Chapter 8: Electrons in Atoms Electromagnetic Radiation • Electromagnetic (EM) radiation is a form of energy transmission propagated as waves moving through space. o We will use a simple model of the wave as a disturbance in the propagating medium An EM wave is generated by accelerating a charged particle, such as an e− Electromagnetic Radiation • A wave is characterized by its: o Wavelength (lambda, λ, in m) is the distance between two adjacent crests on a wave. o Frequency (nu, ν, in s−1) is the number of wavelengths passing a point in one second. o Amplitude is the maximum displacement of the wave. o Speed is how fast the wave travels or propagates in the medium. – 1 • EM radiation in vacuo propagates at a constant speed of c, where c = λν = 3.00 × 108 m s−1, the ‘speed of light.’ • EM radiation spans a wide range of frequencies & wavelengths Practice: An FM radio station broadcasts on a frequency of 91.5 MHz. What is the wavelength of these radio waves in meters? 2 • A property of EM waves is that their amplitudes are “additive.” o Treating amplitudes as signed quantities (+/−), when waves are added the resulting amplitude can increase or decrease. – When waves are in phase, the amplitude increases; this is constructive interference – When waves are out of phase, the amplitude decreases; this is destructive interference • White light contains all the colors of the rainbow; we can see these colors in two ways o Reflect the light off a grooved surface; interference in the reflected light (diffraction) is observed as colorful patterns. o Refract the light by passing it through a prism; the different colored components travel at different speeds in glass and are bent at different angles producing a rainbow spectrum. Atomic Spectra • Light generated by a gas discharge tube or heating salts in a flame consists of a limited number of wavelengths or colors. • Diffracting this light produces an atomic line spectrum. o The line spectrum is the element’s ‘fingerprint.’ 3 • Balmer deduced a formula for the frequencies of the lines observed in the atomic spectrum of hydrogen 𝜈line = 3.2881 × 1015 � 1 1 −1 − �s 22 𝑛 2 4 for 𝑛 = 3,4,5, ⋯ Quantum Theory • As the 19th century came to a close, physicists observed phenomena that could not be explained by classical physics. • Over the course of 30 years, a new theory was developed. o At the heart of this was the proposal that energy is not continuous, but rather is discrete in nature, that is quantized. We will survey some of the people involved. • Max Planck explained the puzzle of “black body radiation” by proposing that radiant heat energy is emitted only in definite amounts called quanta. • We use Planck's result in an equation that shows the energy of electromagnetic radiation is proportional to frequency 𝐸 = ℎ𝜈 where ℎ = 6.626 × 10−34 J s = Planck ' s constant • h (Planck's constant) symbolizes the new quantum physics 5 • When light strikes the surface of a metal in vacuo, an electron may be ejected; this is called the photoelectric effect. • Researchers noted that the energy of the ejected electron did not depend on the intensity of the light but rather on the frequency of the light. • Albert Einstein realized Planck's idea of light appearing as quanta (bundles or photons) was the key to understanding this mystery. Einstein’s explanation is recognized as the first scientific work utilizing quantum theory. • Chemical reactions induced by photons (packets or “particles”) of light are called photoreactions (photochemistry). The Bohr Atom • Niels Bohr (1913) was the first to apply the quantum theory to atomic structure. The most impressive result of the so-called Bohr theory was the way it predicted the spectral lines of atomic hydrogen. 6 • Bohr theory predicted the radii of the stable orbits allowed by quantum theory 𝑟𝑛 = 𝑛2 𝑎0 where 𝑛 = 1,2,3, ⋯ and 𝑎0 = 53 pm and also the energy of an electron in an orbit −𝑅𝐻 −2.179 × 10−18 J 𝐸𝑛 = 2 = 𝑛2 𝑛 where 𝑅𝐻 = 2.179 × 10−18 J • By constructing an energy-level diagram and calculating the energies between orbits, Bohr explained the line spectrum of H 7 Is it likely that one of the electron orbits in the Bohr atom has a radius of 1.00 nm? Is there an energy level for the hydrogen atom, En = −2.69 x 10-20 J? 8 • This model of electrons constrained to move in quantized orbits around a central nucleus was called the Bohr Atom (viz H atom) o Ground state occurs when the electron occupies the orbit with the lowest energy (n = 1); closest to the nucleus. o Excited state occurs when the electron occupies a higher energy orbit with unfilled orbit(s) between itself and the nucleus. • Electron movement between orbits involves energy. This energy can absorbed or released as EM radiation (E = hν). 