Pith. sign in

REVIEW 2 cited by

Compact Objects in Entangled Relativity

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2011.14629 v1 pith:5EEVNBHB submitted 2020-11-30 gr-qc

Denis Arruga , Olivier Rousselle , Olivier Minazzoli This is my paper · ORCID
classification gr-qc
keywords relativitycompactdensityentangledgivenobjectscentralgeneral
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
abstract

We describe the first numerical Tolman-Oppenheimer-Volkoff solutions of compact objects in entangled relativity, which is an alternative to the framework of general relativity that does not have any additional free parameter. Assuming a simple polytropic equation of state and the conservation of the rest-mass density, we notably show that, for any given density, compact objects are always heavier (up to $\sim 8\%$) in entangled relativity than in general relativity -- for any given central density within the usual range of neutron stars' central densities, or for a given radius of the resulting compact object.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Lagrangian Identity and Mass Evolution of Particle-like Objects in Nonminimally Coupled Gravity

    gr-qc 2026-03 conditional novelty 6.0 of 10

    Nambu-Goto p-branes satisfy L_[p]=T_[p]/(p+1), so their rest mass scales as f2^{-p/(p+1)} under nonminimal matter-geometry coupling in FLRW cosmologies.

  2. Numerical evaluation of the exact post-Newtonian parameters in Brans-Dicke and entangled relativity theories

    gr-qc 2026-02 conditional novelty 6.0 of 10

    First numerical evaluation of the exact strong-field post-Newtonian parameters in Brans–Dicke and Entangled Relativity: neutron-star deviations up to ~46% from standard values, and dipolar gravitational-wave predictio...

Pith tools