Nuclear Physics

    Cards (210)

    • Atom

      The building blocks of all matter, incredibly small with a radius of 1 x 10^-10 m
    • Atom
      • Has a tiny, dense nucleus at the centre, with electrons orbiting around the nucleus
      • The radius of the nucleus is over 10,000 times smaller than the whole atom, but it contains almost all of the mass of the atom
      • Consists of a small dense positively charged nucleus, surrounded by negatively charged electrons
    • An atom is a small positive nucleus, surrounded by negative electrons
    • The atom is around 100,000 times larger than the nucleus
    • Rutherford's Experiment

      Involved the scattering of alpha (α) particles by a sheet of thin metal, which supported the nuclear model of the atom
    • Rutherford's Experiment

      1. A beam of alpha particles (He2+ ions) were directed at a thin gold foil
      2. Most of the alpha particles passed straight through the foil
      3. Some of the alpha particles changed direction but continued through the foil
      4. A few of the alpha particles bounced back off the gold foil
    • The bouncing back of alpha particles could not be explained by the Plum Pudding model, so a new model had to be created
    • Rutherford's experiment was the first evidence of the structure of the atom
    • Ion
      An electrically charged atom or group of atoms formed by the loss or gain of electrons
    • Positive ion

      Formed when atoms lose electrons, resulting in more protons than electrons
    • Negative ion

      Formed when atoms gain electrons, resulting in more electrons than protons
    • A stable atom is normally electrically neutral, with the same number of protons and electrons
    • The term 'net charge' refers to the overall charge of an atom
    • Atom
      Structure made up of a positively charged nucleus at the centre (made up of protons and neutrons) and negatively charged electrons in orbit around the nucleus
    • Protons
      Positively charged particles found in the nucleus of an atom
    • Neutrons
      Particles with no charge found in the nucleus of an atom
    • The nucleus is overall positive due to the positive charge of the protons
    • Proton number (Z)

      The number of protons in an atom, which determines the element
    • The atomic number is always the same for a particular element
    • The atomic number is equal to the number of electrons in a neutral atom
    • Nucleon number (A)

      The total number of protons and neutrons in the nucleus of an atom
    • Calculating the number of neutrons

      Nucleon number - Proton number
    • Electrons have a tiny mass compared to protons and neutrons, so their mass is negligible when considering the mass of the nucleus
    • Isotopes
      Atoms of the same element that have the same number of protons but a different number of neutrons
    • Isotopes tend to be more unstable due to their imbalance of protons and neutrons, making them more likely to decay
    • Hydrogen has three naturally occurring isotopes
    • Deuterium and Tritium are rare isotopes of Hydrogen
    • Nuclear fission
      The splitting of a large, unstable nucleus into two smaller nuclei
    • Isotopes of uranium and plutonium
      • They undergo fission and are used as fuels in nuclear power stations
    • Nuclear fission
      1. Neutron collides with unstable nucleus
      2. Nucleus splits into two smaller nuclei (daughter nuclei)
      3. Two or three neutrons emitted
      4. Gamma rays emitted
    • Large nuclei can decay by fission

      Produces smaller nuclei and neutrons with a lot of kinetic energy
    • Nuclear potential energy

      Converted into kinetic energy in the products of fission
    • The mass of the products (daughter nuclei and neutrons) is less than the mass of the original nucleus
    • The remaining mass has been converted into energy which is released during the fission process
    • Nuclide equation for fission
      • 235U + n → 92Kr + 141Ba + 3n + energy
    • Nuclear fusion

      When two light nuclei join to form a heavier nucleus
    • Nuclear fusion requires extremely high temperatures to maintain
    • Stars use nuclear fusion to produce energy
    • Nuclear fusion

      Two hydrogen nuclei fusing to form a helium nucleus
    • Mass-energy equivalence
      E = m × c^2