9 • In the Bohr atom, The energy difference between initial and final energy levels ni and nf is given by −𝑅𝐻 −𝑅𝐻 1 1 1 1 ∆𝐸 = 𝐸f − 𝐸i = � 2 � − � 2 � = 𝑅𝐻 � 2 − 2 � = 2.179 × 10−18 � 2 − 2 � J 𝑛f 𝑛i 𝑛i 𝑛f 𝑛i 𝑛f ∆E > 0 if energy is absorbed (electron excitation) ∆E < 0 if energy is released (electron relaxation) • The energy of the photon either absorbed or emitted is given by (and given ∆E, this allows us to determine the EM frequency) |∆𝐸 | = 𝐸 = ℎ𝜈 Determine the wavelength of light absorbed in an electron transition from n=2 to n=4 in a hydrogen atom. 10 • The Ionization Energy of a hydrogen atom is the energy needed to remove an electron from the atom (ni = 1, nf = ∞). ∆𝐸 = 𝐸f − 𝐸i = 𝑅𝐻 � 1 1 − � = 𝑅𝐻 = 2.179 × 10−18 J 2 2 1 ∞ o This works for any ‘atom’ with one electron, such as He+ or Li2+ by introducing nuclear charge into the equation. The energy of an orbit in such an atom is −𝑧 2 𝑅𝐻 𝐸𝑛 = 𝑛2 where z = atomic number = nuclear charge = # of protons For n = 2 in Hg79+ 𝐸2 = −�802 �𝑅𝐻 4 o The Bohr atom was a revolutionary application of the new quantum theory, but the model only worked for ‘atoms’ with one electron! It did not work for multielectron atoms. o More complex systems needed further refinements to quantum theory 11 Two Ideas Leading to a New Quantum Mechanics • Louis de Broglie posited: If light waves can exhibit particle-like properties (photons), then perhaps particles (electrons) can exhibit wave-like behavior. • The wavelength associated with these “matter waves” is 𝜆= ℎ ℎ = 𝑝 𝑚𝑚 Practice: Assuming Superman has a mass of 91 kg, what is the wavelength associated with him if he is traveling at one-fifth the speed of light? 12 • Werner Heisenberg established that there is a limit to how precisely we can measure the position of a particle (x) and the momentum of that particle (p) simultaneously. The Heisenberg Uncertainty Principle is deep! There is an inherent limit to the precision of a measurement. ℎ ∆𝑥 ∆𝑝 = (∆position)(∆momentum) ≥ 4𝜋 Heisenberg is out for a drive when he's stopped by a traffic cop. The cop says, "Do you know how fast you were going?“ Heisenberg says, Wave Mechanics • All of these new concepts culminated in the formulation of the ‘Wave Mechanics,’ the laws for the motion of electrons in atoms. • A standing wave is a wave motion that reflects back on itself in such a way that the wave contains a certain number of points (nodes) that undergo no motion. • Erwin Schrödinger proposed that an electron’s matter wave could be described by a wave function corresponding to a standing wave (ψ or psi). • The simplest model that shows how ψ relates to the energy levels of an electron is the one-dimensional ‘particle in a box.’ 13 o This model gives quantized energies for ψ. o Note how the wave function changes signs at the nodes 𝑛𝑛𝑥 2 𝜓𝑛 (𝑥 ) = � sin � � 𝐿 𝐿 where n = 1,2,3,… • By applying de Broglie’s relationship (λ=h/p) to the kinetic energy of the particle in the box, we obtain this expression for the kinetic energy of an electron in ψn: 𝑛2 ℎ 2 𝐾𝐾𝑛 = where 𝑛 = 1,2,3, ⋯ 8𝑚 𝐿2 o Note that the kinetic energy is never 0 since n≥1 – The lowest possible energy when n=1 is the zero-point energy. – This is consistent with the Heisenberg Uncertainty Principle because zero KE would violate ∆x ∆p ≥ h/4π. 14 • The most compact form of the Schrödinger equation is Eψ = Hψ. • Schrödinger did not provide physical interpretation for ψ, but Max Born did: ψ2 is the probability of finding an electron at some point in space. • Wave function solutions to the Schrödinger equation are called orbitals (‘like an orbit’) to distinguish them from Bohr’s ‘orbits.’ • We will not go into further mathematics of the Schrödinger Equation except to point out that the solutions yield three quantum numbers that specify a particular orbital; we will look at these quantum numbers, allowed values, and their meaning. 15 Quantum Numbers and Electron Orbitals • Here are the 3 quantum numbers from Schrödinger Equation o n = the principal quantum number – Allowed values: n = 1, 2, 3, 4, … – Meaning: The distance of the orbital from the nucleus – Alternate names: All orbitals with the same value of n are in the same shell or principal electronic shell or principal energy level – Relationship to PT: The period number = n – In electron configuration: leading number (2p) o l = orbital angular momentum quantum number – Allowed values: l = 0, 1, 2, 3, … , n−1 (if n=3, l =0,1,2) – Meaning: The shape of the orbital – Alternate names: All orbitals with the same values of n and l are in the same subshell or sublevel – Relationship to PT: Sets of group numbers = l (for example, groups 1-2 l = 0) – In electron configuration: the letter; to wit l =0 = s, l = 1 = p, l = 2 =d, l=3=f (after this, it’s alphabetical!) o ml = magnetic quantum number – Allowed values: ml = −l, −l+1,…, 0,…, l−1, +l (example: for l = 2 or 5d, ml = −2, −1, 0, +1, +2) – Meaning: The orientation of the orbital in 3 dimensions – Alternate names: This is the true “orbital” occupied by electrons; examples are px, py, pz – Relationship to PT: No permanent association, but we can say that an orbital spans two groups – In electron configuration: no designation, but they do show up as the short line segments in an energy level diagram 16 17 The Fourth and Last Quantum Number! • The fourth quantum number was provided by Wolfgang Pauli to explain how two electrons could occupy the same space (i.e. orbital) at the same time. ms=magnetic spin QN • The Pauli Exclusion Principle: two electrons can occupy the same orbital only if they have opposite spins (↑ or ↓). Corollary: No two electrons in an atom can have the same four quantum numbers (Quantum Numbers = n, l, ml, ms). 