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Structural formula: CuAg3

Force-field: cu_ag_ymwu.eam.alloy

Space group : P6_3/mmc

JARVIS ID: JLMP-1143

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

260.8 137.9 86.6 -0.0 -0.0 17.7
137.9 260.8 86.6 0.0 0.0 -0.0
86.6 86.6 200.6 0.0 -0.0 0.0
-0.0 0.0 0.0 4.4 -0.0 0.0
-0.0 0.0 -0.0 -0.0 4.4 -0.0
17.7 -0.0 0.0 0.0 -0.0 61.5

Bv: 149.4 GPa

Gv: 41.5 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
Cu 2 1.934 Download cif file
Ag 6 0.657 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
-0.0003666326 None
22.6496670195 None
82.3634162992 B2g
85.5556300353 None
86.5194340269 None
98.6138073979 None
98.6368420618 None
107.334302326 None
108.026955043 None
110.240140676 A2u I
126.738196259 None
127.375244481 None
128.53443298 None
180.024678024 None
180.066687531 None
203.58766312 None
204.104519615 None
204.788309681 None
205.254916562 None
220.121074716 B2g
254.78257938 None
268.021238148 A1g R
All phonon mode at Gamma point (cm-1)
-0.0003666445
-0.0001759712
-0.0001302796
22.6496670195
82.3634162992
85.5556300353
86.5194340269
98.6138073979
98.6368420618
107.334302326
108.026955043
110.240140676
126.738196259
127.375244481
128.53443298
180.024678024
180.066687531
203.58766312
204.104519615
204.788309681
205.254916562
220.121074716
254.78257938
268.021238148

See also

Links to other databases or papers are provided below

JVASP-37857

mp-984351

Energy above hull from mp (eV): 0.08548408625