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Updated: Feb 22, 2026
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Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
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Bridging the gap: from massive stars to supernovae
Justyn R Maund1, Paul A Crowther2, Hans-Thomas Janka3
1Department of Physics and Astronomy, University of Sheffield, Hicks Building, Hounsfield Road, Sheffield S3 7RH, UK j.maund@sheffield.ac.uk.
Summary
Massive stars and supernovae are crucial cosmic engines, creating heavy elements and shaping galaxies. Understanding their connection requires bridging stellar evolution and supernova astrophysics communities.
Area of Science:
- Astrophysics
- Stellar Evolution
- Supernova Physics
Background:
- Massive stars and supernovae are fundamental to galactic evolution, producing energy and heavy elements.
- The rapid transition from stellar evolution to supernova explosion involves extreme physics.
- Unanswered questions persist in both massive star evolution and supernova behavior.
Purpose of the Study:
- To bridge the gap between massive star evolution and supernova studies.
- To foster collaboration between theoretical and observational astronomers in these fields.
- To view massive star evolution and supernovae as a continuous process.
Main Methods:
- Convened the Theo Murphy international scientific meeting 'Bridging the gap: from massive stars to supernovae'.
- Facilitated discussion between stellar evolution and supernova astrophysics communities.
- Integrated theoretical and observational approaches to massive star and supernova research.
Main Results:
- Highlighted the interconnectedness of massive star evolution and supernovae.
- Identified the need for a unified approach to studying these phenomena.
- Emphasized the importance of interdisciplinary collaboration.
Conclusions:
- Viewing massive star evolution and supernovae as a single, continuous narrative is essential.
- Bridging the gap between communities will advance understanding of these cosmic events.
- Further integration of theoretical and observational studies is crucial.
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