TY - JOUR
T1 - Efficient circular Dyson Brownian motion algorithm
AU - Buijsman, Wouter
N1 - Publisher Copyright:
© 2024 authors. Published by the American Physical Society.
PY - 2024/4/1
Y1 - 2024/4/1
N2 - Circular Dyson Brownian motion describes the Brownian dynamics of particles on a circle (periodic boundary conditions), interacting through a logarithmic, long-range two-body potential. Within the log-gas picture of random matrix theory, it describes the level dynamics of unitary ("circular") matrices. A common scenario is that one wants to know about an initial configuration evolved over a certain interval of time, without being interested in the intermediate dynamics. Numerical evaluation of this is computationally expensive as the time-evolution algorithm is accurate only on short time intervals because of an underlying perturbative approximation. This work proposes an efficient and easy-to-implement improved circular Dyson Brownian motion algorithm for the unitary class (Dyson index β=2, physically corresponding to broken time-reversal symmetry). The algorithm allows one to study time evolution over arbitrarily large intervals of time at a fixed computational cost, with no approximations being involved.
AB - Circular Dyson Brownian motion describes the Brownian dynamics of particles on a circle (periodic boundary conditions), interacting through a logarithmic, long-range two-body potential. Within the log-gas picture of random matrix theory, it describes the level dynamics of unitary ("circular") matrices. A common scenario is that one wants to know about an initial configuration evolved over a certain interval of time, without being interested in the intermediate dynamics. Numerical evaluation of this is computationally expensive as the time-evolution algorithm is accurate only on short time intervals because of an underlying perturbative approximation. This work proposes an efficient and easy-to-implement improved circular Dyson Brownian motion algorithm for the unitary class (Dyson index β=2, physically corresponding to broken time-reversal symmetry). The algorithm allows one to study time evolution over arbitrarily large intervals of time at a fixed computational cost, with no approximations being involved.
UR - http://www.scopus.com/inward/record.url?scp=85195816913&partnerID=8YFLogxK
U2 - 10.1103/PhysRevResearch.6.023264
DO - 10.1103/PhysRevResearch.6.023264
M3 - Article
AN - SCOPUS:85195816913
SN - 2643-1564
VL - 6
JO - Physical Review Research
JF - Physical Review Research
IS - 2
M1 - 023264
ER -