Charged and radially excited boson stars (in Anti-de Sitter)

Belgium); B. Hartmann (University College London; Brazil); F. Console (University of S\~ao Paulo; UK); Y. Brihaye (University of Mons

REVIEW

Charged and radially excited boson stars (in Anti-de Sitter)

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 2209.07978 v1 pith:J2TCJRTF submitted 2022-09-16 gr-qc hep-thmath-phmath.MP

Y. Brihaye (University of Mons , Belgium) , F. Console (University of São Paulo , Brazil) , B. Hartmann (University College London , UK) This is my paper · ORCID

classification gr-qchep-thmath-phmath.MP

keywords asymptoticallyanti-debosonexcitedradiallysitterspace-timestars

verification ladder T0 review T1 audit T2 compute T3 formal

0 comments

read the original abstract

We study charged and radially excited boson stars in both asymptotically flat as well as asymptotically Anti-de Sitter space-time. We demonstrate that two different types of radially excited solutions exist~: one that persists in the linear limit of small scalar fields, in which analytical arguments suggest the existence of these solutions, and one that appears only in the highly non-linear regime of the model. We also demonstrate that the formation of wavy scalar hair discussed previously for black holes and boson stars in asymptotically flat space-time persists for asymptotically Anti-de Sitter space-time.

Discussion (0). Continue with ORCID to comment.

Pith tools