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VASP自旋轨道耦合计算错误汇总

2019-05-18 5页 doc 104KB 81阅读

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VASP自旋轨道耦合计算错误汇总VASP自旋轨道耦合计算错误汇总静态计算时,报错VERYBADNEWS!Internal内部errorinsubroutine子程序IBZKPT:Reciprocal倒数的latticeandk-latticebelongtodifferentclassoflattices.Oftenresultsarestilluseful...48INCAR参数设置:对策:根据所用集群,修改INCAR中NPAR。将NPAR=4变成NPAR=1,已解决!错误:subspacematrix类错误报错:静态和能带计算中出现警告:WARNING:...
VASP自旋轨道耦合计算错误汇总
VASP自旋轨道耦合计算错误汇总静态计算时,报错VERYBADNEWS!Internal内部errorinsubroutine子程序IBZKPT:Reciprocal倒数的latticeandk-latticebelongtodifferentclassoflattices.Oftenresultsarestilluseful...48INCAR参数设置:对策:根据所用集群,修改INCAR中NPAR。将NPAR=4变成NPAR=1,已解决!错误:subspacematrix类错误报错:静态和能带计算中出现警告:WARNING:Sub-Space-Matrixisnothermitian共轭inDAV结构优化出现错误:WARNING:Sub-Space-MatrixisnothermitianinDA/4-4.681828688433112E-002对策:通过将默认AMIX=0.4,修改成AMIX=0.2(或0.3),问题得以解决。以下是类似的错误:WARNING:Sub-Space-Matrixisnothermitianinrmm-3.00000000000000RMM:22-0.167633596124E+02-0.57393E+00-0.44312E-0113260.221E+00BRMIX:veryseriousproblemstheoldandthenewchargedensitydifferoldchargedensity:28.00003new28.060930.111E+00错误:WARNING:Sub-Space-Matrixisnothermitianinrmm-42.5000000000000ERRORFEXCP:suppliedExchange-correletiontableistoosmall,maximalindex:4794错误:结构优化Bi2Te3时,log文件:WARNINGinEDDIAG:subspacematrixisnothermitian1-0.199E+01RMM:2000.179366581305E+01-0.10588E-01-0.14220E+007180.261E-01BRMIX:veryseriousproblemstheoldandthenewchargedensitydifferoldchargedensity:56.00230new124.7039466F=0.17936658E+01E0=0.18295246E+01dE=0.557217E-02curvature:0.00expectdE=0.000E+00dEforcontlinesearch0.000E+00ZBRENT:fatalerrorinbracketingpleasererunwithsmallerEDIFF,orcopyCONTCARtoPOSCARandcontinue但是,将CONTCAR拷贝成POSCAR,接着算静态没有报错,这样算出来的结果有问题吗?对策1:用这个CONTCAR拷贝成POSCAR重新做一次结构优化,看是否达到优化精度!对策2:用这个CONTCAR拷贝成POSCAR,并且修改EDIFF(目前参数EDIFF=lE-6),默认为10-4错误:WARNING:Sub-Space-MatrixisnothermitianinDA/1-7.626640664998020E-003网上参考解决:对策1:减小POTIM:IBRION=0,标准分子动力学模拟。通过POTIM控制步长。POTIM:当IBRION=1,2或3时,是力的一个缩放常数(相当于确定原子每步移动的大小),默认值为0.5。对策2:改IBRION=1,采用准牛顿算法来优化原子的位置。原IBRION=2,采用共轭梯度算法来优化原子的位置对策3:修改ISMEAR对策4:换成CG弛豫(共轭梯度算法)IBRION=2(决定结构优化过程中,原子如何移动或弛豫)IBRION=2离子是否运动,1不运动但做NSW外循环。0动力学模拟,1准牛顿法离子弛豫2CG法离子弛豫,3采用衰减二阶运动方程离子弛豫,INCARrelax中设置IBRION=2,未解决!对策5:用的CG算符,出现的错误是CG算符不能算,在INCAR中加上IALG=Fast(电子优化采用blockedDavidson方法[IALGO=38:IALG=Normal]和RMM-DIIS算法[IALGO=48:IALG=VeryFast]混合)试一试IALG二Fast(两种方法混用)IALG=Very_Fast等价于IALGO=48)IALG二Normal(等价于IALGO=38)INCAR中加上IALG二Fast已解决!