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The wave nature of matter     221



                                Quantum tunneling is the probability of observing a particle
                                beyond a (non-infinite) potential energy barrier that exceeds the
                                energy of the particle. The effect arises because the amplitude of
                                a wavefunction

                   decreases exponentially within the wavefunction amplitude beyond barrier
                   resulting in non-zero the barrier.
         Related   Quantization of energy and particle-wave   Many-electron atoms (G6)
         topics    duality (G3)
                                                       General features of spectroscopy
                                                       (I1)
                   The structure of the hydrogen atom (G5)




                              Wavefunctions and probabilities

        In the particle-wave duality interpretation of matter and radiation (Topic G3) a particle
        moving in space can also be described as a wave in space with a wavelength related to
        the particle momentum by de Broglie’s equation, λ=h/p. In quantum mechanics, the
        notion of a particle moving in defined trajectories in a system is replaced entirely by this
        description  of  the system in terms of its  wavefunctions,  ψ. The wavefunction
        simultaneously describes all regions of space in which the particle it represents can be
        found. This, in turn, introduces the idea of uncertainty into quantum mechanics because
        the exact position of the particle at each point in time is not defined, only the region of
        space  of  all  its possible positions. The exact  shape of the wavefunction is important
                                                                          2
        because the probability of finding the particle at each point is proportional to ψ  at that
        point; a greater amplitude in  the  wavefunction corresponds to a greater probability
        density in the particle’s distribution.


                                   Schrödinger equation

        The Schrödinger equation is the fundamental equation of quantum mechanics and has
        the general form:
           Hψ i=E iψ i

        Each allowed  wavefunction  ψ 1,  ψ 2,  ψ 3…of a system described by a  Hamiltonian
        operator,  H, is associated with  one  particular  allowed  energy level  E 1,  E 2, E 3… (An
        operator is a mathematical function that represents the action of a physical observable.)
        The Hamiltonian operator is the operator for the total kinetic and potential energy of the
        system. Only an allowed wavefunction of the system, ψ, when operated on by H, returns
        the same wavefunction, multiplied by the associated constant value E. In mathematical
        terminology the Schrödinger equation is an eigenvalue equation; the pairs of E and ψ that
        satisfy the equation are the eigenvalues and eigenfunctions of H, respectively.
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