Pith. sign in

REVIEW 2 cited by

Constraints on massive gravity theory from big bang nucleosynthesis

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 1208.5512 v1 pith:VEGTZG4A submitted 2012-08-27 gr-qc astro-ph.CO

G. Lambiase This is my paper · ORCID
classification gr-qcastro-ph.CO
keywords bangconstraintsgravitymassivenucleosynthesistheoryboundsconsequences
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
read the original abstract

The massive gravity cosmology is studied in the scenario of big bang nucleosynthesis. By making use of current bounds on the deviation from the fractional mass, we derive the constraints on the free parameters of the theory. The cosmological consequences of the model are also discussed in the framework of the PAMELA experiment.

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. Do Pulsar Timing Datasets Favor Massive Gravity?

    astro-ph.CO 2025-07 reject novelty 5.0 of 10

    A one-parameter massive-gravity correlation curve gives lower chi-square than the Hellings-Downs curve for current pulsar-timing data, but the parameter is fitted to the data, so the result is not a prediction.

  2. The new higher-order generalized uncertainty principle and primordial big bang nucleosynthesis

    gr-qc 2024-11 reject novelty 4.0 of 10

    A higher-order GUP is fitted to BBN abundances, but arithmetic errors invalidate the reported parameter bounds.

Pith tools