统计热力学，又称统计力学，是19世纪下半叶和20世纪初随着原子和分子方法的发展而出现的。它解释了经典热力学。它从经典或量子力学的角度考虑单个粒子与其组合运动之间的微观合作。它的解释是基于这样一个事实:系统是由几种粒子或集体运动构成的，每种粒子的分支在某种意义上都是相同的。热力学定律与其他定律不同。总共有四个。它们是从0到4排列的。不是因为它们是按照发现的顺序排列的，而是因为它们特别有编号。第二定律不同于其它定律，对其它定律没有影响。它有不同的公式。第一定律描述了一个系统的内能的量，它是由动能和与环境有关的势能得到的。第一定律把封闭系统间的热传递描述为功。第二定律包括两种理论，即温度和熵。熵从一开始就显示出热力学过程能到达外部系统的功的极限，这个极限被称为不可逆性。温度的影响，这在一定程度上体现在第零定律中，第零定律把能量流动方向上的量作为热在两个系统之间的热连接，这被称为热和冷的常识.
澳洲统计热力学代写:原子和分子方法
Statistical Thermodynamics, also called statistical mechanics, appeared with the development of atomic and molecular approaches in the second half of the 19th century and early 20th century. It shows an explanation of classical thermodynamics. It considers the microscopic cooperation between individual particles and their combined motions, in terms of classical or of quantum mechanics. Its explanation is in terms of data that rest on the fact the system is built of several species of particles or collective motions, the branches of each species individually being in some sense all alike.The laws of thermodynamics are different from others. There’re altogether four of them. They’re arranged from zero to four. Not because they are arranged by discovery in order but because they are numbered some especially. The second law is different from others and there’re no effect on others. It has different formulas. The first law describe the quantity of internal energy of a system, which was found from kinetic energy and from its potential energy which relates to its surroundings. The first law describe the transferring of heat between closed system as work. The second law include two theories which is known as temperature and entropy. Entropy shows the limit which is known as irreversibility from the beginning, on the work that can reach to an external system by thermodynamics process. The effects of temperature, which halfway showed by the zeroth law, which has quantities in the direction of energy flow as heat between two system in thermal connection and which is known as common sense of hot and cold