XKN: a Semi-analytic Framework for the Modelling of Kilonovae
Giacomo Ricigliano, Albino Perego, Ssohrab Borhanian, Eleonora, Loffredo, Kyohei Kawaguchi, Sebastiano Bernuzzi, Lukas Chris Lippold

TL;DR
The paper introduces xkn, a semi-analytic framework for modeling kilonova light curves, incorporating ejecta structure, radiative transfer solutions, and variable physical conditions, to aid in data interpretation and parameter estimation.
Contribution
It presents xkn, a novel semi-analytic model that improves kilonova light curve predictions by including detailed ejecta geometry and radiative transfer solutions.
Findings
xkn-diff significantly outperforms previous semi-analytic models.
The framework accurately reproduces radiative transfer calculations.
xkn is suitable for extensive parameter estimation in kilonova studies.
Abstract
After GW170817, kilonovae have become of great interest for the astronomical, astrophysics and nuclear physics communities, due to their potential in revealing key information on the compact binary merger from which they emerge, such as the fate of the central remnant or the composition of the expelled material. Therefore, the landscape of models employed for their analysis is rapidly evolving, with multiple approaches being used for different purposes. In this paper, we present xkn, a semi-analytic framework which predicts and interprets the bolometric luminosity and the broadband light curves of such transients. xkn models the merger ejecta structure accounting for different ejecta components and non-spherical geometries. In addition to light curve models from the literature based on time scale and random-walk arguments, it implements a new model, xkn-diff, which is grounded on a…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsGamma-ray bursts and supernovae · Astrophysical Phenomena and Observations · Pulsars and Gravitational Waves Research
