CORDIS - EU research results
CORDIS

Three-dimensional spectral modelling of astrophysical transients : unravelling the nucleosynthetic content of supernovae and kilonovae

Project description

Research could shed new light on elements created during stellar explosions

Tracing the origin of chemical element formation is one of the most compelling quests in astronomy. Most elements in the periodic table are believed to be produced by supernovae and kilonovae; however, a growing number of new observational data and advanced modelling capabilities enable researchers to experimentally determine nucleosynthesis and the structure of transient materials. The EU-funded SUPERSPEC project aims to trace element origin by studying the spectra of supernovae and kilonovae in the so-called nebular phase, where the inner regions become visible. New spectral synthesis methods that accurately capture the essential microphysical and macrophysical properties will be developed. The project's results will not only help determine cosmic element production but also provide a testing ground for stellar evolution, nucleosynthesis and explosion process theories.

Objective

Determining the origin of the elements is a fundamental quest in physics and astronomy. Most of the elements in the periodic table are believed to be produced by supernovae and kilonovae. However, this has for decades been little more than a prediction from theory. Now, with a dramatically changing observational situation and new modelling capabilities, it is within our reach to determine the nucleosynthesis production and structure in these transients. To really see what supernovae and kilonovae contain, we must study their spectra in the later so called nebular phase when the inner regions become visible. This project is aimed at establishing the first picture of the origin of elements by determining the yields from supernovae and kilonovae using such analysis. To do this, new spectral synthesis methods need to be developed considering the necessary microphysical (ejecta chemistry, r-process physics, time-dependent gas state) and macrophysical (3D radiation transport) processes to obtain sufficient accuracy. These tools will then be applied to the first 3D explosion simulations of these transients now becoming available. When applied to the growing library of data emerging from automated surveys and follow-up programs, as well to the recent first kilonova observations, this will provide a breakthrough in our understanding of these transients. This development will not only allow a determination of cosmic element production, but also allow tests of theories for stellar evolution, nucleosynthesis, and explosion processes. This will in turn have fundamental impact on several fields of astrophysics such as population synthesis, galactic chemical evolution modelling, and understanding of mass transfer in the progenitor systems. It has a strong connection to recent detections of stellar-mass black holes and merging neutron stars by gravitational waves.

Host institution

STOCKHOLMS UNIVERSITET
Net EU contribution
€ 1 500 000,00
Address
UNIVERSITETSVAGEN 10
10691 Stockholm
Sweden

See on map

Region
Östra Sverige Stockholm Stockholms län
Activity type
Higher or Secondary Education Establishments
Links
Total cost
€ 1 500 000,00

Beneficiaries (1)