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xxiii πανελληνιο συνεδριο φυσικης στερεας καταστασης & επιστημης ...

xxiii πανελληνιο συνεδριο φυσικης στερεας καταστασης & επιστημης ...

xxiii πανελληνιο συνεδριο φυσικης στερεας καταστασης & επιστημης ...

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Grand Canonical Monte Carlo Method for Predicting Hydrogen Adsorption<br />

Tyllianakis Emmanuel 1* , Klontzas Emmanuel 2 , Dimitrakakis K. Georgios 2 , Mpourmpakis Giannis 2 and Frudakis George E. 2<br />

1 Material Science and Technology Department, University of Crete, P.O. Box 2208, Heraklion, Crete, 71003, Greece<br />

2 Department of Chemistry, University of Crete, P.O. Box 2208, Heraklion, Crete, 71003, Greece<br />

*tilman@materials.uoc.gr<br />

A lot effort has been devoted for the study of interaction between hydrogen and nanostructures, in an effort for the hydrogen<br />

uptake to be calculated. From theoretical point of view, the only way to study this hydrogen adsorption is the Grand<br />

Canonical Monte Carlo method, since it permits the total number of particles adsorbed to fluctuate, whereas the chemical<br />

potential, μ, the cell volume, V, and the temperature, T, are kept constant i.e. (μ, V, T) ensemble. In this way, the pressure<br />

and temperature experimental conditions can be simulated, since the chemical potential is explicitly calculated for the<br />

specific thermodynamic state.<br />

Three types of motions occur during the simulation i.e. particle displacement, creation, and destruction. These different<br />

steps are executed with equal frequency. In a creation step, the position of the new particle is chosen randomly within pore<br />

volume V and its potential energy U is calculated. Finally these steps are accepted with the probability min(1; P) with<br />

⎛ U − μ ⎞ V<br />

⎛U<br />

− μ N<br />

P = exp<br />

⎜−<br />

⎟<br />

P<br />

creation<br />

destruction<br />

⎝ kBT<br />

⎠ N + 1<br />

k<br />

BT<br />

⎟ ⎞<br />

⎛ U1<br />

−U<br />

2<br />

⎞<br />

= exp<br />

⎜<br />

P =<br />

⎝ ⎠ V<br />

⎜−<br />

⎟<br />

displacement<br />

exp<br />

⎝ k<br />

BT<br />

⎠<br />

Prior to the GCMC simulation, the exact value of chemical potential for the specific thermodynamic condition is needed, as<br />

referred earlier. For that purpose the Widom test particle method [1] is implemented for bulk hydrogen, at densities that<br />

correspond to that condition. The basic idea of this method is to try to insert at regular intervals, a particle at a random<br />

position. The particle is assumed to have no difference on the rest of the system, but it has an energy, the average of which is<br />

used for the calculation of chemical potential.<br />

The correct form of the function that describes the non-bonded interactions is the central point of this method and to that<br />

direction a lot of classical effective potentials have been used. Among them the Lennard-Jones is the one, most widely used.<br />

According to this potential, the interaction between a pair of particles i and j separated by a distance r is given by the equation<br />

12<br />

6<br />

⎡⎛<br />

σ<br />

⎤<br />

ij<br />

⎞ ⎛σ<br />

ij<br />

⎞<br />

V ⎢⎜<br />

⎟ − ⎜ ⎟ ⎥<br />

ij<br />

= 4 ⋅ε<br />

ij<br />

⎢<br />

⎥<br />

⎣⎝<br />

rij<br />

⎠ ⎝ rij<br />

⎠ ⎦<br />

where i and j denote hydrogen or carbon particles. ε describes the potential depth and σ is the size potential parameters.<br />

Besides this potential, some other functions have also been used like the Silvera-Goldman [2], the Crowell-Brown [3] etc.<br />

The main disadvantage of these potentials is the use of uniform parameters for a given pair of heteroatoms and hence the<br />

absence of varying these values according to the particularities of the system under examination. For that purpose, Monte<br />

Carlo method has often to corporate with accurate ab initio methods for the exact value of these parameters to be calculated.<br />

In addition to these potential some other terms are used also to describe other kind of interactions like electrostatic<br />

interactions, or the contributions of quantum effects which have been proven to contribute significally [4] especially at lower<br />

temperatures.<br />

The application of GCMC methods allows us to compare the efficiency of different nano-structures to adsorb hydrogen and<br />

study the contributions of some factors to that uptake. In that sense, a variety of simulations on different systems has been<br />

performed, including from graphene sheets and carbon nanotubes, that were the first systems to attract the scientific interest<br />

concerning hydrogen uptake, to more novel materials proposed like carbon nanoscrolls and metal organic frameworks. Some<br />

representative results from these calculations can be seen at Figures 1-5.<br />

Figure 1: GCMC calculations for (9-9) nanotube arrays with 0.7 nm intertube distance at pressure of 10 MPa and<br />

temperatures of 77, 175 and 293 K.<br />

193

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