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|  Convergence Behavior of Spin Moments in Noncollinear Magnetic Order. ~ energycutoff and Kgrid ~ |  | 
 Date: 2025/06/02 16:52
 Name: Soichiro Kikuchi
  <akatuki3329@gmail.com>
 
Dear developers,
 My report and question are about Convergence Behavior of Spin Magnetic Moments in Noncollinear Magnetic Order.
 
 I am trying to calculation the spin magnetic moment in noncollinear magnetic order, such as Mn₃Sn and Mn₃CuN."
 
 To investigate the convergence behavior of spin magnetic moments of Mn3Sn, I performed calculations using various values of energy cutoff and Kgrid.
 
 First, I fixed the k-point grid at 12~12~12 and examined the convergence with respect to the energy cutoff. The magnitude of the local spin magnetic moment on the magnetic atom Mn converged at an energy cutoff of around 400–500 Ryd.
 
 However, the total spin magnetic moment, in terms of both its magnitude and orientation, did not show clear convergence until the cutoff was increased to approximately 7000 Ryd, which is significantly higher than the typical values recommended in the manual.
 
 Next, keeping the energy cutoff fixed at 7000 Ryd, I varied the Kgrid to assess its influence. However, the results did not show a clear or systematic convergence behavior, and it became difficult to determine an appropriate Kgrid for reliable calculations.
 
 
 Below is an excerpt from the summary of the convergence results.
 
 ---------------------------------------------------------
 
 Kgrid = 12~12~12
 ‡@cutoff = 200
 local spin moment = 3.38,
 Total spin moment = 0.1424, theta = 89.99, phi = 118.015
 
 ‡Acutoff = 400
 local spin moment = 3,38,
 Total spin moment = 0.0430, theta = 89.88, phi = 118.95
 
 ‡Bcutoff = 600
 local spin moment = 3,38,
 Total spin moment = 0.0135, theta = 89.99, phi = 115.48
 
 ‡Ccutoff = 800
 local spin moment = 3,38,
 Total spin moment = 0.0101, theta = 90.10, phi = 113.55
 
 ‡Dcutoff = 1000
 local spin moment = 3,38,
 Total spin moment = 0.0072, theta = 90.16, phi = 141.72
 
 ‡Ecutoff = 2000
 local spin moment = 3,38,
 Total spin moment = 0.0048, theta = 90.10, phi = 152.68
 
 ‡Fcutoff = 3000
 local spin moment = 3,38,
 Total spin moment = 0.0042, theta = 89.95, phi = 158.50
 
 ‡Gcutoff = 3500
 local spin moment = 3,38,
 Total spin moment = 0.0030, theta = 89.89, phi = 98.42
 
 ‡Hcutoff = 4000
 local spin moment = 3,38,
 Total spin moment = 0.0028, theta = 89.94, phi = 96.16
 
 ‡Icutoff = 5000
 local spin moment = 3,38,
 Total spin moment = 0.0026, theta = 90.17, phi = 94.29
 
 ‡Jcutoff = 6000
 local spin moment = 3,38,
 Total spin moment = 0.0025, theta = 89.99, phi = 93.04
 
 ‡Kcutoff = 7000
 local spin moment = 3,38,
 Total spin moment = 0.0024, theta = 89.99, phi = 91.95
 
 ‡Lcutoff = 8000
 local spin moment = 3,38,
 Total spin moment = 0.0025, theta = 90.00, phi = 93.72
 
 ‡Mcutoff = 9000
 local spin moment = 3,38,
 Total spin moment = 0.0024, theta = 89.98, phi = 91.60
 
 
 energycutoff = 7000
 ‡@Kgrid = 15 15 12
 local spin moment = 3,38,
 Total spin moment = 0.0065, theta = 90.19, phi = 123.92
 
 ‡AKgrid = 18 18 12
 local spin moment = 3,38,
 Total spin moment = 0.014, theta = 89.98, phi = 108.90
 
