The Hayward metric is the simplest description of a black hole which is non-singular. The metric was written down by Sean Hayward as the minimal model which is regular, static, spherically symmetric and asymptotically flat. The metric is not derived from any particular alternative theory of gravity, but provides a framework to test the formation and evaporation of non-singular black holes both within general relativity and beyond. Hayward first published his metric in 2005 and numerous papers have studied it since.
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| - Hayward metric (en)
- Métrica Hayward (pt)
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| - The Hayward metric is the simplest description of a black hole which is non-singular. The metric was written down by Sean Hayward as the minimal model which is regular, static, spherically symmetric and asymptotically flat. The metric is not derived from any particular alternative theory of gravity, but provides a framework to test the formation and evaporation of non-singular black holes both within general relativity and beyond. Hayward first published his metric in 2005 and numerous papers have studied it since. (en)
- A métrica Hayward é a descrição mais simples de um buraco negro que não é singular, um buraco negro regular com carga simétrica esférica. A métrica foi escrita por Sean Hayward como o modelo mínimo que é regular, estático, esfericamente simétrico e assintoticamente plano. Hayward publicou sua métrica pela primeira vez em 2005 e vários artigos a estudaram desde então. (pt)
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| - The Hayward metric is the simplest description of a black hole which is non-singular. The metric was written down by Sean Hayward as the minimal model which is regular, static, spherically symmetric and asymptotically flat. The metric is not derived from any particular alternative theory of gravity, but provides a framework to test the formation and evaporation of non-singular black holes both within general relativity and beyond. Hayward first published his metric in 2005 and numerous papers have studied it since. (en)
- A métrica Hayward é a descrição mais simples de um buraco negro que não é singular, um buraco negro regular com carga simétrica esférica. A métrica foi escrita por Sean Hayward como o modelo mínimo que é regular, estático, esfericamente simétrico e assintoticamente plano. Hayward publicou sua métrica pela primeira vez em 2005 e vários artigos a estudaram desde então. (pt)
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