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Module 1 – Introduction to Atomic Structure

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Evolution of Atomic Theory

1. First clear concept of Atom starts with the Jain School of Thought in 6th Century BC in

India. The Jains considered that matter is made of atoms or “paramanus”. The Jain School also developed an elaborate set of theories on how atoms could combine, move, vibrate, etc.

2. In Western School, the concept of Atom starts in 5th Century BC through Ionian

Philosopher Democritus. The concept of atom was similar to Jain School in the sense that atoms were considered to be fundamental particles that can not be cut or

broken into parts. The word “atom” was coined by him from the Greek adjective “atomos” meaning uncuttable.

3. Atomistic philosophy in Islam was developed around 11th century AD by Imam

Ghazali synthesizing the Jain and Greek Schools of thoughts about Atom. His atomic theory was more in tune with the Jain School rather than of the Greek School.

4. Towards late 18th century scientific developments started renewed philosophical

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Dalton’s Atomic Theory

1. Elements are made of extremely small particles

called atoms.

2. Atoms of a given element are identical in size,

mass, and other properties; atoms of different

elements differ in size, mass, and other

properties.

3. Atoms cannot be subdivided, created, or

destroyed.

4. Atoms of different elements combine in simple

whole-number

ratios

to

form

chemical

compounds.

5. In chemical reactions, atoms are combined,

separated, or rearranged.

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Thomson’s Plum Pudding Model

1. The model was proposed by Thomson in 1904 before the discovery of nucleus.

2. Electrons or “corpuscles” are floating in a soup of positive charge to balance the negative charges. 3. The positive charge was assumed to be like a

“pudding”, and the negatively charged electrons as “plums” and hence the terminology Plum Pudding Model taken from a British dessert.

4. Rutherford-Geiger-Marsden gold foil experiment in 1909 disproved the Plum Pudding Model and showed that instead of a soup of positive charge, an atom consisted of a small nucleus of strong positive charge paving the way to Rutherford’s Atomic Model.

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Rutherford-Geiger-Marsden Experiment

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Rutherford’s Atomic Model

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Limitations of Rutherford’s Model

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Black Body Radiation

A black body is an ideal body which

allows the whole of the incident

radiation to pass into itself ( without

reflecting the energy ) and absorbs

within itself this whole incident

radiation (without passing on the

energy). This propety is valid for

radiation

corresponding

to

all

wavelengths and to all angels of

incidence. Therefore, the black body is

an ideal absorber of incident radaition.

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Basic Laws of Radiation:

1) All objects emit radiant energy.

2) Hotter objects emit more energy than colder

objects (per unit area). The amount of energy

radiated is proportional to the temperature of the

object.

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Ultraviolet (UV) Catastrophe

The Rayleigh-Jeans Law:

* It agrees with experimental

measurements

for

long

wavelengths.

* It predicts an energy output that

diverges

towards

infinity

as

wavelengths grow smaller.

* The failure has become known as

the ultraviolet catastrophe.

4

2

)

,

(

T

ckT

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Planck’s Law of Black Body Radiation

The Planck’s Law of Black Body Radiation states in terms of

wavelength:

1

1

5

2

2

)

,

(

kT

hc

e

hc

T

I

The above equation related intensity of

emission with Temperature and wavelength.

It fits well with experimental observation of

black body radiation.

As opposed to classical model of continuous

energy distribution, energy is emitted in forms of

quantized packets, where h is Planck’s constant

:

c

/

h

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(

m)

1000 100 10 1 0.1 0.01

Earth Sun

Hotter objects emit at

shorter wavelengths.

max

= 3000/T

Hotter objects emit more energy than colder objects

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Applications of Black Body Radiation

Roughly we can say that the stars radiate like

blackbody radiators. This is important because it

means that we can use the theory for blackbody

radiators to infer things about stars like its

effective temperature.

Interesting applications include designing

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Planck-Einstein Relationship

hc

/

h

E

h = Planck’s Constant = 6.626 x 10

-34

joule seconds (J s)

Energy could be gained or lost in individual units or

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Bohr’s Postulates

Bohr’s Atomic Model

1.

In an atom, the electrons revolve around the

nucleus in certain definite circular paths

called orbits, or shells.

2.

Each shell or orbit corresponds to a definite

energy. Therefore, these circular orbits are

also known as energy levels or energy shells.

3.

Electrons in an atom can have only certain

permissible energies .

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Rydberg’s Formula and Bohr’s Theory

Rydberg’s formula is used to explain spectral lines of hydrogen like chemical elements.

Utilizing Bohr’s Postulates, it can be deduced that the energy of a photon emitted by a hydrogen atom is given by the difference of two hydrogen energy levels :

Now in terms of wave-length we have:

Where R is Rydberg’s constant, such that:

R =

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Bohr-Sommerfeld Model

Bohr-Sommerfield Model

Bohr’s model failed in case of

heavier elements where the

spectral lines observed did not

corroborate with the applied

magnetic field. It was found that

spectral lines are not

homogenous but consists of

several convenient lines.

