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- Nov 7, 2018 11:36:24 AM (5 years ago)
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- Tutorials/Magnetic-III
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Tutorials/Magnetic-III/Magnetic-III.htm
r3700 r3725 23 23 <o:Author>Von Dreele</o:Author> 24 24 <o:LastAuthor>vondreele</o:LastAuthor> 25 <o:Revision>2 2</o:Revision>26 <o:TotalTime>7 63</o:TotalTime>25 <o:Revision>23</o:Revision> 26 <o:TotalTime>779</o:TotalTime> 27 27 <o:Created>2012-05-05T14:50:00Z</o:Created> 28 <o:LastSaved>2018-1 0-23T13:56:00Z</o:LastSaved>28 <o:LastSaved>2018-11-07T17:35:00Z</o:LastSaved> 29 29 <o:Pages>1</o:Pages> 30 30 <o:Words>2118</o:Words> 31 <o:Characters>1207 4</o:Characters>31 <o:Characters>12075</o:Characters> 32 32 <o:Lines>100</o:Lines> 33 33 <o:Paragraphs>28</o:Paragraphs> 34 <o:CharactersWithSpaces>1416 4</o:CharactersWithSpaces>34 <o:CharactersWithSpaces>14165</o:CharactersWithSpaces> 35 35 <o:Version>16.00</o:Version> 36 36 </o:DocumentProperties> … … 1283 1283 <p class=MsoNormal>In this tutorials, we continue showing how GSAS-II makes use 1284 1284 of the Bilbao crystallographic server (<a href="http://www.cryst.ehu.es/">www.cryst.ehu.es/</a>) 1285 <i style='mso-bidi-font-style:normal'>Magnetic Symmetry and Applications</i> routine 1286 k-SUBGROUPSMAG (<a href="http://iopscience.iop.org/0953-8984/28/28/286001"><span 1287 style='font-size:10.0pt;font-family:"Arial",sans-serif'>Perez-Mato, JM; <span 1288 class=SpellE>Gallego</span>, SV; <span class=SpellE>Elcoro</span>, L; <span 1289 class=SpellE>Tasci</span>, E and <span class=SpellE>Aroyo</span>, MI, <i>J. of 1290 Phys.: <span class=SpellE>Condens</span> Matter</i> (2016), <b>28</b>:28601</span></a>) 1291 while determining a magnetic crystal structure with a non-zero propagation 1292 vector. If you have not done so already, you may wish to do the Simple Magnetic 1293 Structures tutorial first as it contains some background information that will 1294 not be covered here. It is also helpful to do parts I and II of the series of Magnetic 1295 Structures tutorials. To make this work, your computer must have an internet 1296 connection for GSAS-II to access this site. (We will supply the project file 1297 that results after k-SUBGROUPSMAG is called in case you lack internet access).</p> 1285 <i style='mso-bidi-font-style:normal'>Magnetic Symmetry and Applications</i> 1286 routine k-SUBGROUPSMAG (<a 1287 href="http://iopscience.iop.org/0953-8984/28/28/286001"><span style='font-size: 1288 10.0pt;font-family:"Arial",sans-serif'>Perez-Mato, JM; <span class=SpellE>Gallego</span>, 1289 SV; <span class=SpellE>Elcoro</span>, L; <span class=SpellE>Tasci</span>, E and 1290 <span class=SpellE>Aroyo</span>, MI, <i>J. of Phys.: <span class=SpellE>Condens</span> 1291 Matter</i> (2016), <b>28</b>:28601</span></a>) while determining a magnetic 1292 crystal structure with a non-zero propagation vector. If you have not done so 1293 already, you may wish to do the Simple Magnetic Structures tutorial first as it 1294 contains some background information that will not be covered here. It is also 1295 helpful to do parts I and II of the series of Magnetic Structures tutorials. To 1296 make this work, your computer must have an internet connection for GSAS-II to 1297 access this site. (We will supply the project file that results after 1298 k-SUBGROUPSMAG is called in case you lack internet access).