Easy lessons in Einstein : $b A discussion of the more intelligible features of the theory of relativitySlosson, Edwin E. (Edwin Emery)
Science
Easy lessons in Einstein : $b A discussion of the more intelligible features of the theory of relativity
Slosson, Edwin E. (Edwin Emery)
Einstein, Albert, 1879-1955; Relativity (Physics)
3. The shifting of spectral lines toward the red end of the spectrum
in the case of light coming to us from stars of appreciable mass (not
yet confirmed).
The great attraction of the theory is its logical consistency. If
any deduction from it should prove untenable, it must be given up. A
modification of it seems impossible without destruction of the whole.
No one must think that Newton’s great creation can be overthrown in
any real sense by this or by any other theory. His clear and wide
ideas will forever retain their significance as the foundation on
which our modern conceptions of physics have been built.
A final comment. The description of me and my circumstances in _The
Times_ shows an amusing feat of imagination on the part of the
writer. By an application of the theory of relativity to the taste of
readers, today in Germany I am called a German man of science, and in
England I am represented as a Swiss Jew. If I come to be regarded as
a _bête noire_, the descriptions will be reversed, and I shall
become a Swiss Jew for the Germans and a German man of science for the
English!
FOOTNOTES:
[Footnote 1: Bergson: “Time and Free Will,” p. 221.]
[Footnote 2: Bergson in his “Laughter” traces all humor back to this
fundamental absurdity of making a man act mechanically.]
[Footnote 3: “We can thus say that all these paradoxical phenomena (or
rather negations of phenomena) which have been enumerated above can
only happen after the end or before the beginning of eternity” (De
Sitter).]
[Footnote 4: If you insist upon seeing just what is the difference
between Einstein’s and Newton’s laws of gravitation here it is as given
in _The Scientific Monthly_ of January, 1920:
Any particle or light pulse moves so that the integral of _ds_
between the two points of its path (in four dimensions) is stationary
where
(according to Einstein)
_ds^{2}_ = -(1 - 2_m_/_r_)^{-1}_dr^{2}_-_r^{2}_ _d θ^{2}_ + (1 - 2_m_/_r_)_dt_
or (according to Newton)
_ds^{2}_ = _dr^{2}_ - _r^{2}_ _d θ^{2}_ + (1 - 2_m_/_r_)_dt_
These expressions are in polar coördinates for a particle of
gravitational mass _m_.
The new factor introduced by Einstein is, as shown above,
1/{1-(2_m_/_r_)}
]
[Footnote 5: _Nineteenth Century_, December, 1919.]
[Footnote 6: Quoted by Eddington in _Contemporary Review_,
December, 1919.]
[Footnote 7: Sir Joseph Thomson in _Nature_, December 4, 1919.]
And finally
IF YOU WANT TO READ MORE ABOUT THE EINSTEIN THEORIES
_For the non-mathematical reader_:
ABBOTT, EDWIN.
Flatland, by A Square. Boston, 1891.
An amusing way of leading up to the fourth dimension.
CAMPBELL, NORMAN.
The Commonsense of Relativity. _Philosophical Magazine_,
April, 1911.
CARR, WILDON.
The Metaphysical Implications of the Theory of Relativity.
_Philosophical Review_, Jan., 1915.
CARUS, PAUL.
Public-domain text, read in full here on John Shaqi.
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