熱物理概念

內(nèi)容概要

　　《國(guó)際著名物理圖書·影印版系列：熱物理概念·熱力學(xué)與統(tǒng)計(jì)物理學(xué)（第2版）》詳細(xì)介紹了作為熱力學(xué)和統(tǒng)計(jì)物理學(xué)基礎(chǔ)的一些主要原理以及它們的應(yīng)用。書中以非常清晰的方式介紹和討論了熱力學(xué)和統(tǒng)計(jì)物理學(xué)中一些核心的概念，通過(guò)非常豐富的實(shí)例來(lái)說(shuō)明新的概念、方法和原理，對(duì)于相關(guān)的歷史背景和發(fā)現(xiàn)過(guò)程也作了比較具體的描述。該書關(guān)于概念、原理和方法的應(yīng)用涉及天體物理，大氣物理，信息和通信理論，凝聚態(tài)物理等眾多學(xué)科，體現(xiàn)了基本理論和方法的廣泛適用性。此外，每章末包含了小結(jié)，可以深入學(xué)習(xí)的文獻(xiàn)簡(jiǎn)介以及許多的習(xí)題，有助于加深對(duì)概念、原理和方法的理解?！　　秶?guó)際著名物理圖書·影印版系列：熱物理概念·熱力學(xué)與統(tǒng)計(jì)物理學(xué)（第2版）》可作為綜合大學(xué)或師范院校物理學(xué)以及相關(guān)專業(yè)的熱力學(xué)統(tǒng)計(jì)物理課程的教材。

作者簡(jiǎn)介

作者：（英國(guó)）布隆代爾（Stephen J.Blundell） （英國(guó)）布隆代爾（Katherine M.Blundell）

書籍目錄

前言 第2版前言 Ⅰ準(zhǔn)備知識(shí)  1引言 1.1摩爾是什么？ 1.2熱力學(xué)極限 1.3理想氣體 1.4組合問(wèn)題 1.5本書的計(jì)劃 練習(xí) 2熱量 2.1熱量的定義 2.2熱容量 練習(xí) 3概率 3.1離散概率分布 3.2連續(xù)概率分布 3.3線性變換 3.4方差 3.5線性變換和方差 3.6獨(dú)立變量 3.7二項(xiàng)分布 進(jìn)一步讀物 練習(xí) 4溫度和Boltzmann因子 4.1熱平衡 4.2溫度計(jì) 4.3微觀態(tài)和宏觀態(tài) 4.4溫度的統(tǒng)計(jì)定義 4.5系綜 4.6正則系綜 4.7 Boltzmann分布的應(yīng)用 進(jìn)一步讀物 練習(xí) Ⅱ氣體動(dòng)理學(xué)理論 5 Maxwell—Boltzmann分布 5.1速度分布 5.2速率分布 5.3實(shí)驗(yàn)驗(yàn)證 練習(xí) 6壓強(qiáng) 6.1分子分布 6.2理想氣體定律 6.3 Dolton定律 練習(xí) 7分子瀉流 7.1流密度 7.2瀉流 練習(xí) 8平均自由程和碰撞 8.1平均碰撞時(shí)間 8.2碰撞截面 8.3平均自由程 Ⅲ輸運(yùn)和熱擴(kuò)散 9氣體的輸運(yùn)性質(zhì) 9.1黏性 9.2熱導(dǎo)率 9.3擴(kuò)散 9.4更細(xì)致的理論 進(jìn)一步讀物 練習(xí) 10熱擴(kuò)散方程 10.1熱擴(kuò)散方程的導(dǎo)出 10.2一維熱擴(kuò)散方程 10.3穩(wěn)態(tài) 10.4球的熱擴(kuò)散方程 10.5 Newton冷卻定律 10.6 Prandtl數(shù) 10.7熱源 10.8粒子擴(kuò)散 練習(xí) Ⅳ第一定律 11能量 11.1一些定義 11.2熱力學(xué)第一定律 11.3熱容量 練習(xí) 12等溫過(guò)程和絕熱過(guò)程 12.1可逆性 12.2理想氣體的等溫膨脹 12.3理想氣體的絕熱膨脹 12.4絕熱大氣 練習(xí) Ⅴ第二定律 13熱機(jī)和第二定律 13.1熱力學(xué)第二定律 13.2 Carnot熱機(jī) 13.3 Carnot定理 13.4 Clausius表述與Kelvin表述的等價(jià)性 13.5熱機(jī)實(shí)例 13.6逆向運(yùn)行的熱機(jī) 13.7 Clausius定理 進(jìn)一步讀物 練習(xí) 14熵 14.1熵的定義 14.2不可逆變化 14.3再論第一定律 14.4 Joule膨脹 14.5熵的統(tǒng)計(jì)基礎(chǔ) 14.6混合的熵 14.7 Maxwell妖 14.8熵和概率 練習(xí) 15信息論 15.1信息和Shannon熵 15.2信息和熱力學(xué) 15.3數(shù)據(jù)壓縮 15.4量子信息 15.5條件概率和聯(lián)合概率 15.6 Bayes定理 進(jìn)一步讀物 練習(xí) Ⅵ熱力學(xué)應(yīng)用 16熱力學(xué)勢(shì) 16.1內(nèi)能U 16.2焓H 16.3 Helmholtz函數(shù)F 16.4 Gibbs函數(shù)G 16.5約束 16.6 Maxwell關(guān)系 練習(xí) 17桿，氣泡和磁體 17.1彈性桿 17.2表面張力 17.3電偶極子和磁偶極子 17.4順磁性 練習(xí) 18第三定律 18.1第三定律的不同表述 18.2第三定律的一些結(jié)果 練習(xí) Ⅶ統(tǒng)計(jì)力學(xué) 19能量均分 19.1能量均分定理 19.2應(yīng)用 19.3所作假設(shè) 19.4 Brown運(yùn)動(dòng) 練習(xí) …… Ⅷ超越理想氣體 Ⅸ 特殊專題 A基本常數(shù) B有用的公式 C有用的數(shù)學(xué) D電磁譜 E一些熱力學(xué)定義 F熱力學(xué)展開(kāi)公式 G約化質(zhì)量 H主要符號(hào)總表 參考文獻(xiàn) 索引