 ‡BKgrid = 24 24 12
 local spin moment = 3,38,
 Total spin moment = 0.0033, theta = 90.20, phi = 119.95
 
 ‡CKgrid = 27 27 12
 local spin moment = 3,38,
 Total spin moment = 0.0026, theta = 90.44, phi = 164.10
 
 ‡DKgrid = 30 30 12
 local spin moment = 3,38,
 Total spin moment = 0.00099, theta = 89.91, phi = -67.39
 
 
 energycutoff = 8000
 Kgrid = 25 25 12
 local spin moment = 3.38
 Total spin moment = 0.001584, theta = 90.14, phi = 14.9
 
 -----------------------------------------------------
 
 For comparison, the calculation results obtained using VASP are presented. These results are in good agreement with the experimentally observed values.
 
 -----------------------------------------------------
 
 local spin moment = 2.90,
 Total spin moment = 0.003, theta = 90.00, phi = 0
 
 ------------------------------------------------------
 
 Last, input file used is noted.
 
 
 ------------------------------------------------------
 
 Species.Number                    2
 <Definition.of.Atomic.Species
 Mn    Mn6.0-s3p2d1      Mn_PBE19
 Sn    Sn7.0-s3p2d2      Sn_PBE19
 Definition.of.Atomic.Species>
 
 Atoms.Number                      8
 Atoms.SpeciesAndCoordinates.Unit  FRAC
 <Atoms.SpeciesAndCoordinates
 1  Mn  0.8418997760617231  0.6837995580507723  0.2499994261181939  9.0  6.0  90.0 0.0  90.0 0.0  0 off
 2  Mn  0.1580997540495446  0.3161995080990891  0.7500005346670946  9.0  6.0  90.0 0.0  90.0 0.0  0 off
 3  Mn  0.3162006822288461  0.1581007910616492  0.2499994261181939  9.0  6.0  90.0 -120.0  90.0 -120.0  0 off
 4  Mn  0.6837998848945261  0.8419003491124215  0.7500005346670946  9.0  6.0  90.0 -120.0  90.0 -120.0  0 off
 5  Mn  0.8419001029054840  0.1581007910616492  0.2499994261181939  9.0  6.0  90.0 120.0  90.0 120.0  0 off
 6  Mn  0.1581004642178954  0.8419003491124215  0.7500005346670946  9.0  6.0  90.0 120.0  90.0 120.0  0 off
 7  Sn  0.3333330220499562  0.6666660440999053  0.2499994261181939  7.0  7.0  90.0 0.0  90.0 0.0  0 off
 8  Sn  0.6666665080613186  0.3333330220499562  0.7500005346670946  7.0  7.0  90.0 0.0  90.0 0.0  0 off
 Atoms.SpeciesAndCoordinates>
 
 Atoms.UnitVectors.Unit            Ang
 <Atoms.UnitVectors
 5.5674400329999996    0.0000000000000000    0.0000000000000000
 -2.7837200164999998    4.8215445026000001    0.0000000000000000
 0.0000000000000000    0.0000000000000000    4.4320101738000002
 Atoms.UnitVectors>
 
 scf.Constraint.NC.Spin        off
 
 scf.XcType                    GGA-PBE
 scf.SpinPolarization          nc
 scf.partialCoreCorrection    on
 scf.SpinOrbit.Coupling        on
 scf.ElectronicTemperature    0.0
 scf.energycutoff              600
 scf.maxIter                  1000
 scf.EigenvalueSolver          band
 scf.Kgrid                    12  12  12
 scf.Mixing.Type              rmm-diisk
 scf.Init.Mixing.Weight        0.05
 scf.Min.Mixing.Weight        0.01
 scf.Max.Mixing.Weight        0.30
 scf.Mixing.History            25
 scf.Mixing.StartPulay        15
 scf.criterion                1.0e-8
 
 
 ------------------------------------------------------
 
 
 I would like to know that what is the cause of these problems.
 
 Thank you very much.
 
 
 
 
 
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