Nucleosynthesis in the outflows associated with accretion disks of Type II collapsars

TL;DR

This paper explores nucleosynthesis in outflows from accretion disks of Type II collapsars, revealing the synthesis of heavy elements and their potential to produce observable supernovae.

Contribution

It introduces a model for nucleosynthesis in outflows from Type II collapsar disks, identifying new element synthesis and implications for supernova observations.

Findings

Many new elements like titanium, copper, zinc are produced.

56Ni is abundantly synthesized, indicating potential supernova explosions.

Outflows from He-rich zones are rich in 56Ni, while Si-rich zones remain silicon-rich.

Abstract

We investigate nucleosynthesis inside the outflows from gamma-ray burst (GRB) accretion disks formed by the Type II collapsars. In these collapsars, massive stars undergo core collapse to form a proto-neutron star initially and a mild supernova explosion is driven. The supernova ejecta lack momentum and subsequently this newly formed neutron star gets transformed to a stellar mass black hole via massive fallback. The hydrodynamics and the nucleosynthesis in these accretion disks has been studied extensively in the past. Several heavy elements are synthesized in the disk and much of these heavy elements are ejected from the disk via winds and outflows. We study nucleosynthesis in the outflows launched from these disks by using an adiabatic, spherically expanding outflow model, to understand which of these elements thus synthesized in the disk survive in the outflow. While studying this we find that many new elements like isotopes of titanium, copper, zinc etc. are present in the outflows. 56Ni is abundantly synthesized in most of the cases in the outflow which implies that the outflows from these disks in a majority of cases will lead to an observable supernova explosion. It is mainly present when outflow is considered from the He-rich, 56Ni/54Fe rich zones of the disks. However, outflow from the Si-rich zone of the disk remains rich in silicon. Although, emission lines of many of these heavy elements have been observed in the X-ray afterglows of several GRBs by Chandra, BeppoSAX, XMM-Newton etc., Swift seems to have not detected these lines yet.