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基本宇宙學(xué):從亞里士多德的宇宙到大爆炸(英文)

基本宇宙學(xué):從亞里士多德的宇宙到大爆炸(英文)

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作 者: [美]詹姆斯·J.科拉塔(James J Kolata)
出版社: 哈爾濱工業(yè)大學(xué)出版社
叢編項(xiàng):
標(biāo) 簽: 暫缺

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ISBN: 9787560389387 出版時(shí)間: 2021-06-01 包裝: 平裝-膠訂
開(kāi)本: 16開(kāi) 頁(yè)數(shù): 156 字?jǐn)?shù):  

內(nèi)容簡(jiǎn)介

  《基本宇宙學(xué):從亞里士多德的宇宙到大爆炸(英文)》是一部***的國(guó)外科普著作。中文書(shū)名可譯為——《基本宇宙學(xué):從亞里士多德的宇宙到大爆炸》,作者給出的其內(nèi)容簡(jiǎn)介為:宇宙學(xué)是對(duì)整個(gè)宇宙起源、大小和演化的研究,每一種文化都發(fā)展了一種宇宙論,無(wú)論它是基于宗教、哲學(xué)或科學(xué)原理。在這本書(shū)中,西方傳統(tǒng)文化中對(duì)宇宙的科學(xué)認(rèn)識(shí)是從早期的希臘哲學(xué)家發(fā)展到現(xiàn)代21世紀(jì)的觀點(diǎn)的。這本書(shū)一開(kāi)始是圣母大學(xué)為期一學(xué)期課程的一系列課堂筆記,叫作“基本宇宙學(xué)”。這是一門(mén)為非科學(xué)專業(yè)學(xué)生開(kāi)設(shè)的選修課,旨在讓沒(méi)有數(shù)學(xué)天賦的學(xué)生了解迄今為止宇宙學(xué)領(lǐng)域重要的發(fā)現(xiàn),以及這些發(fā)現(xiàn)是如何不斷改變我們對(duì)宇宙起源和結(jié)構(gòu)的認(rèn)知的?!痘居钪鎸W(xué):從亞里士多德的宇宙到大爆炸(英文)》考察了諸如:宇宙從何而來(lái)?為什么科學(xué)家現(xiàn)在確定它的誕生是在一個(gè)名為大爆炸的宇宙火球中?以及大爆炸本身從何而來(lái)?課程的重點(diǎn)是對(duì)科普讀物的課堂討論,為好奇和聰明的外行人提供閱讀材料,并終聚焦于20世紀(jì)末和21世紀(jì)初宇宙學(xué)中許多有趣和令人興奮的新發(fā)現(xiàn)。這本書(shū)的第二部分追溯了大爆炸理論本身的演變,包括近觀測(cè)到的宇宙本身隨時(shí)間加速膨脹的現(xiàn)象。此外,還討論了現(xiàn)代物理學(xué)對(duì)我們理解大爆炸機(jī)制的貢獻(xiàn),并描述了宇宙在其歷史上各個(gè)時(shí)期的狀態(tài)。后,介紹了一些超出當(dāng)前知識(shí)范圍的對(duì)宇宙學(xué)的推測(cè),并描述了我們對(duì)宇宙未來(lái)發(fā)展的理解。

作者簡(jiǎn)介

  詹姆斯·J.科拉塔(James J Kolata),他是美國(guó)圣母大學(xué)物理名譽(yù)教授,美國(guó)物理學(xué)會(huì)會(huì)員,也是核物理學(xué)界250多種出版物的作者。

圖書(shū)目錄

Preface
Acknowledgements
Author biography
1 The scientific method
1.1 Introduction to the scientific method
1.2 Some mathematics
2 Early astronomy
3 Nebulae
4 Cosmic distances
4.1 The cosmic distance ladder
4.1.1 The parallax view
4.1.2 The color of starlight
4.1.3 The Cepheid variables
4.1.4 The supernova scale
4.2 Spiral nebulae:are they extragalactic?
4.3 The chemical composition of stars
5 Space-time
5.1 The speed of light
5.2 The special theory of relativity
5.3 The general theory of relativity
5.4 Universal expansion
6 The Big Bang
6.1 The structure and history of the Universe
6.2 The geometry of space-time
6.3 The father of the Big Bang
6.4 The creation of the elements
7 Cosmic microwave background radiation
7.1 The 'smoking gun'of the Big Bang
7.2 Decoupling
7.3 How bright is the CMB?
7.4 ‘Matter dominated' versus ‘radiation dominated' Universes
7.5 How uniform is the CMB?
8 Dark matter
8.1 Dark matter defined
8.2 Non-baryonic dark matter
9 The standard model of cosmology
9.1 Nucleosynthesis
9.1.1 The first frame (t = 10-2 s)
9.1.2 The second frame (t = 10-1 s)
9.1.3 The third frame (t = 1 s)
9.1.4 The fourth frame (t = 10 s)
9.1.5 The fifth frame (t = 100 s)
9.1.6 Later frames
9.2 The birth and death of stars
9.3 The size of the Universe
10 The very early Big Bang
10.1 The four forces of nature
10.2 The quantum nature of forces
10.3 The unification of forces
10.4 The quark model
10.5 The leptons
10.6 The gluons
10.7 The standard model of high-energy physics
10.8 The history of the Universe: the early frames
10.9 Why matter rather than antimatter?
11 Inflation
11.1 The horizon problem
11.2 The flatness problem
11.3 The smoothness problem
11.4 The magnetic monopole problem
11.5 Inflation
11.6 How inflation solves the Big Bang problems
12 Dark energy
12.1 The curvature of space-time
12.2 The accelerating universal expansion
12.3 Dark energy and the CMB
12.4 Is there a signature of inflation in the CMB?
13 Higher dimensions
13.1 Field theories
13.2 Kaluza-Klein theory
13.3 Compactification
13.4 QED
13.5 Quantization of the weak and strong forces
13.6 Early attempts at a quantum theory of gravity
14 String theory
14.1 Particles and ‘string'
14.2 M-theory
14.3 The multiverse
15 Black holes and wormholes
15.1 The life of the Sun
15.2 The life of massive stars
15.3 Neutron stars
15.4 Black holes
15.5 Some properties of black holes
15.6 The thermodynamics of black holes
15.7 Hawking radiation
15.8 The singularity at the center of a black hole
16 Reading list
17 Links to astronomy websites
編輯手記

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