Type Ia Supernova cosmology
Type Ia Supernova cosmology
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.
Cosmology, Supernovae
Leibundgut, B.
5a4c0b96-8819-46f5-85eb-c022a8e2aa0b
Sullivan, M.
2f31f9fa-8e79-4b35-98e2-0cb38f503850
March 2018
Leibundgut, B.
5a4c0b96-8819-46f5-85eb-c022a8e2aa0b
Sullivan, M.
2f31f9fa-8e79-4b35-98e2-0cb38f503850
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.
Text
Type Ia Supernova Cosmology
- Accepted Manuscript
More information
Accepted/In Press date: 28 February 2018
e-pub ahead of print date: 12 March 2018
Published date: March 2018
Additional Information:
AM added 12/4/18
Keywords:
Cosmology, Supernovae
Identifiers
Local EPrints ID: 419706
URI: http://eprints.soton.ac.uk/id/eprint/419706
ISSN: 0038-6308
PURE UUID: ac59a943-ca35-466d-b934-9b08057df1de
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Date deposited: 19 Apr 2018 16:30
Last modified: 18 Mar 2024 05:17
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Author:
B. Leibundgut
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