The Astrophysical Processes of Cosmological Hydrogen that Generate the Chemical Elements that Make up the Universe

M. J. Gómez, Salvador Galindo Uribarri, Olga B. Benítez López
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Abstract

The objective of the present article is to explain how all the chemical elements were formed from the big bang generated element: hydrogen. The methodology used was to analyze the main cosmological and astrophysical processes in order to explain the origin of all the known chemical elements. The main results are: Hydrogen cannot be formed in any part of the actual universe; it must come from the Big Bang. Helium and a little bit of lithium can have a cosmological origin associated to the Big Bang nucleosynthesis and the recombination process. The elements with an atomic number between 3 and 26 were, and continue to be, synthetized by nuclear fusion reactions inside the core of massive stars and liberated by explosion when the stars go supernovae, at the end of their lives. In the process of going supernova, elements with a medium atomic number, between 27 and 40, are created. All the elements with an atomic number larger than 40 were generated by neutron star collisions. When Mendeleev and Lothar Meyer designed an ordered arrangement of chemical elements, their tables included the 63 chemical elements known in 1869. A century and a half later, the known elements are 118. By studying different topics related to the elements, it was possible to uncover fundamental particles, such as quarks and leptons, and the strong and weak nuclear forces that form the baryonic part of the universe. The Sun was formed 6000 million years ago and its planets, including earth, were formed 4600 million years ago when and where there were debris of different stars that went supernova, in particular 1A type, and also debris, of at least one of a binary neutron star collision, so to attain, all the elements that have been identified in the solar system, and especially in earth. In addition, the current “periodic table” includes 26 synthetic elements that were produced in neutron star collisions but, because of their short lifetimes, they are not found, on earth. The vast quantities of the elements, produced during the aforementioned astrophysical processes, clustered into planets, stars and galaxies; and at least in one planet, our earth, some chemical elements organized themselves into living creatures.
宇宙氢产生构成宇宙的化学元素的天体物理过程
这篇文章的目的是解释所有的化学元素是如何从大爆炸产生的元素:氢中形成的。所使用的方法是分析主要的宇宙学和天体物理学过程,以解释所有已知化学元素的起源。主要结果是:氢不可能在实际宇宙的任何地方形成;它一定来自大爆炸。氦和少量锂的宇宙起源可能与大爆炸的核合成和重组过程有关。原子序数在3到26之间的元素,过去和现在都是由大质量恒星内部的核聚变反应合成的,当恒星在生命结束时变成超新星时,它们会被爆炸释放出来。在成为超新星的过程中,会产生原子序数在27到40之间的中等元素。所有原子序数大于40的元素都是由中子星碰撞产生的。门捷列夫和洛萨·迈耶设计了一个化学元素的有序排列,他们的元素表包括了1869年已知的63种化学元素。一个半世纪后,已知的元素有118种。通过研究与元素相关的不同主题,有可能发现基本粒子,如夸克和轻子,以及形成宇宙重子部分的强核力和弱核力。太阳形成于60亿年前它的行星,包括地球,形成于46亿年前那里有不同恒星的残骸变成了超新星,特别是1A型,还有至少一个双中子星碰撞的残骸,所以要获得所有在太阳系中被识别的元素,尤其是在地球上。此外,目前的“元素周期表”包括26种合成元素,这些元素是在中子星碰撞中产生的,但由于它们的寿命很短,所以在地球上找不到。在上述天体物理过程中产生的大量元素聚集成行星、恒星和星系;至少在一个星球上,我们的地球上,一些化学元素自己组织成生物。
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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