Titlebook: Introduction to Particle Cosmology; The Standard Model o Cosimo Bambi,Alexandre D. Dolgov Textbook 2016 Springer-Verlag GmbH Germany, part

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使虛弱

General Relativity, This chapter provides a short review of important concepts and some technicalities of the gravitational theory. It can serve as a very brief introduction to the Einstein theory of gravity. It contains all the necessary material to understand the next chapters of this book. With this spirit, we foll

反叛者

The Standard Model of Particle Physics,al forces of Nature except gravity. It is the second fundamental ingredient of the Standard Model of cosmology. Here matter is described by fermions, spin-1/2 particles. Fermions are grouped into two classes, namely leptons and quarks, on the basis of their interaction properties. Leptons participat

Jocose

Cosmological Models, hypothesis, we can derive a number of cosmological models that differ by their matter content. In all the physically interesting cases, the Universe starts from an extremely dense and hot state. The onset of this hot initial state is called big bang. The rate of the expansion and the fate of the Un

盲信者

Awning

Albinism

不法行為

Big Bang Nuclesynthesis,ical predictions of the abundances of deuterium, helium-3, helium-4, and lithium-7 are determined by the Friedmann equations, the matter content of the Standard Model of particle physics, and a large number of particle properties and nuclear reaction rates that can be measured in laboratory. With al

大方一點(diǎn)

Dark Matter,ctuations of the CMB, suggests that most of the matter in the Universe does not emit electromagnetic radiation. This stuff is usually called dark matter and its nature is currently unknown. From the BBN, we can indeed infer that dark matter is unlikely made of ordinary particles (protons, neutrons,

anthropologist

Cosmic Microwave Background,light elements. As the Universe expanded, at a certain point photons in the primordial plasma decoupled from protons and electrons and started freely propagating through the Universe. These are the photons we observe today in the CMB. The spectrum is extremely close to that of a black body with a te