On the extension of Newton's second law to theories of gravitation in curved space-time

dc.creatorArminjon, Mayeul
dc.date2006-09-14
dc.date.accessioned2026-07-07T07:24:01Z
dc.date.available2026-07-07T07:24:01Z
dc.descriptionWe investigate the possibility of extending Newton's second law to the general framework of theories in which special relativity is locally valid, and in which gravitation changes the flat Galilean space-time metric into a curved metric. This framework is first recalled, underlining the possibility to uniquely define a space metric and a local time in any given reference frame, hence to define velocity and momentum in terms of the local space and time standards. It is shown that a unique consistent definition can be given for the derivative of a vector (the momentum) along a trajectory. Then the possible form of the gravitation force is investigated. It is shown that, if the motion of free particles has to follow space-time geodesics, then the expression for the gravity acceleration is determined uniquely. It depends on the variation of the metric with space and time, and it involves the velocity of the particle.
dc.description32 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/0609051
dc.identifierhttp://arxiv.org/abs/gr-qc/0609051
dc.identifierArch.Mech. 48 (1996) 551-576
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/116196
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleOn the extension of Newton's second law to theories of gravitation in curved space-time
dc.typetext

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