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margin-left:0;margin-top:0;width:24pt;height:24pt;z-index:1; mso-wrap-distance-left:6pt;mso-wrap-distance-top:2.25pt; mso-wrap-distance-right:6pt;mso-wrap-distance-bottom:2.25pt; mso-position-horizontal:left;mso-position-vertical-relative:line' o:allowoverlap="f"> <v:imagedata src="%20"/> <w:wrap type="square"/> </v:shape><![endif]--><![if !vml]><img width=32 height=32 src="%20" align=left hspace=8 vspace=3 v:shapes="_x0000_s1026"><![endif]><span style='font-size: 24.0pt;font-family:Helv;color:blue'>Gulzari L. Malli<o:p></o:p></span></h2> <h3><span style='font-size:24.0pt;font-family:Helv;color:blue'><span style='mso-spacerun:yes'> </span><span style='mso-spacerun:yes'></span>Professor Emeritus <o:p></o:p></span></h3> <p class=MsoNormal><span style='font-size:10.0pt'><br> </span><span style='font-size:16.0pt'><span style='mso-spacerun:yes'></span></span><b style='mso-bidi-font-weight:normal'><span style='font-size:22.0pt'>M.Sc., </span></b><st1:place><st1:PlaceName><b style='mso-bidi-font-weight:normal'><span style='font-size:22.0pt'>McMaster</span></b></st1:PlaceName><b style='mso-bidi-font-weight:normal'><span style='font-size:22.0pt'> </span></b><st1:PlaceType><b style='mso-bidi-font-weight:normal'><span style='font-size:22.0pt'>University</span></b></st1:PlaceType></st1:place><b style='mso-bidi-font-weight:normal'><span style='font-size:22.0pt'>, 1960 <br> <span style='mso-spacerun:yes'></span>M.S., Ph.D., 1964, </span></b><st1:place><st1:PlaceType><b style='mso-bidi-font-weight:normal'><span style='font-size:22.0pt'>University</span></b></st1:PlaceType><b style='mso-bidi-font-weight:normal'><span style='font-size:22.0pt'> of </span></b><st1:PlaceName><b style='mso-bidi-font-weight:normal'><span style='font-size:22.0pt'>Chicago</span></b></st1:PlaceName></st1:place><b style='mso-bidi-font-weight:normal'><span style='font-size:22.0pt'> <o:p></o:p></span></b></p> <p class=MsoNormal><span style='font-size:16.0pt;color:lime'><br> </span><span style='color:aqua'><span style='mso-spacerun:yes'></span></span><b style='mso-bidi-font-weight:normal'><span style='font-size:22.0pt;color:lime'>Tel: (604) 291-4880 <br> <span style='mso-spacerun:yes'></span>Fax: (604) 291-3765 <br> <span style='mso-spacerun:yes'></span>e-mail:<a href="mailto:malli@sfu.ca"><span style='font-family:Helv;color:lime'>malli@sfu.ca</span></a> <o:p></o:p></span></b></p> <p class=MsoNormal><b style='mso-bidi-font-weight:normal'><span style='font-size:20.0pt;color:lime'><o:p>&nbsp;</o:p></span></b></p> <div class=MsoNormal align=center style='text-align:center'><b style='mso-bidi-font-weight:normal'><span style='font-size:20.0pt;font-family: Helv'> <hr size=3 width="100%" align=center> </span></b></div> <h3><i style='mso-bidi-font-style:normal'><span style='font-size:26.0pt; font-family:Helv;color:blue;font-weight:normal;mso-bidi-font-weight:bold'>RELATIVISTIC QUANTUM CHEMISTRY</span></i><span style='font-size:26.0pt;font-family:Helv; color:blue;font-weight:normal;mso-bidi-font-weight:bold'>, CHEMICAL<i style='mso-bidi-font-style:normal'> PHYSICS</i><o:p></o:p></span></h3> <h3><span style='font-size:20.0pt;font-family:Helv;color:red;font-weight:normal; mso-bidi-font-weight:bold'>Current Research Program</span><span style='font-size:20.0pt;font-family:Helv;color:lime;font-weight:normal; mso-bidi-font-weight:bold'>:</span><span style='font-size:20.0pt;font-family: Helv;color:blue'> Relativistic Quantum Chemistry of Heavy and Superheavy Elements: Rutherfordium through upto primordial superheavy element ekaplutonium E126 (with Z=126).