论文标题
用喷气机为发光的核心倒塌超新星
Powering luminous core collapse supernovae with jets
论文作者
论文摘要
我检查了具有额外磁力和氦气燃烧的额外能源的发光超新星（LSNE）的最新配件，发现大约一半的LSNE拟合参数有一些问题。在某些LSNE中，这两个能源的总能量大于拟合产生的喷射能量的动能。在其他一些中，延迟中微子爆炸机制的总能量和这两个额外的来源组合小于拟合产生的动能。这些困难表明，就像较早声称喷气机功率超小超新星（SLSNE）一样，喷气机也为发光的LSNE提供动力。磁铁也可能提供能量。但是，在大多数情况下，在爆炸期间，可能在较晚的时候，喷气机提供的能量比磁铁提供了更多的能量。我加强了较早的说法，即在磁塔出生时发射的喷气式飞机不容忽视。我解释了给定氢缺乏核心塌陷超新星（CCSNE）的最大上升时间的趋势，特别是LSNE和SLSNE，其爆炸后很长一段时间的Jets玩具模型。
I examine recent fittings of luminous supernovae (LSNe) with extra energy sources of magnetar and helium burning and find that in about half of these LSNe the fitting parameters have some problems. In some LSNe the total energy of these two energy sources is larger than the kinetic energy of the ejecta that the fitting yields. In some others LSNe the total energy of the delayed neutrino explosion mechanism and these two extra sources combined is smaller than the kinetic energy that the fitting yields. These difficulties suggest that, like earlier claims that jets power superluminous supernovae (SLSNe), jets also power the less luminous LSNe. A magnetar might also supply energy. However, in most cases jets supply more energy than the magnetar, during the explosion and possibly at late times. I strengthen an earlier claim that jets launched at magnetar birth cannot be ignored. I explain the trend of maximum rise time for a given luminosity of hydrogen deficient core collapse supernovae (CCSNe), in particular LSNe and SLSNe, with a toy model of jets that are active for a long time after explosion.
