The holostar - a self-consistent model for a compact self-gravitating object
Michael Petri (Bundesamt fuer Strahlenschutz, Salzgitter, Germany)

TL;DR
The holostar is a novel, exact solution to Einstein's equations that models a black-hole-like object without singularities or horizons, with properties matching cosmological observations and supporting a holographic principle.
Contribution
It introduces the holostar as a self-consistent, horizonless, singularity-free model with properties similar to black holes and the universe, aligning with holographic and thermodynamic principles.
Findings
Holostar's temperature inversely proportional to square root of radius.
Total particle number proportional to boundary area.
Geodesic motion mimics cosmological expansion and temperature decrease.
Abstract
The holostar is an exact spherically symmetric solution to the field equations of general relativity with anisotropic interior pressure. Its properties are similar to a black hole. It has an internal temperature inverse proportional to the square root of the radial coordinate value, from which the Hawking temperature law follows. The number of particles within any concentric region of the holostar's interior is proportional to the proper area of its boundary. The holostar-metric is static throughout the whole space-time. There are no trapped surfaces, no singularity and no event horizon. Information is not lost. The weak and strong energy conditions are fulfilled everywhere, except for a Planck-size region at the center. Geodesic motion of massive particles in a large holostar is similar to what is observed in the universe today: A material observer moving geodesically experiences an…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Relativity and Gravitational Theory
