Transition Metal Oxides A. J. Millis Department of Physics Columbia University NSF DMR 1006282 DOE BES ER 046160 and CMCSN program Copyright A. J. Millis 2013 Columbia University Outline 1. Introduction: History 2. Overview: Phenomena 3. Basic Chemistry and Electronic Structure 4. Theory--General 5. Dynamical Mean Field Theory and Oxides 6. Applications and Prospects Copyright A. J. Millis 2013 Columbia University Transition metal ``oxides’’ Periodic Table of the Elements GROUP 1 IA 1 1 1.00794 H !"#$%&'()$*+, 12$*#3 2 1^gX 2.2 Hydrogen 0.0899 -259.14 =:?'37 13.5984 -252.87 - 3 2 6.941 Li 2 1^gX 0.98 Lithium 0.535 180.54 =$?'152 5.3917 1342 BCC 4 1 1_ 1.57 1.848 1287 =$?'112 9.3227 2470 HCP 11 Na Period 3 2 1^gX 0.82 Rubidium 5 X 12 B\+C'XA `2 24.3050 Mg 1_ 1 1_ 1.00 Calcium Alkali Metals Noble Gas Alkaline Earth Metals Halogens !*A#3)"+'Q+,# !"#$%&'G8AA'R5%" !:#/86,#'I#5A"85" J8A+'#L'(8"),83'9#/8,%"0$A J#3"E$855'&#5A"85" <3+&",#5'G8AA Poor Metals 3 IIIB 21 44.955910 Sc Metalloids 4 IVB 2 @bgX 1.36 Scandium 22 5 VB 47.867 Ti 23 3 UX 1.54 Titanium e k m+ $+c X ,_ +F e U D 2 S hc X 6 VIB 50.9415 V 24 Cr 4 UbgX 1.63 Vanadium 7 1b 1.66 Chromium 25 2.8179403x10 m 1.602176x10-19 J 1.602176x10-19 C 96 485.3399 C/mol 0.0072973525 3.7417749x10-16 W m2 Mn 1+&#56'T86%8"%#5'I#5A"85" 1K++6'#L'9%/0"'%5'8'F8&))$ 1K++6'#L'A#)56'%5'8%,'8"'1V> 1"8568,6'>,+AA),+ 8 VIII 54.938049 6 1agX 1.55 Manganese p h m +gm K R R c R hc ch/k c -15 7 VIIB 51.9961 G R 4,8:%"8"%#5'I#5A"85" G#38,'48A'I#5A"85" G#38,'F#3)$+'=D6+83'48A? >D >385&S'I#5A"85" >,#"#57<3+&",#5'G8AA'T8"%# T26*+,/'I#5A"85" -273.15 °C 1.660539x10-27 kg 23 -1 6.022142x10 mol 2.718281828 -23 1.380650x10 J/K 9.10938215x10-31 kg 0.5110 MeV m) <3+&",#5'T86%)A'=I38AA%&83? <3+&",#5'F#3" <3+$+5",2'I08,/+ U8,8682'I#5A"85" L%5+7A",)&"),+'&#5A"85" U%,A"'T86%8"%#5'I#5A"85" Non Metals Rare Earth Metals BWXC 1#),&+O'K02A%&AP5%A"P/#: Common Constants Solid Synthetic Transition Metals 1 1.31 Magnesium Ca † Liquid Categories Sr 1 1_ 0.95 Strontium Y 2 D3/2 1.22 Yttrium 1.532 2.63 4.472 4.1771 5.6949 6.2173 39.31 688 777 1382 1526 3345 =$?'248 BCC =$?'215 FCC =$?'180 HCP Bh,C'aA ^ Bh,C'aA X Bh,C'W6 ^'aAX `1 `2 `3 132.90545 56 137.327 55 2 1^gX 0.79 Cesium Ba 1 1_ 0.89 Barium 1.879 3.51 3.8939 5.2117 28.44 671 727 1870 =$?'265 BCC =$?'222 BCC Bi+C'eA ^ Bi+C'eA X `1 `2 (223) 88 (226) 87 Fr 7 1^gX 13 IIIA 9 VIII 26 55.845 Fe Iron 5 @W 1.83 27 10 VIII 58.933200 Co 6.67428x10-11 m3 kg-1 s-2 8.314472 J mol-1 K-1 3 0.02241410 m /mol 3.14159265358979 -34 6.626069x10 J s 1836.15267247 10 973 732 m-1 3.289842x1015 Hz 13.6057 eV 0.01438769 m K 299 792 458 m/s 343.2 m/s 101 325 Pa 4 UfgX 1.88 Cobalt 28 11 IB 58.6934 Ni 3 UW 1.91 Nickel 63.546 Cu 2 1^gX 1.90 Copper 10.811 B 8.2980 4000 rhom. 2.26 3550 =:?'77 11.2603 4027 hex 1.251 -210.1 =:?'75 >H^gX 1.61 Aluminum 2.7 5.9858 YWXZ 660.32 2519 =$?'143 FCC B(+C'bA X'bK^ `3 65.409 31 69.723 30 Zn Zinc 1 1_ 1.65 Ga 2 >H^gX 1.81 Gallium 2 1^gX 0.7 Francium - 4.0727 BT5C'cA ^ `1 Ra Nb Mo 6 D1/2 1.60 Niobium 7 S3 2.16 Molybdenum Tc 6 S5/2 1.9 Technetium Ru 5 F5 2.20 Ruthenium Rh 4 F9/2 2.28 Rhodium Pd 1 S0 2.20 Palladium Ag 2 S1/2 1.93 Silver Cd 1 S0 1.69 Cadmium In 2 P°1/2 1.78 Indium 6.511 8.57 10.28 11.5 12.37 12.45 12.023 10.49 8.65 7.31 6.6339 6.7589 7.0924 7.28 7.3605 7.4589 8.3369 7.5762 8.9938 5.7864 1855 4409 2477 4744 2623 4639 2157 4265 2334 4150 1964 3695 1554.9 2963 961.78 2162 321.07 767 156.6 2072 =$?'160 HCP =$?'146 BCC =$?'139 BCC =$?'136 HCP =$?'134 HCP =$?'134 FCC =$?'137 FCC =$?'144 FCC =$?'151 §hex =$?'167 §tetra. Bh,C'W6 X'aAX Bh,C'W6 W'aA^ Bh,C'W6 a'aA^ Bh,C'W6 a'aAX Bh,C'W6 c'aA^ Bh,C'W6 ]'aA^ Bh,C'W6 ^_ Bh,C'W6 ^_'aA^ Bh,C'W6 ^_'aAX Bh,C'W6 ^_'aAX'aK^ +4 `3[a `X[b[W[a[6 `W[7 `X[b[4[e[] `X[3[W `2[W `1 `2 `3 178.49 73 180.9479 74 183.84 75 186.207 76 190.23 77 192.217 78 195.078 79 196.96655 80 200.59 81 204.3833 72 Hf 3 UX 1.3 Ta W 4 UbgX 1.5 Tantalum 985"085%6+'1+,%+A 13.31 5 @_ 2.36 Tungsten Re 6 1agX 1.9 Rhenium Os Ir 5 @W 2.2 Osmium 4 UfgX 2.2 Iridium Pt 3 @b 2.28 Platinum Au 2 1^gX Gold 2.54 Hg 1 1_ 2 Mercury Tl 2 >H^gX 1.62 Thallium 16.65 19.25 21.02 22.61 22.65 21.09 19.3 13.534 10.4375 11.85 6.8251 7.5496 7.8640 7.8335 8.4382 8.9670 8.9588 9.2255 6.1082 2233 4603 3017 5458 3422 5555 3186 5596 3033 5012 2466 4428 1768.3 3825 1064.18 2856 -38.83 356.73 304 1473 =$?'159 HCP =$?'146 BCC =$?'139 BCC =$?'137 HCP =$?'135 HCP =$?'136 FCC =$?'139 FCC =$?'144 FCC =$?'151 §rhom. =$?'170 HCP Bi+C'WL ^W'a6X'eAX Bi+C'WL ^W'a6b'eAX Bi+C'WL ^W'a6W'eAX Bi+C'WL ^W'a6a'eAX Bi+C'WL ^W'a6e'eAX Bi+C'WL ^W'a6c'eAX Bi+C'WL ^W'a6f'eA^ Bi+C'WL ^W'a6^_'eA^ Bi+C'WL ^W'a6^_'eAX B\/C'eK^ +4 `5 `X[b[W[a[6 `X[W[e[7[7^ `X[b[4[e[] `X[b[4[e `X[4 `^[3 `^[2 `1[b (261) 105 (262) 106 (266) 107 (264) 108 (277) 109 (268) 110 (281) 111 (272) 112 (285) 113 104 Rf 1 1_ Radium 3 F2 1.33 Zirconium Hafnium 0.9 5 5.2784 700 1737 BCC BT5C'cA X `2 Zr !&"%5%6+ 1+,%+A 3 UX'd Rutherfordium Db Sg Dubnium Seaborgium Bh Bohrium Hs Hassium Mt Meitnerium Ds Rg Darmstadtium Roentgenium Cn Copernicium Uut Ununtrium >_ Carbon ^ 2 3 X 1 1_ 14 Si 15 >_ Silicon 2.33 8.1517 1414 2900 =:?'111 cubic B(+C'bA X'bKX `X[4[7W 72.64 32 Ge 3 >_ 2.01 Germanium - 5.323 7.8994 938.3 2820 =:?'122 §cubic ^_ X X B!,C'b6 'WA 'WK `X[4 118.710 50 Sn 3 P0 1.96 Tin 7.31 7.3439 231.93 2602 =:?'141 §tetra. Bh,C'W6 ^_'aAX'aKX `X[4 207.2 82 Pb 3 >_ Lead 2.33 1.429 -218.3 =:?'73 13.6181 -182.9 - 1.696 -219.6 =:?'71 4 1HbgX 2.18 4 S°3/2 2.05 Antimony 6.697 8.6084 630.63 1587 =:?'138 §rhom. Bh,C'W6 ^_'aAX'aKb `3[a[73 208.98038 83 Bi 16 1HbgX 2.19 5.727 9.7886 817 614 =:?'119 rhom. ^_ X b B!,C'b6 'WA 'WK `3[a[73 121.760 51 Sb X 4 Arsenic 4 1HbgX 2.02 Bismuth >X Oxygen b 1.823 10.4867 44.2 280.5 =:?'106 § B(+C'bA X'bKb `b[W[5[7b 74.92160 33 3 S 3 >X 2.58 Sulfur 1.96 10.3600 115.21 444.72 =:?'102 FCO B(+C'bA X'bKW `X[W[6[7X 78.96 34 Se 3 >X 2.55 Selenium 4.819 9.7524 221 685 =:?'116 §hex ^_ X W B!,C'b6 'WA 'WK `X[4[e[7X 127.60 52 Te 2 >HbgX 3.16 Br 2 >HbgX 2.96 Bromine 1 1_ - Neon a 3.214 12.9676 -101.5 -34.04 =:?'99 B(+C'bA X'bKa `1[b[a[c[71 79.904 35 21.5645 -246.08 X 18 e B\+C'XA 'XK _ 39.948 Ar 1 1_ - Argon 1.784 15.7596 -189.3 -185.8 =:?'97 B(+C'bA X'bKe _ 83.798 36 Kr I 2 P°3/2 2.66 Iodine 1_ 3 Xe 1 S0 2.60 Xenon 6.24 4.94 5.9 9.0096 10.4513 12.1298 449.51 988 113.7 184.3 -111.8 -108 =:?'135 hex =:?'133 BCO =:?'130 Bh,C'W6 ^_'aAX'aKW Bh,C'W6 ^_'aAX'aKa Bh,C'W6 ^_'aAX'aKe `X[4[e[7X `1[a[c[71 _ (209) 85 (210) 86 (222) 84 Po 3 >X 2.0 Polonium Ununquadium Ununpentium Ununhexium Uuh At 2 >HbgX 2.2 Astatine 302 B\/C'eKa `1[b[a[c[71 117 Rn 1 1_ - Radon 9.73 10.7485 -71 -61.7 =:?'145 B\/C'eKe _ Ununseptium Uuo Ununoctium 6.0 ? BT5C'aL ^W'e6X'cAX'd +4 >+,%#6%&'V8*3+'#L'"0+'<3+$+5"A @+A%/5'*2'F+,"+NWXP&#$ l'X_^^'F+,"+NWX'99IP'!33',%/0"A',+A+,:+6P Lanthanides 57 Actinides References: -(%A"P/#:[';.#3L,8$P&#$'=G8"0+$8"%&?[ ITI'\856*##S'#L'I0+$%A",2'856'>02A%&A ]^A"'<6%"%#5['X___7X__^['856'#"0+,A 1 (or more) from group VIA (O, or S, Se) 118 Uus Notes: 7'@+5A%"2')5%"A'8,+'/g&$ b'L#,'A#3%6A'856'/g9'#,'S/g&$ b'8"' _H'I+3A%)A'L#,'/8A+A 7'!"#$%&'.+%/0"'*8A+6'#5' ^XI 7'='?'%56%&8"+'$8AA'5)$*+,'#L'$#A"'A"8*3+'%A#"#K+ 7'I#$$#5'MN%68"%#5'1"8"+A'%5'*#36 7'<3+&",#5'I#5L%/P'*8A+6'#5'DR>!I'/)%6+3%5+A 7'j'%56%&8"+A'&,2A"83'A",)&"),+'%A')5)A)83'#,'$82',+k)%,+' +NK3858"%#5 7'=$?'G+"833%&',86%)A['=:?'I#:83+5"',86%)A 1 (or more) from transition metal group 1 Krypton 3.12 3.75 11.8138 13.9996 -7.3 59 -157.36 -153.22 =:?'114 BCO =:?'110 ^_ X a ^_ X e B!,C'b6 'WA 'WK B!,C'b6 'WA 'WK `1[a[71 _ 126.90447 54 131.293 53 3 P2 2.10 9.196 8.414 254 962 §cubic B\/C'eKW `X[4 (292) 116 Uup 0.9 -248.59 =:?'69 Chlorine Tellurium 11.34 9.78 7.4167 7.2855 327.46 1749 271.3 1564 =$?'175 FCC =:?'146 §rhom. B\/C'eKX B\/C'eKb `2[W `3[a (289) 115 114 Uuq 17.4228 -188.12 - B\+C'XA 'XK 71 35.453 Cl 20.1797 Ne >HbgX X 17 10 3.98 2 Fluorine W B\+C'XA 'XK 72 32.065 24.5874 -268.93 ^AX _ 18.9984032 14.5341 -195.79 - Phosphorus As 9 F B\+C'XA 'XK `X[3[W[a[7X[73 30.97361 P 15.9994 3.44 X 3 1.90 8 O 1HbgX 0.1785 =:?'32 17 VIIA 3.04 4 Nitrogen X B\+C'XA 'XK `X[4[7W 28.0855 16 VIA 14.0067 N B\+C'XA 'XK `3 26.981538 Al 7 2.55 X 13 12.0107 C >H^gX 2.46 2075 =:?'82 6 15 VA 2.04 2 Boron 12 IIB 29 14 IVA 0.856 1.55 2.985 4.507 6.11 7.14 7.47 7.874 8.9 8.908 8.92 7.14 5.904 4.3407 6.1132 6.5615 6.8281 6.7462 6.7665 7.4340 7.9024 7.8810 7.6398 7.7264 9.3942 5.9993 63.38 759 842 1484 1541 2830 1668 3287 1910 3407 1907 2671 1246 2061 1538 2861 1495 2927 1455 2913 1084.62 2927 419.53 907 29.76 2204 =$?'227 BCC =$?'197 FCC =$?'162 HCP =$?'147 HCP =$?'134 BCC =$?'128 BCC =$?'127 §cubic =$?'126 BCC =$?'125 HCP =$?'124 FCC =$?'128 FCC =$?'134 §hex =$?'135 §BCO ^ X ^ X X X b X a ^ a X e X c X ] X ^_ ^ ^_ X ^_ X ^ B!,C'WA B!,C'WA B!,C'b6 'WA B!,C'b6 'WA B!,C'b6 'WA B!,C'b6 'WA B!,C'b6 'WA B!,C'b6 'WA B!,C'b6 'WA B!,C'b6 'WA B!,C'b6 'WA B!,C'b6 'WA B!,C'b6 'WA 'WK `1 `2 `3 `X[b[4 `X[3[W[5 `X[3[e `2[b[W[e[c `X[3 `2[b `X[3 `^[2 `2 `3 85.4678 38 87.62 39 88.90585 40 91.224 41 92.90638 42 95.94 43 (98) 44 101.07 45 102.90550 46 106.42 47 107.8682 48 112.411 49 114.818 37 Cs 6 2 0.82 Potassium Gas Beryllium 0.968 1.738 5.1391 7.6462 97.72 883 650 1090 =$?'186 BCC =$?'160 HCP B(+C'bA ^ B(+C'bA X `1 `2 39.0983 20 40.078 19 Rb 5 1^gX Sodium K 4 2 0.93 Phase at STP 4.002602 He Helium Free Downloads at Vertex42.com 9.012182 Be ^ B\+C'XA `1 22.989770 2 1.00794 !"#$%&'.+%/0" 2 1^gX -4,#)5671"8"+'9+:+3 2.2 ;<3+&",#5+/8"%:%"2'=>8)3%5/? H (8$+ Hydrogen ;@+5A%"2'B(#"+C 0.0899 13.5984 -D#5%E8"%#5'<5+,/2'=+F? ;G+3"%5/'>#%5"'=HI? -259.14 -252.87 ;J#%3%5/'>#%5"'=HI? FCC I,2A"83'1",)&"),+'B(#"+C !"#$%&',86%)A'=K$?B(#"+C =:?'37 ^A^ <3+&",#5'I#5L%/),8"%#5 `^[7^ >#AA%*3+'MN%68"%#5'1"8"+A'B(#"+C 2 IIA ^A^ `1[7^ 1 18 VIIIA - 138.9055 La 2 @bgX 1.10 Lanthanum 58 140.116 Ce 59 1 G°4 1.12 Cerium Pr 140.90765 4 I°9/2 1.13 60 144.24 Nd 5 I4 1.14 Praseodymium Neodymium 61 Pm (145) 6 H°5/2 - Promethium 62 150.36 Sm 7 F0 1.17 Samarium 63 151.964 Eu 8 S°7/2 - Europium 64 157.25 Gd 9 D°2 1.20 Gadolinium 65 158.92534 Tb 6 H°15/2 - Terbium 66 Dy 162.500 5 I8 1.22 Dysprosium 67 164.93032 Ho 4 I°15/2 1.23 Holmium 68 167.259 Er 3 H6 1.24 Erbium 69 168.93421 Tm 2 F°7/2 1.25 Thulium 70 173.04 Yb 1 S0 - Ytterbium 71 174.967 Lu 2 @bgX 1.27 Lutetium 7.353 5.244 7.901 8.219 8.551 8.795 9.066 9.321 6.57 9.841 6.146 6.689 6.64 7.01 7.264 5.582 5.6437 5.6704 6.1498 5.8638 5.9389 6.0215 6.1077 6.1843 6.2542 5.4259 5.5769 5.5387 5.473 5.5250 920 3464 798 3360 931 3290 1021 3100 1100 3000 1072 1803 822 1527 1313 3250 1356 3230 1412 2567 1474 2700 1497 2868 1545 1950 819 1196 1663 3402 =$?'187 §hex =$?'182 FCC =$?'182 §hex =$?'181 §hex =$?'183 HCP =$?'180 §hex =$?'180 BCC =$?'180 HCP =$?'177 HCP =$?'178 HCP =$?'176 HCP =$?'176 HCP =$?'176 HCP =$?'176 FCC =$?'174 HCP ^ X ^ ^ X b X W X a X e X c X c ^ X f X ^_ X ^^ X ^X X ^b X ^W X ^W Bi+C'a6 'eA Bi+C'WL 'a6 'eA Bi+C'WL 'eA Bi+C'WL 'eA Bi+C'WL 'eA Bi+C'WL 'eA Bi+C'WL 'eA Bi+C'WL 'a6 'eA Bi+C'WL 'eA Bi+C'WL 'eA Bi+C'WL 'eA Bi+C'WL 'eA Bi+C'WL 'eA Bi+C'WL 'eA Bi+C'WL 'a6 ^'eAX +3 +3[W +3[W +3 +3 `X[3 `X[3 +3 +3[W +3 +3 +3 `X[3 `X[3 +3 (227) 90 232.0381 91 231.0359 92 238.0289 93 (237) 94 (244) 95 (243) 96 (247) 97 (247) 98 (251) 99 (252) 100 (257) 101 (258) 102 (259) 103 (262) 89 Ac 2 @bgX 1.1 Actinium 10.07 5.17 1050 3200 FCC BT5C'e6 ^'cAX +3 Th 3 UX 1.3 Thorium 11.724 6.3067 1750 4820 =$?'179 FCC BT5C'e6 X'cAX +4 Copyright A. J. Millis 2013 Pa 4 h^^gX 1.5 Protactinium 15.37 5.89 1572 4000 =$?'163 §tetra BT5C'aL X'e6 ^'cAX `W[5 U 5 L°6 1.38 Uranium 19.05 6.1941 1135 3927 =$?'156 BCP BT5C'aL b'e6 ^'cAX `b[W[a[6 Np 6 L11/2 1.36 Neptunium 20.45 6.2657 644 4000 =$?'155 SO BT5C'aL W'e6 ^'cAX `b[W[5[e Pu 7 F0 1.28 Plutonium 19.816 6.0260 640 3230 =$?'159 §mono. BT5C'aL e'cAX `b[4[a[e Am 8 S°7/2 1.3 Americium 5.9738 1176 2011 =$?'173 HCP BT5C'aL c'cAX +3[W[a[e Cm 9 D°2 1.3 Curium 13.51 5.9914 1345 3110 =$?'174 HCP BT5C'aL c'e6 'cAX +3 Bk 6 H°15/2 1.3 Berkelium 14.78 6.1979 1050 =$?'170 hex BT5C'aL f'cAX +3[W Cf 5 I8 1.3 Californium 15.1 6.2817 900 hex BT5C'aL ^_'cAX +3 Es 4 I°15/2 1.3 Einsteinium 6.42 860 BT5C'aL ^^'cAX +3 Fm 3 H6 1.3 Fermium 6.50 1527 BT5C'aL ^X'cAX +3 Md 2 F°7/2 1.3 Mendelevium 6.58 827 BT5C'aL ^b'cAX `X[3 No 1 S0 1.3 Nobelium 6.65 827 BT5C'aL ^W'cAX `X[3 Lr 2 P°1/2 ? - Lawrencium 4.9 ? 