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Structural formula: Al3Ni2

Force-field: Mishin-Ni-Al-Co-2013.eam.alloy

Space group : P-3m1

JARVIS ID: JLMP-1264

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

204.1 112.3 74.1 -10.4 3.0 -13.2
112.3 204.1 74.1 10.4 -0.0 -0.0
74.1 74.1 228.9 0.0 0.0 -0.0
-10.4 10.4 0.0 46.1 -0.0 0.0
3.0 -0.0 0.0 -0.0 46.1 -10.4
-13.2 -0.0 -0.0 0.0 -10.4 45.9

Bv: 128.7 GPa

Gv: 52.7 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
Al 1 1.794 Download cif file
Al 2 1.89 Download cif file
Ni 2 2.71 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
-0.0002004503 None
178.960025259 Eg R
180.427977675 A2u I
183.906314473 A1g R
230.286887387 Eu I
310.679742724 Eg R
344.789721278 A2u I
360.496437858 Eu I
371.176116435 A1g R
All phonon mode at Gamma point (cm-1)
-0.0002004608
-8.2398e-05
-4.10362e-05
178.960025259
178.960025662
180.427977675
183.906314473
230.286887387
230.286888005
310.679742724
310.679743553
344.789721278
360.496437858
360.496644519
371.176116435

See also

Links to other databases or papers are provided below

JVASP-11950

mp-1057

Energy above hull from mp (eV): 0.0