[Pw_forum] s_psi_nc_ (Lorenzo Paulatto)45

clie clie at aphy.iphy.ac.cn
Mon May 18 15:21:37 CEST 2009


Dear Profssor,
yes, it is the CVS version. Thank you very much.

-----------------------------------------------
Ex5 group Extreme Condition Physics, Institute of Physics, Chinese
Academy of Sciences, P. O. Box 603, Beijing, 100190, People’s Republic of
China

> 
> On Mon, May 18, 2009 14:08, clie wrote:
>>  Dear friends,
>>  I am compiling the QE package,but some error emergences like following
> 
> which version of QE are you compiling? If it is a cvs version you may try
> to rebuild the dependecy tree with "make depend" before compiling.
> 
>>  libpw.a (s_lpsi.o); in function 's_lpsi_':
>>  s_lpsi.f90:(.text+ox1c9) undefined reference to 's_psi_nc_'
>>  make: ***[pw.x] Error 2
> 
> The way this function was called has been changed a bit in the last few
> month but, as far as I know, only in the CVS version
> 
> regards
> 
> -- 
> Lorenzo Paulatto
> SISSA  &  DEMOCRITOS (Trieste)
> phone: +39 040 3787 511
> skype: paulatz
> www:   http://people.sissa.it/~paulatto/
> 
> 
> 
> ----------------------------------------------------------------
>   SISSA Webmail https://webmail.sissa.it/
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> 
> 
> 
> ------------------------------
> 
> Message: 8
> Date: Mon, 18 May 2009 15:07:46 +0200
> From: Gabriele Sclauzero <sclauzer at sissa.it>
> Subject: Re: [Pw_forum] Re hubbard U and stable structure
> To: PWSCF Forum <pw_forum at pwscf.org>
> Message-ID: <4A115DA2.5030303 at sissa.it>
> Content-Type: text/plain; charset=us-ascii; format=flowed
> 
> 
> 
> Naol Regassa wrote:
>> Dear GS
>> 
>> Thank you for responding to my question.
>> In my question I said "more effective"  because I seen some changes on
>> the band structure of cubic ferromagnetic by adding U.But not as
>> effective ( it won't make totally an insulator) as the one I have seen
>> on the (experimentally found) stable structure i.e. hexagonal.
> 
> To figure it out maybe you can have a look at the PDOS in the two cases. The
U term 
> changes the position of the Mn states and consequently the bands which come
from an 
> hybridization between Mn states and other states. You should understand
between which kind 
> of states the gap forms by projecting your bands onto the atomic
wavefunctions (use 
> projwfc.x for this).
> 
> HTH
> 
> GS
> 
> 
>> 
>> 
>> On 5/18/09, pw_forum-request at pwscf.org <pw_forum-request at pwscf.org> wrote:
>>> Send Pw_forum mailing list submissions to
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>>>
>>> Today's Topics:
>>>
>>>    1. Re: Hubbard U and small degauss ... (Gabriele Sclauzero)
>>>    2. Electron-Phonon: loading dVscf file when ldisp=.TRUE.
>>>       (Andrea Marini)
>>>
>>>
>>> ----------------------------------------------------------------------
>>>
>>> Message: 1
>>> Date: Mon, 18 May 2009 10:12:25 +0200
>>> From: Gabriele Sclauzero <sclauzer at sissa.it>
>>> Subject: Re: [Pw_forum] Hubbard U and small degauss ...
>>> To: PWSCF Forum <pw_forum at pwscf.org>
>>> Message-ID: <4A111869.30202 at sissa.it>
>>> Content-Type: text/plain; charset=us-ascii; format=flowed
>>>
>>> Dear Naol,
>>>
>>> Naol Regassa wrote:
>>>> Dear all
>>>>
>>>> I have two questions to ask
>>>>
>>>> a) For the last times I was calculating the effect of Hubbard U on the
>>>> system YMnO_3 using QESPRESSO 4.10. I got an insulator band structure
>>>> using U = 10.5eV though it is completely metal without U (GGA). When I
>>> This is plausible. Though I don't know the physics of your compound, I can
>>> tell you that
>>> for simpler transition metal oxides (like FeO) you find the same change
>>> (i.e. from metal
>>> to insulator) after introducing the Hubbard U. Please have a look at Matteo
>>> Cococcioni's
>>> PhD thesis (from http://www.sissa.it/cm/phd.php) and the related paper (PRB
>>> 2005).
>>>
>>>> got this result I have used small degauss = 0.006. My friend told me
>>>> to use degauss  = 0.015.
>>> Have you asked him the reason? I don't see any...
>>>
>>> In principle you should test convergence of the total energy (and other
>>> quantities you're
>>> interested in) w.r.t all the parameters which introduce significant
>>> approximations to your
>>> result. As you decrease degauss you'll reach the correct result for your
>>> system at T=0
>>> (chosing k-point grids accordingly), so I don't see any reason to choose
>>> higher degauss
>>> other that saving computer time.