1627 BT5C'aL ^W'cAX'cK'd +3 Plus other atoms (playing mainly structural role) Columbia University Some jargon Transition metal series: fill d-shell `Early’ (left side) `Late’ (right side) 3d 4d 5d Copyright A. J. Millis 2013 Columbia University Long history in condensed matter physics Frederich Wohler 1823 WO3: insulator (dull black) add sodium NaxWO3: shiny metal Copyright A. J. Millis 2013 Columbia University In modern terms: doping-driven metal insulator transition NaxTayWO3: # added electrons=x-y Dubson and Holcomb, Phys. Rev. B32 1955 (1985) Copyright A. J. Millis 2013 Columbia University More history 1897: J.J. Thompson discovers electron. Natural inference: transport and optical properties largely determined by electrons 1900: Drude--classical model of electronic conduction Classical mechanics: mean velocity ~ T1/2 idea: conduction should cease as T->0 Copyright A. J. Millis 2013 Columbia University More history Classical mechanics: mean velocity ~ T1/2 idea: conduction should cease as T->0 This idea motivated KamerlinghOnnes to investigate properties of metals at very low T Copyright A. J. Millis 2013 Columbia University More history Classical mechanics: mean velocity ~ T1/2 idea: conduction should cease as T->0 This idea motivated KamerlinghOnnes to investigate properties of metals at very low T Copyright A. J. Millis 2013 =>superconductivity!! Columbia University More history Classical mechanics: mean velocity ~ T1/2 idea: conduction should cease as T->0 This idea motivated KamerlinghOnnes to investigate properties of metals at very low T =>superconductivity!! Importance of theory (even if wrong or incomplete) in motivating experiment Copyright A. J. Millis 2013 Columbia University More history 1920s: Sommerfeld, Peierls, Bloch--quantum theory Fermi statistics=> non-zero electron velocity even at T=0 Neglect electron-electron interactions =>basic equation: � ∇2 i H=− + Vlattice (ri ) 2m i eigenfunctions: ψnk (r) = eik·r unk (r) modulated plane wave, extended throughout solid; propagates at nonzero group velocity=>theory of metallic conduction Copyright A. J. Millis 2013 Columbia University 1931: Enter A. H. Wilson The Master and Fellows of Trinity College Cambridge; taken from http://www.computerhistory.org/ semiconductor/timeline/1931The-Theory.html Note: first sharp statement metal and insulator distinct phases Copyright A. J. Millis 2013 Columbia University Key role of energy gap=> sharp distinction, metal vs insulator Mattheis, PRB5 290 (1972) � ∇2 i H=− + Vlattice (ri ) 2m i µ in bands: metal µ in gap: insulator In this theory, insulator possible only if even # electrons per cell Copyright A. J. Millis 2013 FeO, CoO and NiO: predicted to be metals Columbia University NiO is a very good insulator Discussion of the paper by de Boer and Verwey, reported by N. F. Mott with the help of some notes of R. Peierls 1937 Yamaka and Sawamoto PR 112 1861 1958 Peierls: Importance of electron-electron interactions in partially filled transition metal d-shell. Fundamental modification of usual ``band’’ picture. Need for real-space view of the physics. Copyright A. J. Millis 2013 Columbia University Electronic configuration of atoms complicated basic concept: ‘Hubbard U’ Number of electrons on ion nd configuration: label by nd, other (L,S) quantum numbers Charging energy U: U = E[d nd +1 U E[nd ] = nd (nd − 1) 2 ] + E[d nd −1 ] − 2E[d nd ] In transition metal oxides: Udd big because d wave function small (esp in ‘3d’ series) Copyright A. J. Millis 2013 Columbia University Consequence of ‘Charging energy’: Mott “blocking” effect Copyright A. J. Millis 2013 Columbia University Consequence of ‘Charging energy’: Mott “blocking” effect Copyright A. J. Millis 2013 Columbia University Consequence of ‘Charging energy’: Mott “blocking” effect Copyright A. J. Millis 2013 Columbia University Consequence of ‘Charging energy’: Mott “blocking” effect 2dn=>dn-1dn+1 E~U process suppressed Copyright A. J. Millis 2013 Columbia University Consequence of ‘Charging energy’: Mott “blocking” effect 2dn=>dn-1dn+1 E~U process suppressed Copyright A. J. Millis 2013 Columbia University Consequence of ‘Charging energy’: Mott “blocking” effect 2dn=>dn-1dn+1 E~U process suppressed Copyright A. J. Millis 2013 Columbia University Consequence of ‘Charging energy’: Mott “blocking” effect 2dn=>dn-1dn+1 E~U process suppressed Copyright A. J. Millis 2013 dndn-1=>dn-1dn process allowed Columbia University Consequence of ‘Charging energy’: Mott “blocking” effect 2dn=>dn-1dn+1 E~U process suppressed dndn-1=>dn-1dn process allowed If U large enough, only holes (or doubly occupied sites) can move=> if integer number of electrons per site: Mott insulator Copyright A. J. Millis 2013 Columbia University Something like this actually occurs LaTiO3 http://dmft.rutgers.edu/ LDA/lmto/lmto_run.htm Copyright A. J. Millis 2013 LaTiO3: •# electrons/unit cell is odd •material is insulating! •YTiO3 even more insulating Okimoto et al. PRB51 9581 (1995) Columbia University `Mott’ insulator: fundamental paradigm for oxides But be careful: in many cases ``Mott’’ is not the controlling physics Copyright A. J. Millis 2013 Columbia University Basic properties of transition metals and their oxides Copyright A. J. Millis 2013 Columbia University Transition metal ion: many accessible valence states *Partly filled d-shell =>spin and orbital degrees of freedom active *Multiple valence