Three-dimensional general relativistic Poynting-Robertson effect. III. Static and nonspherical quadrupolar massive source
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19630%2F20%3AA0000022" target="_blank" >RIV/47813059:19630/20:A0000022 - isvavai.cz</a>
Výsledek na webu
<a href="https://journals.aps.org/prd/abstract/10.1103/PhysRevD.101.124031" target="_blank" >https://journals.aps.org/prd/abstract/10.1103/PhysRevD.101.124031</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1103/PhysRevD.101.124031" target="_blank" >10.1103/PhysRevD.101.124031</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Three-dimensional general relativistic Poynting-Robertson effect. III. Static and nonspherical quadrupolar massive source
Popis výsledku v původním jazyce
We investigate the three-dimensional (3D) motion of a test particle in the gravitational field generated by a nonspherical compact object endowed with a mass quadrupole moment, described by the Erez-Rosen metric, and a radiation field, including the general relativistic Poynting-Robertson (PR) effect, coming from a rigidly rotating spherical emitting source located outside of the compact object. We derive the equations of motion for test particles influenced by such radiation field, recovering the two-dimensional (2D) description, and the weak-field approximation. This dynamical system admits the existence of a critical hypersurface, region where gravitational and radiation forces balance. Selected test particle orbits for different set of input parameters are displayed. The possible configurations on the critical hypersurfaces can be either latitudinal drift toward the equatorial ring or suspended orbits. We discuss about the existence of multiple hypersurface solutions through a simple method to perform the calculations. We graphically prove also that the critical hypersurfaces are stable configurations within the Lyapunov theory.
Název v anglickém jazyce
Three-dimensional general relativistic Poynting-Robertson effect. III. Static and nonspherical quadrupolar massive source
Popis výsledku anglicky
We investigate the three-dimensional (3D) motion of a test particle in the gravitational field generated by a nonspherical compact object endowed with a mass quadrupole moment, described by the Erez-Rosen metric, and a radiation field, including the general relativistic Poynting-Robertson (PR) effect, coming from a rigidly rotating spherical emitting source located outside of the compact object. We derive the equations of motion for test particles influenced by such radiation field, recovering the two-dimensional (2D) description, and the weak-field approximation. This dynamical system admits the existence of a critical hypersurface, region where gravitational and radiation forces balance. Selected test particle orbits for different set of input parameters are displayed. The possible configurations on the critical hypersurfaces can be either latitudinal drift toward the equatorial ring or suspended orbits. We discuss about the existence of multiple hypersurface solutions through a simple method to perform the calculations. We graphically prove also that the critical hypersurfaces are stable configurations within the Lyapunov theory.
Klasifikace
Druh
J<sub>imp</sub> - Článek v periodiku v databázi Web of Science
CEP obor
—
OECD FORD obor
10308 - Astronomy (including astrophysics,space science)
Návaznosti výsledku
Projekt
<a href="/cs/project/GA17-16287S" target="_blank" >GA17-16287S: Oscilace a koherentní jevy v akrečních discích kolem kompaktních objektů a jejich observační podpisy</a><br>
Návaznosti
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>S - Specificky vyzkum na vysokych skolach<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2020
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Physical Review D
ISSN
1550-7998
e-ISSN
1550-2368
Svazek periodika
101
Číslo periodika v rámci svazku
12
Stát vydavatele periodika
US - Spojené státy americké
Počet stran výsledku
16
Strana od-do
„124031-1“-„124031-16“
Kód UT WoS článku
000540166200010
EID výsledku v databázi Scopus
2-s2.0-85087024215