To minimise misunderstanding, scientists talk about thermodynamic values in terms of a system and its surroundings. The system’s surroundings are made up of everything that isn’t a part of system. A barrier separates the system from its surroundings. If the system contains one mole of gas in a container, the boundary is merely the container’s inner wall. The container, as well as everything outside of the boundary, is considered the surroundings.
The border must be precisely specified to determine whether a given region of the world is part of the system or not. The system is said to be closed if the matter cannot travel across the boundary; otherwise, it is said to be open. Unless the system is isolated, in which case no matter nor energy can travel across the barrier, a closed system can nevertheless exchange energy with its surroundings.
After knowing the introduction to thermodynamics, let’s discuss the first law of thermodynamics.
The First Law of Thermodynamics
Though it may appear complicated, the concept is quite simple. When you add heat to a system, you can only do one of two things: modify the system’s internal energy or make the system work (or, of course, some combination of the two). All of the heat energy must be used to accomplish these tasks.
Mathematical Representation of the First Law
For the quantities in the first law of thermodynamics, physicists often employ multiple equations of thermodynamics. They are as follows:
• U1 (or Ui) is equal to the initial internal energy of the process at the start
• At the end of the procedure, U2 (or Uf) equals the final internal energy.
• delta-U is equal to U2 – U1 is equal to Internal Energy Change.
• Q is the amount of heat that is moved into (Q > 0) or out of (Q < 0) the system.
• W denotes the amount of work done by the system (W < 0) or on the system (W > 0).
This produces a mathematical representation of the first law that is quite useful and can be rewritten in a variety of ways:
At least in a physics classroom setting, analysing a thermodynamic process often entails analysing a condition in which one of these values is either 0 or at least controllable in a sensible manner. For example, in an adiabatic process, heat transfer (Q) is zero, but work (W) is zero in an isochoric process.
The Second Law of Thermodynamics
This is one of the popular thermodynamics laws that can be expressed in various ways, as will be discussed shortly, but it is essentially a law that, unlike most other laws in physics, deals exclusively with limiting what can be done rather than how to accomplish it.
It is a law that states that nature prevents us from achieving certain outcomes without putting in a lot of effort, and as such, it is intimately linked to the concept of energy conservation, much like the first law of thermodynamics.
The Third Law of Thermodynamics
The third rule of thermodynamics is essentially a statement concerning the capacity to build an absolute temperature scale, with absolute zero being the exact point where a solid’s internal energy is zero.
The following three hypothetical equations of thermodynamics have been found in various sources:
• No system can be reduced to absolute zero in a finite number of operations.
• The energy of a single crystal of an element in its most steady position tends to zero as the temperature approaches absolute zero.
• As a system’s temperature approaches absolute zero, its entropy approaches a constant.
• In practice, this law means that any heat engine or comparable device based on thermodynamic principles cannot be 100% efficient, even in theory.
Consequences of the Laws of Thermodynamics
The thermodynamics laws are quite simple to say and comprehend to the point that it’s easy to overlook their significance. They impose limitations on how energy can be used in the universe, among other things. It’s difficult to overestimate the importance of this topic. The rules of thermodynamics have an impact on practically every element of scientific research in some way.
Conclusion
The thermodynamics laws aren’t very concerned with the how and why of heat transport, which makes sense for laws written before the atomic theory was widely accepted. The laws of thermodynamics have evolved to become some of the most basic rules that must be obeyed when a thermodynamic system undergoes an energy change. They are concerned with the aggregate total of energy and heat transitions inside a system and do not take into account the atomic or molecular nature of heat transference.