</p> 1298 1299 1299 1300 <p class=MsoNormal><span style='mso-no-proof:yes'><!--[if gte vml 1]><v:shapetype … … 1321 1322 <v:imagedata src="Magnetic-III_files/image001.png" o:title=""/> 1322 1323 </v:shape><![endif]--><![if !vml]><img border=0 width=479 height=492 1323 src="Magnetic-III_files/image00 4.gif" v:shapes="Picture_x0020_4"><![endif]></span></p>1324 src="Magnetic-III_files/image002.gif" v:shapes="Picture_x0020_4"><![endif]></span></p> 1324 1325 1325 1326 <p class=MsoNormal>In this example, we will determine the magnetic structure … … 1345 1346 </v:shape><![endif]--><![if !vml]><img width=9 height=19 1346 1347 src="Magnetic-III_files/image008.gif" v:shapes="_x0000_i1025"><![endif]></span><![endif]>m2 1347 with a= 5.64870 Å and c= 5.64870Å. From the structure drawing above, you can1348 with a= 5.64870 Å and c= 14.46580Å. From the structure drawing above, you can 1348 1349 see a tetrameric string of face sharing CoO<sub>6</sub> <span class=SpellE>octahedra</span> 1349 1350 and a separate CoO<sub>4</sub> tetrahedron with one disordered oxygen position … … 1429 1430 <v:imagedata src="Magnetic-III_files/image003.png" o:title=""/> 1430 1431 </v:shape><![endif]--><![if !vml]><img border=0 width=432 height=266 1431 src="Magnetic-III_files/image0 21.gif" v:shapes="Picture_x0020_5"><![endif]></span></p>1432 src="Magnetic-III_files/image010.gif" v:shapes="Picture_x0020_5"><![endif]></span></p> 1432 1433 1433 1434 <p class=MsoNormal style='margin-left:.5in'><span class=GramE>and</span> the … … 1439 1440 <v:imagedata src="Magnetic-III_files/image005.png" o:title=""/> 1440 1441 </v:shape><![endif]--><![if !vml]><img border=0 width=433 height=447 1441 src="Magnetic-III_files/image0 25.gif" v:shapes="Picture_x0020_6"><![endif]></span></p>1442 src="Magnetic-III_files/image012.gif" v:shapes="Picture_x0020_6"><![endif]></span></p> 1442 1443 1443 1444 <p class=MsoNormal style='margin-left:.5in'>We will use the default limits.</p> … … 1499 1500 <v:imagedata src="Magnetic-III_files/image007.png" o:title=""/> 1500 1501 </v:shape><![endif]--><![if !vml]><img border=0 width=430 height=235 1501 src="Magnetic-III_files/image0 28.gif" v:shapes="Picture_x0020_7"><![endif]></span></p>1502 src="Magnetic-III_files/image014.gif" v:shapes="Picture_x0020_7"><![endif]></span></p> 1502 1503 1503 1504 <h3>Step 3. Check powder pattern indexing</h3> … … 1515 1516 <v:imagedata src="Magnetic-III_files/image009.png" o:title=""/> 1516 1517 </v:shape><![endif]--><![if !vml]><img border=0 width=479 height=162 1517 src="Magnetic-III_files/image0 57.gif" v:shapes="Picture_x0020_8"><![endif]></span></p>1518 src="Magnetic-III_files/image016.gif" v:shapes="Picture_x0020_8"><![endif]></span></p> 1518 1519 1519 1520 <p class=MsoNormal>This can use lattice parameters & space groups to … … 1542 1543 <v:imagedata src="Magnetic-III_files/image011.png" o:title=""/> 1543 1544 </v:shape><![endif]--><![if !vml]><img border=0 width=477 height=152 1544 src="Magnetic-III_files/image0 