Section-A
(Very Short Answer Type Questions)
Note:- Answer all questions. As per the nature of the question you delimit your answer in one word, one sentence or maximum up to 30 words. Each question carries 1 (one) mark.
(i). Write down the equation of tangent line to a curve at a given point.
(ii). Define the oscillating circle.
(iii). Write down the formula to the curvature of evolute.
(iv). State Mennier’s theorem.
Section-B
(Short Answer Questions)
Note :- Answer any two questions. Each answer should be given in 200 words. Each question carries 4 marks.
Prove that the torsion of the two Bertrand curves has the same sign and their product is constant.
Show that the vector B^(i)B^i of variable magnitude suffers a parallel displacement along a curve C if and only if :
Prove that an entity whose inner product with an arbitrary tension is a tensor is itself a tensor.
If surface of sphere is a two dimensional Riemannian space. Compute the Christoffel symbols.
Section-C
(Long Answer Questions)
Note :- Answer any one question. Each answer should be given in 800 words. Each question carries 08 marks.
(i). State and prove Meunienis theorem.
(ii). Find the Geodesic curvature of the curve u=u= constant on the surface x=u cos theta,y=u sin theta,z=(1)/(2)au^(2)x=u \cos \theta, y=u \sin \theta, z=\frac{1}{2} a u^2
(i). Find the angle between two tangential direction on the surface in the terms of direction ratio.
(ii). If the tangent and binormal at a point of curve make angles theta,phi\theta, \phi respectively with a fixed directions then:
Write down the equation of the tangent line to a curve at a given point.
Answer:
The equation of the tangent line to a curve at a given point can be determined as follows:
General Formula
If a curve is described by y=f(x)y = f(x), the tangent line at a point (x_(0),y_(0))(x_0, y_0) on the curve is given by:
y-y_(0)=m(x-x_(0)),y – y_0 = m(x – x_0),
where mm is the slope of the tangent line at (x_(0),y_(0))(x_0, y_0). The slope mm is found using the derivative of f(x)f(x) at x_(0)x_0:
m=f^(‘)(x_(0)).m = f'(x_0).
Question:-01(b)
Define the oscillating circle.
Answer:
The oscillating circle (or osculating circle) at a point on a curve is the circle that best approximates the curve near that point. It shares the same tangent, curvature, and radius of curvature as the curve at the given point. The term "osculating" comes from the Latin word osculare, meaning "to kiss," as the circle "kisses" the curve at that point.
Key Features of the Osculating Circle:
Radius of Curvature: The radius of the osculating circle is equal to the reciprocal of the curvature (kk) of the curve at the point:
R=(1)/(k),R = \frac{1}{k},
where kk is the curvature.
Center of the Osculating Circle: The center of the circle, called the center of curvature, lies along the normal to the curve at the given point, at a distance RR from the point.
Curvature Match: The osculating circle has the same curvature as the curve at the point of tangency.
Best Approximation: Among all circles passing through the point, the osculating circle best approximates the curve locally. Its radius and position ensure this close fit.
Formulas:
For a curve given parametrically by (x(t),y(t))(x(t), y(t)):
Center of the Osculating Circle:(x_(c),y_(c))=(x_(0)-R(y^(‘)(t))/(sqrt(x^(‘)(t)^(2)+y^(‘)(t)^(2))),y_(0)+R(x^(‘)(t))/(sqrt(x^(‘)(t)^(2)+y^(‘)(t)^(2)))),\left(x_c, y_c\right) = \left(x_0 – R \frac{y'(t)}{\sqrt{x'(t)^2 + y'(t)^2}}, y_0 + R \frac{x'(t)}{\sqrt{x'(t)^2 + y'(t)^2}}\right),where (x_(0),y_(0))(x_0, y_0) is the point of tangency and RR is the radius of curvature.
Question:-01(c)
Write down the formula to the curvature of evolute.
Answer:
The curvature of the evolute of a given curve is related to the curvature of the original curve as follows:
Formula for the Curvature of the Evolute:
Let the original curve be parameterized by (x(t),y(t))(x(t), y(t)), and let its curvature be k(t)k(t) (with radius of curvature R(t)=1//k(t)R(t) = 1/k(t)).
