JARVIS-FF NIST Disclaimer

Structural formula: Fe2C

Force-field: Fe-C_Hepburn_Ackland.eam.fs

Space group : Pnnm

JARVIS ID: JLMP-1555

Download input files

Elastic tensor (GPa)

Elastic tensor for the conventional cell of the system were calculated with LAMMPS in.elastic script at 0 K [Source] . Similar script can be used for temperature dependent elastic constants and will be available here soon. WARNING! Please note that the starting lattice parameters of crystal structures were taken from density functional theory (DFT) and not from experiments. Generic minimization parameters were chosen for LAMMPS run rather than testing them for each individual case such as energy convergence criterion and so on. Hence, there are chances that the calculation gets trapped in a local energy minima. Please read carefully the assumptions taken during calculations in the in.elastic script and use the data at your own risk

1928.3 1221.9 1796.1 0.0 0.0 0.0
1221.9 2332.0 3284.4 0.0 0.0 0.0
1796.1 3284.4 5337.3 -0.0 -0.0 -0.0
0.0 0.0 -0.0 1147.2 -0.0 -0.0
0.0 0.0 -0.0 -0.0 867.2 0.0
0.0 0.0 -0.0 -0.0 0.0 849.8

Bv: 2466.9 GPa

Gv: 792.5 GPa

Vacancy-formation energy (eV)

Vacancy formation energies were calculated by deleting the symmterically distinct atoms in the system [Source]. In the table, vacancy forming element, its multiplicity, and defect-formation energy are given. The reference element cohesive energies were calculated with the most stable structure for the element found on materials project database. Defect structures were constructed with the fully-relaxed bulk system as input. For defect-structures energetics calculations, constant volume ensemble was used. We impose the defect structures to be at least 1.5 nm large in all directions.

Element Mult. Value
Fe 4 4.191 Download cif file
C 2 3.003 Download cif file

Surface energy (J/m2)

Surface energies were calculated for symmterically distinct crystal surfaces . In the table, (hkl) indices and surface enegies are given. For surface-structure energetics, constant volume ensemble was used. We impose the slab thickness to be at least 2 nm and vaccum size of 2.5 nm. The maximum miller index is taken as 3.

Surface Value
(1 0 1) 2.256 Download cif file
(2 1 2) 2.344 Download cif file
(3 2 3) 2.35 Download cif file
(2 1 3) 2.373 Download cif file
(1 0 0) 2.377 Download cif file
(0 1 1) 2.398 Download cif file
(3 0 1) 2.401 Download cif file
(3 3 2) 2.424 Download cif file
(3 0 2) 2.436 Download cif file
(3 1 3) 2.437 Download cif file
(2 3 3) 2.443 Download cif file
(2 2 1) 2.454 Download cif file
(0 0 1) 2.474 Download cif file
(1 1 3) 2.48 Download cif file
(1 1 0) 2.482 Download cif file
(3 1 0) 2.488 Download cif file
(3 2 2) 2.492 Download cif file
(0 2 1) 2.494 Download cif file
(2 0 3) 2.508 Download cif file
(1 0 3) 2.509 Download cif file
(3 1 2) 2.512 Download cif file
(2 0 1) 2.513 Download cif file
(1 2 1) 2.523 Download cif file
(1 2 2) 2.533 Download cif file
(3 3 1) 2.541 Download cif file
(2 1 1) 2.552 Download cif file
(3 2 1) 2.556 Download cif file
(3 2 0) 2.556 Download cif file
(1 0 2) 2.559 Download cif file
(3 1 1) 2.567 Download cif file
(2 1 0) 2.57 Download cif file
(2 3 1) 2.571 Download cif file
(2 3 0) 2.58 Download cif file
(1 2 0) 2.592 Download cif file
(0 1 3) 2.594 Download cif file
(1 2 3) 2.604 Download cif file
(2 3 2) 2.615 Download cif file
(1 3 2) 2.621 Download cif file
(0 3 1) 2.628 Download cif file
(1 3 3) 2.633 Download cif file
(0 1 2) 2.654 Download cif file
(1 1 2) 2.654 Download cif file
(2 2 3) 2.657 Download cif file
(1 3 1) 2.685 Download cif file
(0 1 0) 2.732 Download cif file
(0 3 2) 2.791 Download cif file
(1 1 1) 2.865 Download cif file
(0 2 3) 2.893 Download cif file
(1 3 0) 2.987 Download cif file

Phonon

Phonons were obtained by making an interface of JARVIS-FF with Phonopy package at 0 K [Source] . For deformed-structures, constant volume ensemble was used. The deofrmed structures were taken of at least 1.5 nm size in all directions. The band-indices for phonon bandstructure was obtained with Pymatgen. The phonon representation were obtained with phonopy. "I" and "R" denotes infrared and Raman active modes respectively

Visualize Phonons here
Phonon mode (cm-1) Representation
-0.3357298884 B1u I
-0.2477697278 B2u I
-0.1458104597 B3u I
234.393686321 B2u I
352.046033847 B1u I
487.070374856 Ag R
502.595893803 Au
508.37064382 B3g R
1135.12820359 B1g R
1136.44872577 B2g R
1962.63994345 Ag R
1968.32087495 B3g R
3608.06180457 Au
3641.51260137 B3u I
4119.04864092 B2u I
4292.86344731 B1u I
4815.57917763 B1u I
4972.26780609 B2u I
All phonon mode at Gamma point (cm-1)
-0.3357298886
-0.2477697278
-0.1458104319
234.393686321
352.046033847
487.070374856
502.595893803
508.37064382
1135.12820359
1136.44872577
1962.63994345
1968.32087495
3608.06180457
3641.51260137
4119.04864092
4292.86344731
4815.57917763
4972.26780609

See also

Links to other databases or papers are provided below

JVASP-20482

mp-1871

Energy above hull from mp (eV): 0.0579305170833