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1 Chapter 6 Electronic Structure of Atoms Table of Contents 6.1. The Wave Nature of Light 6.2. Quantized Energy and Photons 6.3. Line Spectra and the Bohr Model 6.4. The Wave Behavior of Matter 6.5. Many-Electron Atoms 6.6. Electron Configurations 6.7. Electron Configurations and the Periodic Table Spring 2018
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Page 1: Electronic Structure of Atoms - Al Akhawayn Universityaui.ma/.../Files/Chap6_CHE1401_Spring2018.pdf · Electronic Structure of Atoms Table of Contents 6.1. The Wave Nature of Light

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Chapter 6 Electronic Structure

of Atoms

Table of Contents

6.1. The Wave Nature of Light

6.2. Quantized Energy and Photons

6.3. Line Spectra and the Bohr Model

6.4. The Wave Behavior of Matter

6.5. Many-Electron Atoms

6.6. Electron Configurations

6.7. Electron Configurations and thePeriodic Table

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Aim Describe the development of the quantum theory and

how it led to a consistent description of the electronic

structure of the elements.

Quantum theory:

Branch of physics which deals with physical phenomena at

microscopic scales.

Quantum theory is the theoretical basis of modern physics

that explains the nature and behavior of matter and energy

on the atomic and subatomic level.

It provides a mathematical description of much of the

behavior and interactions of energy and matter.

The Wave Nature of Light

The electronic structure of an atom refers to the arrangement of electrons.

Interaction of light (electromagnetic radiation) with matter has provided us with a lot of information about the electronic structure of atoms.

Visible light is a form of electromagnetic radiation, or radiant energy.

Radiation carries energy through space.

Electromagnetic radiation is characterized by its wave nature

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All waves have a characteristic wavelength,

l(lambda), amplitude, A and frequency n.

The speed of a wave is given by its

frequency (hertz) multiplied by its

wavelength.

For light, speed is c = n l

Electromagnetic radiation moves through a vacuum

with a speed of 3.00 x 108 m/s.

Modern atomic theory arose out of studies of

the interaction of radiation with matter.

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The electromagnetic spectrum is a display

of the various types of electromagnetic

radiation arranged in order of increasing

wavelength.

Example: visible radiation has wavelengths

between 400 nm (violet) and 750 nm (red).

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Hot Objects and the Quantization of

Energy

Heated solids emit radiation (blackbody

radiation)

The wavelength distribution depends on

the temperature (i.e., “red hot” objects are

cooler than “blue hot” objects).

Temp. Light emitted

Blue

Infra Red

Red

Orange

Yellow

Infra Red Night Vision

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Temp. Light emitted

Blue

Infra Red

Red

Orange

Yellow

Quantized Energy and Photons

Planck investigated black body radiation.

He proposed that energy can only be

absorbed or released from atoms in

certain amounts called quanta.

A quantum is the smallest amount of

energy that can be emitted or absorbed

as electromagnetic radiation.

The energy of a single quantum:

E =hn where h = 6.626×10-34 J.s (Planck’s constant)

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The photoelectric effect

Phenomenon explained by Albert Einstein (Nobel prize, 1921)

The photoelectric effect

If light shines on a metal surface, there is a point at

which electrons are ejected from the metal

(photoelectric effect).

The electrons will only be ejected if the light source has

sufficient energy:

Below the threshold frequency no electrons are ejected.

Above the threshold frequency, the excess energy appears

as the kinetic energy of the ejected electrons.

Light has wave-like AND particle-like

properties

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Einstein assumed that light traveled in

energy packets called photons.

The energy of one photon:

E =hn

Line Spectra and Bohr Model

Radiation composed of only one

wavelength is called monochromatic.

Radiation that spans a whole array of

different wavelengths is called continuous.

When radiation from a light source, such

as a light bulb, is separated into its

different wavelength components, a

spectrum is produced.

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Continuous Spectrum

White light can be separated into a continuous spectrum of colors.

A rainbow is a continuous spectrum of light produced by the

dispersal of sunlight by raindrops

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Line Spectra

Line Spectra Of Na and H

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Bohr’s Model

Bohr noted the line spectra of certain

elements and assumed the electrons

were confined to specific energy states.

These were called orbits.

Bohr’s Model

Bohr’s model is based on three postulates:

1. Only orbits of specific radii, corresponding to certain definite energies, are permitted for electrons in an atom.

2. An electron in a permitted orbit has a specific energy and is in an "allowed" energy state.

3. Energy is only emitted or absorbed by an electron as it moves from one allowed energy state to another.

(The energy is gained or lost as a photon).

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Energy States of the Hydrogen Atom

Colors from excited gases arise because

electrons move between energy states in the

atom.

Since the energy states are quantized, the

light emitted from excited atoms must be

quantized and appear as line spectra.

Energy States of the Hydrogen Atom

2

18

2H

1)1018.2(

1)(

nJx

nhcRE

Bohr showed mathematically that:

The product hcRH = 2.18 x 10-18 J

n is called the principal quantum number

The first orbit in the Bohr model has n = 1 and is closest to the

nucleus. This is the most stable state and is called ground state.