>>>
>>> In the specific case of DFT+U, you have to be carefull to converge the
local
>>> occupations
>>> too. They are very sensitive to the value of ecutwfc, but also degauss and
>>> number k-points
>>> have to be checked.
>>>
>>> Please tell me how possible (correct) is
>>>> that? I checked the convergence for degauss but it is increasing near
>>>> 0.015.
>>> What is increasing?
>>>
>>>
>>>> b) Is adding U value more effective for the most stable structure ?
>>> Sorry I cannot get this question... in which sense "more effective"?
>>>
>>>> For the unstable states like for my case cubic ferromagnetic phase I
>>>> can't see any change?
>>> What are looking at? Maybe your question is clear to someone who's studying
>>> systems like
>>> yours, so it's because of me that I cannot get the point... but if you
could
>>> be more
>>> precise maybe you would have more change to get help.
>>>
>>>
>>> Regards,
>>>
>>>
>>> GS
>>>
>>>
>>>
>>>> Here is the input for the 'scf'
>>>> &control
>>>>     calculation = 'scf',
>>>>     restart_mode = 'from_scratch',
>>>>     prefix = 'ymo_hcp_ferro'
>>>>     tstress = .true.,
>>>>     tprnfor = .true.,
>>>>     pseudo_dir = '/home/MSC608/Desktop/QESPRESSO_PP',
>>>>     outdir='/home/MSC608/Thesis/Hexagonal/Ferro-Hex/temp'
>>>>  /
>>>>  &system
>>>>     ibrav = 0,
>>>>     celldm(1) = 6.7,
>>>>     nat =  10,
>>>>     ntyp = 4,
>>>>     ecutwfc = 32,
>>>>     ecutrho = 340.0
>>>>     nspin = 2
>>>>     starting_magnetization(2) = 0.7,
>>>>     starting_magnetization(3) = 0.7,
>>>>     occupations = 'smearing',
>>>>     smearing = 'marzari-vanderbilt',
>>>>     degauss = 0.005,
>>>>     lda_plus_u=.true.,
>>>>     Hubbard_U(2) = 10.5,
>>>>     Hubbard_U(3) = 10.5,
>>>>  /
>>>>  &electrons
>>>>     diagonalization = 'david'
>>>>     startingwfc = 'atomic+random'
>>>>     mixing_beta = 0.3,
>>>>     conv_thr =  1.0d-10
>>>>  /
>>>>  ATOMIC_SPECIES
>>>>   Y     88.91     Y.pbe-nsp-van.UPF
>>>>   Mn1   54.94     Mn.pbe-sp-van_mit.UPF
>>>>   Mn2   54.94     Mn.pbe-sp-van_mit.UPF
>>>>   O     15.9994   O.pbe-rrkjus.UPF
>>>>
>>>> CELL_PARAMETERS (alat)
>>>>    0.985236441  -0.266531554  -0.000316189
>>>>   -0.266366323   0.985859979   0.000349871
>>>>    0.000781869  -0.000890980   3.186836665
>>>>
>>>> ATOMIC_POSITIONS (crystal)
>>>> Y       -0.082663260  -0.082649328   0.000174846
>>>> Y       -0.082874577  -0.082880779   0.499813069
>>>> Mn1      0.205305857   0.560245090   0.249986248
>>>> Mn2      0.561457263   0.207812583   0.750012603
>>>> O       -0.027464907  -0.056329933   0.249979343
>>>> O       -0.058482388  -0.031289340   0.750035308
>>>> O        0.247951998   0.582250730   0.083800805
>>>> O        0.582338704   0.248188482   0.916046842
>>>> O        0.582135578   0.247948396   0.583964864
>>>> O        0.247742343   0.582041831   0.416186070
>>>>   K_POINTS automatic
>>>>   3 3 2  1 1 1
>>>>
>>>> Thanks alot in  advance
>>>>  Tamene Regassa
>>>>  AAU
>>>>  Ethiopia
>>>> _______________________________________________
>>>> Pw_forum mailing list
>>>> Pw_forum at pwscf.org
>>>> http://www.democritos.it/mailman/listinfo/pw_forum
>>>>
>>> --
>>>
>>>
>>> o ------------------------------------------------ o
>>> | Gabriele Sclauzero, PhD Student                  |
>>> | c/o:   SISSA & CNR-INFM Democritos,              |
>>> |        via Beirut 2-4, 34014 Trieste (Italy)     |
>>> | email: sclauzer at sissa.it                         |
>>> | phone: +39 040 3787 511                          |
>>> | skype: gurlonotturno                             |
>>> o ------------------------------------------------ o
>>>
>>>
>>> ------------------------------
>>>
>>> Message: 2
>>> Date: Mon, 18 May 2009 10:09:58 +0200 (CEST)
>>> From: Andrea Marini <Andrea.Marini at roma2.infn.it>
>>> Subject: [Pw_forum] Electron-Phonon: loading dVscf file when
>>> 	ldisp=.TRUE.