states=>many electronic configurations, many bonding modalities easily available *energies of different transition metal valences compatible with energies of different oxygen charge states =>tunability of materials properties Copyright A. J. Millis 2013 Columbia University Application: Catalysis (ex: photon-induced water splitting) sciencedirect.com spigse.chem.es.osaka-u.ac.jp Works, in essence, because of multiple d-valence: it is easy to transfer electrons back and forth between free oxygen and transition metal ions. Goal: manipulate band-gap to match solar spectrum Copyright A. J. Millis 2013 Columbia University Application: Respiration etc in biochemistry From the following article Versatility of biological non-heme Fe(II) centers in oxygen activation reactions Elena G Kovaleva & John D Lipscomb Nature Chemical Biology 4, 186 - 193 (2008) Works, in essence, because of multiple d-valence: it is easy to transfer electrons back and forth between free oxygen and Fe complex. Copyright A. J. Millis 2013 Columbia University Application: Batteries http://www.electronicslab.com/articles/ Li_Ion_reconstruct/ Works, in essence, because of multiple d-valence: it is easy to transfer electrons into and out of CoO2 complex Copyright A. J. Millis 2013 Columbia University Application: ``Memristor’’ Nature 453, 80-83 (2008) Electrical observations of filamentary conductions for the resistive memory switching in NiO films D. C. Kim, S. Seo, S. E. Ahn, D.-S. Suh, M. J. Lee et al. Appl. Phys. Lett. 88, 202102 (2006) In oxides works, in essence, because of multiple d-valence: it is easy to transfer electrons into and out of NiO complex Copyright A. J. Millis 2013 Columbia University Many structures possible Monoxide (e.g NiO): rocksalt structure http://www.webelements.com/ compounds/nickel/ nickel_oxide.html Copyright A. J. Millis 2013 Columbia University Many structures possible ABO3 Perovskite (e.g LaNiO3): A and B sites: 2 interpenetrating cubic lattices A-site. Typically electrically inert B-site: in our case, transition metal dont forget oxygen! Fundamental motif: BO6 octahedron Copyright A. J. Millis 2013 Columbia University Many structures possible A2BO4 Perovskite (e.g La2CuO4): Layered structure Octahedra as in perovskite but now organized two dimensionally, with weak interplane coupling Copyright A. J. Millis 2013 Columbia University Many structures possible Ruddlesden-Popper series An+1BnO3n+1 (e.g Sr2RuO4->Sr3Ru2O7->Sr4Ru3O10->SrRuO3) Interpolates between 2 and 3 dimensional coordination Copyright A. J. Millis 2013 Columbia University Many structures possible Double perovskite AA’BB’O6 Sr2FeMoO6 Copyright A. J. Millis 2013 Columbia University Many structures possible Other structures: spinel (2 inequivalent sites: one rocksalt and one tetrahedrally bonded_ tf.uni-kiel.de Copyright A. J. Millis 2013 Columbia University Many structures possible Corundum structure: V2O3; hematite.... Here, only transition metal ions are shown http://www.irm.umn.edu/hg2m/hg2m_b/hg2m_b.html Copyright A. J. Millis 2013 Columbia University Many structures possible Many other structures: for example quasi one dimensional arrays of transition metal ions (e.g. CuGeO3 below), Basic point: multiple configurations of transition metal=>multiple structures possible. Copyright A. J. Millis 2013 Columbia University New development: artificially constructed superlattices LaTiO3/SrTiO3 LaMnO3/SrTiO3 (a): La (b) Ti (c) Mn (d) composite A. Ohtomo, D. A. Muller, J. L. Grazul and H. Hwang, Nature 419 378 (2002) Copyright A. J. Millis 2013 D. Muller Nat. Mat. 9 263 (2009) Columbia University New window onto basic questions Photoemission (many-body density of states--here symmetrized) for n layers of SrVO3 (paramagnetic metal) embedded in SrTiO3 (insulator) As SrVO3 becomes thinner, gap opens Copyright A. J. Millis 2013 Columbia University Strain control of metal-insulator transition in LaNiO3 Son et al Appl. Phys. Lett. 96 062114 (2010) LAO: 1.3% compressive strain LSAT: 0.8% tensile strain DSO: 2.5% tensile strain Critical thickness for metalinsulator transition depends on magnitude and sign of strain Copyright A. J. Millis 2013 Columbia University More exotic: ``design in new properties’’ e.g. Chaloupka/Khalliulin: ?New high-Tc superconductor? Idea: Bulk LaNiO3 Ni [d]7 (1 electron in two degenerate eg bands). Phys. Rev. Lett. 100 016404 (2008) Copyright A. J. Millis 2013 In correctly chosen structure, split eg bands, get 1 electron in 1 band--”like” copperoxide high-Tc Columbia University Structure =>interesting behavior Spins on geometrically frustrated lattices Copyright A. J. Millis 2013 Columbia University Structure =>interesting behavior Anisotropic Transport Copyright A. J. Millis 2013 Columbia University Structure =>interesting behavior Sr2RuO4: p-wave superconductor Sr3Ru2O7: almost ferromagnetic (100x susceptibility enhancement). SrRuO3: Ferromagnetic (Tc ~150K). Power-law conductivity. CaRuO3: no fm, but power law Copyright A. J. Millis 2013 Columbia University Important property of transition oxides: partially filled d-shells Hund’s first rule (maximize total spin) =>magnetism Copyright A. J. Millis 2013 Columbia University Magnetism and full spin polarization at temperatures above room T Nature 395, 677-680 (15 October 1998) Copyright A. J. Millis 2013 Columbia University Hunds second rule: maximize orbital angular momentum In solid state context: occupy a subset of d-orbitals <=> ``orbital order’’=>anisotropic transport Ex: Manganese perovskites band filling x controls orbital ordering=>conductivity Copyright A. J. Millis 2013 Nagaosa/Tokura Science 288 462 Columbia University These effects can be induced by strain Ex: CMR films-substrate-induced strain=>(putative) orbital ordering=> conductivity. Mechanism: ‘orbital ordering’ triggered by strain Konishi et al , J. Phys Soc. Jpn 68 3790 Copyright A. J. Millis 