Chapter 4 many-electron atoms Periodic system and shell structure The empirically determined physical and chemical properties of the atoms and their dependence on the atomic number Z lead to the discovery of the periodic system of the elements. It is one of the goals of atomic physics to understand the ordering and the properties of the chemical elements in periodic system. These are explainable starting from the electronic structures of the atoms. With some important experimental facts, for example, alkali atoms and x-ray spectra, one-electron spectra and many-electron spectra, it leads to the concept of the shell structure of atoms. The periodic system of the elements; Schrödinger equation for a many-electron problem — Hartree-Fock technique; shell structures of the atoms; The periodic system of the elements Atomic volumes and ionisation energies as function of the position in the periodic system of the elements. Particularly noticeable are the (relatively) large atomic volumes of the alkali metal atoms and the large ionisation energies of the noble gas atoms. Properties of elements in periodic table The halogens The transition metals Lanthanides Actinides The alkaline earth metals The Alkali metals The noble gases periodicity With increasing atomic number, the electron configuration of the atoms display a periodic variation. Because of this the elements show periodic variations of both physical and chemical behavior. Atomic Radius: the atomic radii increases top to bottom and right to left in the periodic table. The size of the electron cloud increases as n increases. look down the periodic table, the size of atoms in each group is going to increase. look across the periodic table, all the atoms in each group have the same n. However, for each element, the positive charge on the nucleus increases by one proton, the outer electron cloud is pulled in a little tighter. they tend to decrease in size from left to right across a period of the table. periodicity Ionization Energy: The energy needed to remove the most loosely held electron from an atom. Ionization energies are periodic. In any column or group, there is a gradual decrease in ionization energy as the atomic number increases. Metals typically have a low ionization energy. Nonmetals typically have a high ionization energy. Electron Affinity: The attraction of an atom for an electron. Metals have low electron affinities while nonmetals have high electron affinities. The general trend as you go down a column is a decreasing tendancy to gain electrons. As you go across a row there is also a trend for a greater attraction for electrons. Shell structures and periodic properties of the elements Properties of elements in Group 1A, the alkali metals The alkali metals are the elements Li, Na, K, Rb, Cs. These elements have relatively low melting points. Cesium melts at body temperature, 37o Celsius. They are soft enough that they can be cut with a knife. They react violently with water. Properties of elements in Group 8A, the noble gases • The noble gases, He, Ne, Ar, Kr, Xe, Ra, are nonmetals. • The noble gases are very unreactive. They were once called the inert gases. • The noble gases are so unreactive they are used to protect materials from reaction. Welding is done using argon atmosphere to prevent oxygen in the air from reacting with the hot welded metals. Shell structures and periodic properties of the elements Properties of elements in Group 7A, the halogens The halogens, F, Cl, Br, I, At, are nonmetals. Halogens have lower melting points than the alkali metals. Fluorine and chlorine are gases at room temperature The halogens are corrosive and so reactive that in nature they are only found combined with other elements Properties of elements in Group 2A, the alkaline earth metals • The alkali metals are the elements Be, Mg, Ca, Sr, Ba, Rd. • These elements have higher melting points than the alkali metals. • They are harder and tougher. Magnesium is used to fabricate car parts like wheels. • Calcium reacts with water. Magnesium clearly doesn't react with water. Schrödinger equation for a many-electron problem — Hartree-Fock technique; Strictly speaking, in order to understand the electronic structures of any atoms, and in order to define the quantum numbers of an electron in the atom, one would have to solve the Schrödinger equation for a manyparticle problem, namely for all the electrons in the atom---many body problem---no analytical solution. The problem is solved approximately using the HartreeFock technique, which is based on the model of independent particles. Hartree-Fock technique The basic idea is that instead of trying to calculate the interactions of N-1 electrons with Nth electron, one replaces the Coulomb attraction of the nucleus for the Nth electron by an effective potential. One then calculates the eigenstates and the eigenvalues of the Nth electron in this potential field. These one-particle functions are often referred to in the literature as orbitals. In the actual problem, the Coulomb interaction among the electrons is taken into account. The energy of the Coulomb interaction between the pair of electrons j, k is given by e2/(40rjk) (rjk is the distance between the electrons), so the Halmitonian is: N e 2 N 2 1 e H Hj Hj 2 j k 40 rjk j 1 j k 40 r jk j 1 The next step is to solve the Schrödinger equation: H Et There is no exact solution for the many-body problem, it has to be reduced to a one-electron problem. One-particle problem As we know from the electrostatics, there is an interaction energy between a charge at position r and the charge distribution given by other electrons in the many-electron atom, which is the effective potential V(r): 2 V (r ) 1 40 e (rj ) r r j d j 1 40 e Q ( R j ) r rj d j Where is the charge distribution, is the wave-function, the integral covers the total volume. Then we must solve the Schrödinger equation in which both the Coulomb potential of the nucleus and the interaction energy with all the other electrons. If the chosen electron has the subscript k, and the coordinate Rk: 2 2 1 Ze 2 0 1 V ( r ) ( R ) E k k k k k ( Rk ) 40 rk 2m0 Hartree-Fock method The Hartree-Fock method needs a trial functions (0). The superscript (0) means that we use a given (or guessed) wavefunction to start the whole procedure. The trial wavefunction is belong to a given potential V(0). The next step is to solve the Schrödinger equation with given