◽  
Miles L. Whitmore ◽  
Joseph D. Slivka ◽  
Kevin Ching ◽  
...  
Keyword(s):  

2017 ◽  
Vol 4 (3) ◽  
pp. 225-233
Author(s):  
Y. Tanaka ◽  
K. Tomita ◽  
Y. Inada ◽  
A. Kumada ◽  
K. Hidaka ◽  
...  

This paper briefly introduce research work examples of non-equilibrium studies in switching arcs. In understanding arc behavior, one often assumes local thermodynamic equilibrium (LTE) condition in the arc plasma. However, actual arc plasmas are not completely and not always in LTE state because of strong temperature change temporally and spatially, and high electric field application etc. Recently, we have a collaboration work in numerical simulations and experimental approaches for decaying arcs without LTE assumption. First, our numerical model is presented for decaying arcs without chemical equilibrium assumption. Secondly, two experimental methods are introduced for measuring electron density in decaying arcs without LTE assumption: Laser Thomson Scattering method and the Schack-Hartmann method. Finally, comparison results is shown between the LTE simulation, the chemically non-equilibrium simulation, and the above experimental measurements.


1983 ◽  
Vol 101 ◽  
pp. 245-252
Author(s):  
P. F. Winkler ◽  
C. R. Canizares ◽  
B. C. Bromley

High resolution X-ray spectroscopy of the brightest knot of emission in the Puppis A supernova remnant shows that it is made up of ionizing plasma, far from equilibrium. Flux measurements in several X-ray lines enable us to determine the non-equilibrium conditions: electron temperature, ion populations, and time since the knot was heated by the supernova shock. Imaging and spectroscopic data from the Einstein Observatory together suggest that this knot is a cloud of density about 10 cm−3 which has recently been shocked to a temperature 7 × 106 K. Radio and optical data on the region appear consistent with this picture.


2010 ◽  
Vol 35 (17) ◽  
pp. 2988 ◽  
Author(s):  
Wei Cheng ◽  
Ximiao Hou ◽  
Fangmao Ye

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