physics

Cards (252)

  • Atom
    Positively charged nucleus (which contains neutrons and protons) surrounded by negatively charged electrons
  • Subatomic Particles
    • Proton
    • Neutron
    • Electron
  • Electron
    Relative Mass: 0 (0.0005), Relative Charge: -1
  • Typical radius of an atom: 1 × 10−10 metres
  • Radius of the nucleus is 10 000 times smaller than the atom
  • Most (nearly all) the mass of the atom is concentrated at the nucleus
  • Electron Arrangement

    • Electrons lie at different distances from the nucleus (different energy levels)
    • The electron arrangements may change with the interaction with EM radiation
  • Isotopes
    Atoms of the same element, but with different masses, which have the same number of protons but different number of neutrons
  • Elements
    All atoms of the same element have the same number of protons
  • Neutral Atoms
    Have the same number of electrons and protons
  • Atomic Notation
    𝑍𝑍𝑋𝑋±𝑛𝑛𝐴𝐴 , where X is the letter of the element, A is the mass number, Z is the proton number, and N is the charge
  • Atoms and EM Radiation
    1. When electrons move to a higher orbit (further from the nucleus), the atom has absorbed EM radiation
    2. When the electrons falls to a lower orbit (closer to the nucleus), the atoms has emitted EM radiation
    3. If an electron gains enough energy, it can leave the atom to form a positive ion
  • Dalton said everything was made of tiny spheres (atoms) that could not be divided
  • JJ Thomson discovered the electron
  • Rutherford realised most of the atom was empty space
  • Rutherford Model: Positive nucleus at the centre of the atom, and negative electrons existing in a cloud around the nucleus
  • Bohr produced the final model of the atom
  • Positive charge of nucleus could be subdivided into smaller particles, each with the same amount of charge – the proton
  • James Chadwick provided evidence to prove neutrons existed
  • Radioactive Decay
    Unstable atomic nuclei give out radiation as they change to become more stable. This is a random process.
  • Activity
    The rate at which a source of unstable nuclei decays, measured in Becquerel (Bq)
  • Count-rate
    The number of decays recorded by a detector per second
  • Forms of Radioactive Decay
    • Alpha (α)
    • Beta Minus (β)
    • Gamma (γ)
    • Neutrons
  • Alpha Decay

    • Highly ionising, weakly penetrating (~5cm of air)
  • Beta Decay

    • Medium ionising, medium penetration (~50cm of air, sheet of paper)
  • Gamma Decay

    • Low ionising, highly penetrating (very far in air, few cm of lead)
  • Nuclear Equations
    1. Alpha Decay: 𝑍𝑍𝑋𝑋𝐴𝐴 → 𝑍𝑍−2𝑌𝑌𝐴𝐴−4 + 𝐻𝐻𝑃𝑃24
    2. Beta Decay: 𝑍𝑍𝑋𝑋𝐴𝐴 → 𝑍𝑍+1𝑌𝑌𝐴𝐴 + 𝑃𝑃−10
    3. Gamma Decay: Does not cause the mass or charge to change
  • Half-Life
    The time taken for half the nuclei in a sample to decay or the time taken for the activity or count rate of a sample to decay by half
  • Half-life cannot be predicted when any one nucleus will decay, but it enables the activity of a very large number of nuclei to be predicted during the decay
  • Short Half-Life
    • The source presents less of a risk, as it does not remain strongly radioactive
  • Long Half-Life
    • The source remains weakly radioactive for a long period of time
  • Net Decline
    Calculate the ratio of net decline of radioactive nuclei after X half-lives
  • Contamination
    Radioactive atoms are transferred to an object, lasting for a long period of time
  • Irradiation
    Exposing an object to nuclear radiation, but does not make it radioactive, lasting only for a short period of time
  • Scientific reports on the effects of radiation on humans need to be peer reviewed
  • Background Radiation
    Weak radiation that can be detected from natural / external sources
  • Radiation Dose

    Measured in Sieverts (Sv)
  • Uses of Radioactivity
    • Tracers (e.g. Technetium)
    • Chemotherapy
  • Nuclear Fission
    1. Splitting of a large and unstable nucleus (e.g. uranium or plutonium), releasing energy and neutrons
    2. Spontaneous fission is rare, usually requires absorbing a neutron first
    3. Chain reaction occurs as released neutrons cause further fissions
  • Nuclear Fusion
    Two small nuclei fuse to form a heavier nucleus, releasing energy