论文标题
奇怪的星星介绍
An introduction to strange stars
论文作者
论文摘要
自然观察到的最重的中子星的描述取决于对一般相对论和量子染色体动力学中存在的物理概念的理解。在这项工作中，我们审查了描述由上，向下和奇怪的夸克所构成的奇怪恒星所需的基本概念，这是描述最密集中子恒星的一般特性的可能替代方法之一。我们将回顾Bodmer-witter-terazawa假设，该假说指出，与普通核物质有关的奇怪物质绝对稳定，并讨论表征奇怪恒星的基本特性。我们的目标是提出必要的概念，以了解Astroparpicles的这一重要主题。
The description of the heaviest neutron stars observed in Nature depends on the understanding of the physical concepts present in General Relativity and Quantum Chromodynamics. In this work, we review the basic concepts need to describe strange stars, constituted by up, down and strange quarks, which is one of the possible alternatives to describe the general properties of the most dense neutron stars. We will review the Bodmer-Witten-Terazawa hypothesis, which states that strange matter is absolutely stable in relation to ordinary nuclear matter, and discuss the basic properties that characterize strange stars. Our goal is to present the necessary concepts to understand this important theme of Astroparticles.
