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Titlebook: Astrophysics; An Introduction to T Karl-Heinz Spatschek Textbook 20241st edition The Editor(s) (if applicable) and The Author(s), under exc

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發(fā)表于 2025-3-21 18:27:02 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
期刊全稱(chēng)Astrophysics
期刊簡(jiǎn)稱(chēng)An Introduction to T
影響因子2023Karl-Heinz Spatschek
視頻videohttp://file.papertrans.cn/164/163688/163688.mp4
發(fā)行地址Provides an understandable introduction to astrophysics and cosmology.Suitable for beginners and advanced users.Covers astrophysical fundamentals, an introduction to general relativity and cosmology
圖書(shū)封面Titlebook: Astrophysics; An Introduction to T Karl-Heinz Spatschek Textbook 20241st edition The Editor(s) (if applicable) and The Author(s), under exc
影響因子.This textbook offers a comprehensible introduction to the physical fundamentals of the processes in our universe. The first chapters cover the observational possibilities of astrophysical quantities, cosmic rays, star formation and evolution, and galaxy formation and modeling. Subsequently, the basics of general relativity and different phenomena such as gravitational waves and black holes are covered. The book concludes with an introduction to cosmology: In addition to traditional homogeneous approaches, inhomogeneous cosmology in particular is given a broader scope in this new edition. Current inflationary models are presented.?.The book is intended for students of physics at the undergraduate, bachelor, and master levels, but it also offers a readable and easy-to-understand introduction for people with a basic knowledge of mathematics and physics who are interested in the natural sciences.?.Contents.Some important physical basics - observational possibilities - cosmic rays - stellar structure and stellar evolution - final stages of burning stars - galaxies - Newtonian cosmology - computational rules of ART - ART effects - relativistic stars and stellar dynamics - homogeneous co
Pindex Textbook 20241st edition
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Final Stages of Luminous Starsforms are in the foreground. We discuss compact objects such as white dwarfs and neutron stars, but also quasars and black holes. But ultimately, these states will also continue to change. In part, they will explode or give up their structure through radiation and nuclear decay. In most compact obje
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Textbook 20241st editionences.?.Contents.Some important physical basics - observational possibilities - cosmic rays - stellar structure and stellar evolution - final stages of burning stars - galaxies - Newtonian cosmology - computational rules of ART - ART effects - relativistic stars and stellar dynamics - homogeneous co
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發(fā)表于 2025-3-22 10:05:23 | 只看該作者
Forward Kinematics: Making Things Walkies of celestial bodies and the processes occurring there. One of the most important tasks of astronomical and astrophysical research is the classification of objects in space and time (Kitchin, Astronomical techniques. IoP Publishing, 2003).
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Basics of Actionscript for Animation (Milky Way) and then turn to the classification of the abundance of galaxies [3, 36]. Subsequently, we summarize evidence for the existence of Dark Matter and introduce the important new field of numerical modeling using .CDM models. This ultimately leads to the question of the embedding of galaxies in the universe.?
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Basics of Actionscript for Animationhe one hand. On the other hand, we have already discussed the existence ranges of stable objects. The GRT becomes mandatory in many areas when a tendency towards collapsing structures sets in. The most well-known example is a black hole, whose properties are also illuminated here.
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發(fā)表于 2025-3-23 03:56:52 | 只看該作者
Foundation ActionScript Animationsical” form, in which the cosmos is assumed to be completely homogeneous and isotropic. The Robertson-Walker metric is used in this case. Inhomogeneous cosmology takes into account density and temperature fluctuations. We begin with homogeneous cosmology.
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發(fā)表于 2025-3-23 05:39:03 | 只看該作者
Forward Kinematics: Making Things Walkreby support the described Big Bang scenario. We start with the “oldest” argument for the correctness of Big Bang world models, which is based on a prediction for the nucleosynthesis. Figure 11.1 refers back to Fig. 10.14 and shows further possibilities for verifying a Big Bang world model, which will be presented in the following chapters:
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