Vidaña Isaac
Istituto Nazionale di Fisica Nucleare, Dipartimento di Fisica, Università di Catania, Via Santa Sofia 64, 95123, Catania, Italy.
Proc Math Phys Eng Sci. 2018 Sep;474(2217):20180145. doi: 10.1098/rspa.2018.0145. Epub 2018 Sep 19.
We review the role and properties of hyperons in finite and infinite nuclear systems. In particular, we present different production mechanisms of hypernuclei, as well as several aspects of hypernuclear -ray spectroscopy, and the weak decay modes of hypernuclei. Then we discuss the construction of hyperon-nucleon and hyperon-hyperon interactions on the basis of the meson-exchange and chiral effective field theories. Recent developments based on the so-called approach and lattice quantum chromodynamics will also be addressed. Finally, we go over some of the effects of hyperons on the properties of neutron and proto-neutron stars with an emphasis on the so-called 'hyperon puzzle', i.e. the problem of the strong softening of the equation of state, and the consequent reduction of the maximum mass, induced by the presence of hyperons, a problem which has become more intriguing and difficult to solve due the recent measurements of approximately 2 millisecond pulsars. We discuss some of the solutions proposed to tackle this problem. We also re-examine the role of hyperons on the cooling properties of newly born neutron stars and on the development of the so-called r-mode instability.
我们回顾了超子在有限和无限核系统中的作用及性质。特别地,我们介绍了超核的不同产生机制、超核γ射线光谱学的几个方面以及超核的弱衰变模式。然后我们基于介子交换和手征有效场理论讨论了超子 - 核子和超子 - 超子相互作用的构建。还将探讨基于所谓的 方法和格点量子色动力学的最新进展。最后,我们研究超子对中子星和原中子星性质的一些影响,重点关注所谓的“超子难题”,即由于超子的存在导致状态方程强烈软化以及随之而来的最大质量降低的问题,由于最近对大约2毫秒脉冲星的测量,这个问题变得更加引人入胜且难以解决。我们讨论了为解决这个问题而提出的一些方案。我们还重新审视了超子在新生中子星冷却性质以及所谓的r模式不稳定性发展方面的作用。