Key Concepts of Nuclear Physics: Important Points to Remember for Class 10 Science

Key Concepts of Nuclear Physics: Important Points to Remember for Class 10 Science

Points to Remember - Nuclear Physics | Science

Nuclear Physics (Science)

Points to Remember

  • This phenomenon of spontaneous emission of radiation from certain elements on its own is called 'natural radioactivity'.
  • Curie is defined as the quantity of a radioactive substance, which undergoes 3.7 × 1010 disintegrations in one second. This is actually close to the activity of 1 g of radium-226.
  • Rutherford (Rd) is defined as the quantity of a radioactive substance which produces 106 disintegrations in one second. 1 Rd = 106 disintegrations per second.
  • The SI unit of radioactivity is becquerel. It is defined as the quantity of one disintegration per second.
  • Helium nucleus (2He4) consisting of two protons and two neutrons is known as alpha particle.
  • Beta particles are electrons (-1e0), which are the basic elementary particles present in all atoms.
  • Gamma rays are electromagnetic waves consisting of photons.
  • A nuclear reaction in which an unstable parent nucleus emits an alpha particle and forms a stable daughter nucleus is called as 'alpha decay'.
  • A nuclear reaction in which an unstable parent nucleus emits a beta particle and forms a stable daughter nucleus is called as 'beta decay'.
  • The process of breaking (splitting) up of a heavier nucleus into two smaller nuclei with the release of a large amount of energy is called 'nuclear fission'.
  • The energy released in a nuclear fission process is about 200 MeV.
  • There are some radioactive elements which can be converted into a fissionable material. They are called as 'fertile materials'. e.g. Uranium-238, Thorium-232, Plutonium-240.
  • Controlled chain reaction is used in a nuclear reactor to produce energy in a sustained and controlled manner.
  • The process in which two lighter nuclei combine to form a heavier nucleus is termed as 'nuclear fusion'.
  • Nuclear fusion or thermonuclear reaction is the source of light and heat energy in the Sun and other stars.
  • The safe limit of receiving the radiation is about 100 mR per week.