Singular Strings in the Rotating Astrophysical Sources: a New Conjecture on the QPOs and Jet Phenomena

TL;DR

This paper proposes that singular strings arising from Kerr geometry could explain key astrophysical phenomena like jets and quasi-periodic oscillations in rotating compact objects.

Contribution

It introduces a novel conjecture linking Kerr solution analyticity to singular strings as sources of jets and QPOs.

Findings

Singular strings may originate from Kerr geometry's analyticity.

These strings could be responsible for jets in astrophysical sources.

They may also explain quasi-periodic oscillations in accreting systems.

Abstract

Stringy and disklike sources of the rotating compact astrophysical objects are considered on the base of the Kerr geometry. It is argued that analyticity of the Kerr solutions may result the appearance of singular strings, which may be the source of two important astrophysical effects: the jets and QPOs phenomena.