✦ LIBER ✦

Modelling Turbulent Deflagrations in Type Ia Supernovae

✍ Scribed by J.C. Niemeyer; W. Schmidt; C. Klingenberg

Publisher: Elsevier Science
Year: 2005
Tongue: English
Weight: 322 KB
Volume: 758
Category: Article
ISSN: 0375-9474
DOI: 10.1016/j.nuclphysa.2005.05.080

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

The p-Process Nucleosynthesis in the Car

The p-Process Nucleosynthesis in the Carbon Deflagration Model for Type Ia Supernovae

✍ Motohiko Kusakabe; Nobuyuki Iwamoto; Ken'ichi Nomoto 📂 Article 📅 2005 🏛 Elsevier Science 🌐 English ⚖ 297 KB

Modeling type Ia supernovae

✍ Wolfgang Hillebrandt; Friedrich K. Röpke 📂 Article 📅 2010 🏛 Elsevier Science 🌐 English ⚖ 473 KB

Models of type Ia supernovae

✍ S. Kumagai; K. Iwabuchi; K. Nomoto 📂 Article 📅 1999 🏛 John Wiley and Sons 🌐 English ⚖ 80 KB

Models for type Ia supernovae

✍ S.E. Woosley 📂 Article 📅 2001 🏛 Elsevier Science 🌐 English ⚖ 503 KB

Nucleosynthesis in type Ia supernovae

✍ K. Nomoto; K. Iwamoto; N. Nakasato; F.-K. Thielemann; F. Brachwitz; T. Tsujimoto 📂 Article 📅 1997 🏛 Elsevier Science 🌐 English ⚖ 519 KB

Among the major uncertainties involved in the Chandrasekhar mass models for Type Ia supernovae are the companion star of the accreting white dwarf (or the accretion rate that determines the carbon ignition density) and the flame speed after ignition. We present nucleosynthesis results from relativel

Interpretation of observed type Ia super

Interpretation of observed type Ia supernova spectra with radiative transfer models

✍ D.N. Sauer; P.A. Mazzali 📂 Article 📅 2008 🏛 Elsevier Science 🌐 English ⚖ 237 KB

The different nucleosynthetic yields in type Ia supernovae lead to variation in the observed properties of those objects. Complementary to extensive numerical simulations of the explosion physics the detailed analysis of well observed objects can provide constraints on the explosion mechanism. Using