J 2025

Photons shells inner structure and causal properties

PUGLIESE, Daniela and Zdeněk STUCHLÍK

Basic information

Original name

Photons shells inner structure and causal properties

Edition

Journal of High Energy Astrophysics, 2025, 2214-4048

Other information

Language

English

Type of outcome

Article in a journal

Field of Study

10308 Astronomy

Country of publisher

Netherlands

Confidentiality degree

is not subject to a state or trade secret

References:

Impact factor

Impact factor: 10.500 in 2024

Organization unit

Institute of physics in Opava

UT WoS

001452761400001

EID Scopus

2-s2.0-105000106813

Keywords in English

Lense-Thirring-black holes-accretion;disks-accretion;Hydrodynamics-galaxies: actives

Tags

Tags

International impact, Reviewed
Changed: 15/1/2026 10:50, Mgr. Pavlína Jalůvková

Abstract

In the original language

We shed light on some causal properties of the Kerr super-spinnars emerging through the investigation of the spacetimes photon shells. We define inner structure of the spacetime photon shell, constituted by regions distinguished by specific characteristics of the photons paths. These regions are reflected in the singularity shadow boundaries studied, in particular, in relation to repulsive gravity effects, known in a specific class of slowly spinning super-spinnars. Counter-rotating and co-rotating photons are particularly investigated. Super fast spinning solutions are characterized by "faint" shadow boundaries. The properties emerging from this analysis could be observed from specific regions of the spacetimes photon spheres boundaries. Slowly spinning superspinnars, with (dimensionless) spin 1.