>>> To: Pw_forum at pwscf.org
>>> Message-ID:
>>> 	<alpine.LFD.2.00.0905180949290.25064 at anomaly.roma2.infn.it>
>>> Content-Type: text/plain; charset="us-ascii"
>>>
>>> Dear all,
>>>
>>>  	I am encountering a problem when calculating lambda constants
>>> (PH/elephon.f90). Till now I used to
>>>
>>> 1. calculate first phonons and  dVscf file by using
>>>
>>>    elph=.false.,
>>>    trans=.true.,
>>>    ldisp=.false.,
>>>
>>> in the ph.x input file.
>>>
>>> 2. re-read the dvscf file using a larger k-point grid and changing in the
>>> ph.x input file
>>>
>>>    elph=.true.,
>>>    trans=.false.,
>>>    ldisp=.false.,
>>>
>>> This method works great. If I compare the result of point 2 against the
>>> calculation 1 using elph=.true. the lambda factors are identical.
>>>
>>> Now I am trying to follow points 1 and 2 when ldisp=.TRUE.. Here the
>>> results of the calculation 2, when the dVscf file is read from disk, are
>>> different the case when phonons and lambda's are calculated in the same
>>> run.
>>> More importantly I get that the symmetry of the  lambda factors are not
>>> respected for some q-points when the dVscf file is read from disk:
>>>
>>> < ldisp=.true., trans=.true.,  elph=.true.
>>>> ldisp=.true., trans=.false., elph=.true.
>>> <      q = (    0.500000000  -0.500000000   0.500000000 )
>>> <
>>> <      omega( 1) =       3.751393 [THz] =     125.133833 [cm-1]
>>> <      omega( 2) =       3.751393 [THz] =     125.133833 [cm-1]
>>> <      omega( 3) =       9.121952 [THz] =     304.277585 [cm-1]
>>> <
>>>
>>> <      lambda( 1)=  2.6170   gamma= 1077.54 GHz
>>> <      lambda( 2)=  2.6170   gamma= 1077.54 GHz
>>> <      lambda( 3)=  0.1901   gamma=  462.75 GHz
>>> ---
>>>>      lambda( 1)= 31.9820   gamma=13168.61 GHz
>>>>      lambda( 2)= 23.5894   gamma= 9712.95 GHz
>>>>      lambda( 3)= 19.7009   gamma=47963.51 GHz
>>>
>>> Maybe I am doing something wrong. I would really appreciate is someone
>>> could help me.
>>>
>>> I have attached to this mail a tar.gz file with all inputs to reproduce
>>> the above described error in the simple case of Al bulk. All the runs take
>>> less than 5 minutes. I have already created all the links so if you want
>>> to try, simple
>>>
>>>> cd Alluminum_TEST/
>>>> cd CALCULATE_DVSCF_LDISP_TRUE/
>>>> pw.x < gs.in > gs.out
>>>> ph.x < ph.in > ph.out
>>>> cd ../READ_DVSCF_LDISP_TRUE/
>>>> pw.x < gs.in > gs.out
>>>> ph.x < ph.in > ph.out
>>>> cd CALCULATE_DVSCF_SINGLE_Q/
>>>> pw.x < gs.in > gs.out
>>>> pw.x < nscf.in > nscf.out
>>>> ph.x < ph.in > ph.out
>>>> cd READ_DVSCF_SINGLE_Q
>>>> pw.x < gs.in > gs.out
>>>> pw.x < nscf.in > nscf.out
>>>> ph.x < ph.in > ph.out
>>> The diff between the files CALCULATE_DVSCF_LDISP_TRUE/ph.out and
>>> READ_DVSCF_LDISP_TRUE/ph.out is saved  as DIFF_LDISP_TRUE.
>>>
>>> Cheers
>>>
>>> Andrea
>>>
>>> --------------------------------------------------------------------------
>>>                                 Andrea MARINI
>>>
>>>         Physics Department, University of Rome "Tor Vergata" (Italy)
>>>                - phone: +39-0672594894 - fax: +39-062023507 -
>>>
>>> - andrea.marini at roma2.infn.it -- http://www.yambo-code.org/people/andrea -
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> 
> -- 
> 
> 
> o ------------------------------------------------ o
> | Gabriele Sclauzero, PhD Student                  |
> | c/o:   SISSA & CNR-INFM Democritos,              |
> |        via Beirut 2-4, 34014 Trieste (Italy)     |
> | email: sclauzer at sissa.it                         |
> | phone: +39 040 3787 511                          |
> | skype: gurlonotturno                             |
> o ------------------------------------------------ o
> 
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