Towards a Physical Understanding of the Diversity of Type Ia Supernovae

Mathematics – Logic

Scientific paper

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Scientific paper

Type Ia supernovae {SNe Ia} represent the most mature and productive probe of the dark energy invoked to explain the cosmic acceleration. Considerable resources are being invested with HST and ground-based facilities to detect and measure the properties of distant SNe Ia for this purpose. However, there is not yet a convincing physical model for these events and important correlations have been found between the intrinsic properties of SNe Ia and their host galaxy environment. These suggest diverse ways in which the explosions may occur and highlight the importance of the progenitor metallicity and its relationship to the resulting light curve. We propose a new Target of Opportunity campaign to track and model the time evolution of the UV via spectroscopy of 5 carefully-selected local SNe Ia from soon after the explosion through maximum light. Early phase UV spectroscopy will provide a key diagnostic of the progenitor composition and time-sequence modeling will probe the density structure and its relevance to a variety of explosive models. Recent progress in detailed SNe Ia modeling and in locating early SNe Ia with the highly-successful Palomar Transient Factory now make it practical to embark on such a detailed campaign. The results will significantly improve our ability to understand the validity and limitations of the use of SNe Ia as future cosmological probes.;

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