58.gif" v:shapes="Picture_x0020_9"><![endif]></span></p>1545 src="Magnetic-III_files/image018.gif" v:shapes="Picture_x0020_9"><![endif]></span></p> 1545 1546 1546 1547 <p class=MsoNormal><span class=GramE>showing</span> the lattice constants for … … 1570 1571 <v:imagedata src="Magnetic-III_files/image013.png" o:title=""/> 1571 1572 </v:shape><![endif]--><![if !vml]><img border=0 width=473 height=488 1572 src="Magnetic-III_files/image0 59.gif" v:shapes="Picture_x0020_10"><![endif]></span></b></p>1573 src="Magnetic-III_files/image020.gif" v:shapes="Picture_x0020_10"><![endif]></span></b></p> 1573 1574 1574 1575 <p class=MsoNormal>Ive expanded & shifted the plot slightly to see that a … … 1605 1606 <v:imagedata src="Magnetic-III_files/image015.png" o:title=""/> 1606 1607 </v:shape><![endif]--><![if !vml]><img border=0 width=476 height=152 1607 src="Magnetic-III_files/image0 60.gif" v:shapes="Picture_x0020_11"><![endif]></span></p>1608 src="Magnetic-III_files/image022.gif" v:shapes="Picture_x0020_11"><![endif]></span></p> 1608 1609 1609 1610 <p class=MsoNormal>Notice that the a-axis (11.2974) is now twice the original … … 1611 1612 1612 1613 <p class=MsoNormal><span style='mso-no-proof:yes'><!--[if gte vml 1]><v:shape 1613 id=" Picture_x0020_12" o:spid="_x0000_i1044" type="#_x0000_t75" style='width:356.25pt;1614 height:366.75pt;visibility:visible;mso-wrap-style:square'>1614 id="_x0000_i1044" type="#_x0000_t75" style='width:356.25pt;height:366.75pt; 1615 visibility:visible;mso-wrap-style:square'> 1615 1616 <v:imagedata src="Magnetic-III_files/image017.png" o:title=""/> 1616 1617 </v:shape><![endif]--><![if !vml]><img border=0 width=475 height=489 1617 src="Magnetic-III_files/image0 61.gif" v:shapes="Picture_x0020_12"><![endif]></span></p>1618 src="Magnetic-III_files/image024.gif" v:shapes="_x0000_i1044"><![endif]></span></p> 1618 1619 1619 1620 <p class=MsoNormal>Clearly that did not index all the observed peaks, so we … … 1632 1633 <v:imagedata src="Magnetic-III_files/image019.png" o:title=""/> 1633 1634 </v:shape><![endif]--><![if !vml]><img border=0 width=480 height=493 1634 src="Magnetic-III_files/image0 62.gif" v:shapes="Picture_x0020_13"><![endif]></span></p>1635 src="Magnetic-III_files/image026.gif" v:shapes="Picture_x0020_13"><![endif]></span></p> 1635 1636 1636 1637 <p class=MsoNormal>In this case every powder peak is indexed so a doubling of … … 1663 1664 <v:imagedata src="Magnetic-III_files/image030.png" o:title=""/> 1664 1665 </v:shape><![endif]--><![if !vml]><img border=0 width=277 height=301 1665 src="Magnetic-III_files/image0 63.gif" v:shapes="Picture_x0020_32"><![endif]></span></p>1666 src="Magnetic-III_files/image032.gif" v:shapes="Picture_x0020_32"><![endif]></span></p> 1666 1667 1667 1668 <p class=MsoNormal>These are the controls for running the Bilbao routine. The … … 1700 1701 1701 1702 <p class=MsoNormal><span style='mso-no-proof:yes'><!