Quantum mechanics

Слайд 2

Quantum Physics – introduction Getting ‘into’ the atom

Late in the 19th century, physicists

Quantum Physics – introduction Getting ‘into’ the atom Late in the 19th
explained properties of matter with particle model, light with wave model. Classical physics, which was continuous, had no theoretical limits on size of matter or radiation. Mechanics and electromagnetism together seemed to be enough.
However…

Слайд 3

Black-body radiation remained unexplained

All hot bodies radiate.
The known spectrum did not coincide

Black-body radiation remained unexplained All hot bodies radiate. The known spectrum did
with the theoretical spectrum
Indeed, classical physics violated the law of conservation of energy.

Слайд 4

In 1900, Planck postulated that

All oscillators that emit radiation can only emit

In 1900, Planck postulated that All oscillators that emit radiation can only
discrete energies. That is, radiation comes in packets or quanta (plural of quantum). These quanta are proportional to frequency:
E = hf
where h = 6.63 x 10-34 Js = 4.14 x 10-15 eV-s
h is known as “Planck’s constant”

Слайд 5

Definition


What is one electronvolt?

Definition What is one electronvolt?

Слайд 6

Along comes Albert…

Photoelectric effect

Along comes Albert… Photoelectric effect

Слайд 8

Photoelectric effect

Photoelectric effect

Слайд 9

This equation explained

1) For each metal, there is a threshold frequency below

This equation explained 1) For each metal, there is a threshold frequency
which no electrons are emitted.
2) The number of electrons emitted is proportional to intensity of radiation.
3) Emitted electrons have KE up to a maximum value which depends on frequency of radiation*.
(* unexplained by classical physics)

Слайд 10


For his work on
the photoelectric
Effect, Einstein
was awarded
the Nobel
Prize in 1921

For his work on the photoelectric Effect, Einstein was awarded the Nobel Prize in 1921

Слайд 11

Example 1

a) Find the longest wavelength beyond which no electrons are emitted

Example 1 a) Find the longest wavelength beyond which no electrons are
from a caesium surface if Φcaesium = 1.80 eV.
b) If the surface is illuminated with monochromatic light of wavelength λ = 450 nm, calculate KEmax of emitted photoelectrons.
c) What is the stopping potential which just prevents photoemission in this situation?

Слайд 12

De Broglie equation

During his PhD work, de Broglie proposed that electrons might

De Broglie equation During his PhD work, de Broglie proposed that electrons might behave as waves.
behave as waves.

Слайд 13

Electron diffraction

Using de Broglie equation for electrons accelerated through 1kV gives a

Electron diffraction Using de Broglie equation for electrons accelerated through 1kV gives
wavelength of about _0.0388 nm_.
This is comparable to the wavelength of X-Rays.
Why are electrons easier to use than X-Rays when studying crystalline structures?

Слайд 14

Diffraction patterns due to X-Ray and Electrons passing through aluminium foil

X-ray

Electrons

Diffraction patterns due to X-Ray and Electrons passing through aluminium foil X-ray Electrons

Слайд 15

If all moving objects have an associated wave, why can’t we see

If all moving objects have an associated wave, why can’t we see
the waves associated with buses?

Слайд 16

Wave-particle duality

Sometimes light behaves like a wave, sometimes light behaves like a

Wave-particle duality Sometimes light behaves like a wave, sometimes light behaves like
particle.
Wave-particle duality exists in the universe!
How accurately physical properties can be measured is limited.

Слайд 17

Heisenberg’s uncertainty principle

Heisenberg’s uncertainty principle
Имя файла: Quantum-mechanics.pptx
Количество просмотров: 142
Количество скачиваний: 0