A 3D Simulation of a Type II-P Supernova: From Core Bounce to beyond Shock Breakout Article Swipe
David Vartanyan
,
Benny T.-H. Tsang
,
Daniel Kasen
,
Adam Burrows
,
Tianshu Wang
,
Lizzy Teryoshin
·
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4357/adb1e4
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4357/adb1e4
In order to better connect core-collapse supernova (CCSN) theory with its observational signatures, we have developed a simulation pipeline from the onset of the core collapse to beyond shock breakout from the stellar envelope. Using this framework, we present a 3D simulation study from 5 s to over 5 days following the evolution of a 17 M ⊙ progenitor, exploding with ∼10 51 erg of energy and ∼0.1 M ⊙ of 56 Ni ejecta. The early explosion is highly asymmetric, expanding most prominently along the southern hemisphere. This early asymmetry is preserved to shock breakout, ∼1 day later. Breakout itself evinces strong angle-dependence, with as much as 1 day delay in the shock breakout by direction. The nickel ejecta closely tail the forward shock, with velocities at the breakout as high as ∼7000 km s −1 . A delayed reverse shock forming at the H/He interface on hour timescales leads to the formation of Rayleigh–Taylor instabilities, fast-moving nickel bullets, and almost complete mixing of the metal core into the hydrogen envelope. For the first time, we illustrate the angle-dependent emergent broadband and bolometric light curves from simulations evolved in 3D in entirety, continuing through hydrodynamic shock breakout from a CCSN model of a massive stellar progenitor evolved with detailed, late-time neutrino microphysics and transport. Our case study of a single progenitor underscores that 3D simulations generically produce the cornucopia of observed asymmetries and features in CCSNe observations, while establishing the methodology to study this problem in breadth.
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Metadata
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.3847/1538-4357/adb1e4
- OA Status
- gold
- Cited By
- 14
- References
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- OpenAlex ID
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All OpenAlex metadata
Raw OpenAlex JSON
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https://openalex.org/W4408313725Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.3847/1538-4357/adb1e4Digital Object Identifier
- Title
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A 3D Simulation of a Type II-P Supernova: From Core Bounce to beyond Shock BreakoutWork title
- Type
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
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2025Year of publication
- Publication date
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2025-03-11Full publication date if available
- Authors
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David Vartanyan, Benny T.-H. Tsang, Daniel Kasen, Adam Burrows, Tianshu Wang, Lizzy TeryoshinList of authors in order
- Landing page
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https://doi.org/10.3847/1538-4357/adb1e4Publisher landing page
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YesWhether a free full text is available
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goldOpen access status per OpenAlex
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https://doi.org/10.3847/1538-4357/adb1e4Direct OA link when available
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Physics, Breakout, Supernova, Shock (circulatory), Core (optical fiber), Astrophysics, Type II supernova, Type (biology), Astronomy, Shock front, Shock wave, Mechanics, Optics, Medicine, Finance, Biology, Economics, Internal medicine, EcologyTop concepts (fields/topics) attached by OpenAlex
- Cited by
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14Total citation count in OpenAlex
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2025: 14Per-year citation counts (last 5 years)
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10Other works algorithmically related by OpenAlex
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