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Reverse Monte Carlo (RMC) [1- | '''Reverse Monte Carlo''' (RMC) <ref>[http://dx.doi.org/10.1080/08927028808080958 R. L. McGreevy and L. Pusztai, "Reverse Monte Carlo Simulation: A New Technique for the Determination of Disordered Structures", Molecular Simulation, '''1''' pp. 359-367 (1988)]</ref> is a variation of the standard [[Metropolis Monte Carlo]] method. It is used to produce a 3 dimensional atomic [[models |model]] that fits a set of measurements (neutron diffraction, X-ray-diffraction, EXAFS etc.). | ||
In addition to measured data a number of constraints based on prior knowledge of the system ( | In addition to measured data a number of constraints based on prior knowledge of the system (for example, chemical bonding etc.) can be applied. Some examples are: | ||
*Closest approach between atoms ([[hard sphere model |hard sphere potential]]) | |||
*Coordination numbers. | |||
*Angles in triplets of atoms. | |||
The 3 dimensional structure that is produced by | The 3 dimensional structure that is produced by reverse Monte Carlo is not unique; it is a model consistent with the data and constraints provided. | ||
The algorithm for | The algorithm for reverse Monte Carlo can be written as follows: | ||
#Start with a configuration of atoms with periodic boundary conditions. This can be a random or a crystalline configuration from a different simulation or model. | #Start with a configuration of atoms with [[periodic boundary conditions]]. This can be a random or a crystalline configuration from a different simulation or model. | ||
#Calculate the total radial distribution function <math>g_o^C(r)</math> for this old configuration (''C''=Calculated, ''o''=Old). | #Calculate the total [[radial distribution function]] <math>g_o^C(r)</math> for this old configuration (''C''=Calculated, ''o''=Old). | ||
#Transform to the total structure factor: | #Transform to the total [[Structure factor | structure factor]]: | ||
#:<math>S_o^C (Q)-1=\frac{4\pi\rho}{Q}\int\limits_{0}^{\infty} r(g_o^C(r)-1)\sin(Qr)\, dr</math> | #:<math>S_o^C (Q)-1=\frac{4\pi\rho}{Q}\int\limits_{0}^{\infty} r(g_o^C(r)-1)\sin(Qr)\, dr</math> | ||
#:where ''Q'' is the momentum transfer and <math>\rho</math> the number density. | #:where ''Q'' is the momentum transfer and <math>\rho</math> the number density. | ||
#Calculate the difference between the measured structure factor <math>S^E(Q)</math> and the one calculated from the configuration <math>S_o^C(Q)</math>: | #Calculate the difference between the measured structure factor <math>S^E(Q)</math> (''E''=Experimental) and the one calculated from the configuration <math>S_o^C(Q)</math>: | ||
#:<math>\chi_o^2=\sum_i(S_o^C(Q_i)-S^E(Q_i))^2/\sigma(Q_i)^2</math> | #:<math>\chi_o^2=\sum_i(S_o^C(Q_i)-S^E(Q_i))^2/\sigma(Q_i)^2</math> | ||
#:this sum is taken over all experimental points <math>\sigma</math> is the experimental error. | #:this sum is taken over all experimental points <math>\sigma</math> is the experimental error. | ||
#Select and move one atom at random and calculate the new (''n''=New) distribution function, structure factor and: | #Select and move one atom at random and calculate the new (''n''=New) distribution function, structure factor and: | ||
#:<math>\chi_n^2=\sum_i(S_n^C(Q_i)-S^E(Q_i))^2/\sigma(Q_i)^2</math> | #:<math>\chi_n^2=\sum_i(S_n^C(Q_i)-S^E(Q_i))^2/\sigma(Q_i)^2</math> | ||
#If <math>\chi_n^2<\chi_o^2</math> accept the move and let the new configuration become the old. If <math>\chi_n^2 | #If <math>\chi_n^2<\chi_o^2</math> accept the move and let the new configuration become the old. If <math>\chi_n^2 \geq \chi_o^2</math> then the move is accepted with probability <math>\exp(-(\chi_n^2-\chi_0^2)/2)</math> otherwise it is rejected. | ||
