Effects of Matter Creation on the Heat Engine in the FRW Universe


Sevinç Ö.

İstanbul Yeni Yüzyıl Üniversitesi 10. Bilim Günleri Kongresi, İstanbul, Türkiye, 15 - 16 Nisan 2025, ss.64, (Özet Bildiri)

  • Yayın Türü: Bildiri / Özet Bildiri
  • Basıldığı Şehir: İstanbul
  • Basıldığı Ülke: Türkiye
  • Sayfa Sayıları: ss.64
  • İstanbul Yeni Yüzyıl Üniversitesi Adresli: Evet

Özet

Matter creation in the FRW universe can have significant effects on the operation of a heat engine by altering the equation of state, increasing entropy, modifying energy exchange processes, influencing the expansion rate, and introducing non-equilibrium thermodynamic effects.

In a standard FRW universe, the equation of state relates the pressure p and energy density ρ of the cosmic fluid. Matter creation can alter this relationship, leading to a modified equation of state. This modification can affect the thermodynamic cycles of the heat engine, potentially changing the efficiency and work output. The temperature of the cosmic fluid evolves with the expansion of the universe. Matter creation can affect this temperature evolution, which in turn influences the heat engine's performance. For instance, if matter creation leads to a slower cooling rate, the heat engine might operate over a different temperature range, affecting its efficiency. In a cosmological heat engine, work extraction is related to the expansion of the universe. Matter creation can modify the work extraction process by changing the pressure and energy density of the cosmic fluid. This could either enhance or diminish the amount of work that can be extracted, depending on the specific model of matter creation. The efficiency η of the heat engine is expressed similarly to the Carnot cycle:re, ​ and ​ represent the high temperature of the early universe and the low temperature of the late universe, respectively.In cosmology, the universe can be explained by the laws of thermodynamics, considering it as a heat engine. This approach provides a useful model for displaying data about the universe, such as energy transfer and entropy changes. This model is an important tool, especially in the analysis of modern cosmological problems such as dark energy and the dynamics of the universe.