Abstract
The fragmentation of interstellar molecular clouds has been investigated with great effort by many authors. In this paper, a simple model is given to describe the dynamics of two fragments moving in a special cylindrical potential. Using a modified version of the restricted three-body problem and the corresponding Jacobian integral, some constraints are given for the motion of the fragments.
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Acknowledgements
The first author is grateful for discussions with Drs H. Klahr, F. Biscani and B. Kocsis. This research was partly supported by the OTKA Grant NN-111016.
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Appendix
Appendix
Here, we investigate the linear stability of the collinear equilibrium point found above. First, Eqs. (24) and (25) are linearized (that is, we investigate their behavior at \(x=x_0+\xi \) and \(y=0+\,\eta \), \(x_0\) and 0 being the coordinates of the equilibrium points):
Assuming the solution in the form \(\xi = A e^{\lambda t}\) and \(\eta = B e^{\lambda t}\) with \(A \ne 0\) and \(B \ne 0\), substitution yields
This leads to the characteristic equation with \(\Lambda = \lambda ^2\)
An equilibrium point is stable if and only if \(\Lambda _1, \Lambda _2 < 0\) and real.
Let
and
so that
1.1 \(x_0>b\), the case of \(L_1\)
As \(3x_0^2 > b^2\), the first bracket in C is positive. Using Eq. (30), the second bracket is
In conclusion, C is negative. As \(\Lambda _{1,2}=(-B\pm \sqrt{B^2-4C})/2\) and \(B^2-4C>|B|\), there is always a positive \(\Lambda \) which results in instability.
1.2 \(x_0<-\,b\), the case of \(L_3\)
The first bracket in C is positive again. However, in this case
which concludes that C itself is positive. Equation (39) determines a parabola, which has negative roots if both the position (\(-B/2\)) and the value (\(-B^2/4+C\)) of its minimum are negative. Then, the following equations are to be solved:
and
Assuming again that \(b=0.1\) (see Sect. 4), the condition of stability is \(-\,1.13< x_0 <-\,0.1\) or \(m_1<1.08\), which seems physically reasonable.
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Deme, B., Érdi, B. & Tóth, L.V. The restricted three-body problem in cylindrical clouds. Celest Mech Dyn Astr 130, 73 (2018). https://doi.org/10.1007/s10569-018-9869-x
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DOI: https://doi.org/10.1007/s10569-018-9869-x