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Born rigidity is a concept in special relativity. It is one answer to the question of what, in special relativity, corresponds to the rigid body of non-relativistic classical mechanics. The concept was introduced by Max Born (1909), who gave a detailed description of the case of constant proper acceleration which he called hyperbolic motion. When subsequent authors such as Paul Ehrenfest (1909) tried to incorporate rotational motions as well, it became clear that Born rigidity is a very restrictive sense of rigidity, leading to the Herglotz–Noether theorem, according to which there are severe restrictions on rotational Born rigid motions. It was formulated by Gustav Herglotz (1909, who classified all forms of rotational motions) and in a less general way by Fritz Noether (1909). As a resul

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  • Bornsche Starrheit (de)
  • Rigidez de Born (es)
  • Born rigidity (en)
  • Rigidité de Born (fr)
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  • Die Bornsche Starrheit ist ein Konzept der speziellen Relativitätstheorie und wurde erstmals 1909 von Max Born vorgeschlagen. Es ist eine der möglichen Antworten auf die Frage, inwieweit das Konzept des starren Körpers, das in der klassischen Mechanik von großer Bedeutung ist, auch im Rahmen der speziellen Relativitätstheorie anwendbar ist. Für einen allgemeinen Überblick zu Beschleunigungen in der Minkowski-Raumzeit, siehe Beschleunigung (Spezielle Relativitätstheorie). (de)
  • Born rigidity is a concept in special relativity. It is one answer to the question of what, in special relativity, corresponds to the rigid body of non-relativistic classical mechanics. The concept was introduced by Max Born (1909), who gave a detailed description of the case of constant proper acceleration which he called hyperbolic motion. When subsequent authors such as Paul Ehrenfest (1909) tried to incorporate rotational motions as well, it became clear that Born rigidity is a very restrictive sense of rigidity, leading to the Herglotz–Noether theorem, according to which there are severe restrictions on rotational Born rigid motions. It was formulated by Gustav Herglotz (1909, who classified all forms of rotational motions) and in a less general way by Fritz Noether (1909). As a resul (en)
  • La rigidez de Born es un concepto de la relatividad especial que trata de generalizar la noción de sólido rígido de la mecánica clásica no relativista. El concepto fue introducido por Max Born (1909),​​ quien dio una descripción detallada del caso de aceleración propia constante que llamó . Cuando autores posteriores como Paul Ehrenfest (1909)​ intentaron incorporar también los movimientos de rotación, quedó claro que la rigidez de Born es un sentido muy restrictivo de la rigidez, lo que condujo al teorema de Herglotz-Noether, según el cual existen severas restricciones para los movimientos rígidos de Born de rotación. Fue formulado por (1909, que clasificó todas las formas de movimientos de rotación)​ y de forma menos general por Fritz Noether (1909).​ Como resultado, Born (1910)​ y otro (es)
  • Le critère de rigidité de Born désigne un concept de relativité restreinte introduit par le physicien allemand Max Born. Ce critère permet de définir un équivalent relativiste du concept de corps rigide utilisé en mécanique classique. (fr)
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