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The Universality of Einstein Equations

M. Ferraris, M. Francaviglia, I. Volovich

TL;DR

The paper addresses whether Einstein equations persist as a universal backbone across a wide class of nonlinear gravity theories formulated with a metric and independent connection (Palatini formalism). By examining actions $S(\Gamma,g)=\int_M L(R)\sqrt{g}\,d^nx$ and the universal trace condition $L'(R)R-\frac{n}{2}L(R)=0$, it shows that for $n>2$ the field equations reduce to Einstein dynamics with a cosmological constant $\Lambda= c_i/n$ for real roots $R=c_i$, while in $n=2$ dimensions the system yields a Weyl connection and a constant-curvature constraint; exceptional Lagrangians such as $L(R)=|R|^{n/2}$ and cases with $L'(c_i)=0$ give alternative universal relations. The work provides explicit examples (e.g., $L(R)=aR^2+bR+c$ and $L(R)=R+aR^k$) illustrating bifurcations in the space of Lagrangians and the emergence or modification of Einstein equations, highlighting the role of conformal invariance and degenerate branches. Overall, the results establish a robust link between a broad class of nonlinear Lagrangians and Einstein gravity, with implications for higher-dimensional theories, conformal structures, and potential quantization frameworks.

Abstract

It is shown that for a wide class of analytic Lagrangians which depend only on the scalar curvature of a metric and a connection, the application of the so--called ``Palatini formalism'', i.e., treating the metric and the connection as independent variables, leads to ``universal'' equations. If the dimension $n$ of space--time is greater than two these universal equations are Einstein equations for a generic Lagrangian and are suitably replaced by other universal equations at bifurcation points. We show that bifurcations take place in particular for conformally invariant Lagrangians $L=R^{n/2} \sqrt g$ and prove that their solutions are conformally equivalent to solutions of Einstein equations. For 2--dimensional space--time we find instead that the universal equation is always the equation of constant scalar curvature; the connection in this case is a Weyl connection, containing the Levi--Civita connection of the metric and an additional vectorfield ensuing from conformal invariance. As an example, we investigate in detail some polynomial Lagrangians and discuss their bifurcations.

The Universality of Einstein Equations

TL;DR

The paper addresses whether Einstein equations persist as a universal backbone across a wide class of nonlinear gravity theories formulated with a metric and independent connection (Palatini formalism). By examining actions and the universal trace condition , it shows that for the field equations reduce to Einstein dynamics with a cosmological constant for real roots , while in dimensions the system yields a Weyl connection and a constant-curvature constraint; exceptional Lagrangians such as and cases with give alternative universal relations. The work provides explicit examples (e.g., and ) illustrating bifurcations in the space of Lagrangians and the emergence or modification of Einstein equations, highlighting the role of conformal invariance and degenerate branches. Overall, the results establish a robust link between a broad class of nonlinear Lagrangians and Einstein gravity, with implications for higher-dimensional theories, conformal structures, and potential quantization frameworks.

Abstract

It is shown that for a wide class of analytic Lagrangians which depend only on the scalar curvature of a metric and a connection, the application of the so--called ``Palatini formalism'', i.e., treating the metric and the connection as independent variables, leads to ``universal'' equations. If the dimension of space--time is greater than two these universal equations are Einstein equations for a generic Lagrangian and are suitably replaced by other universal equations at bifurcation points. We show that bifurcations take place in particular for conformally invariant Lagrangians and prove that their solutions are conformally equivalent to solutions of Einstein equations. For 2--dimensional space--time we find instead that the universal equation is always the equation of constant scalar curvature; the connection in this case is a Weyl connection, containing the Levi--Civita connection of the metric and an additional vectorfield ensuing from conformal invariance. As an example, we investigate in detail some polynomial Lagrangians and discuss their bifurcations.

Paper Structure

This paper contains 5 sections, 2 theorems, 52 equations.

Key Result

Proposition 1

(i) If $h_{\mu\nu}$ is a solution of the equation where $R_{\mu\nu}(h)$ is the Ricci tensor of the metric $h_{\mu\nu}$, then the pair $(g,\Gamma)$, where is a solution of eq.s (24) and (25) for any function $\omega$ (here, $\Gamma_{LC}$ is the Levi--Civita connection of $h$). (ii) If $(g,\Gamma)$ is a solution of eq.s (24) and (25), then they have to satisfy the relations where

Theorems & Definitions (2)

  • Proposition 1
  • Theorem 1