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CIE IGCSE Physics (extended)

Topic 5: Nuclear physics

Isotopes, ions, fission and fusion

Study guideThe atomAlpha particle scattering experimentIsotopes, ions, fission and fusionDetection of radioactivityThe three types of nuclear emissionRadioactive decayApplicationsHalf-lifeSafety precautions

Introduction

Understanding the composition and characteristics of an atom is fundamental to the study of physics. In this section, we will explore how atoms can change by forming ions and isotopes, or through processes such as nuclear fission and fusion.

Isotopes

Isotopes are atoms of the same element that have different numbers of neutrons but the same number of protons. This means they have different nucleon numbers (A) but the same proton number (Z).

For example:

  • Carbon-12 has 6 protons and 6 neutrons.

  • Carbon-14 has 6 protons and 8 neutrons.

Despite having different mass numbers, both are still carbon because they have the same number of protons.

Isotopes of an element often have similar chemical properties but different physical properties, such as different levels of radioactivity.

Ions

Atoms can gain or lose electrons to form ions, which are charged particles:

  1. Positive Ion:

    • Formed when an atom loses electrons.

    • The atom becomes positively charged because it has more protons than electrons.

  2. Negative Ion:

    • Formed when an atom gains electrons.

    • The atom becomes negatively charged because it has more electrons than protons.

Nuclear fission and fusion

Nuclear fission and nuclear fusion are processes that involve changes in an atom's nucleus and are crucial for energy production.

  • Nuclear Fission:

    • This is the splitting of a large nucleus into smaller nuclei.

    • Fission releases a significant amount of energy and is the process used in nuclear reactors.

    • An example of fission is when a uranium-235 nucleus absorbs a neutron and splits into two smaller nuclei, releasing energy and more neutrons.

  • Nuclear Fusion:

    • This is the joining of two small nuclei to form a larger nucleus.

    • Fusion releases even more energy than fission and is the process that powers the Sun.

    • In the Sun, hydrogen nuclei fuse to form helium, releasing massive amounts of energy.

Both processes involve changes in mass and energy, as described by Einstein's equation E=mc2. This means that a small amount of mass is converted into a large amount of energy.

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