Holographic Thermodynamics Requires a Chemical Potential for Color
Manus R. Visser

TL;DR
This paper derives a thermodynamic Euler equation for large-N gauge theories from holography, highlighting the necessity of a chemical potential for color and connecting it to black hole thermodynamics.
Contribution
It establishes a holographic derivation of the Euler equation including a chemical potential for color, linking gauge theory thermodynamics to black hole physics.
Findings
The Euler equation relates energy to temperature, entropy, degrees of freedom, and chemical potential.
The Euler equation corresponds to the generalized Smarr formula for AdS black holes.
Thermodynamic variational principles match black hole first law extended to cosmological and gravitational constants.
Abstract
The thermodynamic Euler equation for high-energy states of large- gauge theories is derived from the dependence of the extensive quantities on the number of colors . This Euler equation relates the energy of the state to the temperature, entropy, number of degrees of freedom and its chemical potential, but not to the volume or pressure. In the context of the gauge/gravity duality we show that the Euler equation is dual to the generalized Smarr formula for black holes in the presence of a negative cosmological constant. We also match the fundamental variational equation of thermodynamics to the first law of black hole mechanics, when extended to include variations of the cosmological constant and Newton's constant.
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