1. So we have first, a reversible process.

2. Expansion–contraction is a reversible process.

3. In reversible process, there is the entranspy conservation, that is, no loss of capability of heat transport.

4. They created a similar but reversible process that can either consume or release energy.

5. So for the reversible process, the work done is the integral under the pressure volume state function, the function of state.

6. The reversible process is going to be colder because it has to expend more energy.

7. So a reversible process leads to requiring certain quantities to be maximized.

8. Denaturation in some globular proteins can be a reversible process, unless the conditions causing denaturation are too severe.

9. if it's a reversible process then the equality holds, but if it's irreversible, which means it happens spontaneously, T then dS is greater than this.

10. Compare equilibrium state, intensity, intemal energy and reversible process with particle, force, potential energy and motion. Intercommunity was discovered.

11. So w, the work is less for the irreversible process than the reversible process.

12. Furthermore, the cyclic Voltammetry curve of gingerol indicated that the reaction was half reversible process.

13. This paper questioned the proposition " work done in a reversible process is maximum ", which can be seen in many physical chemistry textbooks.

14. Discussed is a simple closed system of an ideal gas regarded as reversible process[ ], in which only work of volume expansion is dene.

15. How many people vote for that this is a reversible process?

16. The spontaneous emission is controlled by microcavity, it can be enhanced or restrained, even can become a reversible process.

17. And obviously, since it was, since we threw up our hands, just with a simple reversible process like here, it's clear that we're going to throw up our hands a lot.

18. Moreover, if we consider the tunneling process as a reversible process, the result in Hawking radiation via tunneling is consistent with the first and second law of black hole thermodynamics.