Emerging the dark sector from thermodynamics of cosmological systems with constant pressure

  • Alejandro Aviles
  • Norman Cruz
  • Jaime Klapp
  • Orlando Luongo
Research Article

Abstract

We investigate the thermodynamics of general fluids that have the constriction that their pressure is constant. We first consider the more general thermodynamic properties of this class of fluids finding the important result that for them adiabatic and isothermal processes should coincide. We therefore study their behaviors in curved space-times where local thermal equilibrium can be appealed. Thus, we show that this dark fluid degenerates with the dark sector of the \(\Lambda \)CDM model only in the case of adiabatic evolution. We demonstrate that, adding dissipative processes, a phantom behavior can occur and finally we further highlight that an arbitrary decomposition of the dark sector, into ad hoc dark matter and dark energy terms, may give rise to phantom dark energy, whereas the whole dark sector remains non-phantom.

Keywords

Dark sector Thermodynamics of dark energy Dark degeneracy 

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Copyright information

© Springer Science+Business Media New York 2015

Authors and Affiliations

  • Alejandro Aviles
    • 1
  • Norman Cruz
    • 2
  • Jaime Klapp
    • 1
    • 3
  • Orlando Luongo
    • 4
    • 5
    • 6
  1. 1.Departamento de MatemáticasCinvestav del Instituto Politécnico Nacional (IPN)MexicoMexico
  2. 2.Departamento de FísicaUniversidad de Santiago de ChileSantiagoChile
  3. 3.Departamento de FísicaInstituto Nacional de Investigaciones NuclearesMexicoMexico
  4. 4.Dipartimento di FisicaUniversità di Napoli “Federico II”NapoliItaly
  5. 5.Istituto Nazionale di Fisica Nucleare (INFN), Sezione di NapoliNapoliItaly
  6. 6.Instituto de Ciencias NuclearesUniversidad Nacional Autónoma de México (UNAM)MexicoMexico

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