2013 Columbia University Proximity (in energy) of several spin and charge configurations=> interesting and potentially useful transport properties Copyright A. J. Millis 2013 Columbia University Thermoelectric effects Lots of waste heat in the world: Thermal conductivity ∆V S= ∆T A.Maignan, APs tutorial 2010 Copyright A. J. Millis 2013 =>from temperature difference, can get voltage=>current =>recapture some energy Columbia University Thermoelectric figure of merit A.Maignan, APs tutorial 2010 Insulators Semicond. Semimetals Metals S T ZT = ρ (κel + κlattice ) 2 Want: high thermal conductivity, low electrical resistance, low thermal resistance Carrier density (simple band picture) Copyright A. J. Millis 2013 Columbia University (Over)simplification of physics F = Energy − T × Entropy Temperature gradient drives carriers by coupling to entropy Insulators Semicond. Semimetals Metals Insulator: no carriers Metal: entropy per carrier is very small Carrier density (simple band picture) Transition metal oxide: partially filled d-shell=>high density of nearly localized carriers, high spin=>high entropy/carrier Copyright A. J. Millis 2013 Columbia University A.Maignan, APs tutorial 2010 Copyright A. J. Millis 2013 Columbia University More extreme transport anomaly: ``Mott’’ transition V2O3--and other oxides--can be switched from metallic to insulating behavior by modest changes in temperature and pressure. Note! Transitions are first order McWhan et al,PRL 27 941 (1971) Copyright A. J. Millis 2013 Columbia University Device Application: bolometer VO2: thermally driven metal-insulator transition Tune device to critical temperature. Small amount of absorbed heat=>large change in resistance Wu et al, Nanoletters 6 2313 (2006) Copyright A. J. Millis 2013 Columbia University VO2 proposed for actual use Copyright A. J. Millis 2013 Columbia University Hysteresis is a problem hard to ‘reset’ after initial temperature pulse Gurvitch et al http://www.ee.sunysb.edu/~serge/234.pdf Copyright A. J. Millis 2013 Columbia University Partially filled d-shell: ``emergent’’ electronic properties Copyright A. J. Millis 2013 Columbia University Emergent electronic properties ``Colossal’’ Magnetoresistance Copyright A. J. Millis 2013 p-wave superconductivity (and many other phases) Columbia University Colossal Magnetoresistance: Phase competition High T phase: ``insulating’’ (resistivity large and increasing as T is decreased) Low T phase metallic and ferromagnetic Transition appears more or less continuous, and for many years was thought to be second order. BUT...... Copyright A. J. Millis 2013 Columbia University Manganese perovskites Average high-T structure cubic perovskite Many low-T phases ``charge/orbital order’’ (2d slice shown). Note 4 unit cell period Copyright A. J. Millis 2013 Columbia University Transition is first order High T phase has period 4 ordering Adams et al PRL 85 2553 and 3954 2000 Copyright A. J. Millis 2013 Columbia University Transition is first order Low T phase: ferromagnetic. Well defined spin stiffness T phase has period 4 ordering Copyright A. J. Millis 2013 Columbia University Transition is first order Spin stiffness jumps discontinuously as does 1/4,0,0 intensity Copyright A. J. Millis 2013 Morals: --Unusual high T behavior <=>short ranged order --First order transitions (may be hard to see) Columbia University Emergent electronic properties High Tc Superconductivity: in copper oxide and iron arsenide superconductors SCIENCE VOL 329 13 AUGUST 2010 825 J.Zhao, et.al, Nature Mater. 7, 953(2008) Copyright A. J. Millis 2013 Columbia University Copper-oxide high Tc: again competing density-wave phases Wu et al Nature 477 7363 2011 Open question: how much of the physics of oxide superconductivity arises from competing phases Copyright A. J. Millis 2013 Columbia University summary: profusion of emergent electronic phases Manganite Ruthenate FeAs Cuprate Copyright A. J. Millis 2013 Columbia University Key Features of Transition Metal Oxides •Multiple d configurations (both valence and spin/orbital configuration at fixed valence) •``Easy’’ charge exchange with other ions (esp O) •Multiple bonding modalities <=> many possible structures •Unusual transport: high carrier density but low coherence scales •Multiple electronic phases (some, unexpected) All of these properties stem from electron-electron interactions in the partly filled transition metal d-shell The question: relate crystal structure, chemistry to material properties Copyright A. J. Millis 2013 Columbia University Periodic Table to Properties: Stereotypical Theorist’s View Copyright A. J. Millis 2013 Columbia University Periodic Table to Properties: Stereotypical Theorist’s View PeriodicTable Periodic table from J H Wood; quoted in Z Fisk 2010 KITP talk Copyright A. J. Millis 2013 Columbia University Periodic Table to Properties: Stereotypical Theorist’s View PeriodicTable Ignore details: write Quantum Field Theory => κ µνλ � Aµ ∂ν Aλ + ... 2 Periodic table from J H Wood; quoted in Z Fisk 2010 KITP talk Copyright A. J. Millis 2013 Columbia University Periodic Table to Properties: Stereotypical Theorist’s View PeriodicTable Ignore details: write Quantum Field Theory => κ µνλ � Aµ ∂ν Aλ + ... 2 These lectures--where we are on attempts to do better: Periodic table from J H Wood; quoted in Z Fisk 2010 KITP talk Copyright A. J. Millis 2013 Columbia University Periodic Table to Properties: Stereotypical Theorist’s View PeriodicTable Periodic Table of the Elements GROUP 1 IA 1 !"#$%&'()$*+, 12$*#3 2 1^gX 2.2 Hydrogen 0.0899 -259.14 =:?'37 13.5984 -252.87 - 2 IIA ^A^ `1[7^ 3 Li Period 2 1^gX 0.82 Potassium 13 IIIA 5 Gas Mg 1 1_ 1.31 1 1_ 1.00 Calcium Liquid !*A#3)"+'Q+,# !"