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Superheavy Element Research Superheavy Element Research

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The Periodic Table and Relativity<br />

1 18<br />

1 2<br />

H 2 13 14 15 16 17 He<br />

3 4 5 6 7 8 9 10<br />

Li Be B C N O F Ne<br />

11 12 13 14 15 16 17 18<br />

NNa MMg 3 4 5 6 7 8 9 10 11 12 Al Si P S Cl AAr<br />

19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36<br />

K Ca Sc Ti V Cr Mn Fe Co Ni Cu Zn Ga Ge As Se Br Kr<br />

37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54<br />

Rb Sr Y Zr Nb Mo Tc Ru Rh Pd Ag Cd In Sn Sb Te I Xe<br />

55 56 57+* 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86<br />

Cs<br />

87<br />

Ba<br />

88<br />

La<br />

89+"<br />

Hf<br />

104<br />

Ta<br />

105<br />

W<br />

106<br />

Re<br />

107<br />

Os<br />

108<br />

Ir Pt Au Hg<br />

112<br />

Tl Pb Bi Po At Rn<br />

Fr Ra Ac Rf Db Sg Bh Hs 109 110 111 Cn 113 114 115 116 117 118<br />

Mt Ds Rg --- --- --- --- --- ---<br />

* 58 59 60 61 62 63 64 65 66 67 68 69 70 71<br />

Ce Pr Nd Pm Sm Eu Gd Tb Dy Ho Er Tm Yb Lu<br />

" 90 91 92 93 94 95 96 97 98 99 100 101 102 103<br />

Th Pa U Np Pu Am Cm Bk Cf Es Fm Md No Lr<br />

Rel. effects ~Z2 <strong>Element</strong> 114, � member Pronounced in group in heavy 14: elements<br />

-the -Electronic color of Au: conf.: [Rn] 7s<br />

Au: �E (5d conduct. band � Fermi): 2.4 eV (in vis)<br />

Ag: �E (4d conduct. band � Fermi): 3.5 eV (in UV)<br />

2 6d10 5f14 7p 2<br />

1/2<br />

-"Quasi-closed g ( shell" configuration g ) due ( to )<br />

relativistic p<br />

-the "inert pair" 1/2 subshell closure<br />

effect: stabilized 6s electron pair<br />

reduces Evident valency: question: Tl(I), not Tl(III); Pb(II), not Pb(IV),...<br />

-high metallic t ox.states lli (Pb (Pb-like) lik of light )bbehavior, actinides: h i or expanded 5f orbitals<br />

available noble-gas for (Rn-like) chemical bonding: behavior? U(VI) [but no Nd(VI)]<br />

Examples of relativistic orbitals<br />

p1/2 p 3/2<br />

s p d f<br />

RRelativity l ti it in i Chemistry Ch i t<br />

Electrons near nucleus:<br />

v is a large g fraction of c<br />

� relativistic mass increase<br />

1) Direct relativistic effect:<br />

s and d p1/2 orbitals bit l are<br />

stabilized / contracted<br />

2) Indirect relativistic effect:<br />

Other orbitals (p3/2, d, f) are<br />

better shielded from nucleus<br />

� ddestabilized t bili d / expanded d d<br />

3) Spin-orbit splitting:<br />

Heavy atoms: two states per l<br />

� p1/2/p3/2; d3/2/d5/2; f5/2/f7/2 Ch.E. Düllmann – <strong>Superheavy</strong> element research – FIAS Colloquium – Frankfurt Institute for Advanced Studies, Frankfurt – October 20, 2011

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