J 2009

Internal resonance in non-linear disk oscillations and the amplitude evolution of neutron star kilohertz QPOs

ABRAMOWICZ, Marek and Gabriel TÖRÖK

Basic information

Original name

Internal resonance in non-linear disk oscillations and the amplitude evolution of neutron star kilohertz QPOs

Authors

ABRAMOWICZ, Marek and Gabriel TÖRÖK

Edition

Astronomy & Astrophysics, FR - Francouzská republika, 2009, 1432-0746

Other information

Language

English

Type of outcome

Článek v odborném periodiku

Field of Study

10308 Astronomy

Confidentiality degree

není předmětem státního či obchodního tajemství

Organization unit

Faculty of Philosophy and Science in Opava

DOI

http://dx.doi.org/10.1051/0004-6361/200810740

UT WoS

000266730500018

Keywords in English

X-rays:binaries ?Stars:neutron? Accretion, accretion disks

Tags

, GA205-070052, MSM4781305903

Tags

International impact

Links

GA205/07/0052, research and development project. MSM4781305903, plan (intention).
Změněno: 7/12/2020 11:41, Mgr. Pavlína Jalůvková

Abstract

V originále

We explore some properties of twin kilohertz quasiperiodic oscillations (QPOs) in a simple toy-model consisting of two oscillation modes coupled by a general nonlinear force. We examine resonant effects by slowly varying the values of the tunable, and nearly commensurable, eigenfrequencies. The behavior of the actual oscillation frequencies and amplitudes during a slow transition through the 3:2 resonance is examined in detail and it is shown that both are significantly affected by the nonlinearities inthe governing equations. In particular, the amplitudes of oscillations reflect a resonant exchange of energy between the modes, as a result the initially weaker mode may become dominant after the transition.
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