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Zahns Theory of Dynamical Tides and Its Application to Stars

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 نشر من قبل Sergey Chernov
 تاريخ النشر 2017
  مجال البحث فيزياء
والبحث باللغة English
 تأليف S.V. Chernov




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Zahns theory of dynamical tides is analyzed critically. We compare the results of this theory with our numerical calculations for stars with a convective core and a radiative envelope and with masses of one and a half and two solar masses. We show that for a binary system consisting of stars of one and a half or two solar masses and a point object with a mass equal to the solar mass and with an orbital period of one day under the assumption of a dense spectrum and moderately rapid dissipation, the evolution time scales of the semimajor axis will be shorter than those in Zahns theory by several orders of magnitude



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