J 2019

Profiled spectral lines of Keplerian rings orbiting in the regular Bardeen black hole spacetimes

SCHEE, Jan a Zdeněk STUCHLÍK

Základní údaje

Originální název

Profiled spectral lines of Keplerian rings orbiting in the regular Bardeen black hole spacetimes

Autoři

SCHEE, Jan (203 Česká republika, garant, domácí) a Zdeněk STUCHLÍK (203 Česká republika, domácí)

Vydání

European Physical Journal C, 2019, 1434-6044

Další údaje

Jazyk

angličtina

Typ výsledku

Článek v odborném periodiku

Obor

10308 Astronomy

Stát vydavatele

Německo

Utajení

není předmětem státního či obchodního tajemství

Odkazy

Kód RIV

RIV/47813059:19240/19:A0000411

Organizační jednotka

Filozoficko-přírodovědecká fakulta v Opavě

UT WoS

000505552500005

Klíčová slova anglicky

Bardeen black hole; spectral lines; Keplerian rings

Štítky

Příznaky

Mezinárodní význam, Recenzováno

Návaznosti

GB14-37086G, projekt VaV.
Změněno: 20. 3. 2020 08:36, RNDr. Jan Hladík, Ph.D.

Anotace

V originále

Considering the regular Bardeen black hole spacetimes, we test the observational effects of the general relativistic solutions coupled to non-linear electrodynamics (NED) by studying the photon motion in the effective geometry governed by the spacetime geometry and the NED Lagrangian. We focus our attention to the observationally important case of profiled spectral lines generated by rings radiating in a fixed frequency and orbiting the black hole along circular geodesics of the Bardeen spacetime. Such profiled spectral lines are observed in active galactic nuclei and in microquasars, giving sufficient data for the test of regular black holes. We expect that such radiating rings could arise around the Galaxy central supermassive black hole SgrA*, and the related profiled spectral lines could give important additional information to those obtained by direct observations due to the Event Horizon (GRAVITY) Telescope. We demonstrate that the profiled spectral lines of the radiating rings predict strong signatures of the NED effects on the photon motion namely the frequency shift to the red edge of the spectrum, and narrowing of the profile, by more than one order in comparison with the case of the profiles generated purely by the spacetime geometry, for all values of the magnetic charge and the inclination angle of the observer. The specific flux is substantially suppressed and for extended Keplerian disks even the shape of the profiled line is significantly modified due to the NED effect.