← 2016 Paper 2

UPSC 2016 Maths Optional Paper 2 Q6b — Step-by-Step Solution

15 marks · Section B

Sources, sinks, doublets · Mechanics & Fluid Dynamics · asked 8× in 13 yrs · Read the full method →

Question

A simple source of strength mm is fixed at the origin OO in a uniform stream of incompressible fluid moving with velocity Ui^U\hat i. Show that the velocity potential ϕ\phi at any point PP of the stream is mrUrcosθ\dfrac{m}{r}-Ur\cos\theta, where OP=rOP=r and θ\theta is the angle which OP\overrightarrow{OP} makes with the direction i^\hat i. Find the differential equation of the streamlines and show that they lie on the surfaces Ur2sin2θ2mcosθ=Ur^2\sin^2\theta-2m\cos\theta= constant.

Technique

Linear superposition of a point-source potential m/rm/r and a uniform-stream potential Urcosθ-Ur\cos\theta; velocity from q=ϕ\mathbf q=-\nabla\phi in spherical polars; integrate the streamline ODE with the axisymmetric Stokes stream function, yielding ψ=12Ur2sin2θmcosθ\psi=\tfrac12Ur^2\sin^2\theta-m\cos\theta.

Solution

Setup. Use spherical polars (r,θ)(r,\theta) with θ\theta measured from the i^\hat i-axis; the flow is axisymmetric about that axis. Velocity is q=ϕ\mathbf q=-\nabla\phi.

Step 1 — Superpose the two potentials

A simple (point) source of strength mm at OO has potential ϕsrc=mr\phi_{\text{src}}=\dfrac{m}{r} (radial outflow qr=r(m/r)=m/r2q_r=-\partial_r(m/r)=m/r^2).

A uniform stream Ui^U\hat i has potential ϕstream=Ux=Urcosθ\phi_{\text{stream}}=-U x=-Ur\cos\theta (since (Ux)=Ui^-\nabla(-Ux)=U\hat i).

By linearity of Laplace’s equation, superpose:

  ϕ=mrUrcosθ.  \boxed{\;\phi=\frac{m}{r}-Ur\cos\theta.\;}

Each term is harmonic, so 2ϕ=0\nabla^2\phi=0 and the (incompressible, irrotational) motion is admissible.

Step 2 — Velocity components

qr=ϕr=(mr2Ucosθ)=mr2+Ucosθ,q_r=-\frac{\partial\phi}{\partial r}=-\Big(-\frac{m}{r^2}-U\cos\theta\Big)=\frac{m}{r^2}+U\cos\theta, qθ=1rϕθ=1r(Ursinθ)=Usinθ.q_\theta=-\frac1r\frac{\partial\phi}{\partial\theta}=-\frac1r\big(Ur\sin\theta\big)=-U\sin\theta.

(The source adds purely radial flux m/r2m/r^2; far away qUi^q\to U\hat i.)

Step 3 — Differential equation of the streamlines

Streamlines are tangent to q\mathbf q: in the meridian plane

  drqr=rdθqθ,drmr2+Ucosθ=rdθUsinθ.  \boxed{\;\frac{dr}{q_r}=\frac{r\,d\theta}{q_\theta},\qquad\frac{dr}{\dfrac{m}{r^2}+U\cos\theta}=\frac{r\,d\theta}{-U\sin\theta}.\;}

Step 4 — Integrate via the Stokes stream function

For axisymmetric flow the Stokes stream function ψ(r,θ)\psi(r,\theta) satisfies

qr=1r2sinθψθ,qθ=1rsinθψr.q_r=\frac{1}{r^2\sin\theta}\frac{\partial\psi}{\partial\theta},\qquad q_\theta=-\frac{1}{r\sin\theta}\frac{\partial\psi}{\partial r}.

Integrate qr=mr2+Ucosθq_r=\dfrac{m}{r^2}+U\cos\theta:

ψθ=r2sinθ(mr2+Ucosθ)=msinθ+Ur2sinθcosθ,\frac{\partial\psi}{\partial\theta}=r^2\sin\theta\Big(\frac{m}{r^2}+U\cos\theta\Big)=m\sin\theta+Ur^2\sin\theta\cos\theta, ψ=mcosθ+12Ur2sin2θ+g(r).\psi=-m\cos\theta+\tfrac12 Ur^2\sin^2\theta+g(r).

Check qθ=1rsinθψr=1rsinθ(Ursin2θ+g(r))q_\theta=-\dfrac{1}{r\sin\theta}\psi_r=-\dfrac{1}{r\sin\theta}\big(Ur\sin^2\theta+g'(r)\big). For this to equal Usinθ-U\sin\theta we need g(r)=0g'(r)=0. Hence

ψ=12Ur2sin2θmcosθ.\psi=\tfrac12 Ur^2\sin^2\theta-m\cos\theta.

Streamlines are surfaces ψ=\psi= const; multiplying by 22:

Answer

  Ur2sin2θ2mcosθ=constant.  \boxed{\;Ur^2\sin^2\theta-2m\cos\theta=\text{constant}.\;}
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