--[if gte vml 1]><v:shape 1702 id=" _x0000_i1041" type="#_x0000_t75" style='width:357.75pt;height:123.75pt;1703 visibility:visible;mso-wrap-style:square'>1703 id="Picture_x0020_12" o:spid="_x0000_i1041" type="#_x0000_t75" style='width:357.75pt; 1704 height:123.75pt;visibility:visible;mso-wrap-style:square'> 1704 1705 <v:imagedata src="Magnetic-III_files/image023.png" o:title=""/> 1705 1706 </v:shape><![endif]--><![if !vml]><img border=0 width=477 height=165 1706 src="Magnetic-III_files/image0 64.gif" v:shapes="_x0000_i1041"><![endif]></span></p>1707 src="Magnetic-III_files/image034.gif" v:shapes="Picture_x0020_12"><![endif]></span></p> 1707 1708 1708 1709 <p class=MsoNormal>Press <b style='mso-bidi-font-weight:normal'><span … … 1735 1736 1736 1737 <p class=MsoNormal><span style='mso-no-proof:yes'><!--[if gte vml 1]><v:shape 1737 id=" Picture_x0020_33" o:spid="_x0000_i1040" type="#_x0000_t75" style='width:360.75pt;1738 height:293.25pt;visibility:visible;mso-wrap-style:square'>1739 <v:imagedata src="Magnetic-III_files/image0 66.png" o:title=""/>1740 </v:shape><![endif]--><![if !vml]><img border=0 width=4 81 height=3911741 src="Magnetic-III_files/image0 65.gif" v:shapes="Picture_x0020_33"><![endif]></span></p>1738 id="_x0000_i1040" type="#_x0000_t75" style='width:358.5pt;height:323.25pt; 1739 visibility:visible;mso-wrap-style:square'> 1740 <v:imagedata src="Magnetic-III_files/image035.png" o:title=""/> 1741 </v:shape><![endif]--><![if !vml]><img border=0 width=478 height=431 1742 src="Magnetic-III_files/image036.gif" v:shapes="_x0000_i1040"><![endif]></span></p> 1742 1743 1743 1744 <p class=MsoNormal>Notice that the number of unique magnetic atoms is either 3 … … 1745 1746 atoms. Use the <b style='mso-bidi-font-weight:normal'><span style='font-family: 1746 1747 "Calibri",sans-serif;mso-ascii-theme-font:minor-latin;mso-hansi-theme-font: 1747 minor-latin;mso-bidi-theme-font:minor-latin'>Try</span></b> on the first two 1748 entries; they both index every reflection. The two seem identical except for 1749 t he translation vector. Double click the row number for the 1<sup>st</sup> one;1750 apopup will appear</p>1748 minor-latin;mso-bidi-theme-font:minor-latin'>Try</span></b> on the first two entries; 1749 they both index every reflection. The two seem identical except for the 1750 translation vector. Click the space group symbol for the 1<sup>st</sup> one; a 1751 popup will appear</p> 1751 1752 1752 1753 <p class=MsoNormal><span style='mso-no-proof:yes'><!--[if gte vml 1]><v:shape … … 1755 1756 <v:imagedata src="Magnetic-III_files/image027.png" o:title=""/> 1756 1757 </v:shape><![endif]--><![if !vml]><img border=0 width=406 height=440 1757 src="Magnetic-III_files/image0 67.gif" v:shapes="Picture_x0020_14"><![endif]></span></p>1758 src="Magnetic-III_files/image038.gif" v:shapes="Picture_x0020_14"><![endif]></span></p> 1758 1759 1759 1760 <p class=MsoNormal>These are the magnetic symmetry operations for P<sub>c</sub> 1760 1761 -6 c 2. The subscript c on the lattice symbol indicates the c-axis magnetic 1761 centering operation; see the entry <b style='mso-bidi-font-weight:normal'><span 1762 style='font-family:"Calibri",sans-serif;mso-ascii-theme-font:minor-latin; 1763 mso-hansi-theme-font:minor-latin;mso-bidi-theme-font:minor-latin'>for (0<span 1764 class=GramE>,0,1</span>/2)+1</span></b>. The list of operators below it are 1765 in red to indicate the spin inversion is applied for all of them. The Print Ops 1766 button makes a full list on the console; these can be cut & pasted into 1767 other programs as needed. Press <b style='mso-bidi-font-weight:normal'><span 1768 style='font-family:"Calibri",sans-serif;mso-ascii-theme-font:minor-latin; 1769 mso-hansi-theme-font:minor-latin;mso-bidi-theme-font:minor-latin'>OK</span></b>. 