Mougiakakos Stavros, Vanhove Pierre
<a href="https://ror.org/058rvd314">Laboratoire Univers et Théories</a>, Observatoire de Paris, Université PSL, Université Paris Cité, CNRS, F-92190 Meudon, France.
<a href="https://ror.org/00bbtde36">Institut de Physique Théorique</a>, Université Paris-Saclay, CEA, CNRS, F-91191 Gif-sur-Yvette Cedex, France.
Phys Rev Lett. 2024 Sep 13;133(11):111601. doi: 10.1103/PhysRevLett.133.111601.
We apply a formulation of Einstein's general relativity with only cubic interactions for deriving the metric of a Schwarzschild black hole to all orders in perturbation theory. This cubic interactions formulation coupled to effective worldline action of a massive point particle allows to derive a recursion relation for the form factors of the off-shell graviton emission current. The unique solution to the recursion relation leads to the Schwarzschild black-hole solution in four dimensions. This provides the first derivation of the black hole metric from a matter source to all orders in perturbation theory from an amplitude approach.
我们应用一种仅具有三次相互作用的爱因斯坦广义相对论公式,以便在微扰理论中推导史瓦西黑洞度规至所有阶次。这种与大质量点粒子的有效世界线作用耦合的三次相互作用公式,使得能够推导壳外引力子发射流形状因子的递推关系。该递推关系的唯一解导致了四维的史瓦西黑洞解。这从振幅方法出发,首次在微扰理论中从物质源推导黑洞度规至所有阶次。