The evolution of mathematical physics : $b being the Rouse Ball lecture for 1924Lamb, Horace, Sir
History
The evolution of mathematical physics : $b being the Rouse Ball lecture for 1924
Lamb, Horace, Sir
Mathematical physics; Physics -- History
A further feature in the evolution is the gradual recognition of
geometrical or physical meanings in various symbols or groups
of symbols which are of constant recurrence. This is specially
characteristic of the later stages. To Laplace and his school the
potential was simply a convenient mathematical entity; the name
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with its associations came long afterwards from Green. The equation
lost most of its significance when it was
transformed, as was necessary for some purposes, to polar co-ordinates,
and the recognition of the general properties of the function was
delayed. The equation itself first received an explicit interpretation
at the hands of Maxwell, and the same holds with regard to the now
familiar conceptions of ‘divergence,’ ‘concentration,’ and so on.
And it needs hardly to be said that the notion of an operator, as
distinguished from the result, belongs to the later period. The
terminology of physical entities or qualities such as ‘isotropy,’
‘permeability,’ and so on is largely due to Kelvin, with his copious
onomastic faculty.
I have referred mainly to the development of general principles and
methods, but that is, of course, not the whole of the story. A complete
history would have to treat in some detail the special problems which
suggested themselves from time to time. The impulse to general theory
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indeed often came about in this way. For instance, the problem of the
two electrified spheres gave the impulse to Electrostatics, whilst
Chladni’s figures of nodal lines led up by degrees to the theory of
Elasticity. It is, moreover, in the special applications that the skill
of the analyst is particularly evoked, with results often of great
interest and value even from the purely mathematical point of view.
We need not go back to the theory of Attractions, or of the Figure of
the Earth, which evoked Spherical Harmonics. The Conduction of Heat
led incidentally to Bessel Functions, and above all to the theorems
specially associated with the name of Fourier, whilst Poisson’s
problem of the two electrified spheres is a signal instance of the
treatment of a functional equation. To Kelvin we owe the method of
electric inversion, including the astonishing solution of the problem
of the electrified spherical bowl, which had engaged the attention
of Green, and the symmetrical treatment of Spherical Harmonics. To
Maxwell are due the singularly beautiful solution of the problem of
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current sheets, a new interpretation of Spherical Harmonics, and other
interesting results and points of view scattered through his treatise.
As an example of a more systematic application of mathematical
technique we may refer again to Cauchy’s wave-problem, where the
integrals afterwards attributed to Fresnel first make their appearance.
Public-domain text, read in full here on John Shaqi.
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