The secondary supernova machine: Gravitational compression, stored Coulomb energy, and SNII displays

IF 11.7 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Donald D. Clayton, Bradley S. Meyer
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引用次数: 0

Abstract

Radioactive power for several delayed optical displays of core-collapse supernovae is commonly described as having been provided by decays of 56Ni nuclei. This review analyses the provenance of that energy more deeply: the form in which that energy is stored; what mechanical work causes its storage; what conservation laws demand that it be stored; and why its release is fortuitously delayed for about 106 s into a greatly expanded supernova envelope. We call the unifying picture of those energy transfers the secondary supernova machine owing to its machine-like properties; namely, mechanical work forces storage of large increases of nuclear Coulomb energy, a positive energy component within new nuclei synthesized by the secondary machine. That positive-energy increase occurs despite the fusion decreasing negative total energy within nuclei. The excess of the Coulomb energy can later be radiated, accounting for the intense radioactivity in supernovae. Detailed familiarity with this machine is the focus of this review. The stored positive-energy component created by the machine will not be reduced until roughly 106 s later by radioactive emissions (EC and β+) owing to the slowness of weak decays. The delayed energy provided by the secondary supernova machine is a few × 1049 erg, much smaller than the one percent of the 1053 erg collapse that causes the prompt ejection of matter; however, that relatively small stored energy is vital for activation of the late displays. The conceptual basis of the secondary supernova machine provides a new framework for understanding the energy source for late SNII displays. We demonstrate the nuclear dynamics with nuclear network abundance calculations, with a model of sudden compression and reexpansion of the nuclear gas, and with nuclear energy decompositions of a nuclear-mass law. These tools identify excess Coulomb energy, a positive-energy component of the total negative nuclear energy, as the late activation energy. If the value of fundamental charge e were smaller, SNII would not be so profoundly radioactive. Excess Coulomb energy has been carried within nuclei radially for roughly 109 km before being radiated into greatly expanded supernova remnants. The Coulomb force claims heretofore unacknowledged significance for supernova physics.

次超新星机器:引力压缩,储存的库仑能量和SNII显示
核心坍缩超新星的几个延迟光学显示的放射性能量通常被描述为由56Ni核的衰变提供的。这篇综述更深入地分析了这种能量的来源:能量储存的形式;是什么机械功导致了它的储存;什么守恒定律要求它被储存起来?以及为什么它的释放被意外地推迟了大约106秒,进入了一个大大膨胀的超新星包层。我们把这些能量转移的统一图景称为次级超新星机器,因为它具有类似机器的性质;即,机械功迫使储存大量增加的核库仑能,这是二次机合成的新核中的正能量成分。尽管核聚变减少了原子核内的负总能量,但正能量还是增加了。多余的库仑能量后来可以被辐射,这就解释了超新星中强烈的放射性。详细熟悉这台机器是本评论的重点。由于弱衰变的缓慢性,机器产生的储存的正能量成分直到大约106秒后才会被放射性释放(EC和β+)所减少。次级超新星机器提供的延迟能量为几× 1049 erg,远远小于导致物质迅速喷射的1053 erg坍缩的1%;然而,相对较小的储存能量对于激活后期显示是至关重要的。次级超新星机器的概念基础为理解后期SNII显示的能量来源提供了一个新的框架。我们用核网络丰度计算、核气体的突然压缩和再膨胀模型以及核质量定律的核能分解来证明核动力学。这些工具识别多余的库仑能量,总负核能的正能量组成部分,作为后期活化能。如果基本电荷e的值小一些,SNII就不会有如此强烈的放射性。在辐射到膨胀的超新星残骸之前,多余的库仑能量在原子核内径向传播了大约109公里。库仑力在超新星物理学中具有迄今未被承认的重要意义。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
New Astronomy Reviews
New Astronomy Reviews 地学天文-天文与天体物理
CiteScore
18.60
自引率
1.70%
发文量
7
审稿时长
11.3 weeks
期刊介绍: New Astronomy Reviews publishes review articles in all fields of astronomy and astrophysics: theoretical, observational and instrumental. This international review journal is written for a broad audience of professional astronomers and astrophysicists. The journal covers solar physics, planetary systems, stellar, galactic and extra-galactic astronomy and astrophysics, as well as cosmology. New Astronomy Reviews is also open for proposals covering interdisciplinary and emerging topics such as astrobiology, astroparticle physics, and astrochemistry.
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