The Exclusion Principle and the Periodic Table m58587 The Exclusion Principle and the Periodic Table By the end of this section, you will be able to: Explain the importance of Pauli’s exclusion principle to an understanding of atomic structure and molecular bonding Explain the structure of the periodic table in terms of the total energy, orbital angular momentum, and spin of individual electrons in an atom Describe the electron configuration of atoms in the periodic table 306fd5bd-db60-4662-a202-825cc23fdd94 So far, we have studied only hydrogen, the simplest chemical element. We have found that an electron in the hydrogen atom can be completely specified by five quantum numbers: To construct the ground state of a neutral multi-electron atom, imagine starting with a nucleus of charge Ze (that is, a nucleus of atomic number Z) and then adding Z electrons one by one. Assume that each electron moves in a spherically symmetrical electric field produced by the nucleus and all other electrons of the atom. The assumption is valid because the electrons are distributed randomly around the nucleus and produce an average electric field (and potential) that is spherically symmetrical. The electric potential U(r) for each electron does not follow the simple −1/r form because of interactions between electrons, but it turns out that we can still label each individual electron state by quantum numbers, (n,l,m,s,ms). (The spin quantum number s is the same for all electrons, so it will not be used in this section.) The structure and chemical properties of atoms are explained in part by Pauli’s exclusion principle: No two electrons in an atom can have the same values for all four quantum numbers (n,l,m,ms). This principle is related to two properties of electrons: All electrons are identical (“when you’ve seen one electron, you’ve seen them all”) and they have half-integral spin (s=1/2). Sample sets of quantum numbers for the electrons in an atom are given in . Consistent with Pauli’s exclusion principle, no two rows of the table have the exact same set of quantum numbers. Electron States of Atoms n l m ms Subshell symbol No. of electrons: subshell No. of electrons: shell 1 0 0 ½ 1s 2 2 1 0 0 –½ 2 0 0 ½ 2s 2 8 2 0 0 –½ 2 1 –1 ½ 2p 6 2 1 –1 –½ 2 1 0 ½ 2 1 0 –½ 2 1 1 ½ 2 1 1 –½ 3 0 0 ½ 3s 2 18 3 0 0 –½ 3 1 –1 ½ 3p 6 3 1 –1 –½ 3 1 0 ½ 3 1 0 –½ 3 1 1 ½ 3 1 1 –½ 3 2 –2 ½ 3d 10 3 2 –2 –½ 3 2 –1 ½ 3 2 –1 –½ 3 2 0 ½ 3 2 0 –½ 3 2 1 ½ 3 2 1 –½ 3 2 2 ½ 3 2 2 –½
Because of Pauli’s exclusion principle, no two electrons in an atom have the same set of four quantum numbers.
Electrons with the same principal quantum number n are said to be in the same shell, and those that have the same value of l are said to occupy the same subshell. An electron in the n=1 state of a hydrogen atom is denoted 1s, where the first digit indicates the shell (n=1) and the letter indicates the subshell (s,p,d,f…correspond tol=0,1,2,3…). Two electrons in the n=1 state are denoted as 1s2, where the superscript indicates the number of electrons. An electron in the n=2 state with l=1 is denoted 2p. The combination of two electrons in the n=2 and l=0 state, and three electrons in the n=2 and l=1 state is written as 2s22p3, and so on. This representation of the electron state is called the electron configuration of the atom. The electron configurations for several atoms are given in . Electrons in the outer shell of an atom are called valence electrons. Chemical bonding between atoms in a molecule are explained by the transfer and sharing of valence electrons. Electron Configurations of Electrons in an Atom Element Electron Configuration Spin Alignment H 1s1 (↑) He 1s2 (↑↓) Li 1s22s1 (↑) Be 1s22s2 (↑↓) B 1s22s22p1 (↑↓)(↑) C 1s22s22p2 (↑↓)(↑)(↑) N 1s22s22p3 (↑↓)(↑)(↑)(↑) O 1s22s22p4 (↑↓)(↑↓)(↑)(↑) F 1s22s22p5 (↑↓)(↑↓)(↑↓)(↑) Ne 1s22s22p6 (↑↓)(↑↓)(↑↓)(↑↓) Na 1s22s22p63s1 (↑) Mg 1s22s22p63s2 (↑↓) Al 1s22s22p63s23p1 (↑↓)(↑)
The symbol (↑) indicates an unpaired electron in the outer shell, whereas the symbol (↑↓) indicates a pair of spin-up and -down electrons in an outer shell.