<o:p></o:p></span></h3> <p class=MsoNormal><span style='font-size:18.0pt;font-family:Helv'>Our main research interests lie in the general area of ab initio <span style='color: red'>relativistic quantum chemistry</span> of the <span style='color:red'>heavy and superheavy elements</span> with 75 &lt; Z &gt; 126, viz; to develop theoretical and computational methodology for <i><span style='color:red'>ab initio</span></i> <span style='color:blue'>all-electron</span> calculation of the <span style='color:blue'>relativistic</span> as well as <span style='color:lime'>electron correlation effects</span> for molecules, clusters and solids involving heavy and superheavy elements <span style='color:red'>(SHE)</span>, with Z =75-126, where Z is the nuclear charge. Our major contributions to this area of research are summarized below:<o:p></o:p></span></p> <p style='margin-left:60.0pt;text-indent:-33.0pt;mso-list:l1 level1 lfo2; tab-stops:list 60.0pt'><![if !supportLists]><span style='font-size:18.0pt; font-family:Helv;mso-fareast-font-family:Helv;mso-bidi-font-family:Helv'><span style='mso-list:Ignore'>1.<span style='font:7.0pt "Times New Roman"'>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; </span></span></span><![endif]><span style='font-size:18.0pt;font-family:Helv'>Three decades ago we developed the <i>Relativistic</i><span style='color:blue; mso-bidi-font-style:italic'> Self-consistent Field Theory for Closed-Shell Molecules<i>&quot;</i></span><span style='color:blue'>: G.Malli and J.Oreg, J.Chem.Phys.63, 830 (1975</span>). A computer code was developed based upon our formalism and the <i style='mso-bidi-font-style:normal'><span style='color: red'>first</span></i><span style='color:red'> Dirac-Fock SCF calculations</span> using the basis set of Slater-type-orbitals (STOs) were reported on the diatomics Li<sub>2</sub> and Be<sub>2</sub>, see<span style='mso-spacerun:yes'> </span><span style='color:blue'>G.L.Malli and J.Oreg</span>, <span style='color:blue'>Chem.Phys.Letters</span>,<span style='mso-spacerun:yes'> </span>. However, these were preliminary calculations with a minimum of basis set and for the medium and heavy atom molecules very extensive calculations involving extended basis set would be mandatory. As is well-known in <span style='color:lime'>nonrelativisic quantum chemistry</span>, the STOs are unsuitable for molecular calculations in general on polyatomics as first pointed by <span style='color:red'>Boys</span> who proposed the use of <span style='color:blue'>Gaussian type orbitals (GTOs) </span>for quantum mechanical calculations on polyatomics. <o:p></o:p></span></p> <p style='margin-left:60.0pt;text-indent:-33.0pt;mso-list:l1 level1 lfo2; tab-stops:list 60.0pt'><![if !supportLists]><span style='font-size:18.0pt; font-family:Helv;mso-fareast-font-family:Helv;mso-bidi-font-family:Helv'><span style='mso-list:Ignore'>2.<span style='font:7.0pt "Times New Roman"'>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; </span></span></span><![endif]><span style='font-size:18.0pt;font-family:Helv; color:red'>In 1979<b style='mso-bidi-font-weight:normal'> we introduced the Gaussian spinor basis set for relativistic Dirac-Fock SCF calculations on atoms and (molecules):</b></span><span style='font-size:18.0pt;font-family:Helv'> <span style='color:blue'>G.L.Malli, Chem.Phys.Letters, <b style='mso-bidi-font-weight: normal'>68</b>,</span> <span style='color:blue'>529(1979) where we reported the DF SCF calculations for Xe using our G-spinor basis set.</span><o:p></o:p></span></p> <p style='margin-left:60.0pt;text-indent:-33.0pt;mso-list:l1 level1 lfo2; tab-stops:list 60.0pt'><![if !supportLists]><span style='font-size:18.0pt; font-family:Helv;mso-fareast-font-family:Helv;mso-bidi-font-family:Helv; color:purple'><span style='mso-list:Ignore'>3.<span style='font:7.0pt "Times New Roman"'>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; </span></span></span><![endif]><span style='font-size:18.0pt;font-family:Helv'>The <span style='color:lime'>first all-electron fully relativistic calculation</span> on the <span style='color:blue'>heavy diatomic AuH</span> was reported by <span style='color:blue'>Malli and Pyper</span> <span style='color:blue'>[G.L.Malli and N.C.Pyper, Proc.Roy.Soc. A407, 377(1986)]</span> using the <span style='color:red'>numerical DF atomic spinors</span> of Au and H as the basis set. <span style='color:blue'>We showed for the first time</span> that <span style='color:red'>due to relativity</span> (i) there was <span style='color:red'>significant 5d-6s hybridization</span> in the gold atom, (ii) the predicted dissociation energy was <span style='color:red'>doubled, </span><span style='color:black'>and (iii)</span><span style='color:red'> there was a bond contraction of 0.45 bohr.