Free Powerpoint Presentations

Structure of the Atom
Page
3

DOWNLOAD

PREVIEW

WATCH ALL SLIDES

Electron crashes into the nucleus!?

Physics had reached a turning point in 1900 with Planck’s hypothesis of the quantum behavior of radiation.

Slide 15

The Bohr Model of the Hydrogen Atom

The Bohr Model of the Hydrogen Atom

Bohr’s general assumptions:

1. Stationary states, in which orbiting electrons do not radiate energy, exist in atoms and have well-defined energies, En. Transitions can occur between them, yielding light of energy:

E = En − En’ = hn

2. Classical laws of physics do not apply to transitions between stationary states, but they do apply elsewhere.

3. The angular momentum of the nth state is: where n is called the Principal Quantum Number.

Angular momentum is quantized!

Slide 16

The Bohr Model of the Hydrogen Atom

The Bohr Model of the Hydrogen Atom

4.4:

Bohr’s general assumptions:

“Stationary states” (orbiting electrons do not radiate energy) exist in atoms.

E = E1 − E2 = hf

Classical laws of physics do not apply to transitions between stationary states.

The mean kinetic energy of the electron-nucleus system is K = nhforb/2, where forb is the frequency of rotation. This is equivalent to ask that the angular momentum L=nh/(2p)

Slide 17

Consequences of the Bohr Model

Consequences of the Bohr Model

The angular momentum is:

But:

So:

Solving for rn:

So the velocity is:

where:

a0 is called the Bohr radius. It’s the diameter of the Hydrogen atom (in its lowest-energy, or “ground,” state).

Slide 18

Bohr Radius

Bohr Radius

The diameter of the hydrogen atom for stationary states is

Where the Bohr radius is given by

The smallest diameter of the hydrogen atom is

n = 1 gives its lowest energy state (called the “ground” state)

Slide 19

Emission of light occurs when the atom is in an excited state and decays to a lower energy state (nu → nℓ).

Emission of light occurs when the atom is in an excited state and decays to a lower energy state (nu → nℓ).

where n is the frequency of a photon.

R∞ is the Rydberg constant.

The Hydrogen Atom

The energies of the stationary states where E0 = 13.6 eV.

Slide 20

Transitions in the Hydrogen Atom

Transitions in the Hydrogen Atom

The atom will remain in the excited state for a short time before emitting a photon and returning to a lower stationary state. All hydrogen atoms exist in n = 1 (invisible).

Slide 21

Fine Structure Constant

Fine Structure Constant

The electron’s velocity in the Bohr model:

On the ground state,

v1 = 2.2 × 106 m/s ~ less than 1% of the speed of light.

Go to page:
 1  2  3  4  5 

Contents

Last added presentations

© 2010-2024 powerpoint presentations