#$%&'G8AA'R5%" !:#/86,#'I#5A"85" J8A+'#L'(8"),83'9#/8,%"0$A J#3"E$855'&#5A"85" <3+&",#5'G8AA Noble Gas Alkaline Earth Metals Halogens Transition Metals Non Metals Poor Metals 3 IIIB 21 Metalloids 4 IVB 44.955910 Sc 2 @bgX 1.36 Scandium 22 5 VB 47.867 Ti 23 3 UX 1.54 Titanium m) e k m+ $+c X ,_ +F e U D 2 S hc X <3+&",#5'T86%)A'=I38AA%&83? <3+&",#5'F#3" <3+$+5",2'I08,/+ U8,8682'I#5A"85" L%5+7A",)&"),+'&#5A"85" U%,A"'T86%8"%#5'I#5A"85" Rare Earth Metals BWXC 1#),&+O'K02A%&AP5%A"P/#: Common Constants Solid Synthetic Alkali Metals Magnesium Ca † Categories 2 1^gX 0.82 Rubidium Sr 1 1_ 0.95 Strontium Y 2 D3/2 1.22 Yttrium 1.532 2.63 4.472 4.1771 5.6949 6.2173 39.31 688 777 1382 1526 3345 =$?'248 BCC =$?'215 FCC =$?'180 HCP Bh,C'aA ^ Bh,C'aA X Bh,C'W6 ^'aAX `1 `2 `3 132.90545 56 137.327 55 2 1^gX 0.79 Cesium Ba 1 1_ 0.89 Barium 1.879 3.51 3.8939 5.2117 28.44 671 727 1870 =$?'265 BCC =$?'222 BCC Bi+C'eA ^ Bi+C'eA X `1 `2 (223) 88 (226) 87 Fr 7 Phase at STP 1_ 1.57 Beryllium 6 VIB 50.9415 V 4 UbgX 1.63 Vanadium 24 7 1b 1.66 Chromium 25 4,8:%"8"%#5'I#5A"85" G#38,'48A'I#5A"85" G#38,'F#3)$+'=D6+83'48A? >D >385&S'I#5A"85" >,#"#57<3+&",#5'G8AA'T8"%# T26*+,/'I#5A"85" 2.8179403x10-15 m 1.602176x10-19 J 1.602176x10-19 C 96 485.3399 C/mol 0.0072973525 3.7417749x10-16 W m2 1+&#56'T86%8"%#5'I#5A"85" 1K++6'#L'9%/0"'%5'8'F8&))$ 1K++6'#L'A#)56'%5'8%,'8"'1V> 1"8568,6'>,+AA),+ 8 VIII 54.938049 Mn 6 1agX 1.55 Manganese G R -273.15 °C 1.660539x10-27 kg 23 -1 6.022142x10 mol 2.718281828 1.380650x10-23 J/K 9.10938215x10-31 kg 0.5110 MeV 7 VIIB 51.9961 Cr 9 VIII 26 55.845 Fe 5 Iron @W 1.83 27 -11 p h m +gm K R R c R hc ch/k c 4 UfgX 1.88 Cobalt 28 -1 -2 11 IB 58.6934 Ni 3 6.67428x10 m kg s 8.314472 J mol-1 K -1 3 0.02241410 m /mol 3.14159265358979 6.626069x10-34 J s 1836.15267247 -1 10 973 732 m 15 3.289842x10 Hz 13.6057 eV 0.01438769 m K 299 792 458 m/s 343.2 m/s 101 325 Pa 10 VIII 58.933200 Co 2 1^gX 0.7 Francium - 4.0727 BT5C'cA ^ `1 Ra 985"085%6+'1+,%+A 3 UW 1.91 Nickel 63.546 Cu 2 1^gX 1.90 Copper 10.811 B 2 >H^gX 2.04 Boron 2.46 8.2980 2075 4000 =:?'82 rhom. B\+C'XA X'XK^ `3 26.981538 13 Al 2 >H^gX 1.61 Aluminum 2.7 5.9858 660.32 2519 =$?'143 FCC B(+C'bA X'bK^ `3 65.409 31 69.723 YWXZ 12 IIB 29 14 IVA 30 Zn 1 Zinc 1_ 1.65 Ga 2 >H^gX 1.81 Gallium 1_ !&"%5%6+ 1+,%+A Notes: 7'@+5A%"2')5%"A'8,+'/g&$ b'L#,'A#3%6A'856'/g9'#,'S/g&$ b'8"' _H'I+3A%)A'L#,'/8A+A 7'!"#$%&'.+%/0"'*8A+6'#5' ^XI 7'='?'%56%&8"+'$8AA'5)$*+,'#L'$#A"'A"8*3+'%A#"#K+ 7'I#$$#5'MN%68"%#5'1"8"+A'%5'*#36 7'<3+&",#5'I#5L%/P'*8A+6'#5'DR>!I'/)%6+3%5+A 7'j'%56%&8"+A'&,2A"83'A",)&"),+'%A')5)A)83'#,'$82',+k)%,+' +NK3858"%#5 7'=$?'G+"833%&',86%)A['=:?'I#:83+5"',86%)A References: -(%A"P/#:[';.#3L,8$P&#$'=G8"0+$8"%&?[ ITI'\856*##S'#L'I0+$%A",2'856'>02A%&A ]^A"'<6%"%#5['X___7X__^['856'#"0+,A >+,%#6%&'V8*3+'#L'"0+'<3+$+5"A @+A%/5'*2'F+,"+NWXP&#$ l'X_^^'F+,"+NWX'99IP'!33',%/0"A',+A+,:+6P 3 F2 1.33 Zirconium Nb 6 D1/2 1.60 Niobium Mo 7 S3 2.16 Molybdenum Tc 6 S5/2 1.9 Technetium Ru 5 F5 2.20 Ruthenium Rh 4 F9/2 2.28 Rhodium Pd 1 S0 2.20 Palladium Ag 2 S1/2 1.93 Silver Cd 1 S0 1.69 Cadmium In 2 P°1/2 1.78 Indium 6.511 8.57 10.28 11.5 12.37 12.45 12.023 10.49 8.65 7.31 6.6339 6.7589 7.0924 7.28 7.3605 7.4589 8.3369 7.5762 8.9938 5.7864 1855 4409 2477 4744 2623 4639 2157 4265 2334 4150 1964 3695 1554.9 2963 961.78 2162 321.07 767 156.6 2072 =$?'160 HCP =$?'146 BCC =$?'139 BCC =$?'136 HCP =$?'134 HCP =$?'134 FCC =$?'137 FCC =$?'144 FCC =$?'151 §hex =$?'167 §tetra. Bh,C'W6 X'aAX Bh,C'W6 W'aA^ Bh,C'W6 a'aA^ Bh,C'W6 a'aAX Bh,C'W6 c'aA^ Bh,C'W6 ]'aA^ Bh,C'W6 ^_ Bh,C'W6 ^_'aA^ Bh,C'W6 ^_'aAX Bh,C'W6 ^_'aAX'aK^ +4 `3[a `X[b[W[a[6 `W[7 `X[b[4[e[] `X[3[W `2[W `1 `2 `3 178.49 73 180.9479 74 183.84 75 186.207 76 190.23 77 192.217 78 195.078 79 196.96655 80 200.59 81 204.3833 72 Hf 3 UX 1.3 Hafnium Ta 4 UbgX 1.5 Tantalum W 5 @_ 2.36 Tungsten Re 6 1agX 1.9 Rhenium Os Ir 5 @W 2.2 Osmium 4 UfgX 2.2 Iridium Pt 3 @b 2.28 Platinum Au 2 1^gX Gold 2.54 Hg 1 1_ 2 Mercury Tl 2 >H^gX 1.62 Thallium 13.31 16.65 19.25 21.02 22.61 22.65 21.09 19.3 13.534 10.4375 11.85 6.8251 7.5496 7.8640 7.8335 8.4382 8.9670 8.9588 9.2255 6.1082 2233 4603 3017 5458 3422 5555 3186 5596 3033 5012 2466 4428 1768.3 3825 1064.18 2856 -38.83 356.73 304 1473 =$?'159 HCP =$?'146 BCC =$?'139 BCC =$?'137 HCP =$?'135 HCP =$?'136 FCC =$?'139 FCC =$?'144 FCC =$?'151 §rhom. =$?'170 HCP Bi+C'WL ^W'a6X'eAX Bi+C'WL ^W'a6b'eAX Bi+C'WL ^W'a6W'eAX Bi+C'WL ^W'a6a'eAX Bi+C'WL ^W'a6e'eAX Bi+C'WL ^W'a6c'eAX Bi+C'WL ^W'a6f'eA^ Bi+C'WL ^W'a6^_'eA^ Bi+C'WL ^W'a6^_'eAX B\/C'eK^ +4 `5 `X[b[W[a[6 `X[W[e[7[7^ `X[b[4[e[] `X[b[4[e `X[4 `^[3 `^[2 `1[b (261) 105 (262) 106 (266) 107 (264) 108 (277) 109 (268) 110 (281) 111 (272) 112 (285) 113 104 Rf 1 0.9 Radium 5 5.2784 700 1737 BCC BT5C'cA X `2 Zr 3 UX'd Rutherfordium Db Dubnium Sg Seaborgium Bh Bohrium Hs Hassium Mt Meitnerium 4.002602 He 1 1_ - Helium Free Downloads at Vertex42.com 0.856 1.55 2.985 4.507 6.11 7.14 7.47 7.874 8.9 8.908 8.92 7.14 5.904 4.3407 6.1132 6.5615 6.8281 6.7462 6.7665 7.4340 7.9024 7.8810 7.6398 7.7264 9.3942 5.9993 63.38 759 842 1484 1541 2830 1668 3287 1910 3407 1907 2671 1246 2061 1538 2861 1495 2927 1455 2913 1084.62 2927 419.53 907 29.76 2204 =$?'227 BCC =$?'197 FCC =$?'162 HCP =$?'147 HCP =$?'134 BCC =$?'128 BCC =$?'127 §cubic =$?'126 BCC =$?'125 HCP =$?'124 FCC =$?'128 FCC =$?'134 §hex =$?'135 §BCO B!,C'WA ^ B!,C'WA X B!,C'b6 ^'WAX B!,C'b6 X'WAX B!,C'b6 b'WAX B!,C'b6 a'WA^ B!,C'b6 a'WAX B!,C'b6 e'WAX B!,C'b6 c'WAX B!,C'b6 ]'WAX B!,C'b6 ^_'WA^ B!,C'b6 ^_'WAX B!,C'b6 ^_'WAX'WK^ `1 `2 `3 `X[b[4 `X[3[W[5 `X[3[e `2[b[W[e[c `X[3 `2[b `X[3 `^[2 `2 `3 85.4678 38 87.62 39 88.90585 40 91.224 41 92.90638 42 95.94 43 (98) 44 101.07 45 102.90550 46 106.42 47 107.8682 48 112.411 49 114.818 37 Cs 6 Be 1 0.968 1.738 5.1391 7.6462 97.72 883 650 1090 =$?'186 BCC =$?'160 HCP B(+C'bA ^ B(+C'bA X `1 `2 39.0983 20 40.078 19 Rb 5 1^gX Sodium K 4 2 0.93 18 VIIIA 2 1.00794 -!"#$%&'.