Mukhopadhyay, Banibrata (2009) Higher-Order Nonlinearity In Accretion Disks: Quasi-Periodic Oscillations Of Black Hole And Neutron Star Sources And Their Spin. In: Astrophysical Journal, 694 (1). pp. 387-395.
fulltext.pdf - Published Version
Restricted to Registered users only
Download (356Kb) | Request a copy
We propose a unified model to explain Quasi-Periodic Oscillation (QPO), particularly of high frequency, observed from black hole and neutron star systems globally. We consider accreting systems to be damped harmonic oscillators exhibiting epicyclic oscillations with higher-order nonlinear resonance to explain QPO. The resonance is expected to be driven by the disturbance from the compact object at its spin frequency. The model explains various properties parallelly for both types of the compact object. It describes QPOs successfully for ten different compact sources. Based on this, we predict the spin frequency of the neutron star Sco X-1 and specific angular momentum of black holes GRO J1655–40, XTE J1550–564, H1743–322, and GRS 1915+105.
|Item Type:||Journal Article|
|Additional Information:||Copyright of this article belongs to University of Chicago Press.|
|Keywords:||black hole physics;stars:neutron;gravitation;relativity.|
|Department/Centre:||Division of Physical & Mathematical Sciences > Physics|
|Date Deposited:||12 Aug 2009 06:48|
|Last Modified:||19 Sep 2010 05:30|
Actions (login required)