Novikov Coordinates and the Physical Description of Gravitational Collapse
Jaume de Haro

TL;DR
The paper demonstrates how Novikov coordinates, derived from radial geodesics, offer a physically transparent description of gravitational collapse, clarifying the difference between free-fall and static observer perspectives.
Contribution
It provides a direct derivation of Novikov coordinates from geodesics, offering a clear dynamical interpretation of black-hole and white-hole regions in gravitational collapse.
Findings
Novikov coordinates are obtained from radial geodesics with negative energy.
In Novikov coordinates, collapse completes in finite proper time for free-fall observers.
Schwarzschild coordinates depict an infinite time collapse, which is a coordinate artifact.
Abstract
We show that the Novikov coordinates can be obtained in a direct and physically transparent way from the radial geodesics of massive particles with negative energy in the Schwarzschild spacetime. These geodesics form a complete congruence that covers the entire spacetime. By rectifying this family of trajectories using the proper time as the time coordinate, the Novikov variables naturally emerge, providing a clear dynamical interpretation of the different regions usually identified as black-hole and white-hole sectors. In Novikov coordinates, observers at fixed spatial position follow free-fall trajectories. From their perspective, the gravitational collapse of a dust star is completed in a finite proper time, independently of their initial distance from the star. In contrast, observers described by Schwarzschild-Droste coordinates perceive the boundary of the collapsing star as…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Relativity and Gravitational Theory · Astrophysical Phenomena and Observations
