The Toomre stability criterion for a razor-thin isothermal gas disk usesSelf-gravity, represented by , amplifies overdensities. Pressure, represented by , suppresses short wavelengths, while epicyclic motion with frequency suppresses long-wavelength radial collapse. Axisymmetric disturbances are stable for and unstable for .
After a radial Fourier transform, Poisson's equation away from the sheet becomesThe decaying, reflection-symmetric solution is . Integrating Poisson's equation across gives the derivative jumpso . Thus the midplane potential is
Write the perturbations as , radial and azimuthal velocities , and pressure , all proportional to . Linearization in the shearing sheet givesandThe continuity and pressure equations implyEliminating then yields
When , temperature relaxes during a disturbance and the pressure response is isothermal, . When , relaxation is negligible and the response is adiabatic, , so the effective sound speed is . At finite relaxation time the phase lag between compression and pressure also damps stable waves.
At marginal stability write with real . The imaginary part of the pressure factor isFor , , and nonzero , the dispersion relation can have zero imaginary part only when . Thus every marginal mode hasThe marginal equation is consequentlyDefining the isothermal Toomre parameter , its two roots areThey exist when , and the interval between them is unstable when . Finite thermal relaxation therefore leaves the onset criterionequal to the isothermal criterion, regardless of and the nonzero value of .
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