最終更新日:2025/11/20
(physics) a factor arising frequently in special relativity, to calculate the degree of time dilation, length contraction and relativistic mass of an object moving relative to an observer, defined as (1-v²/c²)-0.5, where v and c are relative velocity and the speed of light, respectively
音声機能が動作しない場合はこちらをご確認ください
正解を見る
Lorentz factor
編集履歴(0)