SNSM
Spectral synthesis of multidimensional supernova explosion models
Total Cost €
0EC-Contrib. €
0Partnership
0Views
0SNSM project word cloud
Explore the words cloud of the SNSM project. It provides you a very rough idea of what is the project "SNSM" about.
Project "SNSM" data sheet
The following table provides information about the project.
| Coordinator |
MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV
Organization address contact info |
| 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.
| # | ||||
|---|---|---|---|---|
| 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 |
|---|---|---|---|
| 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 |
Are you the coordinator (or a participant) of this project? Plaese send me more information about the "SNSM" project.
For instance: the website url (it has not provided by EU-opendata yet), the logo, a more detailed description of the project (in plain text as a rtf file or a word file), some pictures (as picture files, not embedded into any word file), twitter account, linkedin page, etc.
Send me an email (fabio@fabiodisconzi.com) and I put them in your project's page as son as possible.
Thanks. And then put a link of this page into your project's website.
The information about "SNSM" are provided by the European Opendata Portal: CORDIS opendata.