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Inelastic stresses and deformations are calculated for rotating variable thickness disks described by two different commonly used disk profile functions i.e. power and exponential forms.
A critical disk profile is determined and the corresponding elastic plastic stresses as well as the residual stress distribution upon removal of the applied pressure are computed and discussed.
Moreover, the values of sensitivity factors Sσ , in and Sσ , e in the considered disk profiles are similar, and the effects of the variations in the thermal loading parameters Qin and Qe on the maximum stress are not influenced by the disk profile.
There is a gap between 4 and 13 AU, which appears to contain a large planet around 20 times the mass of Jupiter, although further examination of the disk profile indicates it might be a more massive object such as a brown dwarf or more than one planet.
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Thickness variation of disks is described by means of a power of linear function, which can be used to describe a fourfold infinity of actual disk profiles.
This paper aims at finding an optimal disk profiles for minimum weight design using the Karush-Kuhn-Tucker method (KKT) as a classical optimization method, simulated annealing (SA) and particle swarm optimization (PSO) as two modern optimization techniques.
We thank S. Majewski and K. Cunha for interesting discussions on the topic, and J. Bovy for help with implementing the disk-flare profile.
In fact, the energy-resolved RMS variability on a time-bin of 2 × 105 s shows a depression around 5 – 7 keV and the degree of the depression as a function of energy is similar to the disk-line profile in the energy spectrum.
If multiple isolates from a given sample exhibited similar disk diffusion susceptibility profiles, genomic profiles as generated by using random amplified polymorphic DNA (RAPD) analysis were compared in the same gel (12 ).
Further validation is provided in Figure 15 where disk-averaged profiles for the two highest resolution 2D runs are shown according to Eq. (94).
When the resolution is increased from (N_{theta}=128) to (N_{theta}=192), the disk-averaged profiles generally agree within their standard deviations, although we observe a continuing trend towards higher gas pressures and magnetic pressures in the outer regions (rin[30mbox{ M},50mbox{ M}]).
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com