The second, third …. orbit in the Bohr model has n=2, 3, 4,5…

(excited states)

As n gets infinite the energy gets closer to zero. (electron is

removed from the nucleus). h: Planck’s constant 6.626 x 10-34 J-s

c: speed of light 3 x 108 m/s

RH : Rydberg constant 1.096776 x 107 m-1

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Energy Level in Hydrogen Atom

Energy states in Hydrogen Atom

Balmer: discovered that the lines in the visible

line spectrum of hydrogen fit a simple equation.

22

18

if

111018.2ν

if nnJxhEEE

If nf is smaller than ni, the electron moves closer to the nucleus,

and E is negative. The atom releases energy.

-

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Limitations of the Bohr Model

The Bohr Model has several limitations:

It cannot explain the spectra of atoms other than hydrogen.

Electrons do not move about the nucleus in circular orbits.

However, the model introduces two important ideas:

The energy of an electron is quantized: electrons exist only in certain energy levels described by quantum numbers.

Energy gain or loss is involved in moving an electron from one energy level to another.

The Wave Behavior of Matter

Knowing that light has a particle nature, it seems

reasonable to ask whether matter has a wave

nature.

This question was answered by Louis deBroglie.

Using Einstein’s and Planck’s equations,

deBroglie derived:

The momentum, mv, is a particle property,

whereas l is a wave property

nl

m

h

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Matter waves

Matter waves is the term used to describe wave

characteristics of material particles.

Therefore, in one equation deBroglie

summarized the concepts of waves and particles

as they apply to low-mass, high-speed objects.

applications: X-ray diffraction, electron microscopy

The Uncertainty Principle

Heisenberg’s uncertainty principle:

we cannot determine the exact position,

direction of motion, and speed of

subatomic particles simultaneously.

Heisenberg: For electrons: we cannot

determine their momentum and position

simultaneously: x x mn > h/4p

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Quantum Mechanics and Atomic Orbitals

Schrödinger proposed an equation containing both wave and particle terms.

Solving the equation leads to wave functions

The wave function describes the electron’s matter wave.

The square of the wave function, 2, gives the probability of finding the electron.

That is, 2 gives the electron density for the atom.

2 is called the probability density.

Electron density

A region of high electron density is one

where there is a high probability of finding

an electron.

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Quantum Numbers

Schrödinger’s equation requires three

quantum numbers:

1.Principal quantum number, n. This is the

same as Bohr’s n.

As n becomes larger, the atom becomes

larger and the electron is further from the

nucleus.

Quantum Numbers

2. Second quantum number, l. This

quantum number depends on the value of

n.

The values of l begin at 0 and increase to

n – 1.

We usually use letters for l (s, p, d and f for l

= 0, 1, 2, and 3).

This quantum number defines the shape of

the orbital. also named “azimuthal” or “angular momentum” quantum number

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Quantum Numbers

3.Magnetic quantum number, ml.

This quantum number depends on l.

The magnetic quantum number has integer

values between –l and +l.

Magnetic quantum numbers give the three-

dimensional orientation of each orbital.

A collection of orbitals with the same value

of n is called an electron shell.

A set of orbitals with the same n and l is

called a subshell.

Each subshell is designated by a number

and a letter.

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Possible Values of quantum Numbers

Representations of Orbitals

All s orbitals are spherical.

As n increases, the s orbitals get larger.

As n increases, the number of nodes increases.

A node is a region in space where the probability

of finding an electron is zero.2 = 0 at a node.

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Representation of S Orbital

The p Orbitals

There are three p orbitals: px, py and pz.

The three p orbitals lie along the x-, y-, and z-

axes of a Cartesian system.

The letters correspond to the allowed values of

ml ( –1, 0, and +1).

The orbitals are dumbbell shaped; each has two

lobes.

As n increases, the p orbitals get larger.

All p orbitals have a node at the nucleus.

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The p Orbitals

The d Orbitals

There are five d orbitals

Three of the d orbitals lie in a plane

bisecting the x-, y-, and z-axes.

Two of the d orbitals lie in a plane aligned

along the x-, y-, and z-axes.

Four of the d orbitals have four lobes

each.

One d orbital has two lobes and a collar.

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The d Orbitals

F orbitals

When n is equal to 4 or larger, there are seven f

orbitals for which l=3.

The shape of f orbitals are very complicated than

those of d orbitals

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Many-Electron Atoms

Orbitals and Their Energies

In a many-electron atom, for a given value

of n, the energy of an orbital increases

with increasing value of l (2s and 2p).

Orbitals of the same energy are said to be

degenerate.

Ordering of Orbital energy levels

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Electron Spin

Line spectra of many-electron atoms show each line as a closely spaced pair of lines.

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Magnetic Quantum Number

Electron is a tiny sphere spinning around its

own axis.

Electron spin is said to be quantized

ms = spin magnetic quantum number = ± ½.

Pauli’s Exclusion Principle

Pauli’s exclusion principle states that no

two electrons in the same orbital can have

the same set of four quantum numbers.

Therefore, two electrons in the same orbital

must have opposite spins.

