Mukhopadhyay, Banibrata (2008) Predicting spin of compact objects from their QPOs: A global QPO model. In: 2nd Kolkata Conference on Observational Evidence for Black Holes in the Universe/Satellite Meeting on Black Holes, Neutron Stars, and Gamma-Ray Bursts, FEB 10-17, 2008, Kolkata.Full text not available from this repository.
We establish a unified model to explain Quasi-Periodic-Oscillation (QPO) observed from black hole and neutron star systems globally. This is based on the accreting systems thought to be damped harmonic oscillators with higher order nonlinearity. The model explains multiple properties parallelly independent of the nature of the compact object. It describes QPOs successfully for several compact sources. Based on it, we predict the spin frequency of the neutron star Sco X-1 and the specific angular momentum of black holes GRO J1655-40, GRS 1915+105.
|Item Type:||Conference Paper|
|Additional Information:||Copyright of this article belongs to American Institute of Physics.|
|Department/Centre:||Division of Physical & Mathematical Sciences > Physics|
|Date Deposited:||30 Mar 2010 07:47|
|Last Modified:||30 Mar 2010 07:47|
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