Lesson Notes By Weeks and Term v4 - SHS 3

ATOMIC PHYSICS

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Subject: Physics

Class: SHS 3

Term: 2nd Term

Week: 17

Grade code: 3.4.1.LI.3

Strand code: 4

Sub-strand code: 1

Content standard code: 3.4.1.CS.1

Indicator code: 3.4.1.LI.3

Theme: ATOMIC AND NUCLEAR PHYSICS

Subtheme: ATOMIC PHYSICS

Lesson Video

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Performance objectives

Lesson summary

This lesson delves into the fascinating world of X-rays, a high-energy form of electromagnetic radiation. We will explore how these invisible rays are produced and learn the fundamental relationships that govern their energy, frequency, and wavelength. Understanding X-rays is crucial not only for physics but also for our daily lives in Ghana. From a doctor at the Korle Bu Teaching Hospital diagnosing a bone fracture to a security officer at Kotoka International Airport scanning luggage, the principles we will learn today are applied every day to keep us safe and healthy. This lesson connects concepts of electricity (voltage), energy, and wave mechanics into a single, powerful application.

Lesson notes

2.1 How are X-rays Produced?

X-rays are produced when fast-moving electrons are suddenly stopped or decelerated. This process typically happens inside a device called an X-ray tube.

Here is a step-by-step breakdown of what happens inside an X-ray tube: Thermionic Emission: A filament (cathode) is heated by a low voltage supply. This heat gives the electrons in the filament enough energy to escape from the metal surface. This process is called thermionic emission. Acceleration: A very high potential difference (voltage), often thousands of volts (kilovolts, kV), is applied between the heated filament (cathode, negative) and a metal target (anode, positive). High-Speed Collision: The emitted electrons are strongly attracted to the positive anode and accelerate across the vacuum tube, gaining a large amount of kinetic energy. Deceleration and Energy Conversion: The high-speed electrons violently collide with the dense metal target (often made of tungsten). Upon impact, they are forced to stop or slow down very abruptly. According to the principle of conservation of energy, the kinetic energy lost by the electrons must be converted into other forms. A small amount becomes heat (about 99%), and a tiny but significant fraction (about 1%) is converted into high-energy electromagnetic radiation – X-ray photons. 2.2 The Physics of X-ray Production: Key Formulas

The entire calculation process hinges on one fundamental principle of energy conservation:

Evaluation guide