Non-geodesic orbital and epicyclic frequencies in vicinity of
slowly rotating magnetized neutron stars

D 2013

Non-geodesic orbital and epicyclic frequencies in vicinity of slowly rotating magnetized neutron stars

BAKALA, Pavel; Zdeněk STUCHLÍK; Eva ŠRÁMKOVÁ; Gabriel TÖRÖK; Martin URBANEC et. al.

Základní údaje

Originální název

Non-geodesic orbital and epicyclic frequencies in vicinity of slowly rotating magnetized neutron stars

Autoři

BAKALA, Pavel; Zdeněk STUCHLÍK; Eva ŠRÁMKOVÁ; Gabriel TÖRÖK a Martin URBANEC

Vydání

Cambridge, UK, Feeding Compact Objects: Accretion on All Scales, Proceedings of the International Astronomical Union, IAU Symposium, od s. 185-186, 2 s. 2013

Nakladatel

Cambridge University Press

Další údaje

Jazyk

angličtina

Typ výsledku

Stať ve sborníku

Obor

10308 Astronomy

Utajení

není předmětem státního či obchodního tajemství

Odkazy

www

Organizační jednotka

Filozoficko-přírodovědecká fakulta v Opavě

ISBN

978-1-107-03379-5

ISSN

DOI

https://doi.org/10.1017/S1743921312019539

Klíčová slova anglicky

Stars: neutron; X-rays: binaries; Stars: magnetic fields

Štítky

FÚ, sbornik

Příznaky

Mezinárodní význam

Změněno: 7. 12. 2020 14:05, Mgr. Pavlína Jalůvková

Anotace

V originále

We study non-geodesic corrections to the quasicircular motion of charged test particles in the field of magnetized slowly rotating neutron stars. The gravitational field is approximated by the Lense-Thirring geometry, the magnetic field is of the standard dipole character. Using a fully-relativistic approach we determine influence of the electromagnetic interaction (both attractive and repulsive) on the quasicircular motion. We focus on the behaviour of the orbital and epicyclic frequencies of the motion. Components of the four-velocity of the orbiting charged test particles are obtained by numerical solution of equations of motion, the epicyclic frequencies are obtained by using the standard perturbative method. The role of the combined effect of theneutron star magnetic field and its rotation in the character of the orbital and epicyclic frequencies is discussed.

Citovat

BAKALA, Pavel; Zdeněk STUCHLÍK; Eva ŠRÁMKOVÁ; Gabriel TÖRÖK a Martin URBANEC. Non-geodesic orbital and epicyclic frequencies in vicinity of slowly rotating magnetized neutron stars. In Feeding Compact Objects: Accretion on All Scales, Proceedings of the International Astronomical Union, IAU Symposium. Cambridge, UK: Cambridge University Press, 2013, s. 185-186. ISBN 978-1-107-03379-5. Dostupné z: https://doi.org/10.1017/S1743921312019539.

@inproceedings{42700,
   author = {Bakala, Pavel and Stuchlík, Zdeněk and Šrámková, Eva and Török, Gabriel and Urbanec, Martin},
   address = {Cambridge, UK},
   booktitle = {Feeding Compact Objects: Accretion on All Scales, Proceedings of the International Astronomical Union, IAU Symposium},
   doi = {https://doi.org/10.1017/S1743921312019539},
   keywords = {Stars: neutron; X-rays: binaries; Stars: magnetic fields},
   language = {eng},
   location = {Cambridge, UK},
   isbn = {978-1-107-03379-5},
   pages = {185-186},
   publisher = {Cambridge University Press},
   title = {Non-geodesic orbital and epicyclic frequencies in vicinity of slowly rotating magnetized neutron stars},
   url = {https://arxiv.org/abs/1212.6938},
   year = {2013}
}

TY  - CONF
ID  - 42700
AU  - Bakala, Pavel - Stuchlík, Zdeněk - Šrámková, Eva - Török, Gabriel - Urbanec, Martin
PY  - 2013
TI  - Non-geodesic orbital and epicyclic frequencies in vicinity of slowly rotating magnetized neutron stars
PB  - Cambridge University Press
CY  - Cambridge, UK
SN  - 9781107033795
KW  - Stars: neutron
KW  - X-rays: binaries
KW  - Stars: magnetic fields
UR  - https://arxiv.org/abs/1212.6938
N2  - We study non-geodesic corrections to the quasicircular motion of charged test particles in the field of magnetized slowly rotating neutron stars. The gravitational field is approximated by the Lense-Thirring geometry, the magnetic field is of the standard dipole character. Using a fully-relativistic approach we determine influence of the electromagnetic interaction (both attractive and repulsive) on the quasicircular motion. We focus on the behaviour of the orbital and epicyclic frequencies of the motion. Components of the four-velocity of the orbiting charged test particles are obtained by numerical solution of equations of motion, the epicyclic frequencies are obtained by using the standard perturbative method. The role of the combined effect of theneutron star magnetic field and its rotation in the character of the orbital and epicyclic frequencies is discussed.
ER  -

BAKALA, Pavel; Zdeněk STUCHLÍK; Eva ŠRÁMKOVÁ; Gabriel TÖRÖK a Martin URBANEC. Non-geodesic orbital and epicyclic frequencies in vicinity of slowly rotating magnetized neutron stars. In \textit{Feeding Compact Objects: Accretion on All Scales, Proceedings of the International Astronomical Union, IAU Symposium}. Cambridge, UK: Cambridge University Press, 2013, s.~185-186. ISBN~978-1-107-03379-5. Dostupné z: https://doi.org/10.1017/S1743921312019539.

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