Spectropolarimetry of Supernovae

dc.creatorWang, Lifan
dc.creatorWheeler, J. Craig
dc.date2008-11-06
dc.date.accessioned2026-07-07T12:15:58Z
dc.date.available2026-07-07T12:15:58Z
dc.descriptionOverwhelming evidence has accumulated in recent years that supernova explosions are intrinsically 3-dimensional phenomena with significant departures from spherical symmetry. We review the evidence derived from spectropolarimetry that has established several key results: virtually all supernovae are significantly aspherical near maximum light; core-collapse supernovae behave differently than thermonuclear (Type Ia) supernovae; the asphericity of core-collapse supernovae is stronger in the inner layers showing that the explosion process itself is strongly aspherical; core-collapse supernovae tend to establish a preferred direction of asymmetry; the asphericity is stronger in the outer layers of thermonuclear supernovae providing constraints on the burning process. We emphasize the utility of the Q/U plane as a diagnostic tool and revisit SN 1987A and SN 1993J in a contemporary context. An axially-symmetric geometry can explain many basic features of core-collapse supernovae, but significant departures from axial symmetry are needed to explain most events. We introduce a spectropolarimetry type to classify the range of behavior observed in polarized supernovae. Understanding asymmetries in supernovae is important for phenomena as diverse as the origins of gamma-ray bursts and the cosmological applications of Type Ia supernovae in studies of the dark energy content of the universe.
dc.descriptionDraft of Annual Review article prior to final copy editing; 85 pages, 13 figures, 1 table
dc.identifierhttps://arxiv.org/abs/0811.1054
dc.identifierhttp://arxiv.org/abs/0811.1054
dc.identifierAnn.Rev.Astron.Astrophys.46:433-474,2008
dc.identifierdoi:10.1146/annurev.astro.46.060407.145139
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/211653
dc.subjectAstrophysics
dc.titleSpectropolarimetry of Supernovae
dc.typetext

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