Equilibrium temperatures of discrete nonlinear systems
Source abstract
Abstract
During the evolution of discrete nonlinear systems with dynamics dictated by the discrete nonlinear Schr\"odinger equation, two quantities are conserved: system energy (Hamiltonian) and system density (number of particles). It is then possible to analyze system evolution in relation to an energy-density phase diagram. Previous works have identified a ``thermalization zone'' on the phase diagram where regular statistical mechanics methods apply. Based on these statistical mechanics methods we have now assigned a specific equilibrium temperature to every point of the thermalization zone. Temperatures were derived in the grand canonical picture through an entropy-temperature relation, modified to suit the nonlinear lattice systems. Generally, everywhere in the thermalization zone of the phase diagram, temperatures along a fixed system-density line, grow monotonously from zero to infinity. Isotherms on the phase diagram are concave.
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Research context
OpenAlex topics: Nonlinear Photonic Systems · Advanced Fiber Laser Technologies · Nonlinear Dynamics and Pattern Formation
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References (34)
Show source-provided references
1. 10.1103/PhysRevLett.84.374010.1103/PhysRevLett.84.3740 ↗
2. 10.1103/PhysRevE.86.01110810.1103/PhysRevE.86.011108 ↗
3. 10.1016/j.physd.2005.11.00210.1016/j.physd.2005.11.002 ↗
4. 10.1103/PhysRevE.89.02292110.1103/PhysRevE.89.022921 ↗
5. 10.1103/PhysRevLett.87.05410210.1103/PhysRevLett.87.054102 ↗
6. 10.1103/PhysRevA.83.01380610.1103/PhysRevA.83.013806 ↗
7. 10.1103/PhysRevE.95.05213510.1103/PhysRevE.95.052135 ↗
8. P. G. Kevrekidis · 200910.1007/978-3-540-89199-4 ↗
9. 10.1016/j.physd.2009.08.00610.1016/j.physd.2009.08.006 ↗
10. 10.1103/PhysRevLett.86.235310.1103/PhysRevLett.86.2353 ↗
11. 10.1103/PhysRevE.93.03221910.1103/PhysRevE.93.032219 ↗
12. 10.1002/cpa.2138810.1002/cpa.21388 ↗
13. 10.1103/PhysRevA.66.05360710.1103/PhysRevA.66.053607 ↗
14. V. S. Bagnato · Rom. Rep. Phys. · 2015 · 67 · 5
15. E. H. Lieb · 2005
16. 10.1103/PhysRevLett.79.495010.1103/PhysRevLett.79.4950 ↗
17. 10.1103/PhysRevA.59.62010.1103/PhysRevA.59.620 ↗
18. 10.1126/science.aaf883410.1126/science.aaf8834 ↗
19. 10.1088/1742-5468/2015/08/P0802810.1088/1742-5468/2015/08/P08028 ↗
20. 10.1088/1367-2630/15/9/09303810.1088/1367-2630/15/9/093038 ↗
21. 10.1038/nature0193610.1038/nature01936 ↗
22. S. Flach · 2016
23. 10.1007/s10955-011-0200-410.1007/s10955-011-0200-4 ↗
24. J. C. Eilbeck · 2003
25. M. J. Ablowitz · 2006
26. 10.1016/0960-0779(94)90114-710.1016/0960-0779(94)90114-7 ↗
27. 10.1103/PhysRevE.89.05291810.1103/PhysRevE.89.052918 ↗
28. 10.1016/j.physa.2006.10.04110.1016/j.physa.2006.10.041 ↗
29. 10.1103/PhysRevE.77.03660610.1103/PhysRevE.77.036606 ↗
30. 10.1103/PhysRevLett.102.23390410.1103/PhysRevLett.102.233904 ↗
31. 10.1103/PhysRevLett.100.05040410.1103/PhysRevLett.100.050404 ↗
32. C. Kittel · 2000
33. 10.2298/TSCI180115012P10.2298/TSCI180115012P ↗
34. 10.1088/1361-6455/aa9a9710.1088/1361-6455/aa9a97 ↗