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Structural formula: C

Force-field: Fe-C_Hepburn_Ackland.eam.fs

Space group : P6_3/mmc

JARVIS ID: JLMP-1532

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

6112.4 5854.3 5964.8 0.0 -0.0 -37.3
5854.3 6112.4 5964.8 0.0 -0.0 0.0
5964.8 5964.8 6494.0 0.0 -0.0 0.0
0.0 0.0 0.0 112.7 0.0 -0.0
-0.0 -0.0 -0.0 0.0 112.7 0.0
-37.3 0.0 0.0 -0.0 0.0 129.1

Bv: 6031.8 GPa

Gv: 133.2 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 -1.922 Download cif file
C 4 -1.819 Download cif file
C 4 -1.925 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.

Visualize Phonons here
Phonon mode (cm-1) Representation
-0.0102758683 A2u I
-0.0010394866 E1u I
152.462185232 E2u
155.10056684 E2g R
269.373006121 E1g R
272.663958433 E1u I
316.00663892 E2u
950.928885206 E2g R
956.541446857 E1u I
964.554903141 E1g R
973.033603038 E2u
986.214886107 E2g R
989.240055546 E1g R
996.59432159 A1g R
1165.15638109 B1u
1168.76702741 B2g
1478.97658657 B1u
1483.14645877 B2g
2027.88468002 A1g R
2028.65338162 A2u I
2132.82596194 A1g R
2140.87630484 A2u I
2360.84642522 B2g
2380.95615972 B1u
All phonon mode at Gamma point (cm-1)
-0.0102758683
-0.0010404542
-0.0010382888
152.462185232
152.462186713
155.10056684
155.100567965
269.373006121
269.373007309
272.663958433
272.663959157
316.00663892
316.006639626
950.928885206
950.928888888
956.541446857
956.541450217
964.554903141
964.554907782
973.033603038
973.033606049
986.214886107
986.214894703
989.240055546
989.240062608
996.59432159
1165.15638109
1168.76702741
1478.97658657
1483.14645877
2027.88468002
2028.65338162
2132.82596194
2140.87630484
2360.84642522
2380.95615972

See also

Links to other databases or papers are provided below

JVASP-25275

mp-611448

Energy above hull from mp (eV): 0.14202627625