原始黑洞以及弦如何在早期宇宙中形成物质

David McGraw Jr.
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摘要

C-中微子是推动宇宙诞生的主要粒子。它衰变成其他粒子,包括质子和电子。原始黑洞对我们宇宙的发展也很重要。它们连接着宇宙射线来源的天体物理学约束。原始黑洞在元素丰度和 CMB 光谱中扮演着重要角色。它们是粒子和物质的创造者。原始黑洞可以是我们时空中任何种类粒子的来源。最终,它们可以为宇宙学问题带来新的启示。原始黑洞是早期宇宙中不均匀原始结构的解决方案。C-中微子是促进创世的粒子,也是我们宇宙中暗物质的组成部分。它是我们宇宙中暗物质的主要来源。在早期宇宙中,宇宙学原理并不存在。我们今天看到的不均匀宇宙是在宇宙诞生后大约 10 亿年演变而来的。
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Primordial Black Holes And How Strings Get Created Into Matter In The Early Universe
The C-Neutralino is the major particle that drives the beginning of our universe. It decays into other particles including protons and electrons. Primordial Black Holes are also important in the development of our universe. They connect astrophysical constraints on sources of cosmic rays. Primordial Black Holes play a role in element abundance and the spectrum of the CMB. They are particle and matter creators. Primordial Black Holes can be a source of any species of particles in our space-time. In the end, they can shed new light on problems in Cosmology. Primordial Black Holes are the solution to inhomogeneous primordial structures in the early universe. C-Neutralinos are the particle that contributes to creation and also contribute to dark matter in our universe. It is the major source of dark matter in our universe. In the early universe, the cosmological principle did not exist. The inhomogeneous universe we see today evolved after about 1 billion years after the creation of our universe.
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