pith. sign in

Sharp bounds on 2m/r of general spherically symmetric static objects

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
abstract

In 1959 Buchdahl \cite{Bu} obtained the inequality $2M/R\leq 8/9$ under the assumptions that the energy density is non-increasing outwards and that the pressure is isotropic. Here $M$ is the ADM mass and $R$ the area radius of the boundary of the static body. The assumptions used to derive the Buchdahl inequality are very restrictive and e.g. neither of them hold in a simple soap bubble. In this work we remove both of these assumptions and consider \textit{any} static solution of the spherically symmetric Einstein equations for which the energy density $\rho\geq 0,$ and the radial- and tangential pressures $p\geq 0$ and $p_T,$ satisfy $p+2p_T\leq\Omega\rho, \Omega>0,$ and we show that $$\sup_{r>0}\frac{2m(r)}{r}\leq \frac{(1+2\Omega)^2-1}{(1+2\Omega)^2},$$ where $m$ is the quasi-local mass, so that in particular $M=m(R).$ We also show that the inequality is sharp. Note that when $\Omega=1$ the original bound by Buchdahl is recovered. The assumptions on the matter model are very general and in particular any model with $p\geq 0$ which satisfies the dominant energy condition satisfies the hypotheses with $\Omega=3.$

citation-role summary

background 1

citation-polarity summary

fields

gr-qc 2

years

2025 1 2019 1

roles

background 1

polarities

background 1

representative citing papers

Buchdahl stars and bounds with cosmological constant

gr-qc · 2025-07-01 · unverdicted · novelty 4.0

Generalized Buchdahl bounds on horizonless object compactness are derived in the presence of a cosmological constant, preserving universality while yielding method-dependent results.

citing papers explorer

Showing 2 of 2 citing papers.

  • Buchdahl stars and bounds with cosmological constant gr-qc · 2025-07-01 · unverdicted · none · ref 3 · internal anchor

    Generalized Buchdahl bounds on horizonless object compactness are derived in the presence of a cosmological constant, preserving universality while yielding method-dependent results.

  • Testing the nature of dark compact objects: a status report gr-qc · 2019-04-10 · accept · none · ref 208

    Current and future observations can test whether dark compact objects are Kerr black holes or exotic alternatives, with null results strengthening the black hole paradigm.