标题： Ia型超新星的爆炸模型：与观测光变曲线、距离、H_o和q_o的比较 显示英文标题

标题： Explosion Models for Type Ia Supernovae: A Comparison with Observed Light Curves, distances, H_o and q_o

摘要： 将理论上的单色光曲线和光球膨胀速度与27颗Ia型超新星（SNe Ia）的观测结果进行了比较。 我们考虑了一组包含37个模型的集合，这些模型涵盖了目前讨论的所有Ia型超新星爆炸情景，包括燃烧波、爆燃、延迟爆燃、脉动延迟爆燃以及Chandra质量的抑制爆燃，还有低质量白矮星的氦爆燃。 这些爆炸使用一维拉格朗日流体力学和辐射流体力学代码（包含核网络）进行计算。 随后，利用我们的LC方案构建了光曲线，该方案包括隐式辐射传输、膨胀不透明度、蒙特卡罗$\gamma $射线传输，以及分子和尘埃形成。 对于某些超新星，已经考虑了详细的非局部热平衡计算结果。 讨论了我们模型系列的观测特性，包括绝对亮度、最大值后下降率、多个时间点的颜色关系等。 所有Ni产量大于0.4太阳质量的模型产生的光曲线亮度相似。 讨论了宇宙红移对光曲线的影响以及星际消光校正的影响。 基于标准差的数据修正，采用了一种定量拟合观测数据的方法来确定自由参数，即正确的模型、距离、消光程度和爆炸时间。 详细讨论了结果，并将其应用于确定H₀和q₀。 显示英文摘要

摘要： Theoretical monochromatic light curves and photospheric expansion velocities are compared with observations of 27 Type Ia supernovae (SNe Ia). A set of 37 models has been considered which encompasses all currently discussed explosion scenarios for Type Ia supernovae including deflagrations, detonations, delayed detonations, pulsating delayed detonations and tamped detonations of Chandra- mass, and Helium detonations of low mass white dwarfs. The explosions are calculated using one-dimensional Lagrangian hydro and radiation-hydro codes with incorporated nuclear networks. Subsequently, light curves are constructed using our LC scheme which includes an implicit radiation transport, expansion opacities, a Monte-Carlo $\gamma $-ray transport, and molecular and dust formation. For some supernovae, results of detailed non-LTE calculations have been considered. Observational properties of our series of models are discussed, the relation between the absolute brightness, post-maximum decline rates, the colors at several moments of time, etc. All models with a Ni production larger than 0.4 solar masses produce light curves of similar brightness. The influence of the cosmological red shift on the light curves and on the correction for interstellar reddening is discussed. Based on data rectification of the standard deviation, a quantitative procedure to fit the observations has been used to the determine the free parameters, i.e. the correct model, the distance, the reddening, and the time of the explosion. The results are discussed in detail and applied to determine Ho and qo.