+%/0" 2 1^gX -4,#)5671"8"+'9+:+3 2.2 ;<3+&",#5+/8"%:%"2'=>8)3%5/? H 9.012182 0.535 1.848 5.3917 9.3227 180.54 1342 1287 2470 =$?'152 BCC =$?'112 HCP B\+C'XA ^ B\+C'XA X `1 `2 22.989770 12 24.3050 11 Na 3 1^gX 0.98 Lithium 4 Ds Rg Darmstadtium Roentgenium Cn Copernicium Uut Ununtrium 6 15 VA 12.0107 C 3 >_ 2.55 Carbon 2.26 11.2603 3550 4027 =:?'77 hex B\+C'XA X'XKX `X[4[7W 28.0855 14 Si 7 14.0067 N 3 >_ 2.01 Germanium 5.323 7.8994 938.3 2820 =:?'122 §cubic B!,C'b6 ^_'WAX'WKX `X[4 118.710 50 Sn 3 P0 1.96 Tin 7.31 7.3439 231.93 2602 =:?'141 §tetra. Bh,C'W6 ^_'aAX'aKX `X[4 207.2 82 Pb 3 >_ Lead 2.33 1HbgX 3.04 Nitrogen P >_ Ge 4 1.251 14.5341 -210.1 -195.79 =:?'75 B\+C'XA X'XKb `X[3[W[a[7X[73 30.97361 15 3 1.90 Silicon 2.33 8.1517 1414 2900 =:?'111 cubic B(+C'bA X'bKX `X[4[7W 72.64 32 16 VIA 4 1HbgX 2.18 Arsenic 4 S°3/2 2.05 Antimony 6.697 8.6084 630.63 1587 =:?'138 §rhom. Bh,C'W6 ^_'aAX'aKb `3[a[73 208.98038 83 Bi 4 1HbgX 2.02 Bismuth S 3 >X 2.58 Sulfur 1.96 10.3600 115.21 444.72 =:?'102 FCO B(+C'bA X'bKW `X[W[6[7X 78.96 34 Se 3 >X 2.55 Selenium 4.819 9.7524 221 685 =:?'116 §hex B!,C'b6 ^_'WAX'WKW `X[4[e[7X 127.60 52 Te >HbgX 3.98 Fluorine 10 20.1797 Ne 1 1_ - Neon 1.696 0.9 17.4228 21.5645 -219.6 -188.12 -248.59 -246.08 =:?'71 =:?'69 B\+C'XA X'XKa B\+C'XA X'XKe 71 _ 35.453 18 39.948 17 Cl 2 >HbgX 3.16 Chlorine 3.214 12.9676 -101.5 -34.04 =:?'99 B(+C'bA X'bKa `1[b[a[c[71 79.904 35 Br 2 >HbgX 2.96 Bromine Ar 1 1_ - Argon 1.784 15.7596 -189.3 -185.8 =:?'97 B(+C'bA X'bKe _ 83.798 36 Kr I 3 P2 2.10 Po 3 >X 2.0 Polonium Ununquadium Ununpentium Ununhexium Uuh 1 1_ 3 Krypton 2 P°3/2 2.66 Iodine Xe 1 S0 2.60 Xenon At 2 >HbgX 2.2 Astatine 302 B\/C'eKa `1[b[a[c[71 117 Rn 1 1_ - Radon 9.73 10.7485 -71 -61.7 =:?'145 B\/C'eKe _ 118 Uus Ununseptium Uuo Ununoctium 6.0 ? 57 138.9055 La 2 @bgX 1.10 Lanthanum 58 140.116 Ce 1 G°4 1.12 Cerium 59 Pr 140.90765 4 I°9/2 1.13 60 144.24 Nd 5 I4 1.14 Praseodymium Neodymium 61 Pm (145) 6 H°5/2 - Promethium 62 150.36 Sm 7 F0 1.17 Samarium 63 151.964 Eu 8 S°7/2 - Europium 64 157.25 Gd 9 D°2 1.20 Gadolinium 65 158.92534 Tb 6 H°15/2 - Terbium 66 Dy 162.500 5 I8 1.22 Dysprosium 67 164.93032 Ho 4 I°15/2 1.23 Holmium 68 167.259 Er 3 H6 1.24 Erbium 69 168.93421 Tm 2 F°7/2 1.25 Thulium 70 173.04 Yb 1 S0 - Ytterbium 71 174.967 Lu 2 @bgX 1.27 Lutetium 7.353 5.244 7.901 8.219 8.551 8.795 9.066 9.321 6.57 9.841 6.146 6.689 6.64 7.01 7.264 5.582 5.6437 5.6704 6.1498 5.8638 5.9389 6.0215 6.1077 6.1843 6.2542 5.4259 5.5769 5.5387 5.473 5.5250 920 3464 798 3360 931 3290 1021 3100 1100 3000 1072 1803 822 1527 1313 3250 1356 3230 1412 2567 1474 2700 1497 2868 1545 1950 819 1196 1663 3402 =$?'187 §hex =$?'182 FCC =$?'182 §hex =$?'181 §hex =$?'183 HCP =$?'180 §hex =$?'180 BCC =$?'180 HCP =$?'177 HCP =$?'178 HCP =$?'176 HCP =$?'176 HCP =$?'176 HCP =$?'176 FCC =$?'174 HCP Bi+C'a6 ^'eAX Bi+C'WL ^'a6 ^'eAX Bi+C'WL b'eAX Bi+C'WL W'eAX Bi+C'WL a'eAX Bi+C'WL e'eAX Bi+C'WL c'eAX Bi+C'WL c'a6 ^'eAX Bi+C'WL f'eAX Bi+C'WL ^_'eAX Bi+C'WL ^^'eAX Bi+C'WL ^X'eAX Bi+C'WL ^b'eAX Bi+C'WL ^W'eAX Bi+C'WL ^W'a6 ^'eAX +3 +3[W +3[W +3 +3 `X[3 `X[3 +3 +3[W +3 +3 +3 `X[3 `X[3 +3 (227) 90 232.0381 91 231.0359 92 238.0289 93 (237) 94 (244) 95 (243) 96 (247) 97 (247) 98 (251) 99 (252) 100 (257) 101 (258) 102 (259) 103 (262) 89 Ac 2 @bgX 1.1 Actinium 10.07 5.17 1050 3200 FCC BT5C'e6 ^'cAX +3 Th 3 UX 1.3 Thorium 11.724 6.3067 1750 4820 =$?'179 FCC BT5C'e6 X'cAX +4 Pa 4 h^^gX 1.5 Protactinium 15.37 5.89 1572 4000 =$?'163 §tetra BT5C'aL X'e6 ^'cAX `W[5 U 5 L°6 1.38 Uranium 19.05 6.1941 1135 3927 =$?'156 BCP BT5C'aL b'e6 ^'cAX `b[W[a[6 Np 6 L11/2 1.36 Neptunium 20.45 6.2657 644 4000 =$?'155 SO BT5C'aL W'e6 ^'cAX `b[W[5[e Pu 7 F0 1.28 Plutonium 19.816 6.0260 640 3230 =$?'159 §mono. BT5C'aL e'cAX `b[4[a[e Am 8 S°7/2 1.3 Americium 5.9738 1176 2011 =$?'173 HCP BT5C'aL c'cAX +3[W[a[e Cm 9 D°2 1.3 Curium 13.51 5.9914 1345 3110 =$?'174 HCP BT5C'aL c'e6 'cAX +3 Bk 6 H°15/2 1.3 Berkelium 14.78 6.1979 1050 =$?'170 hex BT5C'aL f'cAX +3[W Cf 5 I8 1.3 Californium 15.1 6.2817 900 hex BT5C'aL ^_'cAX +3 Es 4 I°15/2 1.3 Einsteinium 6.42 860 BT5C'aL ^^'cAX +3 Fm 3 H6 1.3 Fermium 6.50 1527 BT5C'aL ^X'cAX +3 Md 2 F°7/2 1.3 Mendelevium 6.58 827 BT5C'aL ^b'cAX `X[3 Richer Description of Properties 3.12 3.75 11.8138 13.9996 -7.3 59 -157.36 -153.22 =:?'114 BCO =:?'110 B!,C'b6 ^_'WAX'WKa B!,C'b6 ^_'WAX'WKe `1[a[71 _ 126.90447 54 131.293 53 Tellurium 9.196 8.414 254 962 §cubic B\/C'eKW `X[4 (292) 116 Uup 2 6.24 4.94 5.9 9.0096 10.4513 12.1298 449.51 988 113.7 184.3 -111.8 -108 =:?'135 hex =:?'133 BCO =:?'130 Bh,C'W6 ^_'aAX'aKW Bh,C'W6 ^_'aAX'aKa Bh,C'W6 ^_'aAX'aKe `X[4[e[7X `1[a[c[71 _ (209) 85 (210) 86 (222) 84 11.34 9.78 7.4167 7.2855 327.46 1749 271.3 1564 =$?'175 FCC =:?'146 §rhom. B\/C'eKX B\/C'eKb `2[W `3[a (289) 115 114 Uuq F >X 24.5874 -268.93 ^AX _ 18.9984032 3.44 Oxygen 1HbgX 5.727 9.7886 817 614 =:?'119 rhom. B!,C'b6 ^_'WAX'WKb `3[a[73 121.760 51 Sb O 9 3 1.429 13.6181 -218.3 -182.9 =:?'73 B\+C'XA X'XKW 72 32.065 16 2.19 1.823 10.4867 44.2 280.5 =:?'106 § B(+C'bA X'bKb `b[W[5[7b 74.92160 33 17 VIIA 15.9994 4 Phosphorus As 8 0.1785 =:?'32 BT5C'aL ^W'e6X'cAX'd +4 Lanthanides 2 6.941 2 1 (8$+ Hydrogen ;@+5A%"2'B(#"+C 0.0899 13.5984 -D#5%E8"%#5'<5+,/2'=+F? ;G+3"%5/'>#%5"'=HI? -259.14 -252.87 ;J#%3%5/'>#%5"'=HI? FCC I,2A"83'1",)&"),+'B(#"+C !"#$%&',86%)A'=K$?B(#"+C =:?'37 ^A^ <3+&",#5'I#5L%/),8"%#5 `^[7^ >#AA%*3+'MN%68"%#5'1"8"+A'B(#"+C Actinides 1 1.00794 H No 1 S0 1.3 Nobelium 6.65 827 BT5C'aL ^W'cAX `X[3 Lr 2 P°1/2 ? - Lawrencium 4.9 ? 