Lemaitre model and cosmic mass

Valerio Faraoni (Bishop's University)

Lemaitre model and cosmic mass

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 1506.06358 v1 pith:GCMZLYLW submitted 2015-06-21 gr-qc

Valerio Faraoni (Bishop's University) This is my paper

classification gr-qc

keywords currentenergylemaitremassambiguitiescahillclarifyingconserved

verification ladder T0 review T1 audit T2 compute T3 formal

0 comments

read the original abstract

The mass of a sphere of simmetry in the Lemaitre universe is discussed using the Hawking-Hayward quasi-local energy and clarifying existing ambiguities. A covariantly conserved current introduced by Cahill and McVittie is shown to be a multiple of the Kodama energy current.

Discussion (0). Sign in to comment.

Forward citations

Cited by 1 Pith paper

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

Gravitational Bounce from the Quantum Exclusion Principle
gr-qc 2025-05 reject novelty 5.0 of 10

A closed collapsing fluid ball with a hypothetical maximum density bounces into exponential expansion, which the authors equate with inflation and dark energy, predicting a small negative curvature.

Pith tools