The general relativistic Poynting-Robertson effect: II. A photon flux with nonzero angular momentum

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F11%3A10108956" target="_blank" >RIV/00216208:11320/11:10108956 - isvavai.cz</a>
Result on the web
<a href="http://iopscience.iop.org/0264-9381/28/3/035008/" target="_blank" >http://iopscience.iop.org/0264-9381/28/3/035008/</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1088/0264-9381/28/3/035008" target="_blank" >10.1088/0264-9381/28/3/035008</a>

Result language
angličtina
Original language name
The general relativistic Poynting-Robertson effect: II. A photon flux with nonzero angular momentum
Original language description
The motion of a test particle in a stationary, axially and reflectionsymmetric spacetime of a central compact object, as affected by interaction with a test radiation field of the same symmetries, is studied. Considering the radiation flux with fixed butarbitrary (nonzero) angular momentum, previous results limited to an equatorial plane motion within a zero angular-momentum photon flux in the Kerr and Schwarzschild backgrounds are extended. While a unique equilibriumc ircular orbit exists if the photon flux has zero angular momentum, multiples of such orbits appear if the photon angular momentum is sufficiently high.
Czech name
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Czech description
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Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BE - Theoretical physics
OECD FORD branch
—

Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)

Publication year
2011
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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