论文标题
将超新星建模为光学厚的火球
Modeling Supernovae as an Optically Thick Fireball
论文作者
论文摘要
我们使用开放超新星目录中的数据来计算135个恒星超新星的性质。我们使用球形对称的光学较厚火球模型产生温度,半径,亮度和膨胀速度。这些建模的参数揭示了在不同类型的超新星中常见的趋势。我们已经确定了跨IIA,II,II P和IIB超新星的不同阶段。我们注意到,有很长的合理持续增长(第1阶段),可以证明我们的光学厚火球模型。模型的半径达到最大值,超出其平坦或减小(阶段2)。我们在最大建模半径为4500 K处观察到的温度表明,由于电子重组而引起的不透明度损失设置了时间表,其中我们的光学厚模型不再适用。我们观察到最快的火球速度,最大的建模火球半径以及IA型超新星的最大建模光度。作为一个组,IA型超新星达到的最大发光度比II型超新星高8.5倍。我们提供了一个摘要表,该表包含超新星的建模参数及其按超新星分类类型的时间。
We calculate the properties of 135 stellar supernovae using data from the Open Supernova Catalog. We generate temperatures, radii, luminosities, and expansion velocities using a spherically symmetric optically thick fireball model. These modeled parameters reveal trends that are common across different types of supernovae. We have identified distinct phases that appear across Type Ia, II, II P, and IIb supernovae. We note that there is a long period of reasonable continuous growth (Phase 1), giving credence to our simple model of an optically thick fireball. The modeled radius reaches a maximum value beyond which it is flat or decreases (Phase 2). The temperature we observe at the maximum modeled radius, 4500 K, suggests that the loss of opacity due to electron recombination sets the timeline where our optically thick model no longer applies. We observe the fastest modeled fireball velocities, largest modeled fireball radii, and maximum modeled luminosities for Type Ia supernovae. As a group, Type Ia supernovae reach a maximum luminosity that is 8.5 times more luminous than Type II supernovae. We present a summary table that contains modeled parameters of supernovae and their timings by supernova classification type.