1 Honors Physics 1 Class 18 Fall 2013 Harmonic motion Unit circle and the phasor Solution to the spring differential equation Initial and boundary conditions. Chapter 14 Outline Periodic Motion Oscillations Amplitude, period, frequency Simple harmonic motion Displacement, velocity, and acceleration Energy ...
A more detailed analysis of generated cycles, of their number and analytic properties is given in Theorem 2.2 and related notes in terms of parameter 纬. Since the proofs of Theorems 2.1 and 2.2 are based on the most general properties of Navier-Stokes equations, these theorems can be readily...
Our methods are demonstrated through simulations of two slow-fast models—a gene oscillator, and an oscillating chemical reaction. Notes on possible experimental implementations are provided, the CBC method is discussed, and simulated results are presented for each system. The first test-system is tak...
Book Series: Lecture Notes in Computer Science, Volume 4984 , pp. 604- 613 , Part I , 2008. 12. M.H.F. Zarandi, A. Alaeddini and I.B. Turksen, "A hybrid fuzzy adaptive sampling - Run rules for Shewhart control charts", Information Sciences, Volume 178, Issue 4, pp.1152- 1170...
Versions Notes Abstract We investigate the equilibrium structure and radial oscillations of strange quark stars admixed with fermionic dark matter. For strange quark matter, we employ a stiff equation of state from a color-superconductivity improved bag model. For dark matter, we adopt the cold free...
Review Reports Versions Notes Abstract We imagine spherically symmetric configurations made of both dark matter and dark energy in the halo of spiral galaxies. Adopting a polytropic equation of state for dark matter and the Extended Chaplygin gas equation of state for dark energy, we model the same...
Review Reports Versions Notes Abstract We imagine spherically symmetric configurations made of both dark matter and dark energy in the halo of spiral galaxies. Adopting a polytropic equation of state for dark matter and the Extended Chaplygin gas equation of state for dark energy, we model the same...
Versions Notes Abstract We investigated compact stars consisting of cold quark matter and fermionic dark matter treated as two admixed fluids. We computed the stellar structures and fundamental radial oscillation frequencies of different masses of the dark fermion in the cases of weak and strong self...
Review Reports Versions Notes Abstract To explain the observed X-ray data in a black hole–accreting matter system and understand the physical mechanisms behind QPOs, we have numerically modeled the dynamical and oscillation properties of the shock cone formed around both slowly and rapidly rotating ...
Versions Notes Abstract Strange stars are one of the possible compact stellar objects formed in the core collapse of supernovae. These hypothetical stars are made by deconfined quark matter and are selfbound. In our study, we focus on the torsional oscillations of a non bare strange star, i...