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A new set of spectral quantities characterizing type Ia supernovae: and their correlation with peak luminosity
Stockholm University, Faculty of Science, Department of Physics.
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Identifiers
URN: urn:nbn:se:su:diva-25303OAI: oai:DiVA.org:su-25303DiVA: diva2:199406
Note
Part of urn:nbn:se:su:diva-80Available from: 2004-03-25 Created: 2004-03-25 Last updated: 2010-01-13Bibliographically approved
In thesis
1. Type Ia Supernova Cosmology: Quantitative Spectral Analysis
Open this publication in new window or tab >>Type Ia Supernova Cosmology: Quantitative Spectral Analysis
2004 (English)Doctoral thesis, comprehensive summary (Other academic)
Abstract [en]

Type Ia supernovae have been successfully used as standardized candles to study the expansion history of the Universe. In the past few years, these studies led to the exciting result of an accelerated expansion caused by the repelling action of some sort of dark energy. This result has been confirmed by measurements of cosmic microwave background radiation, the large-scale structure, and the dynamics of galaxy clusters. The combination of all these experiments points to a “concordance model” of the Universe with flat large-scale geometry and a dominant component of dark energy.

However, there are several points related to supernova measurements which need careful analysis in order to doubtlessly establish the validity of the concordance model. As the amount and quality of data increases, the need of controlling possible systematic effects which may bias the results becomes crucial. Also important is the improvement of our knowledge of the physics of supernovae events to assure and possibly refine their calibration as standardized candle.

This thesis addresses some of those issues through the quantitative analysis of supernova spectra. The stress is put on a careful treatment of the data and on the definition of spectral measurement methods. The comparison of measurements for a large set of spectra from nearby supernovae is used to study the homogeneity and to search for spectral parameters which may further refine the calibration of the standardized candle. One such parameter is found to reduce the dispersion in the distance estimation of a sample of supernovae to below 6%, a precision which is comparable with the current lightcurve-based calibration, and is obtained in an independent manner. Finally, the comparison of spectral measurements from nearby and distant objects is used to test the possibility of evolution with cosmic time of the intrinsic brightness of type Ia supernovae.

Place, publisher, year, edition, pages
Stockholm: Fysikum, 2004. 137 p.
Keyword
Supernova, Cosmology, Spectroscopy
National Category
Physical Sciences
Identifiers
urn:nbn:se:su:diva-80 (URN)91-7265-847-9 (ISBN)
Public defence
2004-04-16, sal FA32, AlbaNova universitetscentrum, Roslagstullbacken 21, Stockholm, 10:00
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Available from: 2004-03-25 Created: 2004-03-25Bibliographically approved

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