44Ti and 56Ni in core-collapse supernovae

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dc.creatorMagkotsios, Georgios
dc.creatorTimmes, Francis X.
dc.creatorWiescher, Michael
dc.creatorFryer, Christopher L.
dc.creatorHungerford, Aimee
dc.creatorYoung, Patrick
dc.creatorBennett, Michael
dc.creatorDiehl, Steven
dc.creatorHerwig, Falk
dc.creatorHirschi, Raphael
dc.creatorPignatari, Marco
dc.creatorRockefeller, Gabriel
dc.date2008-11-28
dc.date.accessioned2026-07-07T12:06:18Z
dc.date.available2026-07-07T12:06:18Z
dc.descriptionWe investigate the physical conditions where 44Ti and 56Ni are created in core-collapse supernovae. In this preliminary work we use a series of post-processing network calculations with parametrized expansion profiles that are representative of the wide range of temperatures, densities and electron-to-baryon ratios found in 3D supernova simulations. Critical flows that affect the final yields of 44Ti and 56Ni are assessed.
dc.descriptionTo appear in the Conference Proceedings for the "10th Symposium on Nuclei in the Cosmos (NIC X)", July 27 - August 1 2008, Mackinack Island, Michigan, USA
dc.identifierhttps://arxiv.org/abs/0811.4651
dc.identifierhttp://arxiv.org/abs/0811.4651
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/208615
dc.subjectAstrophysics
dc.title44Ti and 56Ni in core-collapse supernovae
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