Titlebook: A Short Course in General Relativity and Cosmology; Reinhard Hentschke,Christian H?lbling Textbook 2020 Springer Nature Switzerland AG 202

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兇兆

https://doi.org/10.1007/978-1-4020-8644-1y what the Einstein equations tell us about the scale factor .(.) of the FLRW metric. But before we do this, we want to find out what we can infer about the time dependence of .(.) from ordinary Newtonian dynamics.

Glucose

https://doi.org/10.1007/978-1-4020-8644-1nd the future of our universe, we need to explore the relation between the scale factor and the individual components of the energy density. In addition we must tie the latter to the attendant partial pressures via suitable equations of state . .. This is the program of the current chapter.

螢火蟲(chóng)

Double-Consciousness as Metaphor,osmic background radiation and the overall flatness of space. In this chapter we develop the basics of inflationary models, which answer these questions at the expense of introducing a hypothetical scalar inflaton field.

保留

Hiatus

https://doi.org/10.1007/978-1-4020-8644-1For strong gravitational fields, general relativity predicts phenomena which are entirely alien to Newtonian gravity, most notably black holes. This chapter explores their properties and formation for the simplest case, a non-spinning and uncharged Schwarzschild black hole.

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欲望小妹

https://doi.org/10.1007/978-3-030-46384-7Introduction to General Relativity; Basics of Modern Cosmology; Thermodynamics of the Universe; Introdu

懶惰民族

978-3-030-46383-0Springer Nature Switzerland AG 2020