(1QL、2QL已解决,3QL以上未解决)VASPFORUM:theerrorisduetoaLAPCKcall(ZHEGV):ZHEGVcomputesalltheeigenvalues本征值,andoptionally随意地,theeigenvectorsofacomplexgeneralizedHermitian-definiteeigenproblem.theremaybeseveralreasonsforthaterror:theRMM-DIISdiagonalisationalgorithmisnotstableforyourspecificsetupofthecalculation.-->useALGO=Normal(blockedDavidson)orALGO=Fast(5stepsblockedDavidson,RMM-DIIS)用ALGO=NormalIALGO=48或者ALGO=Fast2)maybeyourinputgeometrywasnotreasonable(erroroccursattheveryfirstionicstep,pleasehavealookforthegeometrydataofyourruninOUTCAR)orthelastionicrelaxationstepleadtoanunreasonablegeometry(comparetheinputandoutputgeometriesofthelastionicrelaxationstepsinXDATCAR).Inthatcase(2b)itcanbehelpfulto-->switchtoadifferentrelaxationalgorithm(IBRION-tag)-->reducethestepsizeofthefirststepbysettingPOTIMsmallerthanthedefaultvalue改变IBRION,减少步长POTIMTheinstallationoftheLAPACKonyourmachinewasnotdoneproperly:usetheLAPACKwhichisdeliveredwiththecode(vasp.4.lib/lapack_double.o)IftheerrorpersistalthoughyouswitchedtotheDavidsonalgorithm:onsomearchitectures(especiallySGI)someLAPACKroutinesarenotworkingproperly.However,itispossibletoavoidtheusageoftheZHEGVsubroutinebycommentingtheline#defineUSEZHEEVXindavidson.F,subrot.F,andwavprenoio.FandrecompilingVASP.关于Mixing方法的调试:针对这类错误:DAV:13-0.242323773333E+030.98155E+02-0.87140E+01488320.949E+01BRMIX:veryseriousproblemstheoldandthenewchargedensitydifferoldchargedensity:252.00012new252.299790.809E+01WARNING:Sub-Space-MatrixisnothermitianinDAV90.133520549894753解决办法只需调整AMIX,BMIX的值,把他们设置小一些。Mixing方法:IMIX=typeofmixing混合、混频,AMIX=linearmixingparameter,AMIN=minimalmixingparameter,BMIX=cutoffwavevectorforKerkermixingscheme,AMIX_MAG=linearmixingparameterformagnetization,BMIX_MAG=cutoffwavevectorforKerkermixingschemeformag,WC=weightfactorforeachstepinBroydenmixingscheme,INIMIX=typeofinitialforeachstepinBroydenmixingscheme,MIXPRE=typeofpreconditioninginBroydenmixingscheme,MAXMIX=maximumnumberstepsstoredinBroydenmixer.一般采用其默认值,除非在电子迭代难以收敛的情况,才手动设置AMIX和BMIX等参数值。】对策:grepAMIXOUTCARAMIX=0.40;BMIX=1.00AMIX_MAG=1.60;BMIX_MAG=1.00initialmixingisaKerkertypemixingwithAMIX=0.4000andBMIX=1.0000设置初始值AMIX=0.0100;BMIX=0.0001AMIX=0.1000;BMIX=0.0010AMIX=0.20;BMIX=0.01AMIX=0.2、BMIX=0.001AMIX=0.3、BMIX=0.1AMIX=0.4收敛值AMIX=0.01;BMIX=0.00AMIX=0.10;BMIX=0.00AMIX=0.20;BMIX=0.01AMIX=0.2、BMIX=0.001AMIX=0.3、BMIX=0.1AMIX=0.40;BMIX=1.00结果计算无误计算无误计算无误计算无误计算无误静态log:WARNINGinEDDRMM:callto**AMIX=0.02AMIX=0.1AMIX=0.02;BMIX=1.00AMIX=0.10;BMIX=1.00计算无误静态log:WARNINGinEDDRMM:calltoZHEGVfailed,returncode=63**,能带一样**AMIX=0.3AMIX=0.30;BMIX=1.00静态log:WARNINGinEDDRMM:calltoZHEGVfailed,returncode=63**,能带一样**BMIX=0.0001AMIX=0.40;BMIX=0.00以上参数设置,得到的能带图都一样,如下图:综上:设置AMIX=0.2(或0.3),BMIX默认(省事,算出正确的能带。