potential V(0), and we have the new wavefunction (1). (1) again is belong to a given potential V(1). Then repeat the same process… Seen schematically, we have the calculation procedure: ( 0) V ( 0) (1) V (1) ( 2) V ( 2) ( j ) The was achieve by a series of iteratively process, and the calculations were done by computers. We will not involve in detailed calculations. The results are interesting for the structures of many-electron atoms. Orbitals and quantum numbers Orbitals: the one-electron function calculated by Hartree-Fock method is referred to in the literature as orbitals, which are the eigenstates and eigenvalues of the Nth electron in the manyelectron atom. Similar to one electron atom, H, it needs quantum numbers to characterise the atomic structures: The principal quantum number: n = 1, 2, 3, 4…; The orbital quantum number: l = 0, 1, 2, 3, …, n-1; The magnetic quantum number: ml = 0, ±1, ±2, …, ±l; The magnetic spin quantum number: ms = ±1/2. The electronic configuration The electronic configuration: a particular states of the energy levels or terms of an atoms by electrons is called electronic configuration of the atom in that state – in this case, the ground state. The questions for the electronic configuration: What are the possible electronic configurations in the atoms; Which are particularly stable; How the electrons of an atom are distributed among the possible quantum number. Pauli principle Pauli principle (Pauli 1925): the electronic states of an atom can only be occupied in such a way that no two electron have exactly the same set of quantum numbers. The electrons must therefore differ in at least one quantum number. A set of quantum numbers: n, l, ml, ms. A state of an atom, the states with the lowest energies are naturally the occupied ones. Shell structures Shell: the group of the electrons with the same principal quantum number n. The shell is also refer to energy level or term. n = 1, 2, 3, 4, 5, … refers to K, L, M, N, O shells, … Electron in K shell is much closer to the nucleus than L shell. Subshell: the group of the electrons with the same principal quantum number n and the same orbital quantum number l. l = 0, 1, 2, 3, 4, … refers to S, P, D, F, G, … subshells, … subshells Shell structures level or shell number of subshells type of subshells Maximun number of electrons in shell 2n2 n=1 1 S 2 n=2 2 S and P 8 n=3 3 S, P, D 18 n=4 4 S, P, D, F 32 n=5 5 S, P, D, F, G - n=6 6 S, P, D, F, G, H - n=7 7 S, P, D, F, G, H, I - the number of electrons (112) in the biggest atom known can be accommodated by using only the common s, p, d, and f sublevels. The subshells g, h, i etc. are never needed. Distance between nucleus and an electron The principal quantum number "n" is very useful. It tells the relative energy for an electron in an atom and it also indicates the average distance between the nucleus and an electron. The higher the value for "n" the greater the distance between the nucleus and the electron. An electron in the first level, n = 1, is closer to the nucleus on average than an electron in the n = 4 shell Subshells s, p, d and f The shape for all "s" orbitals is spherical with the center of the sphere at the nucleus. The size of the sphere increases for increasing quantum numbers. The 1s has a smaller diameter than the 2s and so forth. Subshells s, p, d and f The p orbitals have a double lobe shape with the point of contact of the lobes at the center of the nucleus. The three different p orbitals are each aligned along one of the three coordinate axes x, y, or z Number of orbitals in a shell orbital type S p d f maximum number of orbitals in a subshell 1 3 5 7 number of electrons that can fit into orbital type 2 6 10 14 The maximum number of electrons with a given principal quantum number which can be bound to an atom: For a given n there are n different values for l; For every value of l there are 2l+1 different values of ml; For each pair of l and ml there are two different values of ms; Thus for each pair of numbers n and l, there are at most 2(2l+1) electrons. The maximum number of electrons in a shell with a given value of n is: n 1 2 2 ( 2 l 1 ) 2 n l 0 It is the possible electronic configuration of many-electron atoms. The shell structure of the atomic energy levels and their ordering, for the last added electron and for the inner electrons What is the electronic configuration for the elements? He(2) B(5) Ni(28) (1s)2 (1s)2(2s)2(2p)1 (1s)2(2s)2(2p)6(3s)2(3p)6(4s)2(3d)8 Orbital diagram Electronic configurations Na(11) Mg(12) Al(13) Si(14) P(15) S(16) Cl(17) Ar(18) 2 2 6 1 1s 2s 2p 3s 2 2 6 2 1s 2s 2p 3s 1s22s22p63s23p1 1s22s22p63s23p2 1s22s22p63s23p3 2 2 6 2 4 1s 2s 2p 3s 3p 2 2 6 2 5 1s 2s 2p 3s 3p 1s22s22p63s23p6 The orbital diagrams Many-electron atoms Examples of the filling of the electron configurations Element He Li Be O Cl K Electrons in Element 2 3 4 8 17 19 Electron Configuration 1s2 1s22s1 1s22s2 1s22s22p4 1s22s22p63s23p5 1s22s22p63s23p64s1 Closed shell A closed shell or noble gas configuration occurs whenever the next electron to be added would occupy the s state of the next higher principal quantum number n, and it is not necessary that all the states belong to the lower principal quantum numbers be filled. The electrons in the closed shells are more closer to the nucleus and are more strongly bound. The angular momentum and magnetic moments add up to zero, so that the closed shells are spherically symmetrical and is especially stable. The closed shells are particularly stable electronic configurations. 2He (1s)2 (1s)2(2s)2(2p)6 18Ar (3s)2(3p)6 10Ne 36Kr (4s)2(3d)10(4p)6 54Xe (5s)2(4d)10(5p)6 86Rn (6s)2(4f)14(5d)10(6p)6 Electron configuration and the periodic table The transition metals The noble gases The halogens The Alkali metals The alkaline earth metals Lanthanides Actinides •The left-most columns include the alkali metals and the alkaline earth metals. In these elements the valence s orbitals are being filled •On the right hand side, the right-most block of six elements are those in which the valence p orbitals are being filled These two groups comprise the main-group elements •In the middle is a block of ten columns that contain transition metals. These are elements in which d orbitals are being filled •Below this group are two rows with 14 columns. These are commonly referred to the f-block metals. In these columns the f orbitals are being filled homework 19.1, 19.4, 19.6, 19.7