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Chandler Wobble and Free Core Nutation of Neutron Stars

Published online by Cambridge University Press:  19 July 2016

Alexander Gusev  and
Irina Kitiashvili
Alexander Gusev
Affiliation:
Kazan State University, Kremlevskaya str.18, Kazan, 420008, Russia
Irina Kitiashvili
Affiliation:
Kazan State University, Kremlevskaya str.18, Kazan, 420008, Russia

Abstract

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Extending the theory of core-mantle differential rotation of a planet, we have obtained the periods PCW and PFCN for different pulsars in the second approximation. We have investigated the dependence of these periods on the equation of state of neutron liquid, flatness of mantle and crust of the neutron star.

Type
Part 1: Neutron Star Formation and Evolution
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 45 - 46
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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