2009
DOI: 10.1142/s0217732309032137
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Self-Gravitating Astrophysical Mass With Singular Central Density Vibrating in Fundamental Mode

Abstract: The fluid-dynamical model of a self-gravitating mass of viscous liquid with singular density at the center vibrating in fundamental mode is considered in juxtaposition with that for Kelvin fundamental mode in a homogeneous heavy mass of incompressible inviscid liquid. Particular attention is given to the difference between spectral formulae for the frequency and lifetime of f -mode in the singular and homogeneous models. The newly obtained results are discussed in the context of theoretical asteroseismology of… Show more

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Cited by 4 publications
(5 citation statements)
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“…Note that this result differs from that of a uniform-density self-gravitating body, σ G = [(8/3)πGρl(l − 1)/(2l + 1)] 1/2 [32]. Bastrukov has recently obtained a similar spectrum for a self-gravitating liquid droplet with radially-varying density distribution ρ(r < a) ∝ 1/r, having a singular density at the center [33].…”
Section: Appendixmentioning
confidence: 99%
“…Note that this result differs from that of a uniform-density self-gravitating body, σ G = [(8/3)πGρl(l − 1)/(2l + 1)] 1/2 [32]. Bastrukov has recently obtained a similar spectrum for a self-gravitating liquid droplet with radially-varying density distribution ρ(r < a) ∝ 1/r, having a singular density at the center [33].…”
Section: Appendixmentioning
confidence: 99%
“…Regarding the difference between node-free oscillatory behavior of solid sphere and spherical mass of an incompressible liquid it is appropriate to note that the liquid sphere is able to sustain solely spheroidal node-free vibrations of fluid velocity. The canonical example is the Kelvin fundamental mode of oscillating fluid velocity in a heavy spherical mass of incompressible homogeneous liquid restored by forces represented as gradient of pressure and gradient of potential of self-gravity [36]. In the meantime, the node-free vibrations of solid sphere restored by elastic force (represented as divergence of shear mechanical stresses) are characterized by two eigenmodes.…”
Section: A the Energy Methodsmentioning
confidence: 99%
“…As shown in [18], this vacuum field is stable against collapse due to self-gravitation, i.e., the equivalent Jeans length is greater than the radius of the universe. (See [27] for a model of a self-gravitating liquid mass which vibrates.) The NLKG equation is used (as opposed to the non-linear Schödinger equation), because relativistic effects are essential in this context.…”
Section: Nlkg In An Arbitrary Metricmentioning
confidence: 99%