Fractional dark energy: phantom behavior and negative absolute temperature
Ricardo G. Landim

TL;DR
This paper explores an extended fractional dark energy model incorporating chemical potential and negative absolute temperatures, revealing potential phantom behavior and cosmological implications consistent with observations.
Contribution
It introduces a thermodynamic extension of the fractional dark energy model with chemical potential and links it to negative absolute temperatures in cosmology.
Findings
The model can describe phantom regimes thermodynamically.
Constraints from Planck data limit the chemical potential to temperature ratio.
Negative absolute temperatures are compatible with cosmological evolution at high redshift.
Abstract
The fractional dark energy (FDE) model describes the accelerated expansion of the Universe through a nonrelativistic gas of particles with a noncanonical kinetic term. This term is proportional to the absolute value of the three-momentum to the power of , where is simply the dark energy equation of state parameter, and the corresponding energy leads to an energy density that mimics the cosmological constant. In this paper we expand the fractional dark energy model considering a non-zero chemical potential and we show that it may thermodynamically describe a phantom regime. The Planck constraints on the equation of state parameter put upper limits on the allowed value of the ratio of the chemical potential to the temperature. In the second part, we investigate the system of fractional dark energy particles with negative absolute temperatures (NAT). NAT are possible in quantum…
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