Pith. sign in

REVIEW

Gamma-ray flares from black hole coronae

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 1104.2300 v1 pith:D23OXQDT submitted 2011-04-12 astro-ph.HE

Gustavo E. Romero , Florencia L. Vieyro This is my paper
classification astro-ph.HE
keywords blackholeflaresparticlephotonaccountaccretingannihilation
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We present results of a study of non-thermal, time-dependent particle injection in a corona around an accreting black hole. We model the spectral energy distribution of high-energy flares in this scenario. We consider particle interactions with magnetic, photon and matter fields in the black hole magnetosphere. Transport equations are solved for all species of particles and the electromagnetic output is predicted. Photon annihilation is taken into account for the case of systems with early-type donor stars.

Discussion (0). Sign in to comment.

Pith tools