[CP2K-user] [CP2K:22122] Re: The KERKER mixing method may be more suitable than the BROYDEN mixing method for calculations involving magnetic systems.
yis...@163.com
yisichi at 163.com
Fri Feb 27 13:28:30 UTC 2026
Thank you for your reply. However, based on the test results, it is still
difficult to converge.
在2026年2月26日星期四 UTC+8 18:43:32<Shiyang Wang (W0728)> 写道:
> Dear yisichi-design,
>
> For BROYDEN_MIXING, you should use NBROYDEN instead of BETA to help
> convergence. Default NBROYDEN is 4, which often hinders convergence. You
> can increase it to 8 or even 12. BETA is used for KERKER_MIXING.
>
> For such systems, reducing the ALPHA value does indeed help with
> convergence (the default is 0.4), and this is often done in practice (we
> often use 0.3 or even 0.15). However, setting ALPHA too small may lead to
> numerical issues.
>
> To understand what *“Spin contamination estimate not implemented for
> k‑points”* means, you may need to look up what *spin contamination*
> refers to. In CP2K, in most cases this warning can be safely ignored.
>
> If there’s anything else that needs to be discussed, feel free to add it
> at any time.
>
> 在2026年2月26日星期四 UTC+8 12:37:55<yis... at 163.com> 写道:
>
>> Hello CP2K developers,
>> A few days ago on GitHub, we discussed whether the KERKER or
>> BROYDEN mixing method is more suitable for magnetic system calculations.
>> Following up on that, I have done some tests and found that the KERKER
>> mixing method may be more appropriate for magnetic systems than BROYDEN.
>> Below is my testing procedure.
>> I used two test models: a unit cell model of NiFe(OH)₂ and
>> the (010) surface of gamma-NiOOH. For the NiFe(OH)₂ unit cell, the test
>> procedure was as follows. First, with SMEAR enabled, the number of
>> iterations for the SCF calculation was set to 100. I then tested the
>> effects of different mixing methods, ALPHA, and BETA on convergence. The
>> test results are shown in Table 1. Figure 1 shows a screenshot of the SCF
>> results for the first 50 steps of Test1, which used the KERKER mixing
>> method with ALPHA = 0.2 and BETA at its default value. Both Table 1 and
>> Figure 1 indicate that under these parameters, SCF does not converge and
>> shows no trend toward convergence. In Test2, ALPHA was reduced to 0.03
>> while keeping other parameters the same as in Test1. Figure 1 and Table 1
>> show that a convergence trend appears, albeit slowly. After 100 iterations,
>> the convergence value reached 0.00041471. Although it has not yet met the
>> convergence criterion, I believe that increasing the number of iterations
>> would lead to successful convergence. Test3 further reduced BETA to 0.8
>> based on Test2. After 100 iterations, the convergence value was 0.00159217,
>> which is slower than Test2. However, based on my previous experience, if
>> the parameters in Test2 struggle to converge, trying the parameters in
>> Test3 can be a useful alternative.
>> [image: 图片2.jpg]
>> [image: 图片3.jpg]
>> Fingure 1 Convergence results for unit
>> cell
>> I further tested BROYDEN as the wavefunction mixing method, as
>> shown in Figure 1 and Table 1. Compared to KERKER, its convergence
>> performance is noticeably worse. The SCF results show persistent
>> oscillations without a clear trend of convergence. Additionally, compared
>> to Test4, reducing both ALPHA and BETA to 0.01 still resulted in a
>> convergence value of 0.07070099 after 100 iterations, but without a
>> distinct convergence trend. Subsequently, I disabled SMEAR and reran the
>> same tests. The results are shown in the lower half of Table 1. Compared to
>> the cases with SMEAR enabled, convergence did not improve. For the same
>> wavefunction mixing method, ALPHA, and BETA, convergence actually worsened.
>> For example, with SMEAR disabled, using the KERKER method with ALPHA = 0.03
>> gave a convergence value of 0.00082845 after 100 iterations, which is
>> higher than the case with SMEAR enabled. For the BROYDEN method with ALPHA
>> = 0.2 and default BETA, the convergence value increased to 0.07480723,
>> still worse than KERKER. Moreover, as shown in Figure 1, when appropriate
>> ALPHA and BETA values are used with the KERKER method, convergence steadily
>> improves with increasing iterations rather than oscillating continuously.
>> Based on these results, I draw the following conclusions:
>> 1. The KERKER mixing method may be more suitable for magnetic
>> systems than BROYDEN.
>> 2. Default parameters for KERKER generally struggle to achieve
>> convergence; ALPHA needs to be reduced to 0.03 or even lower.
>> Further, I selected the (010) surface of gamma-NiOOH to test
>> SCF convergence. The results are shown in Table 2 and Figure 2. First, I
>> tested convergence with SMEAR enabled and ADDED_MOS set to 20. Similar to
>> the unit cell calculations, when ALPHA = 0.2, KERKER failed to converge and
>> showed no trend toward convergence. For TEST3 and TEST4, after lowering
>> ALPHA, an interesting phenomenon was observed. In both cases, a clear
>> convergence trend initially appeared, but after reaching a certain value,
>> the convergence residual began to increase again. For TEST3 (ALPHA reduced
>> to 0.03), the residual gradually decreased to 0.0350084 within the first 50
>> iterations, but then it started to diverge. For TEST4 (BETA reduced to 0.8
>> and ALPHA reduced to 0.01), the residual decreased to 0.00089041 within the
>> first 75 steps, then gradually increased to 0.02504273.
>> [image: 图片4.jpg]
>> [image: 图片5.jpg]
>> Figure 2 Convergence results for slab
>> For BROYDEN, the convergence behavior was more complex. With
>> ALPHA = 0.2 and BETA = 0.8, the residual reached 0.05432726 after 200
>> iterations. However, when ALPHA and BETA were both reduced to 0.01, the
>> convergence worsened, and the SCF residual oscillated continuously without
>> a clear trend.
>> Considering that unoccupied orbitals might affect
>> convergence, I set ADDED_MOS to -1 -1 and reran the tests. The results in
>> the lower half of Table 2 show no significant differences.
>> In summary, I conclude:
>> 1. KERKER may be more suitable than BROYDEN for convergence
>> in magnetic systems.
>> 2. Default parameters for KERKER generally struggle to
>> achieve convergence; ALPHA needs to be reduced to 0.03 or even lower.
>> The difficulty of achieving SCF convergence for magnetic
>> systems in CP2K has been a longstanding issue. I would like to ask the CP2K
>> developers to review my testing procedure and input files and provide
>> suggestions for optimizing the input. Additionally, I have a question:
>> 1. What does the warning "WARNING in qs_scf_post_gpw.F:1841 ::
>> Spin contamination estimate not implemented for k-points" mean, and how can
>> it be resolved?
>> The input files and results have been compressed into a ZIP file
>> and are provided as an attachment.
>> Thank you very much
>>
>>
>>
--
You received this message because you are subscribed to the Google Groups "cp2k" group.
To unsubscribe from this group and stop receiving emails from it, send an email to cp2k+unsubscribe at googlegroups.com.
To view this discussion visit https://groups.google.com/d/msgid/cp2k/51b02e82-5915-4eb9-bed3-3fd168fec5c0n%40googlegroups.com.
-------------- next part --------------
An HTML attachment was scrubbed...
URL: <https://lists.cp2k.org/archives/cp2k-user/attachments/20260227/ca82c67c/attachment.htm>
More information about the CP2K-user
mailing list