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Electron Configurations

Electron configurations tell us how the

electrons are distributed among the

various orbitals of an atom.

The most stable configuration, or ground

state, is that in which the electrons are in

the lowest possible energy state.

When writing ground-state electronic

configurations:

electrons fill orbitals in order of increasing

energy with no more than two electrons per

orbital.

no two electrons can fill one orbital with the

same spin (Pauli).

for degenerate orbitals, electrons fill each

orbital singly before any orbital gets a

second electron (Hund’s rule).

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How do we show spin?

An arrow pointing upwards has ms = + ½

(spin up).

An arrow pointing downwards has ms = – ½

(spin down).

Hund's Rule

for degenerate orbitals, the lowest energy

is attained when the number of electrons

with the same spin is maximized. Thus,

electrons fill each orbital singly with their

spins parallel before any orbital gets a

second electron.

By placing electrons in different orbitals,

electron-electron repulsions are

minimized.

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Summary For Quantum Mechanical

Model For The Atom

Every electron in an atom has a probability

region in which it resides.

Probability region is described by wave

function and a wave equation

Solving the wave equation produces four

Quantum Numbers.

The complete set of four Quantum Numbers

most adequately describes the physical

features of the probability region.

Principle Quantum Number (n)

n the energy level of orbitals.

Allowable values of n = 1,2,3,4....

Maximum number of electrons in a

given shell is 2n2

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Azimuthal Quantum Number (l)

It defines the shape of the orbital

Allowable values- l = 0,1,2.....n-1

l=0 called an "S" region. It can have a maximum of 2 electrons assigned to it, and is shaped spherical

l=1 called a "P" region. It can have a maximum of 6 electrons assigned to it, and is shaped double lobed (two spheres tangent to one another.

l=2 called a “d" region. It can have a maximum of 10 electrons assigned to it, and is shaped as an quadra-lobed region.

l=3 called an “f" region. It can have a maximum of 14 electrons assigned to it, and is shaped as an octa lobed region.

Magnetic Quantum Number (ml)

It defines the direction the region

extends to

Allowable values for ml = -l< ml <+l

What values of "m" are possible for a

probability region that is partially

described by an l=3 value?

ml = -3, -2, -1, 0, +1, +2, +3

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Spin Quantum Number (s)

It defines the direction of spin electron

particle may have

Allowable values- +1/2 or -1/2

Pauli Exclusion Principle

No two electrons can have the same

exact set of quantum numbers (ie:

electrons must have paired spins in the

same orbital)

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Hund’s Rule

For degenerate orbitals, the lowest

energy is attained when the number of

electrons with the same spin is

maximized.

Octet Rule

The most stable atoms are those whose

valence outermost regions have eight

electrons. Exceptions are Hydrogen

and Helium atoms which have 1 and 2

respectively)

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Assigning Electronic Configuration of

a given atom

The following sequence is used:

1s,2s,2p,3s,3p,4s,3d,4p,5s,4d,5p,6s,4f, 5d,

6p,7s,5f,6d.....

You begin with the first orbital, 1s, and

add electrons until the maximum

number for that orbital is reached,

Assigning Electronic Configuration of

a given atom

1s

2s 2p

3s 3p

4s 3d 4p

5s 4d 5p

6s 4f 5d 6p

7s 5f 6d 7p

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Klechkowski’s rule

Madelung’s rule

“n+l rule”

Energy ordering rule

Electron Configuration of Lighter

Elements

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Condensed Electron Configurations

Electron configurations may be written

using a shorthand notation (condensed

electron configuration):

Condensed Electron Configurations

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Transition Metals

After Ar the d orbitals begin to fill.

After the 3d orbitals are full the 4p orbitals

begin to fill.

The ten elements between Sc and Zn are

called the transition metals, or transition

elements.

Transition Metals

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Lanthanide and Actinide Elements

The 15 elements corresponding to the

filling of 4f orbitals are called lanthanide

elements (or rare earth elements).

The 15 elements corresponding to the

filling of 5f orbitals are called actinide

elements.

Most actinides are not found in nature

(they are synthesized).

Electron Configurations and the Periodic

Table

The periodic table can be used as a guide

for electron configurations.

The period number is the value of n.

Groups 1A and 2A have their s orbitals

being filled.

Groups 3A – 8A have their p orbitals being

filled.

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The s-block and p-block of the periodic table contain the representative, or main-group, elements.

Transition metals have their d orbitals being filled.

The lanthanides and actinides have their f orbitals being filled.

The actinides and lanthanide elements are collectively referred to as the f-block metals.

Note that the 3d orbitals fill after the 4s orbital. Similarly, the 4f orbitals fill after the 5d orbitals.

Electron Configuration of lanthanide

La [Xe] 6s2 5d1 4f 0

Lu [Xe] 6s2 5d1 4f 14

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Anomalous Electron Configurations

There are many elements that appear to

violate the electron configuration guidelines.

Examples:

Chromium is [Ar]3d54s1 instead of [Ar]3d44s2.

Copper is [Ar]3d104s1 instead of [Ar]3d94s2.

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