scholarly journals Cluster evolution and critical cluster sizes for the square and triangular lattice Ising models using lattice animals and Monte Carlo simulations

2012 ◽  
Vol 85 (21) ◽  
Author(s):  
G. Eising ◽  
B. J. Kooi
2003 ◽  
Vol 593 (2) ◽  
pp. 772-787 ◽  
Author(s):  
J. M. Fregeau ◽  
M. A. Gurkan ◽  
K. J. Joshi ◽  
F. A. Rasio

2010 ◽  
Vol 81 (10) ◽  
Author(s):  
Iver Bakken Sperstad ◽  
Einar B. Stiansen ◽  
Asle Sudbø

2007 ◽  
Vol 3 (S246) ◽  
pp. 151-155 ◽  
Author(s):  
Sourav Chatterjee ◽  
John M. Fregeau ◽  
Frederic A. Rasio

AbstractWe systematically study the effects of collisions on the overall dynamical evolution of dense star clusters using Monte Carlo simulations over many relaxation times. We derive many observable properties of these clusters, including their core radii and the radial distribution of collision products. We also study different aspects of collisions in a cluster taking into account the shorter lifetimes of more massive stars, which has not been studied in detail before. Depending on the lifetimes of the significantly more massive collision products, observable properties of the cluster can be modified qualitatively; for example, even without binaries, core collapse can sometimes be avoided simply because of stellar collisions.


1992 ◽  
Vol 03 (05) ◽  
pp. 821-824
Author(s):  
DIETER W. HEERMANN

We briefly review some of the results on metastable and unstable states as observed by Monte Carlo simulations of short- and long-range Ising models.


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