#repeat from step 5. | #repeat from step 5. | ||
When <math>\chi^2</math> have reached an equilibrium the configuration is saved and can be analysed. | When <math>\chi^2</math> have reached an equilibrium the configuration is saved and can be analysed. | ||
== References == | |||
<references/> | |||
;Related reading | |||
*[http://dx.doi.org/10.1088/0953-8984/13/46/201 R. L. McGreevy, "Reverse Monte Carlo modelling", Journal of Physics: Condensed Matter '''13''' pp. R877-R913 (2001)] | |||
*[http://dx.doi.org/10.1016/S1359-0286(03)00015-9 R. L. McGreevy and P. Zetterström, "To RMC or not to RMC? The use of reverse Monte Carlo modelling", Current Opinion in Solid State and Materials Science. '''7''' pp. 41-47 (2003)] | |||
*[http://dx.doi.org/10.1088/0953-8984/17/5/001 G. Evrard, L. Pusztai, "Reverse Monte Carlo modelling of the structure of disordered materials with RMC++: a new implementation of the algorithm in C++", Journal of Physics: Condensed Matter '''17''' pp. S1-S13 (2005)] | |||
*[http://dx.doi.org/10.1016/j.molliq.2015.02.044 V. Sánchez-Gil, E. G. Noya, L. Temleitner, L. Pusztai "Reverse Monte Carlo modeling: The two distinct routes of calculating the experimental structure factor", Journal of Molecular Liquids '''207''' pp. 211-215 (2015)] | |||
[[Category:Monte Carlo]] | |||
Latest revision as of 17:57, 25 May 2015
Reverse Monte Carlo (RMC) [1] is a variation of the standard Metropolis Monte Carlo method. It is used to produce a 3 dimensional atomic model that fits a set of measurements (neutron diffraction, X-ray-diffraction, EXAFS etc.). In addition to measured data a number of constraints based on prior knowledge of the system (for example, chemical bonding etc.) can be applied. Some examples are:
- Closest approach between atoms (hard sphere potential)
- Coordination numbers.
- Angles in triplets of atoms.
The 3 dimensional structure that is produced by reverse Monte Carlo is not unique; it is a model consistent with the data and constraints provided.
The algorithm for reverse Monte Carlo can be written as follows:
- Start with a configuration of atoms with periodic boundary conditions. This can be a random or a crystalline configuration from a different simulation or model.
- Calculate the total radial distribution function for this old configuration (C=Calculated, o=Old).
- Transform to the total structure factor:
- where Q is the momentum transfer and the number density.
- Calculate the difference between the measured structure factor (E=Experimental) and the one calculated from the configuration :
- this sum is taken over all experimental points is the experimental error.
- Select and move one atom at random and calculate the new (n=New) distribution function, structure factor and:
- If accept the move and let the new configuration become the old. If then the move is accepted with probability otherwise it is rejected.
- repeat from step 5.
When have reached an equilibrium the configuration is saved and can be analysed.
References[edit]
- Related reading
- R. L. McGreevy, "Reverse Monte Carlo modelling", Journal of Physics: Condensed Matter 13 pp. R877-R913 (2001)
- R. L. McGreevy and P. Zetterström, "To RMC or not to RMC? The use of reverse Monte Carlo modelling", Current Opinion in Solid State and Materials Science. 7 pp. 41-47 (2003)
- G. Evrard, L. Pusztai, "Reverse Monte Carlo modelling of the structure of disordered materials with RMC++: a new implementation of the algorithm in C++", Journal of Physics: Condensed Matter 17 pp. S1-S13 (2005)
- V. Sánchez-Gil, E. G. Noya, L. Temleitner, L. Pusztai "Reverse Monte Carlo modeling: The two distinct routes of calculating the experimental structure factor", Journal of Molecular Liquids 207 pp. 211-215 (2015)