1762 centering operation; see the entry <span style='font-family:"Calibri",sans-serif; 1763 mso-ascii-theme-font:minor-latin;mso-hansi-theme-font:minor-latin;mso-bidi-theme-font: 1764 minor-latin'>for (0<span class=GramE>,0,1</span>/2)+1</span>. The list of 1765 operators below it are in red to indicate the spin inversion is applied for all 1766 of them. The Print Ops button makes a full list on the console; these can be 1767 cut & pasted into other programs as needed. Press <b style='mso-bidi-font-weight: 1768 normal'><span style='font-family:"Calibri",sans-serif;mso-ascii-theme-font: 1769 minor-latin;mso-hansi-theme-font:minor-latin;mso-bidi-theme-font:minor-latin'>OK</span></b>. 1770 1770 Since the 1<sup>st</sup> two solutions seem reasonable, well try these.</p> 1771 1771 … … 1783 1783 <v:imagedata src="Magnetic-III_files/image029.png" o:title=""/> 1784 1784 </v:shape><![endif]--><![if !vml]><img border=0 width=479 height=246 1785 src="Magnetic-III_files/image0 68.gif" v:shapes="Picture_x0020_15"><![endif]></span></p>1785 src="Magnetic-III_files/image040.gif" v:shapes="Picture_x0020_15"><![endif]></span></p> 1786 1786 1787 1787 <p class=MsoNormal>Do <b style='mso-bidi-font-weight:normal'><span … … 1795 1795 <v:imagedata src="Magnetic-III_files/image031.png" o:title=""/> 1796 1796 </v:shape><![endif]--><![if !vml]><img border=0 width=297 height=297 1797 src="Magnetic-III_files/image0 69.gif" v:shapes="Picture_x0020_16"><![endif]></span></p>1797 src="Magnetic-III_files/image041.gif" v:shapes="Picture_x0020_16"><![endif]></span></p> 1798 1798 1799 1799 <p class=MsoNormal>This shows all magnetic phases that were marked Keep in the … … 1810 1810 <v:imagedata src="Magnetic-III_files/image033.png" o:title=""/> 1811 1811 </v:shape><![endif]--><![if !vml]><img border=0 width=378 height=165 1812 src="Magnetic-III_files/image0 70.gif" v:shapes="Picture_x0020_17"><![endif]></span></p>1812 src="Magnetic-III_files/image042.gif" v:shapes="Picture_x0020_17"><![endif]></span></p> 1813 1813 1814 1814 <p class=MsoNormal>Since the chemical phase had three Co atoms, having three … … 1845 1845 <v:imagedata src="Magnetic-III_files/image037.png" o:title=""/> 1846 1846 </v:shape><![endif]--><![if !vml]><img border=0 width=625 height=330 1847 src="Magnetic-III_files/image0 71.gif" v:shapes="Picture_x0020_18"><![endif]></span></p>1847 src="Magnetic-III_files/image043.gif" v:shapes="Picture_x0020_18"><![endif]></span></p> 1848 1848 1849 1849 <p class=MsoNormal>Select Atoms, enter <b style='mso-bidi-font-weight:normal'><span … … 1864 1864 <v:imagedata src="Magnetic-III_files/image039.png" o:title=""/> 1865 1865 </v:shape><![endif]--><![if !vml]><img border=0 width=454 height=864 1866 src="Magnetic-III_files/image0 72.gif" v:shapes="Picture_x0020_19"><![endif]></span></p>1866 src="Magnetic-III_files/image044.gif" v:shapes="Picture_x0020_19"><![endif]></span></p> 1867 1867 1868 1868 <p class=MsoNormal>Do <b style='mso-bidi-font-weight:normal'><span … … 1881 1881 style='mso-bidi-font-weight:normal'><span