The holographic screen at low temperatures

TL;DR

This paper explores how the holographic screen's vibrational spectrum at low temperatures influences thermal energy distribution and gravity laws, aligning with galactic rotation observations and connecting holographic parameters with MOND.

Contribution

It introduces a modified holographic screen model that explains galactic rotation curves and links holographic parameters with MOND acceleration.

Findings

Modified energy distribution over bits at low temperatures

Altered gravity law consistent with galaxy rotation curves

Connection between holographic parameters and MOND acceleration

Abstract

A permissible spectrum of transverse vibrations for the holographic screen modifies both a distribution of thermal energy over bits at low temperatures and the law of gravitation at small accelerations of free fall in agreement with observations of flat rotation curves in spiral galaxies. This modification relates holographic screen parameters in de Sitter space-time with the Milgrom acceleration in MOND.