Consider the incompressible, irrotational, 2D flow, where the stream function is given by: 4 = 424 Determine the velocity field. Prove that the flow is both Physically possible and irrotational.
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- (a) Discuss your understanding of the concepts of the symmetry of a mechanical system, a conserved quantity or quantities within the mechanical system and the relation between them. Illustrate your answer with an example, but not the example in the Lecture Notes. What is the benefit of symmetry when analysing a mechanical system? (b) Consider the Lagrangian function on R? (defined by the Cartesian coordinates (x, y)) given by 1 L m (i² – ý²) + a(y² – x²), where m and a are constants. (i) Show to first order in e (that is, ignore terms of order e? and higher), that L is invariant under the transform (x, y) + (x + €Y, Y + ex). (ii) Find the integral of motion predicted by Noether's theorem for the Lagrangian function L.(0, 1, 0) is Consider a two-dimensional incompressible flow in the xz plane: u = - ey x Vo, where e the unit vector perpendicular to the xz plane. Denote the two velocity components in the xz plane as u and w in the x, z directions, respectively. Write down the expressions for them in terms of o. If the function of o assumes = x2² calculate the values of u and w at the coordinate x = = 2, z = 1. Ou= Ou= 86 əz > Ou=- - 86 əx W= ap dz 7 W= W= 8p Əz ap əz " ap " əI u = 4, w = -1 u = -1, w = 4 u = −4, w = 1 86 0₂7 86 Ou=- W=- u= -1, w = -4 5 dr =Sketch how water curls down a sink, say, in clock-wise rotation. Draw the resulting vector of the curl-operator applied on this water flow.
- The dynamics of a particle moving one-dimensionally in a potential V (x) is governed by the Hamiltonian Ho = p²/2m + V (x), where p = is the momentuin operator. Let E, n = of Ho. Now consider a new Hamiltonian H given parameter. Given A, m and E, find the eigenvalues of H. -ih d/dx 1, 2, 3, ... , be the eigenvalues Ho + Ap/m, where A is a %3|please solveConsider a 3-body system again. This time, let the particles be the Sun, the Earth, and the Moon. (a) Write the relative vector equations of motion for the Moon relative to the Earth. (b) At the very instance where the following right angle triangle geometry is achieved, compute the dominant and perturbing accelerations. Compare the magnitudes of both accelerations, is it reasonable to model the Moon's motion by considering a two-body problem with the Earth? Explain your answer.