[Pw_forum] Problem with nbnd in clusters

Stefano de Gironcoli degironc at sissa.it
Wed Nov 21 10:39:30 CET 2007


methfessel-paxton smearing is  dangerous (because it is not 
positive-defnite) when  k-point sampling is not sufficient.

When dealing with a "fake metal" as your molecule where the Fermi energy 
should fall in gap of the spectrum I think it is more advisable to use 
simple gaussian or marzari-vanderbilt smearing. The spurious negative 
weights of m-p smearing the occupation of levels just above the Fermi 
energy can lock some spourios state that shouldn't be there ... If you 
have many kpoints this (in my experience... Nicola has a different 
opinion) is never a problem.

In any case the  smearing contribution for a molecule should be  zero 
... which is not the case in your  output ... particularly so  for the 
problematic cases  with 12 or 25 bands..

TEST>  grep -e TS -e ! Fe*.out
Fe_dimer_gamma_nbnd12.scf.out:!    total energy              =  
-121.76376536 Ry
Fe_dimer_gamma_nbnd12.scf.out:     smearing contrib. (-TS)   =    
-0.00157785 Ry
Fe_dimer_gamma_nbnd20.scf.out:!    total energy              =  
-121.76907297 Ry
Fe_dimer_gamma_nbnd20.scf.out:     smearing contrib. (-TS)   =     
0.00048313 Ry
Fe_dimer_gamma_nbnd25.scf.out:!    total energy              =  
-121.76376546 Ry
Fe_dimer_gamma_nbnd25.scf.out:     smearing contrib. (-TS)   =    
-0.00157856 Ry

Does the problem (at least the one with 25 bands) disappears if you use 
"m-v" of "gaussian" smearing ?
I would expect so... otherwise there is still something else.
hope it helps,
stefano

Cyrille Barreteau wrote:
> Dear Paolo,
>
> Maybe I found the second exception due to another very special
> phase of the moon:-) What do I win in this case:-)
>
> You will find at the following links:
> the input file, the pseudo file and the three output
> corresponding to nbnd=12,20,25 respectively.
>
> http://www-drecam.cea.fr/spcsi/cbarreteau/tempo/Fe_dimer.scf.in
> http://www-drecam.cea.fr/spcsi/cbarreteau/tempo/Fe.pw91.vdb.UPF
> http://www-drecam.cea.fr/spcsi/cbarreteau/tempo/Fe_dimer_gamma_nbnd12.scf.out
> http://www-drecam.cea.fr/spcsi/cbarreteau/tempo/Fe_dimer_gamma_nbnd20.scf.out
> http://www-drecam.cea.fr/spcsi/cbarreteau/tempo/Fe_dimer_gamma_nbnd25.scf.out
>
> thanks for having a look at this case.
>
>    cyrille
>
> - 
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>
>
>
> Paolo Giannozzi wrote:
>
>   
>> On Nov 20, 2007, at 15:55 , Cyrille Barreteau wrote:
>>
>>  
>>
>>     
>>> Does anyone has experience about the behaviour
>>> of the various diagonalization schemes?
>>> Which one is better, in which case?
>>>    
>>>
>>>       
>> the so-called conjugate-gradient diagonalization basically
>> never fails; it uses less memory but it is much slower than
>> the block Davidson algorithm. The latter is also quite
>> robust but there is a tiny probability to end up in the wrong
>> ground state. The only such case I know happens in some
>> high-symmetry perovskites, if you start from superposition
>> of atomic states, with occupied states only, and if the phase
>> of the moon is close to 42. The problem disappears if you
>> add a few more states, or if you start from random wavefunctions.
>> I am quite surprised to hear that there is a case in which
>> you get good results with 12 states and bad with 20.
>> I wouldn't be surprised by the opposite. Could you please
>> post one jobs showing the problem?
>>
>> Paolo
>> ---
>> Paolo Giannozzi, Dept of Physics, University of Udine
>> via delle Scienze 208, 33100 Udine, Italy
>> Phone +39-0432-558216, fax +39-0432-558222
>>
>>
>>
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>
>
> -
>
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