计算无误K"M等于1.0),可以保证计算过程无误。还需进一步调整其他参数,ZHEGVfailed,returncode=63**,能带一样警告:算1QL弛豫、静态、能带时,都有这个提示:ADVICETOTHISUSERRUNNING'VASP/VAMP'(HEARYOURMASTER'SVOICE...):Youhavea(moreorless)'smallsupercell'andforsmallercellsitisrecommendedtousethereciprocal-spaceprojectionscheme!Therealspaceoptimizationisnotefficientforsmallcellsanditisalsolessaccurate...ThereforesetLREAL=.FALSE.intheINCARfile对策:对于较小的晶胞(原子数小于20),设置LREAL=.FALSE.,计算结果比较精确。而对于较大的晶胞,设置LREAL=Auto,这样计算速度比较快。本体系含原子5个,INCAR中LREAL=Auto。设置所有INCAR中的LREAL=.FALSE.,重新算一遍。对于1QL2QL3QL原子数分别为5、10、15,LREAL=.False.对于4QL5QL6QL原子数分别为20、25、30,LREAL=Auto自旋轨道耦合计算时,静态和能带计算中出现的错误:ERROR:noncollinearcalculationsrequirethatVASPiscompiledwithouttheflag-DNGXhalfand-DNGZhalf分析:VASP手册中关于自旋轨道耦合计算的描述(翻译版):非线性计算和自旋轨道耦合:旋量是由GeorgKresse在VASP代码中引入的。这个代码是由DavidHobbs编写,用于处理非线性磁结构。自旋轨道耦合计算是由OlivierLebacqandGeorgKresse共同实现的。只有VASP4.5以上的版本才支持旋量的计算。在INCAR中设置LNONCOLLINEAR=.TRUE•允许执行完全非线性磁结构的计算。VASP有能力读入之前非磁或非线性计算得到的WAVECAR和CHGCAR文件,然而它不可能扭转局域在指定原子处的磁场。因此在实际操作中,我们推荐分两步执行非线性计算:第一步,计算计算非磁性基态,产生WAVECAR和CHGCAR文件。第二步,读入WAVECAR和CHGCAR文件,通过设置MAGMOM参数,提供初始的磁矩。对于非线性设置,在MAGMOM这一行,每个离子必须设置三个值。这三项分别对应每个离子在x,y,z方向的初始局域磁矩值。MAGMOM=100010这一行,给第一个原子赋予的初始磁矩值沿x方向,第二个原子的初始磁矩值沿y方向。注意:只有在ICHARG=2(即不读入之前CHGCAR的情况)或者CHGCAR文件中只包含电荷但是不包括磁密度数据的情况(即之前那一步进行了非磁的计算)下,才需要通过MAGMOM设定初始磁矩值。LSORBIT-tagSupportedasofVASP.4.5.【设置LSORBIT=.TRUE.表示计算自旋轨道耦合,并附带自动设置了LNONCOLLINEAR=.TRUE.】LSORBIT=.TRUE.只能用于PAW赝势,不能用于超软赝势。如果不考虑自选轨道耦合,则能量不依赖磁矩的方向,也就是说,旋转所有的磁矩以同一个角度,让它们拥有相等的能量。不考虑自选轨道耦合的时候,不需要定义自旋量子化坐标。开启自旋轨道耦合设置以下参数:LSORBIT=.TRUE.SAXIS=s_xs_ys_z(自旋量子化轴,默认值SAXIS=(0+,0,1))GGA_COMPAT=.FALSE.!应用球面截断能到梯度场其中SAXIS默认=(0+,0,1)(0+表示沿x轴方向一个无穷小的正数)。当需要计算亚meV能量尺度的微小能量差异(一般指磁各向异性计算的情况)时,需要设置GGA_COMPAT这个参数。现在所有关于坐标轴(Sx,Sy,Sz)的磁矩都给出来了,我们采用VASP中给出关于这个坐标轴所有磁矩和自旋状量子读写惯例。这包括INCAR文件中的MAGMOM行,OUTCAR和PROCAR文件中的总和局域磁矩,WAVECAR文件中的类自旋轨道,CHGCAR文件中的磁密度。笛卡尔坐标系中的磁分量由以下等式得到:m=cos(P)cos(a)加曲$—sin(a)maxis+sin(P)*cos(a)maxisTOC\o"1-5"\h\zxxyzm=cos(P)sin(a)m+cos(a)maxis+sin(P)sin(a)m«xisyxyzm=—sin(P)maxis+cos(P)maxiszxz其中,maxis是外部可见的磁矩值,此处的a是SAXIS矢量(sx,sy,sz)和笛卡尔坐标x轴的夹角,卩是SAXIS矢量和笛nIs2+s2|卡尔坐标z轴的夹角,以下等式得到逆变化:P=atan—szmaxis=cos(P)cos(a)m+cos(P)sin(a)m+sin(P)mTOC\o"1-5"\h\zxxyzmaxis=—sin(a)m+cos(a)myxymaxis=sin(P)cos(a)m+sin(P)sin(a)m+cos(P)m,xyz不难看出,默认值(sx,sy,sz)=(0+,0,1),两个角度都是0,即卩=0和a=0。在这种情况下,内部转换简单地等于外部地转换:mx=呼,my=彎,mz=maxis,第二种重要的情况,是mr=0和營s=0,在这种情况下:m=sin(P)*cos(a)maxis=maxiss/、s2+s2+s2xzzz'xyzm=ym=cos(P)maxis=maxiss/、、.s2+s2+s2zxzzxyz因此现在磁矩是平行于SAXIS矢量。这样有两种方式去旋转自旋到任意方向,即通过改变初始的磁矩MAGMOM或改变SAXIS。为了给计算赋予平行于一个选定的矢量(x,y,z)的初始磁矩,可以通过设定(假定是单原子原胞):MAGMOM=xyzSAXIS=001!局域磁矩xyz!