A History of MechanicsRoutledge, 1955 - 671 стор. |
З цієї книги
Результати 1-3 із 53
Сторінка 491
... Einstein does not hesitate to arrange for the system S ' to be accompanied by clocks which , at each point in space , keep the local time t of the system S ; this in order to demonstrate the fact that the simultaneity he introduces only ...
... Einstein does not hesitate to arrange for the system S ' to be accompanied by clocks which , at each point in space , keep the local time t of the system S ; this in order to demonstrate the fact that the simultaneity he introduces only ...
Сторінка 532
... Einstein's spatially closed universe can be put in the form ds2 = - R2 [ d02 + sin2 0 ( dq2 + sin2 ydw2 ) ] + dt2 ( Einstein , Sitzungsber . , Berlin , 1917 , p . 150 ) . It is also possible to write it in the form x2 + x2 + x2 + x2 R2 ...
... Einstein's spatially closed universe can be put in the form ds2 = - R2 [ d02 + sin2 0 ( dq2 + sin2 ydw2 ) ] + dt2 ( Einstein , Sitzungsber . , Berlin , 1917 , p . 150 ) . It is also possible to write it in the form x2 + x2 + x2 + x2 R2 ...
Сторінка 627
... Einstein and two of his collaborators.1 A physical theory must be both correct and complete . Einstein does not concern himself with the correctness of quantum mechanics— that is , its agreement with experiment . By a " complete theory ...
... Einstein and two of his collaborators.1 A physical theory must be both correct and complete . Einstein does not concern himself with the correctness of quantum mechanics— that is , its agreement with experiment . By a " complete theory ...
Зміст
Nicholas Copernicus 14721543 His system of the world | 5 |
The priority of Herman and Euler in the matter of dAlemberts | 6 |
Transformation of Maxwells equations including convection | 11 |
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Загальні терміни та фрази
acceleration Albert of Saxony Archimedes Aristotle assumed axis Bernoulli Blasius of Parma Carnot centre of gravity classical mechanics concept conservation considered coordinates d'Alembert Daniel Bernoulli deduced Descartes differential direction displacement distance Duhem dynamics Earth Einstein elastic electron energy equal equations equilibrium Euler experiment fall Fermat fluid function Galileo generalised given heavy body Huyghens hypothesis impact impetus inclined plane inertia instant Jean Bernoulli Kepler Lagrange least action Leibniz length Leonardo lever living forces Louis de Broglie mass Maupertuis means moving body natural necessary Newton observation obtained Oresme oscillation particle pendulum physical problem projectile proportional Proposition quantity of motion quantum mechanics ratio relation relative resistance rest Roberval rotation solution space sphere statics supposed surface theory trajectory travelled treatise uniformly variables velocity vertical wave weight XIIIth Century ди ду дх