On magnetic-field-induced corrections to the orbital and
epicyclic frequencies: paper II. Slowly rotating magnetized
neutron stars

J 2012

On magnetic-field-induced corrections to the orbital and epicyclic frequencies: paper II. Slowly rotating magnetized neutron stars

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

Basic information

Original name

On magnetic-field-induced corrections to the orbital and epicyclic frequencies: paper II. Slowly rotating magnetized neutron stars

Authors

BAKALA, Pavel, Zdeněk STUCHLÍK, Eva ŠRÁMKOVÁ, Gabriel TÖRÖK and Martin URBANEC

Edition

Classical and Quantum Gravity, GB - Spojené království Velké Británie a, 2012, 0264-9381

Other information

Language

English

Type of outcome

Článek v odborném periodiku

Field of Study

10308 Astronomy

Confidentiality degree

není předmětem státního či obchodního tajemství

References:

URL

Organization unit

Faculty of Philosophy and Science in Opava

DOI

http://dx.doi.org/10.1088/0264-9381/29/6/065012

UT WoS

000301175600013

Keywords in English

Quasi-periodicoscillations; X-ray binaries; Integrated relativistic tori; Charged black-holes

Links

GA202/09/0772, research and development project. GPP209/12/P740, research and development project. LC06014, research and development project. MSM4781305903, plan (intention).

Změněno: 7/4/2021 08:20, Mgr. Pavlína Jalůvková

Abstract

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, and the magnetic field is of the standard dipole character. Using a fully relativistic approach, we determine the influence of the electromagnetic interaction (both attractive and repulsive) on the quasicircular motion. We focus on the behaviour of the orbital and epicyclic frequencies ofthe motion. Components of the four-velocity of the orbiting charged test particles are obtained by the numerical solution of equations of motion, and the epicyclic frequencies are obtained by using the standard perturbative method. The role of the combined effect of the neutron star magnetic field and its rotation in the character of the orbital and epicyclic frequencies is discussed. It is demonstrated that even in the Lense-Thirring spacetime, particles being static relative to distant

Citovat

BAKALA, Pavel, Zdeněk STUCHLÍK, Eva ŠRÁMKOVÁ, Gabriel TÖRÖK and Martin URBANEC. On magnetic-field-induced corrections to the orbital and epicyclic frequencies: paper II. Slowly rotating magnetized neutron stars. Classical and Quantum Gravity. GB - Spojené království Velké Británie a, 2012, vol. 29, No 6, 21 pp. ISSN 0264-9381. Available from: https://dx.doi.org/10.1088/0264-9381/29/6/065012.

@article{42118,
   author = {Bakala, Pavel and Stuchlík, Zdeněk and Šrámková, Eva and Török, Gabriel and Urbanec, Martin},
   article_location = {GB - Spojené království Velké Británie a},
   article_number = {6},
   doi = {http://dx.doi.org/10.1088/0264-9381/29/6/065012},
   keywords = {Quasi-periodicoscillations; X-ray binaries; Integrated relativistic tori; Charged black-holes},
   language = {eng},
   issn = {0264-9381},
   journal = {Classical and Quantum Gravity},
   title = {On magnetic-field-induced corrections to the orbital and epicyclic frequencies: paper II. Slowly rotating magnetized neutron stars},
   url = {https://iopscience.iop.org/article/10.1088/0264-9381/29/6/065012/pdf},
   volume = {29},
   year = {2012}
}

TY  - JOUR
ID  - 42118
AU  - Bakala, Pavel - Stuchlík, Zdeněk - Šrámková, Eva - Török, Gabriel - Urbanec, Martin
PY  - 2012
TI  - On magnetic-field-induced corrections to the orbital and epicyclic frequencies: paper II. Slowly rotating magnetized neutron stars
JF  - Classical and Quantum Gravity
VL  - 29
IS  - 6
SN  - 02649381
KW  - Quasi-periodicoscillations
KW  - X-ray binaries
KW  - Integrated relativistic tori
KW  - Charged black-holes
UR  - https://iopscience.iop.org/article/10.1088/0264-9381/29/6/065012/pdf
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, and the magnetic field is of the standard dipole character. Using a fully relativistic approach, we determine the influence of the electromagnetic interaction (both attractive and repulsive) on the quasicircular motion. We focus on the behaviour of the orbital and epicyclic frequencies ofthe motion. Components of the four-velocity of the orbiting charged test particles are obtained by the numerical solution of equations of motion, and the epicyclic frequencies are obtained by using the standard perturbative method. The role of the combined effect of the neutron star magnetic field and its rotation in the character of the orbital and epicyclic frequencies is discussed. It is demonstrated that even in the Lense-Thirring spacetime, particles being static relative to distant
ER  -

BAKALA, Pavel, Zdeněk STUCHLÍK, Eva ŠRÁMKOVÁ, Gabriel TÖRÖK and Martin URBANEC. On magnetic-field-induced corrections to the orbital and epicyclic frequencies: paper II. Slowly rotating magnetized neutron stars. \textit{Classical and Quantum Gravity}. GB - Spojené království Velké Británie a, 2012, vol.~29, No~6, 21 pp. ISSN~0264-9381. Available from: https://dx.doi.org/10.1088/0264-9381/29/6/065012.

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