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SNSM

Spectral synthesis of multidimensional supernova explosion models

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EC-Contrib. €

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Partnership

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Project "SNSM" data sheet

The following table provides information about the project.

Coordinator
MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV 

Organization address
address: HOFGARTENSTRASSE 8
city: MUENCHEN
postcode: 80539
website: n.a.

contact info
title: n.a.
name: n.a.
surname: n.a.
function: n.a.
email: n.a.
telephone: n.a.
fax: n.a.

 Coordinator Country Germany [DE]
 Project website https://star.pst.qub.ac.uk/wiki/doku.php/users/ajerkstrand/start
 Total cost 171˙460 €
 EC max contribution 171˙460 € (100%)
 Programme 1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
 Code Call H2020-MSCA-IF-2015
 Funding Scheme MSCA-IF-EF-ST
 Starting year 2016
 Duration (year-month-day) from 2016-10-01   to  2018-09-30

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV DE (MUENCHEN) coordinator 171˙460.00

Map

 Project objective

Core-collapse supernovae are the explosive deaths of massive stars. They are the main production sites of the heavy elements in the Universe, drive galactic dynamic and chemical evolution, and produce exotic remnants such as black holes and neutron stars. To interpret observations and advance our understanding of the origin of the elements, sophisticated spectral models are needed. The main science objective in this proposal is to compute the first spectral models of multi-dimensional core-collapse explosion simulations. These models will then be compared with available high-quality data to derive information on nucleosynthesis yields and supernova structure. The proposed work involves the development of spectral modelling tools from current 1D to multi-D capability, and application of these to recently computed state-of-the-art 3D explosion simulations. This innovative project will allow a milestone in supernova research to be reached by producing the first light curves and spectra of modern 3D simulations, and will approach us to solving an almost 50 year standing mystery of how supernovae explode and how the elements are produced.

 Publications

year authors and title journal last update
List of publications.
2017 A Jerkstrand, T Ertl, H-T Janka, E Müller, T Sukhbold, S E Woosley
Emission line models for the lowest mass core-collapse supernovae – I. Case study of a 9 M⊙ one-dimensional neutrino-driven explosion
published pages: 277-305, ISSN: 0035-8711, DOI: 10.1093/mnras/stx2877
Monthly Notices of the Royal Astronomical Society 475/1 2019-05-09

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