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相关论文: On the Mechanism of Type Ia Supernovae

200 篇论文

Type Ia supernovae (SNe Ia) are a prime tool in observational cosmology. A relation between their peak luminosities and the shapes of their light curves allows to infer their intrinsic luminosities and to use them as distance indicators.…

太阳与恒星天体物理 · 物理学 2010-02-15 F. K. Roepke , W. Hillebrandt , D. Kasen , S. E. Woosley

Motivated by the fact that calibrated light curves of Type Ia supernovae (SNe Ia) have become a major tool to determine the expansion history of the Universe, considerable attention has been given to, both, observations and models of these…

宇宙学与河外天体物理 · 物理学 2013-02-27 W. Hillebrandt , M. Kromer , F. K. Röpke , A. J. Ruiter

Empirically, Type Ia supernovae are the most useful, precise, and mature tools for determining astronomical distances. Acting as calibrated candles they revealed the presence of dark energy and are being used to measure its properties.…

宇宙学与河外天体物理 · 物理学 2011-06-15 D. Andrew Howell

Type Ia supernovae (SNe Ia) are the largest thermonuclear explosions in the Universe. Their light output can be seen across great distances and has led to the discovery that the expansion rate of the Universe is accelerating. Despite the…

天体物理学 · 物理学 2009-11-11 M. Zingale , A. S. Almgren , J. B. Bell , M. S. Day , C. A. Rendleman , S. E. Woosley

Type Ia supernovae (SNe Ia) are used as distance indicators to infer the cosmological parameters that specify the expansion history of the universe. Parameter inference depends on the criteria by which the analysis SN sample is selected.…

宇宙学与河外天体物理 · 物理学 2021-02-19 Alex G. Kim

Modeling type Ia supernova (SN Ia) explosions in three dimensions allows to eliminate any undetermined parameters and provides predictive power to simulations. This is necessary to improve the understanding of the explosion mechanism and to…

天体物理学 · 物理学 2009-11-11 F. K. Roepke , W. Hillebrandt

Type Ia Supernovae hold great promise to measure the cosmic deceleration. The diversity observed among these explosions, however, complicates their ability to measure cosmological parameters considerably. The comparison of near and distant…

天体物理学 · 物理学 2007-05-23 B. Leibundgut

We give an overview of the current understanding of Type Ia supernovae relevant for their use as cosmological distance indicators. We present the physical basis to understand their homogeneity of the observed light curves and spectra and…

天体物理学 · 物理学 2007-05-23 P. Hoeflich

I review the use of type-Ia supernovae (SNe) for cosmological studies. After briefly recalling the main features of type-Ia SNe that lead to their use as cosmological probes, I briefly describe current and planned type-Ia SNe surveys, with…

天体物理学 · 物理学 2008-11-26 Ramon Miquel

Observations of Type Ia supernovae (SNe Ia) reveal correlations between their luminosities and light-curve shapes, and between their spectral sequence and photometric sequence. Assuming SNe Ia do not evolve at different redshifts, the…

天体物理学 · 物理学 2007-05-23 Weidong Li , Alexei V. Filippenko

Spectroscopic and photometric evidence indicates that Type Ia supernovae (SNe Ia) are the thermonuclear explosions of accreting white dwarfs. However, the progenitor binary systems and hydrodynamical models for SNe Ia are still…

天体物理学 · 物理学 2009-10-30 Ken'ichi Nomoto , Koichi Iwamoto , Nobuhiro Kishimoto

The application of Type Ia supernovae (SNe Ia) as distance indicators in cosmology calls for a sound understanding of these objects. Recent years have seen a brisk development of astrophysical models which explain SNe Ia as thermonuclear…

天体物理学 · 物理学 2009-06-23 F. K. Roepke

Supernovae of type Ia (SNe Ia) are very important for cosmography. To exclude systematic effects in linking the observed light of distant SNe Ia to the parameters of cosmological models, one has to understand the nature of supernova…

天体物理学 · 物理学 2009-11-07 S. Blinnikov , E. Sorokina

Type Ia supernovae (SNe Ia) are thermonuclear exploding stars that can be used to put constraints on the nature of our universe. One challenge with population analyses of SNe Ia is Malmquist bias, where we preferentially observe the…

宇宙学与河外天体物理 · 物理学 2024-07-24 Benjamin M. Boyd , Matthew Grayling , Stephen Thorp , Kaisey S. Mandel

Type Ia Supernovae (SNe Ia) are used as reliable cosmic distance indicators and their standardization is necessary for a more accurate measurement of the cosmological parameters of the Universe. However, the Hubble diagram still shows some…

高能天体物理现象 · 物理学 2024-06-17 Anastasia Baluta , Maria Pruzhinskaya , Philippe Rosnet , Nicoleta Pauna

Type Ia supernovae are bright stellar explosions distinguished by standardizable light curves that allow for their use as distance indicators for cosmological studies. Despite their highly successful use in this capacity, the progenitors of…

太阳与恒星天体物理 · 物理学 2015-06-05 Alan C. Calder , Brendan K. Krueger , Aaron P. Jackson , Dean M. Townsley , Edward F. Brown , Francis X. Timmes

In the next decade Type Ia supernovae (SNe Ia) will be used to test theories predicting changes in the Dark Energy equation of state with time. Ultimately this requires a dedicated space mission like JDEM. SNe Ia are mature cosmological…

The major role type Ia supernovae play in many fields of astrophysics and in particular in cosmological distance determinations calls for self-consistent models of these events. Since their mechanism is believed to crucially depend on…

天体物理学 · 物理学 2015-06-03 F. K. Roepke

The remarkable uniformity of Type Ia supernovae (SNe Ia) has allowed astronomers to use them as distance indicators to measure the properties and expansion history of the Universe. However, SNe Ia exhibit intrinsic variation in both their…

天体物理学 · 物理学 2009-09-29 William Michael Wood-Vasey
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