量子轴平行于z轴或者MAGMOM=00total_magnetic_moment!局域磁矩平行于SAXISSAXIS=xyz两种设置都必须在相同能量的标准/辐射(原则、!量子轴平行于矢量(x,y,z)根源)场,但是要实现第二种方法,通常更加精确。第二种方法,也允许读入之前存在的WAVECAR文件(由线性计算还是非线性计算产生的都可以),然后继续用一个不同的自旋方向计算。当读入一个非线性WAVECAR文件,自旋假定平行于SAXIS(因此VASP将仅仅输出一个z轴方向的磁矩)。推荐计算磁各项异性的步骤如下:先做线性计算,得到一个WAVECAR和CHGCAR文件。加入以下参数:LSORBIT=.TRUE.ICHARG=11!非自洽计算,读入CHGCARLMAXMIX=4!对于d电子元素设置LMAXMIX=4,f电子元素设置LMAXMIX=6!在线性计算中,需要设置LMAXMIXSAXIS=xyz!磁场的方向NBANDS=2*线性计算能带数GGA_COMPAT=.FALSE.!在梯度场中应用球面截断能VASP读入WA/ECAR和CHGCAR文件,将自旋量子轴对齐SAXIS矢量,这意味着现在磁场平行于SAXIS矢量,执行非线性计算。通过比较不同方向的能量,可以确定磁各向异性。请记住,原则上,在VASP中一个完全地自洽计算(ICHARG=1)也是有可能的,但是这种情况将会允许自旋波函数从它们的初始值旋转到平行于SAXIS矢量,直到获得正确的基态,也就是,直到磁矩平行于易磁化轴。实际操作中,这种旋转非常缓慢,直到自旋获得少量能量重新定位。因此,如果收敛标准太精确,完全地自洽计算可以得到一个比较合理的结果(我们实验过的几种自洽计算都没有问题。)要非常小心对称性。我们建议选择计算自旋轨道耦合时,完全关掉对称性(ISYM=0)。通常会从一个自旋方向到另一个自旋方向k点的设置会发生改变,进而恶化转换的结果(如果k点改变WA/ECAR将不会被正确地重新读取)。GGA_COMPAT通常需要,应该被设置,因为磁各向异性能量通常需要精确到亚meV数量级。当计算自旋轨道耦合,特别是磁各向异性时通常需要非常小心:能量差异非常小,k点的收敛冗长而且缓慢,需要耗费大量的计算时间。此外,这一特征-尽管长期存在于VASP中-在最新的版本中依然存在,你可以尝试频繁地升级发现这一点。不敢保证,你的结果是有用的!此处根据README文件做了一个小小的总结:20.11.2003:提出的GGA程序轻微的破坏了非正交体系晶胞的对称型。球面截断能应用于梯度及互逆空间中的所有中间结果。GGA引起的轻微的改变(通常每个原子0.1meV),却对磁各项异性很重要。05.12.2003:继续…现在VASP.4.6默认旧的行为GGA_COMPAT=.TRUE.,新的行为将可以通过在INACR中设置GGA_COMPAT=.FALSE得至V。12.08.2003:主要的错误出现在symmetry.F和paw.F:非线性计算的对称性例程没有正确的执行。如果你阅读了以上内容,就会意识到在VASP.4.6和VASP.5.2版本中进行非线性计算推荐设置GGA_COMPAT=.FALSE.,这样可以提升GGA计算的数值精度。VASP:Non-collinearcalculationsandspinorbitcoupling:Spinors旋量wereincludedbyGeorgKresseintheVASPcode.Thecoderequiredforthetreatment处理ofnon-collinearmagneticstructureswaswrittenbyDavidHobbs,andspin-orbitcouplingwasimplemented实施、执行byOlivierLebacqandGeorgKresse.SpinorsareonlysupportedasofVASP.4.5.Subsections:分段、子章节、下一级栏目LNONCOLLINEAR-tagSupported支持asofVASP.4.5.ySettingLNONCOLLINEAR=.TRUE.intheINCARfileallowstoperformfullynon-collinearmagneticstructurecalculations.VASPiscapable有能力的ofreadingWAVECARandCHGCARfilesfromprevious之前的non-magnetic非磁orcollinear线性calculations,itishowevernotpossibletorotate旋转、转动themagneticfieldlocallyonselectedatoms.Hence因此,inpractice在实践中,werecommend推荐toperformnon-collinearcalculationsintwosteps:First,calculatethenonmagneticgroundstate基态andgenerateaWAVECARandCHGCARfile.Second,readtheWAVECARandCHGCARfile,andsupply提供initialmagneticmomentsbymeansoftheMAGMOMtag(compareSec.6.13).Foranon-collinearsetup,threevaluesmustbesuppliedforeachionintheMAGMOMline.Thethreeentriescorrespondtotheinitiallocalmagneticmomentforeachioninx,yandzdirectionrespectively.ThelineMAGMOM=100010Initialises赋初值themagneticmomentonthefirstatominthex-direction,andonthesecondatomintheydirection.Mind,thattheMAGMOMlinesuppliesinitialmagneticmomentsonlyifICHARG=2,oriftheCHGCARfilecontainsonlychargebutnomagnetisationdensity.LSORBIT=.TRUE.Switches接通、开启onspin-orbitcouplingandautomaticallysetsLNONCOLLINEAR=.TRUE..Thisoption选项、选择worksonlyforPAWpotentialsandisnotsupportedforultrasoftpseudopotentials.Ifspin-orbitcouplingisnotincluded,theenergydoesnotdependon依赖thedirectionofthemagneticmoment,i.e.