- ...
.
- In what follows it is convenient to
represent different energy scales in dimensionless form. There are two
natural units of energy per unit mass in our problem: the first associated the stellar
cusp - GM/ra and the second associated with the internal structure of star itself -
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For the dimensionless quantities expressed in terms of the
first unit we will use the calligraphic style while the quantities
expressed in terms of the second unit will be denoted by tilde.
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- ... waves
- Note that it is important to distinguish between the effect
of emission of gravitational waves by perturbations of the white dwarf
and the effect of emission of gravitational waves due to the
orbital motion of the star. The former effect is important as a
major process of mode energy loss while the latter significantly influences the
orbital evolution and may provide a source of gravitational waves
during the late stages of orbital evolution, see below.
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- ... form
- A more accurate expression has been derived in IP. See also this paper for the references on numerical and analytical studies of the stochastic instability.
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- ...)
- Note an alternative form of
Eq. (38) has already been provided in other studies, see e.g. Hopman
Alexander (2005), their Eq. (17) and references therein. To obtain this we
write
,
where
characterises the total number of stars having binding energies per unit mass of order of E, we introduce the global relaxation time scale
and use Eqs. (2), (4) and (35).
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- ...

- Note a misprint in Appendix of Peters
Mathews (1963) in their expression for g(n,e). The fifth term in the braces must
contain the factor (4/e)2 contrary to the factor (4/e2)2 as
in the text.
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- ...H
- Note that the average number of globular clusters is meaningful only when
Mpc, where 70 Mpc is a typical distance between the elements
of the Large Scale Structure in the Universe.
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