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Structural formula: Zr2Ni

Force-field: Ni-Zr_Mendelev_2014.eam.fs

Space group : I4/mcm

JARVIS ID: JLMP-1670

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

292.2 184.6 179.4 0.0 -0.0 0.0
184.6 292.2 179.4 -0.0 -0.0 -0.0
179.4 179.4 305.5 -0.0 0.0 -0.0
0.0 -0.0 -0.0 66.8 0.0 -0.0
-0.0 -0.0 0.0 0.0 66.8 0.0
0.0 -0.0 -0.0 -0.0 0.0 53.8

Bv: 219.6 GPa

Gv: 60.6 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
Zr 8 4.469 Download cif file
Ni 4 1.983 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
-0.0001364655 None
130.377838469 B1g R
148.221514082 A2u I
150.362242702 A2g
150.411059305 Eg R
156.289948622 Eu I
166.570288127 B1u
172.555564842 A1g R
198.971430965 B2g R
202.745471498 Eg R
213.93764995 Eu I
233.40616355 A2g
All phonon mode at Gamma point (cm-1)
-0.0001364914
-9.49344e-05
-9.47839e-05
106.248619043
120.626318074
122.812993403
130.377838469
130.490833535
133.261597698
139.156999114
148.221514082
150.362242702
150.411059305
156.289948622
160.470826193
166.570288127
172.555564842
175.315216252
198.104019327
198.971430965
202.745471498
204.035545596
206.429669131
213.93764995
217.485182407
229.525450389
233.40616355

See also

Links to other databases or papers are provided below

JVASP-14657

mp-328

Energy above hull from mp (eV): 0.0