</span> <span style='color:purple'><o:p></o:p></span></span></p> <p style='margin-left:27.0pt'><span style='font-size:18.0pt;font-family:Helv'>(4) <span style='color:lime'>We performed the <i style='mso-bidi-font-style:normal'>first</i></span> limited <span style='color:blue'>relativistic Configuration Interaction (RCI) </span>calculation for AuH and we reported the <span style='color:blue'>effects of relativity and electron correlation on bond length, vibrational frequency, dissociation energy</span> (and<span style='color:lime'> dipole moment)</span>. Later we reported such results for the diatomic hydrides of the sixth row elements. <span style='color:red'>A 50% reduction of the dipole moment was predicted by relativity for AuH:</span> <span style='color:blue'>A.F.Ramos, N.C.Pyper and G.L.Malli, Phys.Rev. A 38, 2729(1989).No such calculations had been reported for any heavy atom molecule.<o:p></o:p></span></span></p> <p style='margin-left:27.0pt'><span style='font-size:18.0pt;font-family:Helv; color:aqua'>We extended our relativistic DF SCF theory</span><span style='font-size:18.0pt;font-family:Helv'> to <span style='color:red'>a general class of open shell molecular systems [G.L.Malli, Chem.Phys.Lett.73, 510(1980)] and </span>its application to AuH+ was reported <span style='color:blue'>[Y.Ishikawa, G.L.Malli and N.C.Pyper, Chem.Phys.Lett.194, 481(1992)].<o:p></o:p></span></span></p> <p style='margin-left:27.0pt'><span style='font-size:18.0pt;font-family:Helv'>(5) We have developed the Universal Gaussian Basis set <span style='color:blue'>[G.L.Malli et al</span>, <span style='color:blue'>Phys.Rev. <b style='mso-bidi-font-weight: normal'>A 47</b>,143 (1993),</span> <i style='mso-bidi-font-style:normal'><span style='color:blue'>ibid</span></i><span style='color:blue'>, Chem.Phys.Lett, <b style='mso-bidi-font-weight:normal'>201</b>, 37 (1993);<i style='mso-bidi-font-style: normal'>ibid</i> J.Chem.Phys. 1<b style='mso-bidi-font-weight:normal'>01</b>,6829 (1994);<i style='mso-bidi-font-style:normal'>ibid,</i> J.Chem.Phys.<b style='mso-bidi-font-weight:normal'>109</b>,8759(1998)]</span> for the <i><span style='color:lime'>first ab initio all-electron</span></i><span style='color:lime'> Dirac-Fock (DF) relativistic self-consistent field (RSCF) calculations</span> for <span style='color:blue'>a large number of diatomics and polyatomics</span> involving <span style='color:blue'>heavy</span> and <span style='color:blue'>superheavy</span> elements(SHE).<o:p></o:p></span></p> <p style='margin-left:27.0pt'><span style='font-size:18.0pt;font-family:Helv'>(6)We <span style='color:red'>have performed the first</span> Dirac- scattered wave (DSW) SCF calculations on <span style='color:blue'>gold clusters with 3 to 13 gold atoms in various geometries</span> including <span style='color:lime'>the first Icosahedral (I<b style='mso-bidi-font-weight:normal'><sub>h</sub></b>*) and cuboctahedron geometries for 13 gold atoms</span> and we discussed the relative stabilities for the 13 gold -atom geometrical configurations: <o:p></o:p></span></p> <p style='margin-left:27.0pt'><span style='font-size:18.0pt;font-family:Helv'>(7) Recently we have investigated <span style='color:blue'>both</span> the <span style='color:red'>effects of relativity</span> and <span style='color:red'>electron correlation</span> using our fully relativistic Dirac-Fock, relativistic Moller-Plesset second order perturbation theory (MP2<span style='color:red'>), coupled-cluster single and doubles (RCCSD) and RCCSD(T) calculations </span>which treat the triple excitations as perturbation.for a large number of molecules involving <span style='color:blue'>heavy actinides</span> and SHE elements up to <span style='color:red'>the primordial SHE E126 ekaplutonium.