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Type Ia Supernova Cosmology

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Abstract

The primary agent for Type Ia supernova cosmology is the uniformity of their appearance. We present the current status, achievements and uncertainties. The Hubble constant and the expansion history of the universe are key measurements provided by Type Ia supernovae. They were also instrumental in showing time dilation, which is a direct observational signature of expansion. Connections to explosion physics are made in the context of potential improvements of the quality of Type Ia supernovae as distance indicators. The coming years will see large efforts to use Type Ia supernovae to characterise dark energy.

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Acknowledgements

B.L. acknowledges support for this work by the Deutsche Forschungsgemeinschaft through the TransRegio Project TRR33 “The Dark Universe”.

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  1. European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748, Garching, Germany

    B. Leibundgut

  2. Excellence Cluster Universe, Technische Universität München, Boltzmannstrasse 2, 85748, Garching, Germany

    B. Leibundgut

  3. Department of Physics and Astronomy, University of Southampton, Southampton, Hampshire, SO17 1BJ, UK

    M. Sullivan

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Leibundgut, B., Sullivan, M. Type Ia Supernova Cosmology. Space Sci Rev 214, 57 (2018). https://doi.org/10.1007/s11214-018-0491-8

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