\(\renewcommand{\AA}{\text{Å}}\)
pair_style ilp/graphene/hbn command
Accelerator Variant: ilp/graphene/hbn/opt
Syntax
pair_style [hybrid/overlay ...] ilp/graphene/hbn cutoff tap_flag
cutoff = global cutoff (distance units)
tap_flag = 0/1 to turn off/on the taper function
Examples
pair_style hybrid/overlay ilp/graphene/hbn 16.0 1
pair_coeff * * ilp/graphene/hbn BNCH.ILP B N C
pair_style hybrid/overlay rebo tersoff ilp/graphene/hbn 16.0 coul/shield 16.0
pair_coeff * * rebo CH.rebo NULL NULL C
pair_coeff * * tersoff BNC.tersoff B N NULL
pair_coeff * * ilp/graphene/hbn BNCH.ILP B N C
pair_coeff 1 1 coul/shield 0.70
pair_coeff 1 2 coul/shield 0.695
pair_coeff 2 2 coul/shield 0.69
Description
The ilp/graphene/hbn style computes the registry-dependent interlayer potential (ILP) potential as described in (Leven1), (Leven2) and (Maaravi). The normals are calculated in the way as described in (Kolmogorov).
Where \(\mathrm{Tap}(r_{ij})\) is the taper function which provides a continuous cutoff (up to third derivative) for interatomic separations larger than \(r_c\) (Maaravi). The definitions of each parameter in the above equation can be found in (Leven1) and (Maaravi).
It is important to include all the pairs to build the neighbor list for calculating the normals.
Note
This potential (ILP) is intended for interlayer interactions between two different layers of graphene, hexagonal boron nitride (h-BN) and their hetero-junction. To perform a realistic simulation, this potential must be used in combination with intralayer potential, such as AIREBO or Tersoff potential. To keep the intralayer properties unaffected, the interlayer interaction within the same layers should be avoided. Hence, each atom has to have a layer identifier such that atoms residing on the same layer interact via the appropriate intralayer potential and atoms residing on different layers interact via the ILP. Here, the molecule id is chosen as the layer identifier, thus a data file with the “full” atom style is required to use this potential.
The parameter file (e.g. BNCH.ILP), is intended for use with metal units, with energies in meV. Two additional parameters, S, and rcut are included in the parameter file. S is designed to facilitate scaling of energies. rcut is designed to build the neighbor list for calculating the normals for each atom pair.
Note
The parameters presented in the parameter file (e.g. BNCH.ILP), are fitted with taper function by setting the cutoff equal to 16.0 Angstrom. Using different cutoff or taper function should be careful. The parameters for atoms pairs between Boron and Nitrogen are fitted with a screened Coulomb interaction coul/shield. Therefore, to simulated the properties of h-BN correctly, this potential must be used in combination with the pair style coul/shield.
Note
Four new sets of parameters of ILP for 2D layered Materials with bilayer and bulk configurations are presented in (Ouyang1) and (Ouyang2), respectively. These parameters provide a good description in both short- and long-range interaction regimes. While the old ILP parameters published in (Leven2) and (Maaravi) are only suitable for long-range interaction regime. This feature is essential for simulations in high pressure regime (i.e., the interlayer distance is smaller than the equilibrium distance). The benchmark tests and comparison of these parameters can be found in (Ouyang1) and (Ouyang2).
This potential must be used in combination with hybrid/overlay. Other interactions can be set to zero using pair_style none.
This pair style tallies a breakdown of the total interlayer potential energy into sub-categories, which can be accessed via the compute pair command as a vector of values of length 2. The 2 values correspond to the following sub-categories:
E_vdW = vdW (attractive) energy
E_Rep = Repulsive energy
To print these quantities to the log file (with descriptive column headings) the following commands could be included in an input script:
compute 0 all pair ilp/graphene/hbn
variable Evdw equal c_0[1]
variable Erep equal c_0[2]
thermo_style custom step temp epair v_Erep v_Evdw
Styles with a gpu, intel, kk, omp, or opt suffix are functionally the same as the corresponding style without the suffix. They have been optimized to run faster, depending on your available hardware, as discussed on the Accelerator packages page. The accelerated styles take the same arguments and should produce the same results, except for round-off and precision issues.
These accelerated styles are part of the GPU, INTEL, KOKKOS, OPENMP, and OPT packages, respectively. They are only enabled if LAMMPS was built with those packages. See the Build package page for more info.
You can specify the accelerated styles explicitly in your input script by including their suffix, or you can use the -suffix command-line switch when you invoke LAMMPS, or you can use the suffix command in your input script.
See the Accelerator packages page for more instructions on how to use the accelerated styles effectively.
Mixing, shift, table, tail correction, restart, rRESPA info
This pair style does not support the pair_modify mix, shift, table, and tail options.
This pair style does not write their information to binary restart files, since it is stored in potential files. Thus, you need to re-specify the pair_style and pair_coeff commands in an input script that reads a restart file.
Restrictions
This pair style is part of the INTERLAYER package. It is only enabled if LAMMPS was built with that package. See the Build package page for more info.
This pair style requires the newton setting to be on for pair interactions.
The BNCH.ILP potential file provided with LAMMPS (see the potentials directory) are parameterized for metal units. You can use this potential with any LAMMPS units, but you would need to create your own custom BNCH.ILP potential file with coefficients listed in the appropriate units, if your simulation does not use metal units.
Default
tap_flag = 1
(Ouyang1) W. Ouyang, D. Mandelli, M. Urbakh and O. Hod, Nano Lett. 18, 6009-6016 (2018).
(Ouyang2) W. Ouyang et al., J. Chem. Theory Comput. 16(1), 666-676 (2020).
(Leven1) I. Leven, I. Azuri, L. Kronik and O. Hod, J. Chem. Phys. 140, 104106 (2014).
(Leven2) I. Leven et al, J. Chem.Theory Comput. 12, 2896-905 (2016).
(Maaravi) T. Maaravi et al, J. Phys. Chem. C 121, 22826-22835 (2017).
(Kolmogorov) A. N. Kolmogorov, V. H. Crespi, Phys. Rev. B 71, 235415 (2005).