style='font-family:"Calibri",sans-serif; 1882 1882 mso-ascii-theme-font:minor-latin;mso-hansi-theme-font:minor-latin;mso-bidi-theme-font: 1883 minor-latin'>Refine unit cell</span></b> box for each. Then go to Sample 1884 parametersfor the PWDR data set, set goniometer radius to <b style='mso-bidi-font-weight:1883 minor-latin'>Refine unit cell</span></b> box for each. Then go to Sample parameters 1884 for the PWDR data set, set goniometer radius to <b style='mso-bidi-font-weight: 1885 1885 normal'><span style='font-family:"Calibri",sans-serif;mso-ascii-theme-font: 1886 1886 minor-latin;mso-hansi-theme-font:minor-latin;mso-bidi-theme-font:minor-latin'>650</span></b> … … 1916 1916 <v:imagedata src="Magnetic-III_files/image047.png" o:title=""/> 1917 1917 </v:shape><![endif]--><![if !vml]><img border=0 width=475 height=799 1918 src="Magnetic-III_files/image0 73.gif" v:shapes="Picture_x0020_23"><![endif]></span></p>1918 src="Magnetic-III_files/image045.gif" v:shapes="Picture_x0020_23"><![endif]></span></p> 1919 1919 1920 1920 <p class=MsoNormal>The fit to the powder pattern looks quite good</p> … … 1925 1925 <v:imagedata src="Magnetic-III_files/image049.png" o:title=""/> 1926 1926 </v:shape><![endif]--><![if !vml]><img border=0 width=480 height=377 1927 src="Magnetic-III_files/image0 74.gif" v:shapes="Picture_x0020_24"><![endif]></span></p>1927 src="Magnetic-III_files/image046.gif" v:shapes="Picture_x0020_24"><![endif]></span></p> 1928 1928 1929 1929 <p class=MsoNormal>But we should try the other solution to see if it is better. … … 1953 1953 <v:imagedata src="Magnetic-III_files/image051.png" o:title=""/> 1954 1954 </v:shape><![endif]--><![if !vml]><img border=0 width=479 height=247 1955 src="Magnetic-III_files/image0 75.gif" v:shapes="Picture_x0020_25"><![endif]></span></p>1955 src="Magnetic-III_files/image048.gif" v:shapes="Picture_x0020_25"><![endif]></span></p> 1956 1956 1957 1957 <p class=MsoNormal>Do <b style='mso-bidi-font-weight:normal'><span … … 1965 1965 <v:imagedata src="Magnetic-III_files/image031.png" o:title=""/> 1966 1966 </v:shape><![endif]--><![if !vml]><img border=0 width=297 height=297 1967 src="Magnetic-III_files/image0 69.gif" v:shapes="Picture_x0020_26"><![endif]></span></p>1967 src="Magnetic-III_files/image041.gif" v:shapes="Picture_x0020_26"><![endif]></span></p> 1968 1968 1969 1969 <p class=MsoNormal>We already tried the 1<sup>st</sup> one; now select the 2<sup>nd</sup> … … 1975 1975 <v:imagedata src="Magnetic-III_files/image053.png" o:title=""/> 1976 1976 </v:shape><![endif]--><![if !vml]><img border=0 width=378 height=165 1977 src="Magnetic-III_files/image0 76.gif" v:shapes="Picture_x0020_27"><![endif]></span></p>1977 src="Magnetic-III_files/image050.gif" v:shapes="Picture_x0020_27"><![endif]></span></p> 1978 1978 1979 1979 <p class=MsoNormal>It looks very similar to what we had before; close … … 1992 1992 <v:imagedata src="Magnetic-III_files/image055.png" o:title=""/> 1993 1993 </v:shape><![endif]--><![if !vml]><img border=0 width=484 height=249 1994 src="Magnetic-III_files/image0 77.gif" v:shapes="Picture_x0020_28"><![endif]></span></p>1994 src="Magnetic-III_files/image052.gif" v:shapes="Picture_x0020_28"><![endif]></span></p> 1995 