Polarization vector transport in Kerr geometry
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F14%3A00451155" target="_blank" >RIV/67985815:_____/14:00451155 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Polarization vector transport in Kerr geometry
Original language description
In this paper the authors proved a set of practical formulae that are helpful in calculating the orientation of polarization vectors that are parallel transported from a region of strong gravitational field of a Kerr black hole to a distant observer.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2014
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Proceedings of RAGtime 14/16: Workshops on black holes and neutron stars
ISBN
9788075101266
ISSN
2336-5668
e-ISSN
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Number of pages
11
Pages from-to
39-49
Publisher name
Silesian University
Place of publication
Opava
Event location
Opava
Event date
Sep 18, 2012
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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