章節(jié)摘錄

版權(quán)頁(yè)：   插圖：   1.2 The thermodynamic limit In this section, we will explain how the large numbers of molecules ina typical thermodynamic system mean that it is possible to deal withaverage quantities. Our explanation proceeds using an analogy: imaginethat you are sitting inside a tiny hut with a fiat roof. It is rainingoutside, and you can hear the occasional raindrop striking the roof. Theraindrops arrive randomly, so sometimes two arrive close together, butsometimes there is quite a long gap between raindrops. Each raindroptransfers its momentum to the roof and exerts an impulse2 on it. If youknew the mass and terminal velocity of a raindrop, you could estimatethe force on the roof of the hut. The force as a function of time wouldlook like that shown in Fig. 1.1(a), each little blip corresponding to theimpulse from one raindrop. Now imagine that you are sitting inside a much bigger hut with a fiatroof a thousand times the area of the first roof. Many more raindropswill now be falling on the larger roof area and the force as a function oftime would look like that shown in Fig. 1.1(b). Now scale up the areaof the fiat roof by a further factor of one hundred and the force wouldlook like that shown in Fig. 1.1. Notice two key things about thesegraphs: (1) The force, on average, gets bigger as the area of the roof getsbigger. This is not surprising because a bigger roof catches moreraindrops. (2) The fluctuations in the force get smoothed out and the force lookslike it stays much closer to its average value. In fact, the fluctuations are still big but, as the area of the roof increases, they growmore slowly than the average force does. The force grows with area, so it is useful to consider the pressure, whichis defined as The average pressure due to the falling raindrops will not change as thearea of the roof increases, but the fluctuations in the pressure will decrease. In fact, we can completely ignore the fluctuations in the pressurein the limit that the area of the roof grows to infinity. This is preciselyanalogous to the limit we refer to as the thermodynamic limit. Consider now the molecules of a gas which are bouncing around in acontainer. Each time the molecules bounce off the walls of the container,they exert an impulse on the walls. The net effect of all these impulses isa pressure, a force per unit area, exerted on the walls of the container. Ifthe container were very small, we would have to worry about fluctuationsin the pressure (the random arrival of individual molecules on the wall,much like the raindrops in Fig. 1.1(a)). However, in most cases that onemeets, the number of molecules in a container of gas is extremely large,so these fluctuations can be ignored and the pressure of the gas appearsto be completely uniform. Again, our description of the pressure of thissystem can be said to be "in the thermodynamic limit", where we havelet the number of molecules be regarded as tending to infinity in such away that the density of the gas is a constant.

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《熱物理概念:熱力學(xué)與統(tǒng)計(jì)物理學(xué)(第2版)》可作為綜合大學(xué)或師范院校物理學(xué)以及相關(guān)專業(yè)的熱力學(xué)統(tǒng)計(jì)物理課程的教材。

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