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Improvements to type Ia supernova mo...
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Saunders, Clare M.
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Improvements to type Ia supernova models.
紀錄類型:
書目-電子資源 : Monograph/item
正題名/作者:
Improvements to type Ia supernova models./
作者:
Saunders, Clare M.
出版者:
Ann Arbor : ProQuest Dissertations & Theses, : 2016,
面頁冊數:
91 p.
附註:
Source: Dissertation Abstracts International, Volume: 78-06(E), Section: B.
Contained By:
Dissertation Abstracts International78-06B(E).
標題:
Astrophysics. -
電子資源:
http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=10191598
ISBN:
9781369558531
Improvements to type Ia supernova models.
Saunders, Clare M.
Improvements to type Ia supernova models.
- Ann Arbor : ProQuest Dissertations & Theses, 2016 - 91 p.
Source: Dissertation Abstracts International, Volume: 78-06(E), Section: B.
Thesis (Ph.D.)--University of California, Berkeley, 2016.
Type Ia Supernovae provided the first strong evidence of dark energy and are still an important tool for measuring the accelerated expansion of the universe. However, future improvements will be limited by systematic uncertainties in our use of Type Ia supernovae as standard candles. Using Type Ia supernovae for cosmology relies on our ability to standardize their absolute magnitudes, but this relies on imperfect models of supernova spectra time series. This thesis is focused on using data from the Nearby Supernova Factory both to understand current sources of uncertainty in standardizing Type Ia supernovae and to develop techniques that can be used to limit uncertainty in future analyses. (Abstract shortened by ProQuest.).
ISBN: 9781369558531Subjects--Topical Terms:
535904
Astrophysics.
Improvements to type Ia supernova models.
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Type Ia Supernovae provided the first strong evidence of dark energy and are still an important tool for measuring the accelerated expansion of the universe. However, future improvements will be limited by systematic uncertainties in our use of Type Ia supernovae as standard candles. Using Type Ia supernovae for cosmology relies on our ability to standardize their absolute magnitudes, but this relies on imperfect models of supernova spectra time series. This thesis is focused on using data from the Nearby Supernova Factory both to understand current sources of uncertainty in standardizing Type Ia supernovae and to develop techniques that can be used to limit uncertainty in future analyses. (Abstract shortened by ProQuest.).
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