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    This article describes a scientific and mathematical term. For other meanings see half-life (disambiguation).The half-life of a quantity subject to exponential decay is the time required for the quantity to decay to half of its initial value. The concept originated in the study of radioactive decay, but applies to many other fields as well, including phenomena which are described by non-exponential decays.



    The table at right shows the reduction of the quantity in terms of the number of half-lives elapsed.

    It can be shown that, for exponential decay, the half-life t_ obeys this relation:
    t_ = rac

    where
      lambda is the decay constant, a positive constant used to describe the rate of exponential decay.

    The half-life is related to the mean lifetime τ by the following relation:
    t_ = ln (2) cdot au



        Half-life
            Examples
            Decay by two or more processes
            Derivation
            Validation
            See also

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    Examples


    The generalized constant lambda can represent many different specific physical quantities, depending on what process is being described.

      In an RC circuit or RL circuit, lambda is the reciprocal of the circuit's time constant au (the symbol is the same as the mean lifetime, noted above; the two quantities happen to be equal). For simple RC and RL circuits, lambda equals RC or L/R, respectively.
      In biology (specifically pharmacokinetics), from MeSH: Half-Life: The time it takes for a substance (drug, radioactive nuclide, or other) to lose half of its pharmacologic, physiologic, or radiologic activity. Year introduced: 1974 (1971).

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    Decay by two or more processes
    Some quantities decay by two processes simultaneously (see Exponential decay#Decay by two or more processes). In a fashion similar to the previous section, we can calculate the new total half-life T_ and we'll find it to be:

    T_ = rac ,


    or, in terms of the two half-lives

    T_ = rac ,


    where t _1 is the half-life of the first process, and t _2 is the half life of the second process.

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    Derivation
    Quantities that are subject to exponential decay are commonly denoted by the symbol N. (This convention suggests a decaying number of discrete items. This interpretation is valid in many, but not all, cases of exponential decay.) If the quantity is denoted by the symbol N, the value of N at a time t is given by the formula:

    N(t) = N_0 e^ ,


    where N_0 is the initial value of N (at t = 0)

    When t = 0, the exponential is equal to 1, and N(t) is equal to N_0. As t approaches infinity, the exponential approaches zero. In particular, there is a time t_ , such that

    N(t_) = N_0cdot rac.


    Substituting into the formula above, we have

    N_0cdot rac = N_0 e^, ,


    e^ = rac, ,


    - lambda t_ = ln rac = - ln, ,


    t_ = rac. ,


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    Validation
    The half-life of a process can be determined easily by experiment. In fact, some methods do not require advance knowledge of the law governing the decay rate, be it exponential decay or another pattern.

    Most appropriate to validate the concept of half-life for radioactive decay, in particular when dealing with a small number of atoms, is to perform experiments and correct computer simulations. See in * how to test the behavior of the last atoms. Validation of physics-math models consists in comparing the model's behavior with experimental observations of real physical systems or valid simulations (physical and/or computer). The references given here describe how to test the validity of the exponential formula for small number of atoms with simple simulations, experiments, and computer code.

    In radioactive decay, the exponential model does not apply for a small number of atoms (or a small number of atoms is not within the domain of validity of the formula or equation or table). The DIY experiments use pennies or M&M's candies. *, *. A similar experiment is performed with isotopes of a very short half-life, for example, see Fig 5 in *. See how to write a computer program that simulates radioactive decay including the required randomness in * and experience the behavior of the last atoms. Of particular note, atoms undergo radioactive decay in whole units, and so after enough half-lives the remaining original quantity becomes an actual zero rather than asymptotically approaching zero as with continuous systems.

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    See also

      For non-exponential decays, see half-life in the article Rate equation
     

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    This article is licensed under the GNU Free Documentation License [copyleft]. It uses material from the Wikipedia article "Half-life". link