18 Summary of the 4 Quantum Numbers • n = the principal quantum number (shell) o n = 1, 2, 3, 4, … o Distance of the orbital from the nucleus • l = orbital angular momentum quantum number (subshell) o l = 0, 1, 2, 3, … , n−1 o Shape of the orbital; l=0=s, l=1=p, l=2=d, l=3=f • ml = magnetic quantum number o ml = −l, −l+1, …, 0, …, l−1, +l o Orientation of the orbital in 3D • ms = electron spin quantum number o ms = +½, −½ (also denoted by ↑ and ↓) 19 Degenerate and Non-Degenerate Orbitals • Degenerate orbitals all have the same energy. • In a hydrogen atom all orbitals in a shell (principal energy level) are degenerate. • In a multi-electron atom orbitals within a subshell are degenerate, but subshells with a shell are not degenerate. Interactions between electrons remove degeneracy. 20 Electron Configurations • We use the energy ordering of shells and subshells, and the number of orbitals per subshell to write electron configurations o The electronic configuration of an atom or ion lists orbitals that are occupied (i.e. have electrons in them) • Subshells are occupied in the following order 1s 2s 2p 3s 3p 4s 3d 4p 5s 4d 5p 6s 4f 5d 6p 7s 5f 6d 7p • How do we remember this? The Periodic Table! 21 • Subshells have these maximum occupancies: 1s2 2s2 2p6 3s2 3p6 4s2 3d10 4p6 5s2 4d10 5p6 6s2 4f14 5d10 6p6 7s2 5f14 6d10 7p6 • Let’s look at some guiding principles for filling orbitals: o Aufbau principle: ‘building up’ principle; electrons occupy the lowest energy orbitals first; this yields the ground state configuration. o Hund’s Rule: when degenerate orbitals (within a subshell) are being filled, the electrons occupy the orbitals singly first, all with the same spin, before pairing up. o Pauli exclusion principle: an orbital can hold at most two electrons; electrons in same orbital must have opposite spins. • GS electron configurations can be written a few different ways: spdf notation (condensed) spdf notation (expanded) orbital diagram Noble gas shorthand You can mix and match these! 22 Identify the element having the electron configuration 1s2 2s2 2p6 3s2 3p6 4s2 3d2 Use spdf condensed notation to show the electron configuration of iodine. How many electrons does the iodine atom have in its 3d subshell? How many unpaired electrons are in an iodine atom? 1s 2s 2p 3s 3p 4s 3d 4p 5s 4d 5p 6s 4f Represent electron configuration of iron with an orbital diagram __ 1s __ 2s __ __ __ 2p __ 3s __ __ __ 3p __ 4s __ __ __ __ __ 3d Represent the electron configuration of bismuth with an orbital diagram; use the Noble gas shorthand __ 6s __ __ __ __ __ __ __ 4f __ __ __ __ __ 5d __ __ __ 6p Practice: For an atom of Sn, indicate the number of (a) electron shells that are either filled or partially filled; (b) 3p electrons; (c) 5d electrons; and (d) unpaired e− 1s 2s 2p 3s 3p 4s 3d 4p 5s 4d 5p 6s 4f 5d 6p For home practice, look at the ‘Concept Assessment’ on page 323. 23 • We have a few concepts left to consider o Valence electrons are those electrons in the highest numbered shell and any unfilled d or f subshells. (Only valence electrons are involved in chemical bonding and reactions.) o Core electrons are those electrons that are not valence electrons! Electrons in filled shells that may have empty d or f subshells. (Core electrons are too tightly held to get involved in chemical bonding or reactions.) o Penetration refers to the fact that the radial probabilities of subshells interpenetrate; this explains the following. (See also pictures below.) o The 4s subshell fills before the 3d because the 4s subshell penetrates inside the 3d subshell. An electron fills the 4s subshell first because it will be closer to the nucleus and have lower energy (Aufbau principle). o Shielding (screening) means that core electrons ‘shield’ valence electrons from the attraction of the full nuclear charge (more in chapter 9). o Electron configurations of Cr and Cu and the stability of halffilled subshells. 24 In multielectron atoms, the 3s electrons penetrate most deeply into the inner orbitals, are least shielded, and experience the greatest effective nuclear charge. The 3d electrons penetrate least. This accounts for the energy ordering of the sublevels: d>p>s. 25 Assessing electron configurations 26
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