Shear-induced structural and thermodynamic phase transitions in micellar systems

2017 ◽  
Vol 40 (2) ◽  
Author(s):  
Angelina Martín del Campo ◽  
J. Paulo García-Sandoval ◽  
J. F. Armando Soltero ◽  
Fernando Bautista ◽  
Octavio Manero ◽  
...  
1991 ◽  
Vol 02 (01) ◽  
pp. 201-208
Author(s):  
ROBERT H. SWENDSEN

Monte Carlo simulations of thermodynamic phase transitions are usually hampered by long relaxation times due to the phenomenon of “critical slowing down.” Using a mapping due to Fortuin and Kasteleyn, a cluster approach to Monte Carlo simulations has been developed, which greatly reduces relaxation times, improving efficiency by up to two or three orders of magnitude. New developments and extensions of this approach are also discussed.


2020 ◽  
Vol 35 (39) ◽  
pp. 2050326
Author(s):  
Abdul Jawad ◽  
Shahid Chaudhary

Among many open questions in theoretical physics, consistent quantum gravity theory is still a major issue to be solved. Recent major works in phase transitions of black holes (BH) can be helpful for quantum interpretation of classical gravity. We study the new effective method to discuss the thermodynamic phase transitions onto well renowned regular BHs. Ordinary approaches of phase transitions depend upon equation of state and it is impossible to obtain all critical points with ordinary approaches. This study is derived from the slope of temperature versus entropy and it provides the possibility of finding all the critical points analytically. This technique provides pressure, which is different from standard relation of pressure and independent of other thermodynamical relations. We discuss some issues in ordinary methods and provide an easy approach to investigate the critical behavior of thermodynamical quantities. We find out the phase transitions points and horizon radii of non-physical range for BHs. We also use the new thermodynamical relations to briefly study well-known Joule–Thomson (JT) effect on regular BH.


2003 ◽  
Vol 367 (3-4) ◽  
pp. 344-350 ◽  
Author(s):  
A Michaelides ◽  
M.-L Bocquet ◽  
P Sautet ◽  
A Alavi ◽  
D.A King

Calphad ◽  
1992 ◽  
Vol 16 (1) ◽  
pp. 63-72 ◽  
Author(s):  
B.H. Erné ◽  
A.J. van der Weijden ◽  
A.M. van der Eerden ◽  
J.B.H. Jansen ◽  
J.C. van Miltenburg ◽  
...  

2001 ◽  
Vol 10 (06) ◽  
pp. 807-809 ◽  
Author(s):  
SAURYA DAS ◽  
J. GEGENBERG ◽  
V. HUSAIN

We investigate thermodynamic properties of two types of asymptotically anti-de Sitter spacetimes: black holes and singular scalar field spacetimes. We describe the possibility that thermodynamic phase transitions can transform one spacetime into another, suggesting that black holes can radiate to naked singularities.


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