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Book Boris V. Vasiliev Astrophysics

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Astrophysics

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Chapter 8<br />

The angular velocity of the<br />

apsidal rotation in binary<br />

stars<br />

8.1 The apsidal rotation of close binary stars<br />

The apsidal rotation (or periastron rotation) of close binary stars is a result of their<br />

non-Keplerian movement which originates from the non-spherical form of stars. This<br />

non-sphericity has been produced by rotation of stars around their axes or by their<br />

mutual tidal effect. The second effect is usually smaller and can be neglected. The<br />

first and basic theory of this effect was developed by A.Clairault at the beginning of<br />

the XVIII century. Now this effect was measured for approximately 50 double stars.<br />

According to Clairault’s theory the velocity of periastron rotation must be approximately<br />

100 times faster if matter is uniformly distributed inside a star. Reversely,<br />

it would be absent if all star mass is concentrated in the star center. To reach an<br />

agreement between the measurement data and calculations, it is necessary to assume<br />

that the density of substance grows in direction to the center of a star and here it runs<br />

up to a value which is hundreds times greater than mean density of a star. Just the<br />

same mass concentration of the stellar substance is supposed by all standard theories<br />

of a star interior. It has been usually considered as a proof of astrophysical models.<br />

But it can be considered as a qualitative argument. To obtain a quantitative agreement<br />

between theory and measurements, it is necessary to fit parameters of the stellar<br />

substance distribution in each case separately.<br />

Let us consider this problem with taking into account the gravity induced electric<br />

polarization of plasma in a star. As it was shown above, one half of full mass of a<br />

star is concentrated in its plasma core at a permanent density. Therefor, the effect<br />

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