Quantum particle statistics on the holographic screen leads to Modified Newtonian Dynamics (MOND)
E. Pazy, N. Argaman

TL;DR
This paper derives Modified Newtonian Dynamics (MOND) from a thermodynamic and quantum statistical perspective of holographic screens, linking the acceleration scale to quantum properties of fermionic or bosonic excitations.
Contribution
It introduces a novel quantum statistical mechanical framework for MOND, connecting the acceleration scale to the Fermi energy and deriving the interpolating function from first principles.
Findings
Derived the MOND acceleration scale from holographic fermionic degrees of freedom.
Calculated the MOND interpolating function using quantum statistics and matched it with phenomenological models.
Reinterpreted cosmological implications of MOND, linking $a_0$ to the Hubble constant and cosmological constant.
Abstract
Employing a thermodynamic interpretation of gravity based on the holographic principle and assuming underlying particle statistics, fermionic or bosonic, for the excitations of the holographic screen leads to Modified Newtonian Dynamics (MOND). A connection between the acceleration scale appearing in MOND and the Fermi energy of the holographic fermionic degrees of freedom is obtained. In this formulation the physics of MOND results from the quantum-classical crossover in the fermionic specific heat. However, due to the dimensionality of the screen, the formalism is general and applies to two dimensional bosonic excitations as well. It is shown that replacing the assumption of the equipartition of energy on the holographic screen by a standard quantum-statistical-mechanics description wherein some of the degrees of freedom are frozen out at low temperatures is the physical basis…
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