1995 1996 1996 <p class=MsoNormal>Select the Atoms tab & set <span class=SpellE>Mz</span> … … 2024 2024 Finally use <b style='mso-bidi-font-weight:normal'><span style='font-family: 2025 2025 "Calibri",sans-serif;mso-ascii-theme-font:minor-latin;mso-hansi-theme-font: 2026 minor-latin;mso-bidi-theme-font:minor-latin'>6</span></b> background coefficients 2027 and refine <b style='mso-bidi-font-weight:normal'><span style='font-family: 2028 "Calibri",sans-serif;mso-ascii-theme-font:minor-latin;mso-hansi-theme-font: 2029 minor-latin;mso-bidi-theme-font:minor-latin'>XU</span></b> for the chemical 2030 phase atoms and <b style='mso-bidi-font-weight:normal'><span style='font-family: 2031 "Calibri",sans-serif;mso-ascii-theme-font:minor-latin;mso-hansi-theme-font: 2032 minor-latin;mso-bidi-theme-font:minor-latin'>XUM</span></b> for the magnetic 2033 atoms. Do <b style='mso-bidi-font-weight:normal'><span style='font-family:"Calibri",sans-serif; 2034 mso-ascii-theme-font:minor-latin;mso-hansi-theme-font:minor-latin;mso-bidi-theme-font: 2035 minor-latin'>Calculate/Refine</span></b> a few times until it converges. I got <span 2036 class=SpellE>wR</span> = 7.47% which is only slightly better than the result 2037 for the first model. In this case the tetrahedral Co atom carries the large 2038 magnetic moment while the octahedral ones have nearly zero moment. This is 2039 probably the better model because it is similar to the magnetic structures 2040 found for related materials. We can see if the moment is fully on the 2041 tetrahedral Co; set <span class=SpellE><b style='mso-bidi-font-weight:normal'><span 2042 style='font-family:"Calibri",sans-serif;mso-ascii-theme-font:minor-latin; 2043 mso-hansi-theme-font:minor-latin;mso-bidi-theme-font:minor-latin'>Mz</span></b></span><b 2026 minor-latin;mso-bidi-theme-font:minor-latin'>6</span></b> background 2027 coefficients and refine <b style='mso-bidi-font-weight:normal'><span 2028 style='font-family:"Calibri",sans-serif;mso-ascii-theme-font:minor-latin; 2029 mso-hansi-theme-font:minor-latin;mso-bidi-theme-font:minor-latin'>XU</span></b> 2030 for the chemical phase atoms and <b style='mso-bidi-font-weight:normal'><span 2031 style='font-family:"Calibri",sans-serif;mso-ascii-theme-font:minor-latin; 2032 mso-hansi-theme-font:minor-latin;mso-bidi-theme-font:minor-latin'>XUM</span></b> 2033 for the magnetic atoms. Do <b style='mso-bidi-font-weight:normal'><span 2034 style='font-family:"Calibri",sans-serif;mso-ascii-theme-font:minor-latin; 2035 mso-hansi-theme-font:minor-latin;mso-bidi-theme-font:minor-latin'>Calculate/Refine</span></b> 2036 a few times until it converges. I got <span class=SpellE>wR</span> = 7.47% 2037 which is only slightly better than the result for the first model. In this case 2038 the tetrahedral Co atom carries the large magnetic moment while the octahedral 2039 ones have nearly zero moment. This is probably the better model because it is 2040 similar to the magnetic structures found for related materials. We can see if 2041 the moment is fully on the tetrahedral Co; set <span class=SpellE><b 2044 2042 style='mso-bidi-font-weight:normal'><span style='font-family:"Calibri",sans-serif; 2045 2043 