date: 2018-01-26T08:43:34Z pdf:PDFVersion: 1.5 pdf:docinfo:title: Visualization of Thomas?Wigner Rotations xmp:CreatorTool: LaTeX with hyperref package access_permission:can_print_degraded: true subject: It is well known that a sequence of two non-collinear Lorentz boosts (pure Lorentz transformations) does not correspond to a Lorentz boost, but involves a spatial rotation, the Wigner or Thomas?Wigner rotation. We visualize the interrelation between this rotation and the relativity of distant simultaneity by moving a Born-rigid object on a closed trajectory in several steps of uniform proper acceleration. Born-rigidity implies that the stern of the boosted object accelerates faster than its bow. It is shown that at least five boost steps are required to return the object's center to its starting position, if in each step the center is assumed to accelerate uniformly and for the same proper time duration. With these assumptions, the Thomas?Wigner rotation angle depends on a single parameter only. Furthermore, it is illustrated that accelerated motion implies the formation of a ``frame boundary''. The boundaries associated with the five boosts constitute a natural barrier and ensure the object's finite size. dc:format: application/pdf; version=1.5 pdf:docinfo:creator_tool: LaTeX with hyperref package access_permission:fill_in_form: true pdf:encrypted: false dc:title: Visualization of Thomas?Wigner Rotations modified: 2018-01-26T08:43:34Z cp:subject: It is well known that a sequence of two non-collinear Lorentz boosts (pure Lorentz transformations) does not correspond to a Lorentz boost, but involves a spatial rotation, the Wigner or Thomas?Wigner rotation. We visualize the interrelation between this rotation and the relativity of distant simultaneity by moving a Born-rigid object on a closed trajectory in several steps of uniform proper acceleration. Born-rigidity implies that the stern of the boosted object accelerates faster than its bow. It is shown that at least five boost steps are required to return the object's center to its starting position, if in each step the center is assumed to accelerate uniformly and for the same proper time duration. With these assumptions, the Thomas?Wigner rotation angle depends on a single parameter only. Furthermore, it is illustrated that accelerated motion implies the formation of a ``frame boundary''. The boundaries associated with the five boosts constitute a natural barrier and ensure the object's finite size. pdf:docinfo:subject: It is well known that a sequence of two non-collinear Lorentz boosts (pure Lorentz transformations) does not correspond to a Lorentz boost, but involves a spatial rotation, the Wigner or Thomas?Wigner rotation. We visualize the interrelation between this rotation and the relativity of distant simultaneity by moving a Born-rigid object on a closed trajectory in several steps of uniform proper acceleration. Born-rigidity implies that the stern of the boosted object accelerates faster than its bow. It is shown that at least five boost steps are required to return the object's center to its starting position, if in each step the center is assumed to accelerate uniformly and for the same proper time duration. With these assumptions, the Thomas?Wigner rotation angle depends on a single parameter only. Furthermore, it is illustrated that accelerated motion implies the formation of a ``frame boundary''. The boundaries associated with the five boosts constitute a natural barrier and ensure the object's finite size. pdf:docinfo:creator: Georg Beyerle PTEX.Fullbanner: This is pdfTeX, Version 3.14159265-2.6-1.40.17 (TeX Live 2016/W32TeX) kpathsea version 6.2.2 meta:author: Georg Beyerle trapped: False meta:creation-date: 2017-11-29T12:44:59Z created: Wed Nov 29 13:44:59 CET 2017 access_permission:extract_for_accessibility: true Creation-Date: 2017-11-29T12:44:59Z Author: Georg Beyerle producer: pdfTeX-1.40.17 pdf:docinfo:producer: pdfTeX-1.40.17 dc:description: It is well known that a sequence of two non-collinear Lorentz boosts (pure Lorentz transformations) does not correspond to a Lorentz boost, but involves a spatial rotation, the Wigner or Thomas?Wigner rotation. We visualize the interrelation between this rotation and the relativity of distant simultaneity by moving a Born-rigid object on a closed trajectory in several steps of uniform proper acceleration. Born-rigidity implies that the stern of the boosted object accelerates faster than its bow. It is shown that at least five boost steps are required to return the object's center to its starting position, if in each step the center is assumed to accelerate uniformly and for the same proper time duration. With these assumptions, the Thomas?Wigner rotation angle depends on a single parameter only. Furthermore, it is illustrated that accelerated motion implies the formation of a ``frame boundary''. The boundaries associated with the five boosts constitute a natural barrier and ensure the object's finite size. Keywords: special relativity; Thomas?Wigner rotation; accelerated frame; visualization access_permission:modify_annotations: true dc:creator: Georg Beyerle description: It is well known that a sequence of two non-collinear Lorentz boosts (pure Lorentz transformations) does not correspond to a Lorentz boost, but involves a spatial rotation, the Wigner or Thomas?Wigner rotation. We visualize the interrelation between this rotation and the relativity of distant simultaneity by moving a Born-rigid object on a closed trajectory in several steps of uniform proper acceleration. Born-rigidity implies that the stern of the boosted object accelerates faster than its bow. It is shown that at least five boost steps are required to return the object's center to its starting position, if in each step the center is assumed to accelerate uniformly and for the same proper time duration. With these assumptions, the Thomas?Wigner rotation angle depends on a single parameter only. Furthermore, it is illustrated that accelerated motion implies the formation of a ``frame boundary''. The boundaries associated with the five boosts constitute a natural barrier and ensure the object's finite size. dcterms:created: 2017-11-29T12:44:59Z Last-Modified: 2018-01-26T08:43:34Z dcterms:modified: 2018-01-26T08:43:34Z title: Visualization of Thomas?Wigner Rotations xmpMM:DocumentID: uuid:0c51233e-00ec-4908-b799-445ac5a99628 Last-Save-Date: 2018-01-26T08:43:34Z pdf:docinfo:keywords: special relativity; Thomas?Wigner rotation; accelerated frame; visualization pdf:docinfo:modified: 2018-01-26T08:43:34Z meta:save-date: 2018-01-26T08:43:34Z pdf:docinfo:custom:PTEX.Fullbanner: This is pdfTeX, Version 3.14159265-2.6-1.40.17 (TeX Live 2016/W32TeX) kpathsea version 6.2.2 Content-Type: application/pdf X-Parsed-By: org.apache.tika.parser.DefaultParser creator: Georg Beyerle dc:subject: special relativity; Thomas?Wigner rotation; accelerated frame; visualization access_permission:assemble_document: true xmpTPg:NPages: 19 access_permission:extract_content: true access_permission:can_print: true pdf:docinfo:trapped: False meta:keyword: special relativity; Thomas?Wigner rotation; accelerated frame; visualization access_permission:can_modify: true pdf:docinfo:created: 2017-11-29T12:44:59Z