<o:p></o:p></span></span></p> <p style='margin-left:27.0pt'><span style='font-size:18.0pt;font-family:Helv'>(8) Currently we are using the relativistic coupled-cluster methodology for atoms and molecules of heavy and SHE. These calculations are performed using <span style='color:blue'>our universal Gaussian basis set (UGBS)</span> for atoms of the heaviest elements (Z=104-126) assuming a Gaussian nuclear model using the MOLFDIR code. <o:p></o:p></span></p> <p style='margin-left:27.0pt'><span style='font-size:18.0pt;font-family:Helv; color:blue'>(9) All-electron</span><span style='font-size:18.0pt;font-family: Helv'> <span style='color:blue'>fully relativistic 4-component DF SCF calculations </span>have been performed for <span style='color:lime'>over 200 molecules of the transactinides and their lighter homologs</span> which include the following:<span style='color:red'>tetrachlorides</span> of Zr, Hf and Rf (Z=104); <span style='color:red'>pentachlorides</span> of Nb, Ta and Ha (Z=105); <span style='color:red'>hexachlorides</span> of Mo, W and Sg (Z=106);<span style='color:red'>oxychlorides</span> TaOCl<sub>3</sub> HaOCl<sub>3</sub> , SgOCl<sub>4</sub> , SgO<sub>2</sub>Cl<sub>2</sub> ; <span style='color:red'>hexafluorides</span> and hexachlorides of E110 ( Z=110); tetra,penta,and hexachlorides and the corresponding-bromides of Rf, Ha, Sg , Ns( Z=107) and E111 ( Z=111),<span style='color:red'>hexafluoride and hexachloride of E126</span> ( ekaplutonium).<o:p></o:p></span></p> <p><span style='font-size:18.0pt;font-family:Helv'><span style='mso-spacerun:yes'></span>(10)We have also investigated the <span style='color:red'>stability and atomization (binding) energy </span>of the various <span style='color:red'>actinide and superheavy element carbonyls M(CO)n</span> <span style='color:lime'>and isocarbonyls M(OC)n</span> (n=1-6, M=Th, U,Pu, Rf,Sg,E110, E112, E118,E122,E124,E126),etc.<o:p></o:p></span></p> <p><span style='font-size:18.0pt;font-family:Helv;color:blue'>Our gargantuan calculations which required thousands of CPU hrs and huge disk space were performed at Cray C90 and IBM RS 6000 Seaborg<span style='mso-spacerun:yes'> </span>supercomputers at National Energy Research Scientific Computing Center (NERSC</span><span style='font-size:18.0pt;font-family:Helv;color:red'>), </span><span style='font-size:18.0pt;font-family:Helv;color:lime'>supported by the Office of Science of the U.S. Department of Energy and at the Cray supercomputer centre at </span><st1:place><st1:PlaceName><span style='font-size:18.0pt;font-family: Helv;color:lime'>Chippewa</span></st1:PlaceName><span style='font-size:18.0pt; font-family:Helv;color:lime'> </span><st1:PlaceType><span style='font-size: 18.0pt;font-family:Helv;color:lime'>Falls</span></st1:PlaceType></st1:place><span style='font-size:18.0pt;font-family:Helv;color:lime'> through the generosity of Cray Inc, </span><st1:country-region><st1:place><span style='font-size:18.0pt; font-family:Helv;color:lime'>Canada</span></st1:place></st1:country-region><span style='font-size:18.0pt;font-family:Helv;color:lime'>.<o:p></o:p></span></p> <p><span style='font-size:18.0pt;font-family:Helv;color:blue'>Our recent research in the chemistry and physics of the heavy and superheavy elements was featured in<span style='mso-spacerun:yes'> </span>the <b style='mso-bidi-font-weight: normal'>Chemical &amp; Engineering News (C &amp; EN): Heavy Elements, </b></span><st1:date Year="1998" Day="23" Month="3"><b style='mso-bidi-font-weight:normal'><span style='font-size:18.0pt;font-family:Helv;color:blue'>March 23,1998</span></b></st1:date><b style='mso-bidi-font-weight:normal'><span style='font-size:18.0pt;font-family: Helv;color:blue'> issue, see pp 54-55.