Please use this identifier to cite or link to this item: https://doi.org/10.1016/j.cpc.2004.11.006
DC FieldValue
dc.titleSolving the master equation for extremely long time scale calculations
dc.contributor.authorLee, H.K.
dc.contributor.authorOkabe, Y.
dc.contributor.authorCheng, X.
dc.contributor.authorJalil, M.B.A.
dc.date.accessioned2014-10-07T04:36:29Z
dc.date.available2014-10-07T04:36:29Z
dc.date.issued2005-06-15
dc.identifier.citationLee, H.K., Okabe, Y., Cheng, X., Jalil, M.B.A. (2005-06-15). Solving the master equation for extremely long time scale calculations. Computer Physics Communications 168 (3) : 159-164. ScholarBank@NUS Repository. https://doi.org/10.1016/j.cpc.2004.11.006
dc.identifier.issn00104655
dc.identifier.urihttp://scholarbank.nus.edu.sg/handle/10635/83034
dc.description.abstractThe dynamics of magnetic reversal process plays an important role in the design of the magnetic recording devices in the long time scale limit. In addition to long time scale, microscopic effects such as the entropic effect become important in magnetic nano-scale systems. Many advanced simulation methods have been developed, but few have the ability to simulate the long time scale limit and to accurately model the microscopic effects of nano-scale systems at the same time. We develop a new Monte Carlo method for calculating the dynamics of magnetic reversal at arbitrary long time. For example, actual calculations were performed up to 1050 Monte Carlo steps. This method is based on microscopic interactions of many constituents and the master equation for magnetic probability distribution function is solved symbolically. © 2005 Elsevier B.V. All rights reserved.
dc.description.urihttp://libproxy1.nus.edu.sg/login?url=http://dx.doi.org/10.1016/j.cpc.2004.11.006
dc.sourceScopus
dc.subjectDynamics
dc.subjectMagnetic reversal
dc.subjectMaster equation
dc.subjectMonte Carlo
dc.typeArticle
dc.contributor.departmentELECTRICAL & COMPUTER ENGINEERING
dc.description.doi10.1016/j.cpc.2004.11.006
dc.description.sourcetitleComputer Physics Communications
dc.description.volume168
dc.description.issue3
dc.description.page159-164
dc.description.codenCPHCB
dc.identifier.isiut000229984900002
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