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Structural formula: ZrNi5

Force-field: Ni-Zr_Mendelev_2010.eam.fs

Space group : F-43m

JARVIS ID: JLMP-1630

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

257.5 102.6 102.6 0.0 -0.0 0.0
102.6 257.5 102.6 0.0 -0.0 0.0
102.6 102.6 257.5 0.0 -0.0 0.0
0.0 0.0 0.0 67.8 0.0 -0.0
-0.0 -0.0 -0.0 0.0 67.8 0.0
0.0 0.0 0.0 -0.0 0.0 67.8

Bv: 154.2 GPa

Gv: 71.7 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
Zr 4 5.19 Download cif file
Ni 4 -0.185 Download cif file
Ni 16 -0.705 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
-7.40312e-05 None
93.0156218488 None
122.919475684 None
177.274992383 None
204.254171153 None
254.403303831 None
350.694341086 A1 R
All phonon mode at Gamma point (cm-1)
-7.39476e-05
-7.38689e-05
-7.36897e-05
90.6759170606
93.0156218488
109.235333702
112.720507928
122.919475684
127.353146195
136.770853942
155.577593267
160.865040956
168.203481147
177.274992383
180.793004024
182.114917483
204.254171153
216.719276938
254.403303831
288.512255274
294.238879575
350.694341086

See also

Links to other databases or papers are provided below

JVASP-14553

mp-2439

Energy above hull from mp (eV): 0.000715927916661