mso-ascii-theme-font:minor-latin;mso-hansi-theme-font:minor-latin;mso-bidi-theme-font: 2046 minor-latin'>=0</span></b> for the other two and set their refinement flags to 2047 just <b style='mso-bidi-font-weight:normal'><span style='font-family:"Calibri",sans-serif; 2048 mso-ascii-theme-font:minor-latin;mso-hansi-theme-font:minor-latin;mso-bidi-theme-font: 2049 minor-latin'>XU</span></b>. Do <b style='mso-bidi-font-weight:normal'><span 2050 style='font-family:"Calibri",sans-serif;mso-ascii-theme-font:minor-latin; 2051 mso-hansi-theme-font:minor-latin;mso-bidi-theme-font:minor-latin'>Calculate/Refine</span></b>. 2052 My final <span class=SpellE>wR</span>=7.476% shows that probably all the 2053 magnetic moment is on the tetrahedral Co atoms. The Atoms list </p> 2044 minor-latin'>Mz</span></b></span><b style='mso-bidi-font-weight:normal'><span 2045 style='font-family:"Calibri",sans-serif;mso-ascii-theme-font:minor-latin; 2046 mso-hansi-theme-font:minor-latin;mso-bidi-theme-font:minor-latin'>=0</span></b> 2047 for the other two and set their refinement flags to just <b style='mso-bidi-font-weight: 2048 normal'><span style='font-family:"Calibri",sans-serif;mso-ascii-theme-font: 2049 minor-latin;mso-hansi-theme-font:minor-latin;mso-bidi-theme-font:minor-latin'>XU</span></b>. 2050 Do <b style='mso-bidi-font-weight:normal'><span style='font-family:"Calibri",sans-serif; 2051 mso-ascii-theme-font:minor-latin;mso-hansi-theme-font:minor-latin;mso-bidi-theme-font: 2052 minor-latin'>Calculate/Refine</span></b>. My final <span class=SpellE>wR</span>=7.476% 2053 shows that probably all the magnetic moment is on the tetrahedral Co atoms. The 2054 Atoms list </p> 2054 2055 2055 2056 <p class=MsoNormal><span style='mso-no-proof:yes'><!--[if gte vml 1]><v:shape … … 2058 2059 <v:imagedata src="Magnetic-III_files/image084.png" o:title=""/> 2059 2060 </v:shape><![endif]--><![if !vml]><img border=0 width=482 height=110 2060 src="Magnetic-III_files/image0 78.gif" v:shapes="Picture_x0020_29"><![endif]></span></p>2061 src="Magnetic-III_files/image054.gif" v:shapes="Picture_x0020_29"><![endif]></span></p> 2061 2062 2062 2063 <p class=MsoNormal><span class=GramE>gives</span> <span class=SpellE>Mz</span>=3.347(43); … … 2071 2072 <v:imagedata src="Magnetic-III_files/image086.png" o:title=""/> 2072 2073 </v:shape><![endif]--><![if !vml]><img border=0 width=237 height=480 2073 src="Magnetic-III_files/image0 79.gif" v:shapes="Picture_x0020_30"><![endif]><!--[if gte vml 1]><v:shape2074 src="Magnetic-III_files/image056.gif" v:shapes="Picture_x0020_30"><![endif]><!--[if gte vml 1]><v:shape 2074 2075 id="Picture_x0020_31" o:spid="_x0000_i1025" type="#_x0000_t75" style='width:187.5pt; 2075 2076 height:358.5pt;visibility:visible;mso-wrap-style:square'> 2076 2077 <v:imagedata src="Magnetic-III_files/image088.png" o:title=""/> 2077 2078 </v:shape><![endif]--><![if !vml]><img border=0 width=250 height=478 2078 src="Magnetic-III_files/image08 0.gif" v:shapes="Picture_x0020_31"><![endif]></span></p>2079 src="Magnetic-III_files/image081.gif" v:shapes="Picture_x0020_31"><![endif]></span></p> 2079 2080 2080 2081 <p class=MsoNormal>Ive placed the doubled c-axis chemical structure so you can -
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