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f(R) is a type of modified gravity theory which generalizes Einstein's general relativity. f(R) gravity is actually a family of theories, each one defined by a different function, f, of the Ricci scalar, R. The simplest case is just the function being equal to the scalar; this is general relativity. As a consequence of introducing an arbitrary function, there may be freedom to explain the accelerated expansion and structure formation of the Universe without adding unknown forms of dark energy or dark matter. Some functional forms may be inspired by corrections arising from a quantum theory of gravity. f(R) gravity was first proposed in 1970 by Hans Adolph Buchdahl (although ϕ was used rather than f for the name of the arbitrary function). It has become an active field of research following

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  • F(R) gravity (en)
  • Teoria f(R) (it)
  • F(R)重力 (ja)
  • Teorias f(R) de gravitação (pt)
  • F(R)引力 (zh)
rdfs:comment
  • La teoria f(R) racchiude un insieme di teorie sulla gravitazione ottenute estendendo la relatività generale. La prima versione di queste teorie fu proposta nel 1970 da . Esse sono divenute un importante campo di ricerca a partire dall'opera di Hagen Kleinert e di Brian Schmidt, manifestando una serie di problemi irrisolti. Sono state proposte come possibile spiegazione dell'accelerazione dell'espansione dell'universo indipendente dall'ipotesi dell'energia oscura. (it)
  • f(R)重力（f(R)じゅうりょく）とはアインシュタインの一般相対性理論に補正を加えた重力理論の中の一つである。f(R)重力は、リッチスカラーの函数により定義される一連の理論である。最も単純な場合が、この函数がスカラーに等しいときで、これが一般相対論である。任意の函数を導入するために、暗黒物質やダークエネルギーの存在を加えることなく宇宙の(structure formation)や(accelerated expansion)を説明出来る可能性を持っている。重力の量子論に起源をもつ汎函数形式も考えられている。f(R)重力は1970年に(Hans Adolph Buchdahl)により導入された。 （このときは、φが任意函数の名前で f の代わりで使われていた。） (ja)
  • Teorias f(R) de Gravitação ou teorias f(R) são um tipo de teoria da interação gravitacional que generaliza a teoria da Relatividade Geral. A forma da função f(R), que na formulação Lagrangeana da Relatividade Geral é idêntica ao escalar de Ricci, se torna arbitrária, podendo ser construída de tal maneira a modificar a relação entre geometria e a dinâmica do espaço-tempo. (pt)
  • 引力理论是一种修改引力理论，它是爱因斯坦广义相对论的一种推广。 引力实际上是一系列理论，每个理论都由里奇标量 的不同函数 定义。最简单的情况是，这就对应广义相对论。这一引入任意函数的自由度有可能在不添加未知形式的暗能量或暗物质的情况下解释宇宙的加速膨胀和结构形成。某些函数形式可能受到量子引力理论修正的启发。 引力最早由Hans Adolph Buchdahl于1970年提出（尽管使用的是 而非 表示任意函数）。继Starobinsky对宇宙暴胀的研究之后， 引力成为了一个活跃的研究领域。采用不同的函数可以从这个理论中产生广泛的现象；然而，许多函数形式被观测所排除，或者在理论上是病态的。 (zh)
  • f(R) is a type of modified gravity theory which generalizes Einstein's general relativity. f(R) gravity is actually a family of theories, each one defined by a different function, f, of the Ricci scalar, R. The simplest case is just the function being equal to the scalar; this is general relativity. As a consequence of introducing an arbitrary function, there may be freedom to explain the accelerated expansion and structure formation of the Universe without adding unknown forms of dark energy or dark matter. Some functional forms may be inspired by corrections arising from a quantum theory of gravity. f(R) gravity was first proposed in 1970 by Hans Adolph Buchdahl (although ϕ was used rather than f for the name of the arbitrary function). It has become an active field of research following (en)
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