We gratefully acknowledge support from
the Simons Foundation and member institutions.
Full-text links:

Download:

Current browse context:

astro-ph.HE

Change to browse by:

References & Citations

Bookmark

(what is this?)
CiteULike logo BibSonomy logo Mendeley logo del.icio.us logo Digg logo Reddit logo

Astrophysics > High Energy Astrophysical Phenomena

Title: Observed Trends in FRB Population and Bi-modality in the Luminosity Density Distribution

Abstract: We have considered both non-CHIME and CHIME FRBs in the present study. Our robust conclusion is that there are two categories of non-CHIME FRBs - high luminosity density and low luminosity density events, with majority of the repeaters falling in the latter category. In order to circumvent the non-availability of measured fluence and flux density of the CHIME FRBs, we have devised a novel dimensionless approach that utilizes the ratio of the estimated CHIME lower limits to the fluence as well as to the flux density to investigate the presence of trends and patterns in both non-CHIME as well as CHIME FRB population. We have introduced several physically meaningful dimensionless quantities, and one of the robust results is that the computed values of these are almost same for both CHIME and non-CHIME events. This universality is also seen in the distributions of the computed dimensionless quantities and the underlying trends. In the case of CHIME repeaters, distributions of few of the dimensionless quantities hint at the existence of two modes of repeating radio transients.
Comments: Submitted to EPL
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE); General Relativity and Quantum Cosmology (gr-qc)
Cite as: arXiv:2310.11992 [astro-ph.HE]
  (or arXiv:2310.11992v1 [astro-ph.HE] for this version)

Submission history

From: Patrick Das Gupta [view email]
[v1] Wed, 18 Oct 2023 14:23:29 GMT (2087kb,D)
[v2] Sun, 21 Apr 2024 07:14:31 GMT (1525kb,D)

Link back to: arXiv, form interface, contact.