An operator is a mathematical rule, or set or rules, which transforms one function into another without necessarily specifying any particular function. Mathematically, we define the general operator, , as
Examples of might be (1) multiply by x or (2) take the first derivative with respect to x. In the first case, is simply x and g( x) = xf( x) . In the second case, is d/ dx and g( x) = df( x)/ dx.
Some of the basic rules of operator algebra are as follows:
| (H.1) |
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| (H.2) |
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| (H.3) |
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| (H.4) |
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| (H.5) |
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where C is a constant. The identity operator, , is the operator which leaves the function unchanged; the null operator, , is the operator which yields zero when operating on any function:
| (H.6) |
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| (H.7) |
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Note that, in Eqs. (H.4) and (H.5), we dropped any explicit reference to the function f( x) . This is the usual way of writing the equations of operator algebra.
Most operators encountered in the physical sciences are linear operators. An operator, , is linear if
| (H.8) |
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An example of a nonlinear operator is the square-root execution. In general, the results from two operations do not commute, so that
=
. Hence, if we define the commutator, [ ,
], as
| (H.9) |
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the operators and
can...
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