</span></b><span style='font-size:18.0pt; font-family:Helv'> <span style='color:blue'>More recently, our research in</span><span style='color:black'> </span><span style='color:red'>Transactinde Chemistry</span><span style='color:black'> was highlighted in</span><span style='color:aqua'> </span><b style='mso-bidi-font-weight:normal'><span style='color:blue'>Chemical &amp; Engineering News (C &amp; EN</span></b><span style='color:aqua'> </span><span style='color:blue'>)<b style='mso-bidi-font-weight:normal'> December 16, 2002 issue,p.11,</b></span><span style='color:aqua'> </span><span style='color:blue'>devoted to <b style='mso-bidi-font-weight:normal'>Chemistry Highlights 2002</b> under <b style='mso-bidi-font-weight:normal'> HEAVY WEIGHTS YIELD TO COMPUTATION</b>.</span><span style='color:aqua'> <o:p></o:p></span></span></p> <p><span style='font-size:18.0pt;font-family:Helv'><o:p>&nbsp;</o:p></span></p> <div class=MsoNormal align=center style='text-align:center'><span style='font-size:18.0pt;font-family:Helv'> <hr size=3 width="100%" align=center> </span></div> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><b><span style='font-size:26.0pt; font-family:Helv;color:#FF6600'>Selected Publications</span></b><b><span style='font-size:10.0pt;font-family:Helv'> </span></b><b><span style='font-size:26.0pt;font-family:Helv;color:#FF6600'>(1995-2005)</span></b><b><span style='font-size:10.0pt;font-family:Helv'><o:p></o:p></span></b></p> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:10.0pt; font-family:Helv'><span style='mso-spacerun:yes'></span></span><span style='font-size:18.0pt'><span style='mso-spacerun:yes'></span></span><span style='font-size:18.0pt;font-family:Palatino'><o:p></o:p></span></p> <p class=MsoBodyTextIndent2><span style='font-size:18.0pt'>103.<span style='mso-tab-count:1'> </span>Malli, G.L., J. Styszynki, and A.B.F. DaSilva (1995).<span style='mso-spacerun:yes'> </span>Ab Initio Calculation of Relativistic and Electron Correlation Effects in Polyatomics using the universal Gaussian Basis set : XeF<sub>2</sub> . <i style='mso-bidi-font-style:normal'>Int. J. Quantum. Chem.,</i> <u>55</u>, 213-225<o:p></o:p></span></p> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt; font-family:Palatino'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt; font-family:Palatino'>104.<span style='mso-tab-count:1'> </span>Styszynski, J. and Malli, G.L. (1995). Electron Correlation and Relativistic Effects in Xenon Tetrafluoride, <i style='mso-bidi-font-style:normal'>Int. J. Quantum. Chem.,</i> <u>55</u>, 227-235.<o:p></o:p></span></p> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt; font-family:Palatino'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.0pt 59.3pt 82.1pt'><span style='font-size:18.0pt; font-family:Palatino'>105.<span style='mso-tab-count:1'> </span>Malli, G.L. and<span style='mso-spacerun:yes'> </span>Styszynki J. (1996)<span style='mso-spacerun:yes'> </span>Ab <i style='mso-bidi-font-style:normal'>initio </i>all-electron Dirac-Fock-Breit calculations for UF<sub>6</sub>, <i style='mso-bidi-font-style:normal'>J. Chem. Phys.</i> <u>104:,</u><span style='mso-spacerun:yes'> </span>1012-1017.<o:p></o:p></span></p> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.0pt 59.3pt 82.1pt'><span style='font-size:18.0pt; font-family:Palatino'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt; font-family:Palatino'>106<span style='mso-tab-count:1'> </span><span style='mso-tab-count:1'> </span>Styszynski, J. Xiaoping, C., Malli, G.L. and L. Visscher (1997). Relativistic All-Electron Dirac-Fock-Breit Calculations on Xenon Fluorides (XeF<sub>n</sub>, n=1,2,4,6), J<i style='mso-bidi-font-style: normal'>. Computational Chem., </i><b style='mso-bidi-font-weight:normal'>18</b> , 601-608.<o:p></o:p></span></p> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt; font-family:Palatino'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt; font-family:Palatino'>107<span style='mso-tab-count:2'> </span>Malli, G.L. (1997) .Ab Initio Relativistic Quantum Chemistry of Superheavy Transactinide Elements:Rutherfordium through Eka-Astatine , Proceedings of The Robert A.Welch Foundation XXXXI Conference on Chemical Research The Transactinide Elements , 197-228 , Houston, Texas, U.S.A.