JARVIS-FF NIST Disclaimer

Structural formula: C

Force-field: Fe-C_Hepburn_Ackland.eam.fs

Space group : Cmmm

JARVIS ID: JLMP-1517

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

1551.1 2663.2 2642.2 -0.0 -0.0 -0.0
2663.2 5350.0 5255.2 -0.0 0.0 -0.0
2642.2 5255.2 5527.0 -0.0 0.0 -0.0
-0.0 -0.0 -0.0 101.7 0.0 -0.0
-0.0 0.0 0.0 0.0 39.6 0.0
-0.0 -0.0 -0.0 -0.0 0.0 195227.7

Bv: 3727.7 GPa

Gv: 39198.3 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
C 4 116.01 Download cif file
C 4 98.039 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 2 0) -3.233 Download cif file
(1 1 0) -3.172 Download cif file
(3 1 0) -3.122 Download cif file
(3 2 0) -2.973 Download cif file
(1 0 0) -2.938 Download cif file
(2 1 0) -2.531 Download cif file
(2 3 0) -2.381 Download cif file
(1 3 0) -1.944 Download cif file
(3 0 1) -1.299 Download cif file
(3 1 1) -1.159 Download cif file
(1 0 3) -1.149 Download cif file
(3 2 1) -0.839 Download cif file
(0 0 1) -0.835 Download cif file
(2 0 1) -0.817 Download cif file
(1 0 2) -0.627 Download cif file
(2 1 1) -0.525 Download cif file
(2 0 3) -0.502 Download cif file
(3 0 2) -0.404 Download cif file
(0 1 3) -0.345 Download cif file
(2 2 1) -0.298 Download cif file
(0 1 2) -0.296 Download cif file
(3 3 1) -0.284 Download cif file
(3 2 2) -0.184 Download cif file
(2 3 1) -0.057 Download cif file
(0 2 3) -0.056 Download cif file
(0 1 1) -0.017 Download cif file
(1 0 1) -0.012 Download cif file
(3 2 3) 0.007 Download cif file
(2 1 3) 0.097 Download cif file
(3 1 2) 0.124 Download cif file
(0 3 2) 0.155 Download cif file
(1 1 3) 0.163 Download cif file
(1 2 1) 0.203 Download cif file
(1 2 3) 0.209 Download cif file
(3 1 3) 0.21 Download cif file
(0 3 1) 0.228 Download cif file
(2 3 2) 0.335 Download cif file
(1 2 2) 0.366 Download cif file
(2 1 2) 0.37 Download cif file
(2 2 3) 0.377 Download cif file
(0 1 0) 0.4 Download cif file
(1 1 2) 0.44 Download cif file
(3 3 2) 0.516 Download cif file
(2 3 3) 0.546 Download cif file
(1 3 3) 0.548 Download cif file
(0 2 1) 0.766 Download cif file
(1 1 1) 1.075 Download cif file
(1 3 2) 1.301 Download cif file
(1 3 1) 1.72 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
-111.411015154 B3g R
-0.1527920964 B1u I
-0.1494532653 B2u I
-0.1281093063 B3u I
351.33060008 B3g R
365.144194863 B2u I
371.661759611 B2g R
1145.33535574 Ag R
1286.39267475 B3u I
1306.99733374 B2g R
2720.2803874 Ag R
2864.30346667 B1u I
All phonon mode at Gamma point (cm-1)
-111.411015154
-104.288309453
-0.1527921006
-0.149453265
-0.1281093047
89.2448586085
194.700376688
290.540298865
312.883946861
351.33060008
365.144194863
371.661759611
403.545261894
1145.33535574
1286.39267475
1291.7472721
1302.59931496
1306.99733374
1389.78225404
2013.63597406
2203.05311924
2465.01220955
2720.2803874
2864.30346667

See also

Links to other databases or papers are provided below

JVASP-25054

mp-1008374

Energy above hull from mp (eV): 0.43726209875