Abstract:A method is presented to analyze and observe, in molecular dynamic simulations, the statistical properties of instantaneous cluster transitions, mainly fusions and fissions for a homogeneous vapor at equilibrium. The method yields the way to obtain mean lives, branching ratios and, to some extent, transition rates as well. To the best of our knowledge branching rations in cluster decays have not been measured before (simulationally or experimentally). An application of this method to a model system provides a … Show more
“…Soto and Cordero [19] have developed Hill's criterion, and Barrett [16] has performed Monte Carlo modelling of molecular configurations, excluding those which decay in molecular dynamics within a suitable period. The idea of introducing a residence time has also been discussed by both Bahadur and McClurg [20] and Pugnaloni and Vericat [21].…”
Molecular configurations which count as snapshots of a quasi-bound cluster are identified through a retrospective dynamical definition. The trajectory of a molecular cluster is followed, and a clear evaporation event is considered to have occurred when a molecule moves a very long distance away from the others. The cluster is judged to have broken before this condition is satisfied, however, at the instant that the energy of the departing molecule in the centre of mass frame becomes positive. The decay of a cluster is therefore defined dynamically as the production of a molecule with positive energy on a separating trajectory. Not all positive energy molecules created by the system follow such a trajectory, hence the need to examine the subsequent behaviour in molecular dynamics. We simulate a sequence of decays by repairing broken clusters as they occur. This approach enables us to calculate mean decay rates of isolated Lennard-Jones clusters in what promises to be a physically realistic fashion.
“…Soto and Cordero [19] have developed Hill's criterion, and Barrett [16] has performed Monte Carlo modelling of molecular configurations, excluding those which decay in molecular dynamics within a suitable period. The idea of introducing a residence time has also been discussed by both Bahadur and McClurg [20] and Pugnaloni and Vericat [21].…”
Molecular configurations which count as snapshots of a quasi-bound cluster are identified through a retrospective dynamical definition. The trajectory of a molecular cluster is followed, and a clear evaporation event is considered to have occurred when a molecule moves a very long distance away from the others. The cluster is judged to have broken before this condition is satisfied, however, at the instant that the energy of the departing molecule in the centre of mass frame becomes positive. The decay of a cluster is therefore defined dynamically as the production of a molecule with positive energy on a separating trajectory. Not all positive energy molecules created by the system follow such a trajectory, hence the need to examine the subsequent behaviour in molecular dynamics. We simulate a sequence of decays by repairing broken clusters as they occur. This approach enables us to calculate mean decay rates of isolated Lennard-Jones clusters in what promises to be a physically realistic fashion.
“…assuming the integration limits do not depend on r 1 . Fortunately, the second term on the right hand side of equation (19) can be simplified. We represent the derivative of the delta function as the limit of…”
Section: B the Potential Of Mean Force In Statistical Mechanicsmentioning
confidence: 99%
“…Implicit in any microscopic theory of nucleation, however, is the need for a clear definition of what is meant by a cluster. This is a subtle matter, and one which has received considerable attention 6,7,[15][16][17][18][19][20][21][22][23][24][25][26] . Intuitively, a cluster should comprise a set of molecules located close to one another.…”
Section: Introductionmentioning
confidence: 99%
“…We have recently developed a definition of a cluster involving energy rather than position 24 . It is widely recognised that an energetic rather than a positional criterion is an indicator of a quasi-bound structure 19,23,27 . We have added the essential feature that in order to escape from a cluster, a molecule needs not only to acquire positive energy, through thermal fluctuations, but must also be able to move away from the cluster, avoiding recapture.…”
We show that evaporation from a quasistable molecular cluster may be treated as a kinetic problem involving the stochastically driven escape of a molecule from a potential of mean force. We derive expressions for the decay rate, and a relationship between the depth of the potential and the change in system free energy upon loss of a molecule from the cluster. This establishes a connection between kinetic and thermodynamic treatments of evaporation, but also reveals differences in the prefactor in the rate expression. We perform constant energy molecular dynamics simulations of cluster dynamics to calculate potentials of mean force, friction coefficients and effective temperatures for use in the kinetic analysis, and to compare the results with the directly observed escape rates. We also use the simulations to estimate the escape rates by a probabilistic analysis. It is much more efficient to calculate the decay rate by the methods we have developed than it is to monitor escape directly, making these approaches potentially useful for the assessment of molecular cluster stability.
“…This point of view is fundamental for classical nucleation theory, but has also been adopted in early computational investigations [8], followed by many others [9][10][11][12], for its relevance in many areas and primarily in atmospheric science. At equilibrium, the homogeneous nucleation equilibrium can be summarized by the reactions…”
Section: Main Assumptions and Steady-state Hypothesismentioning
Abstract. An overview of the physics of homogeneous nucleation is presented, focusing on the main theoretical approaches that are currently available. We review the microscopic assumptions behind classical nucleation theory, as well as several improvements with various degrees of empiricism. The increasing role played by molecular simulations in testing and correcting nucleation theories is discussed. Typical laboratory experiments on homogeneous nucleation are also reviewed, emphasizing how experimental observables can be compared with theoretical predictions. Finally, the more specific challenges of nucleation in astrophysical media are discussed.
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