不出名 发表于 2025-3-27 00:37:41
V. Gupta,M. D. Lechner,R. Guptaovern the temporal, regular or chaotic modulations of the amplitudes of the excited modes. These amplitude equations have been calculated and solved for realistic population I (Classical) Cepheid models, which have an internal resonance of the type Ω. ≃ 2 Ω. and exhibit a secondary bump on their lig聋子 发表于 2025-3-27 02:19:41
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R. Gupta,V. Gupta,M. D. Lechner,R. Gupta with the second law of thermodynamics, (ii) the relation between the information flow rate ( = Kolmogorov entropy), Lyapunov exponents, and dimensions of the attractor, (iii) the discussion of generalized dimensions and entropies related to the flow of Renyi informations, (iv) the measurements of tfreight 发表于 2025-3-27 16:32:08
R. Gupta,V. Gupta,M. D. Lechner,R. Gupta presence of a mean magnetic field, limited by a of large magnetic Reynolds number R. An asymptotic procedure relying on a presumed geometry of flux ropes and sheets is used. Our results suggest that alpha has a finite nonzero limit as R → ∞. We express this limit in terms of the geometry of certainCAB 发表于 2025-3-27 20:23:38
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R. Gupta,V. Gupta,M. D. Lechner,R. Guptan applied to obtain a Hamiltonian formalism. The numerical results presented here show that the nonradial modes can cause a much more irregular motion than the radial modes. First, there are many near-resonant nonradial frequencies, and second, there is a nonlinear velocity-dependent term in the Hamjumble 发表于 2025-3-28 05:02:23
http://reply.papertrans.cn/23/2239/223880/223880_38.png小溪 发表于 2025-3-28 09:47:23
https://doi.org/10.1007/978-3-642-41556-2rate limit cycles are identified, one of which is responsible for shell flashes in red giants and the second provides the underlying mechanism for X-ray burst sources..When the impact of the burst luminosity on the accretion rate is introduced, the system is shown to exhibit a complex temporal behav轻推 发表于 2025-3-28 12:41:42
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