Other
Scientific paper
May 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011phrvd..83j3526j&link_type=abstract
Physical Review D, vol. 83, Issue 10, id. 103526
Other
1
Particle-Theory And Field-Theory Models Of The Early Universe, Thermodynamic Functions And Equations Of State, Nonequilibrium And Irreversible Thermodynamics, Dark Energy
Scientific paper
We discuss thermodynamics of electromagnetic radiation, with p=(1/3)ρ and S∝T3V, and of cosmic string loops, with p=-(1/3)ρ and S∝T-3V, where p stands for pressure, T temperature, ρ energy density, S entropy, and V volume. We write the thermodynamic formalisms under a common framework that illustrates their formal relationship and allows us to go from one to the other through a smooth transformation. From a microscopic perspective, these relations arise from the energy relations u(λ)=hc/λ for the photons of electromagnetic radiation, and u(l)=(c4/a2G)l for cosmic string loops, a being a numerical (dimensionless) constant and λ and l the radiation wavelength and the length of a loop; G, c, and h are the gravitational constant, the speed of light in vacuo, and the Planck constant, respectively. The corresponding thermodynamic behaviors are seen to be connected through a related thermal duality corresponding to the change of T by T*=Tc2/T, with Tc a reference temperature related to h, c, and G.
Jou David
Mongiovì Maria Stella
Sciacca Michele
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