Bondi mass with a cosmological constant

TL;DR

This paper demonstrates that the Bondi mass can be generalized to include a cosmological constant without correction, ensuring positive energy loss for gravitational waves, especially in the quadrupole case, and clarifies previous proposals.

Contribution

It shows that the Bondi mass with a cosmological constant can be taken as the usual Bondi mass without correction, simplifying the understanding of energy loss in such spacetimes.

Findings

The generalized Bondi mass $M_ ext{Lambda}$ equals the usual $M_B$ for any $ ext{Lambda}$.

Energy carried away by quadrupole gravitational waves is positive-definite for $ ext{Lambda}>0$.

Higher multipole moments preserve positivity under certain weakness conditions.

Abstract

The mass loss of an isolated gravitating system due to energy carried away by gravitational waves with a cosmological constant $\Lambda\in\R$ was recently worked out, using the Newman-Penrose-Unti approach. In that same article, an expression for the Bondi mass of the isolated system, $M_\Lambda$, for the $\Lambda>0$ case was proposed. The stipulated mass $M_\Lambda$ would ensure that in the absence of any incoming gravitational radiation from elsewhere, the emitted gravitational waves must carry away a positive-definite energy. That suggested quantity however, introduced a $\Lambda$-correction term to the Bondi mass $M_B$ (where $M_B$ is the usual Bondi mass for asymptotically flat spacetimes) which would involve not just information on the state of the system at that moment, but ostensibly also its past history. In this paper, we derive the identical mass-loss equation using an integral formula on a hypersurface formulated by Frauendiener based on the Nester-Witten identity, and argue that one may adopt a generalisation of the Bondi mass with $\Lambda\in\R$ \emph{without any correction}, viz. $M_\Lambda=M_B$ for any $\Lambda\in\R$. Furthermore with $M_\Lambda=M_B$, we show that for \emph{purely quadrupole gravitational waves} given off by the isolated system (i.e. when the "Bondi news" $\sigma^o$ comprises only the $l=2$ components of the "spherical harmonics with spin-weight 2"), the energy carried away is \emph{manifestly positive-definite} for the $\Lambda>0$ case. For a general $\sigma^o$ having higher multipole moments, this perspicuous property in the $\Lambda>0$ case still holds if those $l>2$ contributions are weak --- more precisely, if they satisfy any of the inequalities given in this paper.