<o:p></o:p></span></p> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt; font-family:Palatino'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt; font-family:Palatino'>108<span style='mso-tab-count:2'> </span>Malli, G.L. and J.Styszynski (1998) Ab Initio all-electron fully Relativistic Dirac-Fock-Breit Calculations for Molecules of the Transactinide Superheavy Elements: Rutherfordium Tetrachloride <i style='mso-bidi-font-style:normal'>, J.Chem.Phys</i>, <b style='mso-bidi-font-weight:normal'>109</b>, 4448-4455.<o:p></o:p></span></p> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt; font-family:Palatino'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt; font-family:Palatino'>109.<span style='mso-tab-count:1'> </span>Malli, G.L and Y. Ishikawa (1998) The Generator Coordinate Dirac-Fock Method for Open-Shell Atomic Systems , J.Chem.Phys., <b style='mso-bidi-font-weight:normal'>109</b> , 8759-8763<o:p></o:p></span></p> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt; font-family:Palatino'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt; font-family:Palatino'>110<span style='mso-tab-count:1'> </span>.<span style='mso-tab-count:1'> </span>Malli, G.L. (2001) Relativistic Quantum Chemistry of Superheavy Transactinide Elements. <i style='mso-bidi-font-style: normal'>New Trends in Quantum Systems in Chemistry and Physics, Volume <b style='mso-bidi-font-weight:normal'>1</b>, </i>243-255<i style='mso-bidi-font-style: normal'>.<o:p></o:p></i></span></p> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><i style='mso-bidi-font-style: normal'><span style='font-size:18.0pt;font-family:Palatino'><o:p>&nbsp;</o:p></span></i></p> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt; font-family:Palatino'>111<span style='mso-tab-count:2'> </span>Malli, G.L. (2001) Relativistic all-electron Dirac-Fock calculations on RnF<sub>6</sub> and its ions. Journal of Molecular Structure (Theochem), <b style='mso-bidi-font-weight: normal'>537,</b>: 71-77. <o:p></o:p></span></p> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt; font-family:Palatino'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt; font-family:Palatino'>112. <span style='mso-tab-count:1'> </span>Malli, G.L. (2002) Prediction of the existence of radon carbonyl: RnCO. Int. J Quantum Chem, <b style='mso-bidi-font-weight:normal'>90</b>, 611-615.<o:p></o:p></span></p> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt; font-family:Palatino'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt; font-family:Palatino'>113.<span style='mso-tab-count:1'> </span>Malli, G.L. (2002) Ab initio all-electron fully relativistic Dirac-Fock self-consistent field calculations for molecules of superheavy elements: Seaborgium hexabromide. J. Chem. Phys, <b style='mso-bidi-font-weight:normal'>116, </b>5476.<o:p></o:p></span></p> <p class=MsoNormal style='margin-left:31.5pt;text-align:justify;text-indent: -31.5pt;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt; font-family:Palatino'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino'>114.<span style='mso-tab-count: 1'> </span>Malli, G.L. (2002) (<span style='color:blue'>Communication</span>) Dramatic relativistic effects in atomization energy and volatility of the superheavy Hassium tetroxide and OsO<sub>4</sub>, J. Chem. Phys, <b style='mso-bidi-font-weight:normal'>117</b>, 10441-10443. <o:p></o:p></span></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino'>115.<span style='mso-tab-count: 1'> </span>Malli, G.L. (2003<i style='mso-bidi-font-style:normal'>). </i>Ab initio all-electron fully relativistic Dirac-Fock Self-consistent field calculations for UCl<sub>6</sub>. Mol. Phys., <b style='mso-bidi-font-weight: normal'>101</b>, 287-294.<o:p></o:p></span></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino'>116.<span style='mso-tab-count: 1'> </span>Malli, G.L., Siegert, M and.Turner, D.P (2004) Relativistic <span style='mso-spacerun:yes'></span>and Electron Correlation Effects for Molecules of Heavy Elements: An initio Fully Relativistic Coupled-Cluster Calculations for PbH<sub>4</sub> , Int. J. Quantum Chem.<b style='mso-bidi-font-weight:normal'>99</b>, 940-949<o:p></o:p></span></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino'>117.<span style='mso-tab-count: 1'> </span>Malli,G.L. (2004) Relativistic Quantum Chemistry of Heavy and Superheavy Elements: Fully Relativistic Coupled-Cluster Calculations for Molecules of Heavy and Transactinide Superheavy Elements. <i style='mso-bidi-font-style: normal'>Fundamental World of Quantum Chemistry, <b style='mso-bidi-font-weight: normal'>Vol. III</b>, </i>323-363<i style='mso-bidi-font-style:normal'>, </i>E.J.Brandas and E.S.Kryachko (eds), Kluwer Academic Publishers.<o:p></o:p></span></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><i style='mso-bidi-font-style:normal'><span style='font-size:18.0pt;font-family: Palatino'><o:p>&nbsp;</o:p></span></i></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino'>118.<span style='mso-tab-count: 1'> </span>Arratia-Perez, R., Hernandez-Acvedo, L, and Malli, G.L.,<o:p></o:p></span></p> <p class=MsoNormal style='margin-left:9.0pt;text-align:justify;mso-pagination: none;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt; font-family:Palatino'>. Calculated optical and magnetic properties of hexafluorouranate(V) anion:UF<sub>6</sub> <sup></sup>, J.Chem.Phys.<b style='mso-bidi-font-weight:normal'>121</b>,7743-7747 (2004).<o:p></o:p></span></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino'>119.<span style='mso-tab-count: 1'> </span>Malli, G.L., (2005).<span style='color:blue'>(Communication), </span><span style='color:#333333'>Electronic structure and<o:p></o:p></span></span></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino'><span style='mso-spacerun:yes'> </span><span style='mso-spacerun:yes'></span>prediction of atomization energy of naked homoleptic uranium hexacarbonyl U(CO)<sub>6 ,</sub> J.Chem.Phys. (accepted </span><st1:date Year="2005" Day="21" Month="11"><span style='font-size:18.0pt;font-family:Palatino'>Nov 21, 2005</span></st1:date><span style='font-size:18.0pt;font-family:Palatino'>,<b style='mso-bidi-font-weight:normal'>in press</b>) <o:p></o:p></span></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino'>120.<span style='mso-tab-count: 1'> </span> Malli, G.L.,(2005).<span style='color:blue'> (Communication),</span><span style='color:#333333'> Dissociation energy of ekaplutonium fluoride E126F: The first diatomic with molecular spinors consisting of g atomic spinors, </span>J.Chem.Phys. (</span><span style='font-size:20.0pt;font-family:Palatino'>J.Chem.Phys. (</span><span style='font-size:18.0pt;font-family:Palatino'>accepted </span><st1:date Year="2005" Day="30" Month="11"><span style='font-size:18.0pt;font-family:Palatino'>Nov 30, 2005</span></st1:date><b style='mso-bidi-font-weight:normal'><span style='font-size:18.0pt;font-family:Palatino'> in press</span></b><span style='font-size:18.0pt;font-family:Palatino'>)<o:p></o:p></span></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 30.0pt 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino'><span style='mso-tab-count:1'> </span></span><b style='mso-bidi-font-weight:normal'><u><span style='font-size:22.0pt; font-family:Palatino;color:blue'>BOOKS <o:p></o:p></span></u></b></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 30.0pt 59.3pt 82.1pt'><u><span style='font-size:18.0pt;font-family:Palatino'><o:p><span style='text-decoration: none'>&nbsp;</span></o:p></span></u></p> <p class=MsoNormal style='margin-left:30.0pt;text-align:justify;text-indent: -30.0pt;mso-pagination:none;mso-list:l5 level1 lfo5;tab-stops:-.25in 59.3pt 82.1pt'><![if !supportLists]><span style='font-size:18.0pt;font-family:Palatino;mso-fareast-font-family:Palatino; mso-bidi-font-family:Palatino;color:blue'><span style='mso-list:Ignore'>1.