也就是说rotating旋转allmagneticmoments磁矩bythesameangleresultsexactlyinthesameenergy.Hence因此thereisnoneedtodefinethespinquantizationaxis自旋量子化坐标轴,aslongas只要spin-orbitcouplingisnotincluded.Spin-orbitcoupling,however,couples一对、一双thespintothecrystalstructure.Spinorbitcouplingisswitchedon开启byselectingLSORBIT=.TRUE.SAXIS=s_xs_ys_z(quantisationaxisforspin自旋量子化轴)GGA_COMPAT=.FALSE.!applyspherical球面cutoff截断能ongradientfield梯度场wherethedefaultforSAXIS=(0+,0,l)(thenotation符号0+implies意味着aninfinitesimal无穷小smallpositivenumberinxdirection).TheflagGGA_COMPAT(seeSec.6.42)isoptional选项andshouldbesetwhensmallenergydifferencesinthesub副、下标meVregime体制、状态needtobecalculated(oftenthecaseformagneticanisotropycalculations磁各向异性计算).Allmagneticmomentsarenowgivenwithrespectto关于theaxis坐标轴(Sx,Sy,Sz),wherewehaveadopted应用theconvention“惯例0thatallmagneticmomentsandspinor-likequantitieswrittenorreadbyVASParegivenwithrespecttothisaxis.ThisincludestheMAGMOMlineintheINCARfile,thetotalandlocalmagnetizationsintheOUTCARandPROCARfile,thespinor自旋量-likeorbitalsintheWAVECARfile,andthemagnetizationdensityintheCHGCARfile.Withrespecttothecartesian笛卡尔latticevectorsthecomponents组件、部分ofthemagnetizationare(internally内部地、内在的)givenbym=cos(卩)cos(a)maxis-sin(a)maxis+sin(卩)*cos(a)maxisTOC\o"1-5"\h\zxxyzm=cos(卩)sin(a)m+cos(a)maxis+sin(卩)sin(a)maxisyxyzm=—sin(卩)mEs+cos(卩)mEszxzWheremaxisistheexternally夕卜部地visible可得到的,现有的,可见的magneticmomentHere,aistheanglebetweenthe/X入SAXISvector(s%,s『,sz)andthecartesianvectorx,and卩istheanglebetweenthevectorSAXISandthecartesianvectorz:snIs2+s2|a=atanT,p=atan~厂ssxzTheinverse倒转、翻转transformation转化、转换isgivenbymaxis=cos(P)cos(a)m+cos(P)sin(a)m+sin(P)myzxxmaxis=—sin(a)m+cos(a)mxyy-maxis=sin(P)cos(a)m+sin(P)sin(a)m+cos(P)m”xyzItiseasytoseethatforthedefault(sx,s『,sz)=(0+,0,l),bothanglesrepresentationissimplyequivalenttotheexternalrepresentation:arezero,i.e.0a0da=0.Inthiscase,theinternalm=maxis,m=maxis,m=maxisxxyyzzThesecondimportantcase,ismaxjs=°andmaxis=0.Inthiscasem=sin(卩)*cos(a)肌曲=maxiss/、:s2+s2+s2zzzXyzm=ym=cos(卩}maxis=maxiss/s2+s2+s2zxzzxyzHence因此、今后nowthemagneticmomentisparalleltothevectorSAXIS.Thustherearetwowaystorotatethespinsinanarbitrary任意的direction,eitherbychangingtheinitialmagneticmomentsMAGMOMorbychangingSAXIS.Toinitialisecalculationswiththemagneticmomentparalleltoachosenvector(x,y,z),itistherefore因此possibletoeitherspecify扌旨定(assuming假定、假设asingleatominthecell)MAGMOM=xyz!localmagneticmomentinx,y,zSAXIS=001!quantisationaxisparalleltozorMAGMOM=00total_magnetic_moment!localmagneticmomentparalleltoSAXISSAXIS=xyz!quantisationaxisparalleltovector(x,y,z)Bothsetupsshouldinprincipleyieldexactlythesameenergy,butforimplementation实现reasonsthesecondmethodisusuallymoreprecise精确.ThesecondmethodalsoallowstoreadapreexistingWAVECARfile(fromacollinearornoncollinearrun),andtocontinuethecalculationwithadifferentspinorientation.WhenanoncollinearWAVECARfileisread,thespinisassumed假定tobeparalleltoSAXIS(hence因此VASPwillinitiallyreportamagneticmomentinthez-directiononly).Therecommended被推荐的procedure过程、步骤forthecalculationofmagneticanisotropiesistherefore因而、表示结果(pleasecheckthesectiononLMAXMIX6.63):StartwithacollinearcalculationandcalculateaWAVECARandCHGCARfile.AddthetagsLSORBIT=.TRUE.ICHARG=11!nonselfconsistentrun,readCHGCARLMAXMIX=4!fordelementsincreaseLMAXMIXto4,f:LMAXMIX=6!youneedtosetLMAXMIXalreadyinthecollinearcalculationSAXIS=xyz!directionofthemagneticfieldNBANDS=2*numberofbandsofcollinearrunGGA_COMPAT=.FALSE.!applysphericalcutoffongradientfieldVASPreadsintheWAVECARandCHGCARfiles,aligns排列thespinquantizationaxisparalleltoSAXIS,whichimplies意味着thatthemagneticfieldisnowparalleltoSAXIS,andperformsanonselfconsistentcalculation.Bycomparingtheenergiesfordifferentorientationsthemagneticanisotropycanbedetermined确定.Pleasemind,thatacompletelyselfconsistentcalculation(ICHARG=1)isinprinciple大体上、原则上alsopossiblewithVASP,butthiswouldallowthethespinorwavefunctionstorotatefromtheirinitialorientationparalleltoSAXISuntilthecorrectgroundstateisobtained,i.e.untilthemagneticmomentisparalleltotheeasyaxis(?=theeasymagneticaxis).Inpracticethisrotationwillbeslow,sincereorientation再定位ofthespingains获得littleenergy.Thereforeiftheconvergence收敛criterion标准isnottootight,sensible明智的resultsmightbeobtainedevenforfullyselfconsistentcalculations(inthefewcaseswehavetried可靠地,试验过的selfconsistentcyworkedwithoutproblems).Beverycarefulwithsymmetry.Werecommend建议toswitchoff关掉symmetry(ISYM=0)altogether完全地,whenspinorbitcouplingisselected.Oftenthek-pointsetchangesfromonetotheotherspinorientation,worsening恶化thetransferabilityoftheresults(alsotheWAVECARfilecannotberereadproperly正确地ifthenumberofk-pointschanges).TheflagGGA_COMPATisusuallyrequiredandshouldbeset,sincemagneticanisotropyenergiesareofteninthesubmeVregime(seeSec.6.42).Generallybeextremely非常careful,whenusingspinorbitcouplingand,specifically特别地,magneticanisotropies:energydifferencesaretiny微小的,k-pointconvergence收敛istedious冗长乏味andslow,andthecomputertimemightbehuge.Additionally此夕卜,thisfeature这一特征--althoughlongimplemented应用inVASP--isstillinalatebetast,aageyoumightdeducefrom推断,从…得出结论thefrequent频繁的updates升级、更新.Nopromise允诺,thatyourresultswillbeuseful!Hereisasmallsummary总结fromtheREADMEfile:20.11.2003:Thepresent提出GGAroutine程序breaksthesymmetryslightly轻微地fornonorthorhombic正交晶系cells.Aspherical球面的cutoffisnowimposedon应用于thegradientsandallintermediate中间的resultsinreciprocal互逆space.ThischangestheGGAresultsslightly(usuallyby0.1meVperatom),butisimportantformagneticanisotropies.05.12.2003:continue...NowVASP.4.6defaultstotheoldbehaviorGGA_COMPAT=.TRUE.,thenewbehaviorcanbeobtainedbysettingGGA_COMPAT=.FALSE.intheINCARfile.12.08.2003:MAJOR主要的BUG故障FIX固定insymmetry.Fandpaw.F:fornon-collinearcalculationsthesymmetryroutines惯例didnotworkproperly正确地Ifyouhavereadthepreviouslines,youwillrealizethatitisrecommended推荐tosetGGA_COMPAT=.FALSE.fornoncollinearcalculationsinVASP.4.6andVASP.5.2,sincethisimprovesthenumericalprecisionofGGAcalculations.degree:BSc:BachelorofScience理科学士MDMS:master硕士PhD:DoctorofPhilosophy博士学位AAAssociatedegreeofArts大专文科学位AASAssociatedegreeofArtsandScience大专文理科学位ASAssociatedegreeofScience大专理科学位BABachelorofArts文科本科学位BSBachelorofScience理科本科学位MAMasterofArts文科硕士MBAMasterofBusinessAdministration商学硕士MSMasterofScience理科硕士Ph.D.DoctorofPhiolosphy哲学(通才)博士JDDoctorofJournalism新闻博士MDDoctorofMedicine医学博士DVMDoctorofVeterinry兽医博士CalltoZHEGVfailedErrorEDDDAV:CalltoZHEGVfailed.Returncode=1318Theearliersolutionsuggestedbyadmin(DOS操作系统中,超级管理员。行政、管理)(suppressing制止的theline#defineUSE_ZHEEVXindavidson.F,subrot.F,andwavpre_noio.FandrecompilingVASP)doesnotwork,i.e.thesameerrormessages,andthesameindication迹象、表示ofZHEGVfailure,stillappear出现.ImayaddnowthattheproblemappearsbothwiththelapackwhichcomeswithVASPandwithasystem-nativelapacklibrary.Thewarningsgivensuggestthattheproblemactuallyappearsatanearlierstage阶段,inwhichamatrixisgeneratedwithinadequate不适当的valueswhichmakeitnonhermitian,andconsequentlyZHEGVfailsevenifworkingcorrectly;thesolutionthuswouldnotbetoavoidusingZHEGV,buttoavoidanincorrectgenerationofthesaidmatrix.Cansomeonegiveanideatoreallysolvetheproblem?答:Pleasetryifitworksbyadding"LSCALAPACK=.FALSE."inyourINCAR.对策:grepLSCALAPACKOUTCAR空设置:LSCALAPACK=.FALSE问:No;adding"LSCALAPACK=.FALSE."inINCARmakesnodfference,theproblemcontinuesthesame.问:Iwassuccessfultofixthisproblem解决此问题byusingIALGO=48insteadofIALGO=Default。unfortunately,whenisetIALGO=48,thenewwarningis:WARNINGinEDDRMM:calltoZHEGVfailed,returncode=6314howtosolvethisproblem?whatdoes"ZBRENT"mean?