1627 BT5C'aL ^W'cAX'cK'd +3 Understand and control what situations give which properties These lectures--where we are on attempts to do better: Periodic table from J H Wood; quoted in Z Fisk 2010 KITP talk Copyright A. J. Millis 2013 Columbia University Basic chemistry and physics •Crystal type and nominal valence •Crystal structure and level ordering •Energetics •Interactions •Charge transfer •Hybridization •Classification and Summary Copyright A. J. Millis 2013 Columbia University Crystal type and nominal valence Basic idea --Oxygen: very electronegative. In vacuum: 1s22s22p4 In solid: oxygen ``wants`` to fill up p-shell (O2-: 1s22s22p6) --Transition metal: less electronegative In vacuum: [Ar]dn4s2 In solid: ``wants`` to lose 4s electrons, change # d =>[Ar]dn+m By controlling number of oxygen per transition metal, and number and electronegativity of other elements, can control filling of d-shell Copyright A. J. Millis 2013 Columbia University Crystal type and nominal valence Monoxide: rocksalt structure Simple picture: removal energy of Ni 4s low; electron affinity of O 2p high => Ni: [Ar]3d8 O: [He]2s22p6 http://www.webelements.com/ compounds/nickel/ nickel_oxide.html Complication: Ni-O hybridization Ni: [Ar]3d8+x O: [He]2s22p6-x ??how big is x?? Copyright A. J. Millis 2013 Columbia University Crystal type and nominal valence ABO3 perovskite, cubic phase A-site. Typically electrically inert; choice of A ion controls valence of B site B-site: in our case, transition metal with partly filled d-shell dont forget oxygen! http://en.wikipedia.org/wiki/File:Perovskite.jpg Copyright A. J. Millis 2013 Columbia University Crystal type and nominal valence ABO3: Presence of A-site ion stabilizes different valence Simple picture: removal energies of La 5d, 6s V 4s, 3d low; electron affinity of O2p high =>LaVO3 La3+ [Xe] V3+: [Ar]3d2 O2-: [He]2s22p6 Complication: V-O hybridization V: [Ar]3d2+3x Copyright A. J. Millis 2013 ??how big is x?? O: [He]2s22p6-x Columbia University Crystal type and nominal valence Vary A-site ion: change valence Simple picture: removal energies of La 5d, 6s V 4s, 3d low; electron affinity of Simple picture: removal energies O2p high of La 5d, 6s V 4s, 3d low; =>LaVO3 electron affinity of O2p high La3+ [Xe] V3+: [Ar]3d2 O2-: [He]2s22p6 =>SrVO3 Complication: V-O hybridization V4+: [Ar]3d1+3x O2-: [He]2s22p6-x V: [Ar]3d2+3x Copyright A. J. Millis 2013 ??how big is x?? O: [He]2s22p6-x Columbia University Crystal structure and level ordering Basic idea --d-levels degenerate in free space. --Solid state: local environment breaks the symmetry By controlling the local (point) symmetry of the transition metal ion, can control which orbitals are occupied. Copyright A. J. Millis 2013 Columbia University Symmetry breaking: Group Theory Simplest example: nearly cubic environment Free space (no spin orb) Cubic O(3) Oh group: representation L=2 eg t2g x2-y2; 3z2-r2 xy; xz; yz picture http://winter.group.shef.ac.uk/ orbitron/AOs/3d/index.html Copyright A. J. Millis 2013 Columbia University Electrostatic contribution to crystal field splitting small Simple estimate: point charge model: O charge -2 at distance RO~2A; ``size’’ of d orbital Rd~0.5A -2 -2 V(�r) = i=1...6 -2 4e2 � i| |�r − R Level splitting: expand for small r. First deviation from spherical symmetry is quadrupole term -2 Vquad Copyright A. J. Millis 2013 � 4e2 ∼ RO � Rd RO �4 ∼ 0.1eV Columbia University Dominant contribution: hybridization to ligand (oxygen) tpd + - + dx2 −y2 - + pσ εd εp p-d anti bonding p-d bonding In almost all transition metal oxides, the near-fermi surface states are p-d ANTIBONDING states. Question: how much d and how much p character Copyright A. J. Millis 2013 Columbia University d-p overlap stronger for eg than t2g - + in solid (cubic symm) pσ dxy Copyright A. J. Millis 2013 free ion eg − pσ antibonding t2g − pπ antibonding t2g − pπ bonding eg − pσ bonding - - + - dx2 −y2 + - - + + + pπ Columbia University Lower than cubic symmetry Rondinelli and Spaldin, Adv. Mater. 23 3363 (2011) (Recall! what is depicted are the p-d antibonding bands) Copyright A. J. Millis 2013 Columbia University Jahn-Teller (cubic-tetragonal) distortion Define distortions Copyright A. J. Millis 2013 Columbia University Consequence of structural distortion: change of hybridization Jahn-Teller type: change Tm-O bond length Change transition metaloxygen distance: hybridization changes. =>shifts bondingantibonding splitting Copyright A. J. Millis 2013 Columbia University Alternative: GdFeO3 distortion Rotate octahedra about two axes Induced by choice of A-site ion. If dAA<2dBO then B-O-B bond is under compressive strain. B-O bond relatively rigid =>B-O-B bond buckles. Angle can be as small as 140o Change in bandwidth: 30% Copyright A. J. Millis 2013 Columbia University Consequence of structural distortion: change of hybridization dxy - + - + pπ + + - + - tpd - GdFeO3 type dxy Move oxygen out of alignment: overlap decreases Copyright A. J. Millis 2013 Columbia University How big are these effects? Cubic perovskite structure: eg-t2g splitting ~2eV Copyright A. J. Millis 2013 Columbia University Cartoon p O p θ Tm 1 tpd → tpd cos θ Copyright A. J. Millis 2013 Tm 2 Bandwidth ∼ cos2 θ Columbia University Density of states of t2g antibonding band as function of amplitude of GdFeO3 distortion: ``LaVO3’’ (H. T. Dang) Bandwidth varies from ~2.5eV to ~1.6eV Copyright A. J. Millis 2013 Columbia University Jahn-Teller (cubic-tetragonal) distortion Analyse band structure in distorted case λ : 2 − 3eV/Å Copyright A. J. Millis 2013 Ederer and AJM, PRB 76 155105 (2007) Popovic and Satpathy, PRL 84 1603 (2000) Yin et al PRL 96 116405 (2006) Columbia University GdFeO3 rotation (trigonal) distortion Analyse band structure in distorted case ◦ θ = 12 Local basis rotated WRT mean crystal structure θ = 12 Level splitting : 0.15eV ◦ θ = 20 Level splitting : 0.25eV ◦ Pavarini et al PRL 92 176403 (2004) Copyright A. J. Millis 2013 Columbia University free-space d-orbital: 5-fold degenerate lattice effects lift degeneracy Rondinelli and Spaldin, Adv. Mater. 23 3363 (2011) Jahn-Teller (0.1/AA: 0.2eV) GdFeO3 Rotations (15o: 0.2eV) Splittings from structural effects by themselves are typically small compared to bandwidths. Overall band-width renormalization important. ?Enhancement of splitting by manybody effects: orbital ordering? Copyright A. J. Millis 2013 Columbia University