Sommerfield proposed that not

only do electrons travel in certain

orbits but the orbits have

different shapes and the orbits

could tilt in the presence of a

magnetic field. This explained

well the splitting of spectral lines

observed for heavier elements

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Advantages and Disadvantages of Bohr-Sommerfield Model

• Sommerfield’s Model predicted the splits in the spectrum. The electrons moving on the two orbits of the same n number but of different shape have a bit different energies which explained the splitting of spectral lines or very closely spaced spectral lines.

Sommerfield’s Model also showed that

orbits don’t have to lie on the same plane and could tilt in the presence of a magnetic field.

The fundamental flaw was that

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Hydrogen Spectral Series

The Hydrogen Spectral Series can be explained through Rydberg’s formula:

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Balmer Spectral Series

The Balmer series is particularly useful in astronomy

because the Balmer lines appear in numerous stellar

objects due to the abundance of hydrogen in the universe,

and therefore are commonly seen and relatively strong

compared to lines from other elements.

The familiar red H-alpha spectral line of hydrogen gas in

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Particles act like Waves!

p

h

/

De- Broglie’s Matter waves was a brilliant idea.

It proposed:

If light (which is a wave) is quantized (like

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Heisenberg’s Uncertainity Principle

It is impossible to know

both

the position and momentum

exactly, i.e.,

D

x

=0 and

D

p

=0

These uncertainties are inherent in the physical world and

have nothing to do with the skill of the observer

Because

h

is so small, these uncertainties are not

observable in normal everyday situations

4

/

.

p

h

x

D

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Another Consequence of

Heisenberg’s Uncertainty Principle

A quantum particle can never be in a state of rest,

as this would mean we know both its position and

momentum precisely

The more accurately we know the energy of a body,

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Orbitals

Orbitals are regions in space where an electron

is likely to be found:

90% of the time the electron is within the

boundaries described by the electron density map

The exact path of an electron in a given orbital is

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Describing Orbitals

Use quantum numbers to describe orbitals.

A given orbital can be described by a set of 3

quantum numbers:

1. Principal quantum number (n)

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Principal Quantum Number (n)

(

n) describes the size and energy of the orbital:

Possible values: whole number integer

1, 2, 3, …

As “n” increases so does the size and energy of

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Angular momentum quantum number (

l)

(l) is related to the shape of the orbital:

Possible values: (

l)

is an integer between 0 and

n-1

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Angular momentum quantum number (

l)

(

l)

Value

Letter Designation

0

s

1

p

2

d

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n

Possible

l

values

Designation

1

0

1s

2

0

1

2s

2p

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Magnetic quantum number (m

l

)

(m

l

) is related to the orientation of the orbital

in 3-D space:

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Magnetic quantum number (m

l

)

Consider the p orbital…it has an l value of 1

and thus the possible m

l

values are -1, 0, +1

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M

l

and Orbitals

l

m

l

# orbitals

0 (s)

0

1

1 (p)

-1, 0, 1

3

2 (d)

-2, -1, 0, 1, 2

5

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Quantum Number Summary

A set of 3 quantum numbers describes a specific

orbital

Energy and size - n

Shape -

l

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4

th

Quantum Number!

A 4

th

quantum number was added to describe

the spin on a given electron.

Called the electron spin quantum number - m

s
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More on electron spin

Each orbital can hold a maximum of 2

electrons of opposite spin.

Pauli exclusion principle states that no two

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Summary

Three quantum numbers describe a specific

orbital

Energy and size, shape, and orientation

Four quantum numbers describe a specific

electron in an atom

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Stern-Gerlach Experiment

The Stern–Gerlach experiment involves sending a beam of particles through an inhomogeneous magnetic field and observing their deflection. The results show that particles possess an intrinsic angular momentum that is most closely

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Aufbau Principle

The

Aufbau principle

from the German

Aufbau

meaning

"building up, construction":

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Pauli’s Exclusion Principle

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Hund’s Rule

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Schrodinger’s Equation

Schrodinger Equation gives the understanding of Quantum

Mechanics Model:

What did this equation do for knowing more about atomic structure?

1. Schroëdinger's equation eliminated the illogical quantum jump of

electrons from one orbit to another as seen in Bohr’s Model, replacing it with a transitional process in which the wave pattern gradually fades out, while the new wave pattern fades in, during which time radiation is being emitted.

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Particle in a 1-D Box

An electron in a chemical bond is a real time example of a Particle in a 1-D box

How is it so?

Imagine an electron in a C-C single bond. Since carbon atoms are roughly 24000 times more massive than an electron, thinking classically for a moment, this would be like a ball-bearing between two wrecking balls, which would certainly seem like two infinitely high walls. The box length for a C-C single bond would be roughly 1.5 Å giving a defined confined space.

Uses:

1. Particle in a 1-D box model can be used to predict the wavelength of maximum absorbance for highly conjugated organic molecules.

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Applications of Particle in a 1-D Box in Nanotechnology

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A Quantum Harmonic Oscillator

Representing a ball on a spring in a classical

harmonic oscillator, a quantum harmonic

oscillator is applicable for vibrational

motion of a diatomic molecule where, two

atoms are assumed to be attached to a

spring representing the chemical bond.

The energy solution is given by:

The energy of a system described by a harmonic oscillator potential cannot have zero energy . Thus, physical systems such as atoms in a solid lattice or in

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References

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