对策:grepIALGOOUTCARIALGO=68algorithm(INCARALGO=Fast)设置:IALGO=48pleasetryoneofthefollowing:chooseadifferentalgorithmforionicoptimization(IBRION=1)采用准牛顿算法来优化原子位置setADDGRID=.True.inINCAR(onlyforvaspreleases发布管理、释放、豁免445andnewer)对策:grepADDGRIDOUTCAR空grepIBRIONOUTCARIBRION=2ionicrelax:0-MD1-quasi-New2-CG设置ADDGRID=.True.InINCAR设置IBRION=1inINCAR错误:internalERRORRSPHER:runningoutofbuffer001310nonlr.F:OutofbufferRSPHER得到的CONTCAR是空的!结构优化出现错误:Internal内部的、内在的ERRORRSPHER:runningoutofbuffer缓冲001310nonlr.F:OutofbufferRSPHER解决:将-NPAR=-1-修改成4(或者-2)-,问-题得以解决。分两步-Gsc-f非磁线性计算,bands读取-CHGCAR、WAVECAR-做非线性自旋轨道耦合计算),能带计算出错:ERROR:whilereadingWAVECAR,-planewavecoefficients系数•changed5728628837Solution:Youhavetocontinuewiththeconverged收敛CHGCAR,becausemostprobably,youwillincrease增^加/change改变thek-meshtogetadenser密集的、浓厚的k-gridtocalculatetheDOSaccurately.Then,WAVECARwillnotbereadcorrectlybecausethewavefunction-coefficients波函数-系数arestored存储k-pointwise明智的concerning涉及theREADerrorofCHGCAR:pleasecheckwhethertheFFTmesheshavechanged.pleasemakesurethattheCHGCARreallyisintheworkingdirectory目录atruntime运行时间thefftmeshesofCHGCARarecompatible兼容的Themainpointsisinthissentence"planewavecoefficientschanged",IthinktheISMEARyouusedinscfandnoscfprocessisdifferent,therefore,theplanewavecoefficientschangedinthesetwoprocessisnotidentical完全相同的.YoucanfindthevaluesofNGXF,NGYFandNGZFintheCHGCARorOUTCARofthescf,andthenaddthesethreeparametersintheINCARofthenonscf.OK,theproblemisresolved.在静态计算的CHGCAR或者OUTCAR中找到NGXF,NGYF和NGZF,将这些参数加到非静态计算的INCAR中:grepNGXFOUTCARdimensionx,y,zNGXF=64NGYF=64NGZF=840supportgridNGXF=64NGYF=64NGZF=840NGXF,Y,Zisequivalenttoacutoffof25.43,25.43,25.05a.u.对策:在能带计算INCAR中加入NGXF=64——NG¥F=-64-NGZF=-840修改之后,bands中出现错误:ERROR:-non-collinear-calculations-require-that-VASPis-compiled-without-theflag-DNGXhalfand--DNGZhalf解决:待解决!网上经验:noncollinearcalculationsrequirethatVASPiscompiledwithouttheflag-DNGXhalfand-DNGZhalf.一、请加入SOC1)INCAR中加入LNONCOLLINEAR=.True.LSORBIT=.True.LORBMOM=.True.ISYM=-1(?不对,ISYM取值0,l,2,3)【SAXIS=自旋轴方向;MAGMOM=每个原子的初始磁矩值】2)不要忘记toincludeSOC,please1)addthefollowinglinestoINCARLNONCOLLINEAR二.True.SimplecubeMCenterofanedgeRCornerpointXCenterofafaceFace-centeredcubicLSORBIT二.True.SAXIS=#pleasegivethespinquantizationaxishere,like001forthez-axis)MAGMOM=#pleasegiveatripletofnumbersforeachatomhere,andpleasehavealookatthemanual(chapternon-collinearcalculationsandspin-orbittag)onhowthedirectionofthemagneticmomentshastobedefinedwithrespecttothes
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