Foreword |
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vii | |
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Preliminary notions of Kinematics. Translations, proper rotations SO(3), Galilei group transformations |
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1 | (6) |
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Preliminary notions of Analytical Dynamics. Newton's Equations. |
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7 | (3) |
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Constraints. Work. The Principle of Least Action. Euler-Lagrange Equations |
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10 | (6) |
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14 | (2) |
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Poincare Lemma and its converse |
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16 | (6) |
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Linear partial differential equations. The method of characteristics |
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19 | (3) |
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The Inverse Variational Problem. Helmholtz's Conditions |
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22 | (22) |
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33 | (6) |
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The matrix σ. Tr σα is conserved quantity |
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39 | (5) |
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Instructive example of Cislo |
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44 | (8) |
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Instructive example of Douglas |
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50 | (1) |
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Instructive example of Pardo |
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51 | (1) |
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Construction of an autonomous one-particle Lagrange function in (3+1) space-time dimensions yielding rotationally covariant Euler-Lagrange Equations coinciding with the Newton Equations. |
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52 | (18) |
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Canonical variables. Equivalence problem of the Lagrange functions |
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66 | (4) |
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All Lagrange functions, s-equivalent to the Lagrange function L = 1/2x2 -- U (|x|), in (3+1) space-time dimensions |
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70 | (43) |
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The case U (|x|) ≠ αx2 + β, where α, β -- constants |
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75 | (11) |
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The case U (|x|) = αx2 + βW |
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86 | (6) |
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The Hamilton formalism for the model investigated in Subsections 8.1 - 8.3. Equivalence sets of Lagrange functions |
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92 | (5) |
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97 | (16) |
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Example of Henneaux and Shepley |
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98 | (3) |
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101 | (3) |
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104 | (3) |
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107 | (2) |
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109 | (4) |
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The model of Subsections 8.1 - 8.4 for n ≠ 3 |
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113 | (2) |
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All autonomous s-equivalent one-particle Lagrange functions for (1+1) space-time dimensions |
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115 | (7) |
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All s-equivalent one-particle Lagrange functions for (1+1) space-time dimensions |
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120 | (2) |
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Construction of the most general autonomous one-particle Lagrange function in (3+1) space-time dimensions giving rise to rotationally covariant Euler-Lagrange Equations |
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122 | (22) |
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Evaluation of the Function Gij |
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124 | (13) |
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Symmetry of Gij and evaluation of the Lagrange function |
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137 | (4) |
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Symmetry properties of the Lagrange function |
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141 | (3) |
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The largest set of Lagrange functions of one-particle system in a (3+1) dimensional space-time, s-equivalent to a given Lagrange function yielding rotationally forminvariant Equations of Motion (formulation of the problem) |
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144 | (11) |
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Construction of the most general two-particle Lagrange function in (1+1) space-time dimensions giving rise to Euler-Lagrange Equations covariant under Galilei transformation |
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155 | (12) |
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Galilei forminvariance of the Euler-Lagrange Equations for two particles in (1 + 1) space-time dimensions |
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163 | (4) |
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Construction of the most general two-particle Lagrange function in (3+1) space-time dimensions giving rise to Euler-Lagrange Equations covariant under Galilei transformations |
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167 | (13) |
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Galilei forminvariance of the Euler-Lagrange Equations for two particles in (3 + 1) space-time dimensions |
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177 | (3) |
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All two-particle Lagrange functions s-equivalent to a given autonomous Lagrange function yielding Galilei forminvariant Equations of Motion in (1 + 1) space-time dimensions |
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180 | (31) |
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All Euler-Lagrange Equations, forminvariant under the Galilei transformations |
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181 | (17) |
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184 | (8) |
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192 | (6) |
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198 | (6) |
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Generalization of the set of Lagrange functions L (admission of Euler-Lagrange Equations not covariant under Galilei transformations) |
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204 | (4) |
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Case of Galilei forminvariant Newton's Equations corresponding to Euler-Lagrange Equations which are not Galilei covariant (formulation of the problem) |
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208 | (3) |
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An Outlook. Application in the Feynman Approach to Quantum Mechanics |
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211 | (9) |
Index |
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220 | |