The non-linear behavior of the black hole system GRS 1915+105

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The Non - Linear Behavior of the Black Hole System Grs 1915 + 105

Using non-linear time series analysis, along with surrogate data analysis, it is shown that the various types of long term variability exhibited by the black hole system GRS 1915+105, can be explained in terms of a deterministic non-linear system with some inherent stochastic noise. Evidence is provided for a non-linear limit cycle origin of one of the low frequency QPO detected in the source, ...

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The chaotic behavior of the black hole system GRS 1915 + 105

A modified non-linear time series analysis technique, which computes the correlation dimension D2, is used to analyze the X-ray light curves of the black hole system GRS 1915+105 in all twelve temporal classes. For four of these temporal classes D2 saturates to ≈ 4 − 5 which indicates that the underlying dynamical mechanism is a low dimensional chaotic system. Of the other eight classes, three ...

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Black hole spin in GRS 1915 + 105

Microquasars are galactic black hole binary systems with radio jets which can sometimes be spatially resolved to show superluminal motion. The first and best known of this class of objects is GRS 1915+105, the brightest accreting source in our Galaxy. There is persistent speculation that strong jet emission could be linked to black hole spin. If so, the high spin should also be evident in accre...

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ژورنال

عنوان ژورنال: Advances in Space Research

سال: 2006

ISSN: 0273-1177

DOI: 10.1016/j.asr.2005.10.061