Schwarzschild-de Sitter Metric and Inertial Beltrami Coordinates

TL;DR

This paper derives a new inertial coordinate form of the Schwarzschild-de Sitter metric within de Sitter general relativity, clarifying the distinction between gravitational and inertial effects in dS spacetime.

Contribution

The paper introduces a new Schwarzschild-de Sitter solution in inertial Beltrami coordinates, separating gravity from inertial effects in de Sitter spacetime.

Findings

New S-BdS metric in inertial coordinates

Clarification of gravity-inertia mixing effects

Potential applications in cosmology and gravitational physics

Abstract

Under consideration of coordinate conditions, we get the Schwarzschild-Beltrami-de Sitter (S-BdS) metric solution of the Einstein field equations with a cosmological constant $\Lambda$. A brief review to the de Sitter invariant special relativity (dS-SR), and de Sitter general relativity (dS-GR, or GR with a $\Lambda$) is presented. The Beltrami metric $B_{\mu\nu}$ provides inertial reference frame for the dS-spacetime. By examining the Schwarzschild-de Sitter (S-dS) metric $g_{\mu\nu}^{(M)}$ existed in literatures since 1918, we find that the existed S-dS metric $g_{\mu\nu}^{(M)}$ describes some mixing effects of gravity and inertial-force, instead of a pure gravity effect arisen from "solar mass" $M$ in dS-GR. In this paper, we solve the vacuum Einstein equation of dS-GR, with the requirement of gravity-free metric $g_{\mu\nu}^{(M)}|_{M\rightarrow 0}=B_{\mu\nu}$. In this way we find S-BdS solution of dS-GR, written in inertial Beltrami coordinates. This is a new form of S-dS metric. Its physical meaning and possible applications are discussed.