The maximum number of electrons in a subshell depends on the value of the angular momentum quantum number, l. For a given a value l, there are 2l+1 orbital angular momentum states. However, each of these states can be filled by two electrons (spin up and down, ↑↓). Thus, the maximum number of electrons in a subshell is In the 2s (l=0) subshell, the maximum number of electrons is 2. In the 2p (l=1) subshell, the maximum number of electrons is 6. Therefore, the total maximum number of electrons in the n=2 shell (including both the l=0 and 1 subshells) is 2+6 or 8. In general, the maximum number of electrons in the nth shell is 2n2. Subshells and Totals for <m:math><m:mrow><m:mi>n</m:mi><m:mo>=</m:mo><m:mn>3</m:mn></m:mrow></m:math> How many subshells are in the n=3 shell? Identify each subshell and calculate the maximum number of electrons that will fill each. Show that the maximum number of electrons that fill an atom is 2n2. Strategy Subshells are determined by the value of l; thus, we first determine which values of l are allowed, and then we apply the equation “maximum number of electrons that can be in a subshell =2(2l+1)” to find the number of electrons in each subshell. Solution Because n=3, we know that l can be 0, 1, or 2; thus, there are three possible subshells. In standard notation, they are labeled the 3s, 3p, and 3d subshells. We have already seen that two electrons can be in an s state, and six in a p state, but let us use the equation “maximum number of electrons that can be in a subshell =2(2l+1)” to calculate the maximum number in each: The equation “maximum number of electrons that can be in a shell =2n2” gives the maximum number in the n=3 shell to be Significance The total number of electrons in the three possible subshells is thus the same as the formula 2n2. In standard (spectroscopic) notation, a filled n=3 shell is denoted as 3s23p63d10. Shells do not fill in a simple manner. Before the n=3 shell is completely filled, for example, we begin to find electrons in the n=4 shell. The structure of the periodic table () can be understood in terms of shells and subshells, and, ultimately, the total energy, orbital angular momentum, and spin of the electrons in the atom. A detailed discussion of the periodic table is left to a chemistry course—we sketch only its basic features here. In this discussion, we assume that the atoms are electrically neutral; that is, they have the same number of electrons and protons. (Recall that the total number of protons in an atomic nucleus is called the atomic number, Z.) First, the periodic table is arranged into columns and rows. The table is read left to right and top to bottom in the order of increasing atomic number Z. Atoms that belong to the same column or chemical group share many of the same chemical properties. For example, the Li and Na atoms (in the first column) bond to other atoms in a similar way. The first row of the table corresponds to the 1s (l=0) shell of an atom. Consider the hypothetical procedure of adding electrons, one by one, to an atom. For hydrogen (H) (upper left), the 1s shell is filled with either a spin up or down electron (↑or↓). This lone electron is easily shared with other atoms, so hydrogen is chemically active. For helium (He) (upper right), the 1s shell is filled with both a spin up and a spin down (↑↓) electron. This “fills” the 1s shell, so a helium atom tends not to share electrons with other atoms. The helium atom is said to be chemically inactive, inert, or noble; likewise, helium gas is said to be an inert gas or noble gas. Build an atom by adding and subtracting protons, neutrons, and electrons. How does the element, charge, and mass change? Engage the Phet simulation below to explore the answers to these questions.