Chi-square test of the relativistic precession model through the neutron star IGR J17511-3057

Ivan Z. Stefanov

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arXiv · 2308.15759

Chi-square test of the relativistic precession model through the neutron star IGR J17511-3057

Ivan Z. Stefanov

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Abstract

The aim of the current paper is to apply the method of Bambi (Bambi, 2015) to a source which contains two or more simultaneous triads of variability components. The joint chi-square variable that can be composed in this case, unlike some previous studies, allows the goodness of the fit to be tested. It appears that a good fit requires one of the observation groups to be disregarded. Even then, the model prediction for the mass of the neutron star in the accreting millisecond pulsar IGR J17511-3057 is way too high to be accepted.

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Ivan Z. Stefanov. 2023-08-30. Chi-square test of the relativistic precession model through the neutron star IGR J17511-3057. https://arxiv.org/abs/2308.15759

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