<span style='font:7.0pt "Times New Roman"'>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; </span></span></span><![endif]><span style='font-size:18.0pt;font-family:Palatino; color:blue'>Fraga, S. and G.L. Malli (1968). Many-electron Systems, Properties and Interactions, W.B. Saunders, </span><st1:place><st1:City><span style='font-size:18.0pt;font-family:Palatino;color:blue'>Philadelphia</span></st1:City><span style='font-size:18.0pt;font-family:Palatino;color:blue'>, </span><st1:country-region><span style='font-size:18.0pt;font-family:Palatino;color:blue'>U.S.A.</span></st1:country-region></st1:place><span style='font-size:18.0pt;font-family:Palatino;color:blue'>, pp. 196.<o:p></o:p></span></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino;color:blue'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='margin-left:30.0pt;text-align:justify;text-indent: -30.0pt;mso-pagination:none;mso-list:l5 level1 lfo5;tab-stops:-.25in 59.3pt 82.1pt'><![if !supportLists]><span style='font-size:18.0pt;font-family:Palatino;mso-fareast-font-family:Palatino; mso-bidi-font-family:Palatino;color:blue'><span style='mso-list:Ignore'>2.<span style='font:7.0pt "Times New Roman"'>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; </span></span></span><![endif]><span style='font-size:18.0pt;font-family:Palatino; color:blue'>Malli, G.L. (Ed.) (1983). Relativistic Effects in Atoms, Molecules and Solids, Plenum Press, pp. 554, </span><st1:place><st1:City><span style='font-size:18.0pt;font-family:Palatino;color:blue'>New York</span></st1:City><span style='font-size:18.0pt;font-family:Palatino;color:blue'>, </span><st1:country-region><span style='font-size:18.0pt;font-family:Palatino;color:blue'>U.S.A.</span></st1:country-region></st1:place><span style='font-size:18.0pt;font-family:Palatino;color:blue'> Proceedings of the NATO ASI directed and organized by Professor G.L. Malli, and held at U.B.C., </span><st1:date Year="1981" Day="10" Month="8"><span style='font-size:18.0pt;font-family:Palatino; color:blue'>August 10-21, 1981</span></st1:date><span style='font-size:18.0pt; font-family:Palatino;color:blue'>.<o:p></o:p></span></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino;color:blue'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='margin-left:30.0pt;text-align:justify;text-indent: -30.0pt;mso-pagination:none;mso-list:l5 level1 lfo5;tab-stops:-.25in 59.3pt 82.1pt'><![if !supportLists]><span style='font-size:18.0pt;font-family:Palatino;mso-fareast-font-family:Palatino; mso-bidi-font-family:Palatino;color:blue'><span style='mso-list:Ignore'>3.<span style='font:7.0pt "Times New Roman"'>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; </span></span></span><![endif]><span style='font-size:18.0pt;font-family:Palatino; color:blue'>Malli, G.L. (Ed.) (1994). Relativistic and Electron Correlation Effects in Molecules and Solids, Plenum Press, pp. 486, </span><st1:place><st1:City><span style='font-size:18.0pt;font-family:Palatino;color:blue'>New York</span></st1:City><span style='font-size:18.0pt;font-family:Palatino;color:blue'>, </span><st1:country-region><span style='font-size:18.0pt;font-family:Palatino;color:blue'>U.S.A.</span></st1:country-region></st1:place><span style='font-size:18.0pt;font-family:Palatino;color:blue'>, Proceedings of the NATO ASI directed and organized by Professor G.L. Malli, and held at U.B.C., </span><st1:date Year="1992" Day="10" Month="8"><span style='font-size:18.0pt;font-family:Palatino; color:blue'>August 10-21, 1992</span></st1:date><span style='font-size:18.0pt; font-family:Palatino;color:blue'>.<o:p></o:p></span></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 30.0pt 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino;color:blue'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 30.25pt 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='margin-left:49.5pt;text-align:justify;text-indent: -31.5pt;mso-list:skip;tab-stops:-.25in 30.0pt 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino'><o:p>&nbsp;</o:p></span></p> <p class=MsoNormal style='text-align:justify;tab-stops:-.25in 30.0pt 59.3pt 82.1pt'><span style='font-size:18.0pt;font-family:Palatino'><o:p>&nbsp;</o:p></span></p> </div> </body> </html>