The curvature of the evolute, denoted as k_(“evolute”)(t)k_{\text{evolute}}(t), is given by:
R(t)=1//k(t)R(t) = 1/k(t) is the radius of curvature of the original curve.
rho(t)\rho(t) is the radius of the osculating circle measured along the evolute (distance to the center of curvature).
Explanation
Evolute: The evolute of a curve is the locus of the centers of curvature of the original curve.
Geometry: The curvature of the evolute depends on how the curvature of the original curve changes relative to the distance from the curve to its center of curvature.
This formula accounts for the relationship between the geometry of the evolute and the original curve.
Question:-01(d)
State Mennier’s theorem.
Answer:
Meunier’s Theorem is a fundamental result in the geometry of surfaces in differential geometry. It relates the normal curvature of a surface to the principal curvatures at a given point. The theorem states:
Statement of Meunier’s Theorem:
The normal curvaturek_(n)k_n of a surface in a given direction is equal to the cosine-weighted average of the principal curvaturesk_(1)k_1 and k_(2)k_2. Specifically:
k_(1)k_1 and k_(2)k_2 are the principal curvatures of the surface at the point under consideration.
theta\theta is the angle between the given direction and the direction of the first principal curvature (k_(1)k_1).
Question:-02
Prove that the torsion of the two Bertrand curves has the same sign and their product is constant.
Answer:
To prove that the torsion of two Bertrand curves has the same sign and their product is constant, we proceed as follows:
Bertrand Curves
Two curves are said to be Bertrand curves if each point on one curve corresponds to a point on the other such that the principal normal vectors of the curves at corresponding points are the same.
Let the two Bertrand curves be alpha(s)\boldsymbol{\alpha}(s) and beta(s)\boldsymbol{\beta}(s), parameterized by their arc length ss, with the following properties:
beta(s)=alpha(s)+lambda N(s)\boldsymbol{\beta}(s) = \boldsymbol{\alpha}(s) + \lambda \boldsymbol{N}(s), where N(s)\boldsymbol{N}(s) is the principal normal of alpha(s)\boldsymbol{\alpha}(s) and lambda\lambda is a constant.
The principal normal directions of alpha(s)\boldsymbol{\alpha}(s) and beta(s)\boldsymbol{\beta}(s) coincide at corresponding points.
Definitions of Curvature and Torsion
For a space curve alpha(s)\boldsymbol{\alpha}(s):
The curvature is kappa(s)\kappa(s).
The torsion is tau(s)\tau(s).
For the Bertrand mate beta(s)\boldsymbol{\beta}(s):
Let its curvature and torsion be kappa _(beta)(s)\kappa_\beta(s) and tau _(beta)(s)\tau_\beta(s), respectively.
This shows that the product is proportional to tau(s)^(2)\tau(s)^2, which remains constant if tau(s)\tau(s) does not change.
Step 4: Signs of the Torsions
The torsions tau(s)\tau(s) and tau _(beta)(s)\tau_\beta(s) depend on (1-lambda kappa(s))^(2)(1 – \lambda \kappa(s))^2, which is always positive. Thus, the signs of tau(s)\tau(s) and tau _(beta)(s)\tau_\beta(s) must be the same.
Conclusion
The torsions of the two Bertrand curves have the same sign.
The product of their torsions is constant:tau(s)*tau _(beta)(s)=(tau(s)^(2))/((1-lambda kappa(s))^(2)).\tau(s) \cdot \tau_\beta(s) = \frac{\tau(s)^2}{(1 – \lambda \kappa(s))^2}.
Question:-03
Show that the vector B^(i)B^i of variable magnitude suffers a parallel displacement along a curve CC if and only if:
A vector B^(i)B^i undergoes parallel displacement along a curve CC if its covariant derivative along the tangent to the curve is zero. This condition is written as:
(DB^(i))/(Ds)=0,\frac{D B^i}{Ds} = 0,
where ss is the arc length parameter along the curve, and (D)/(Ds)\frac{D}{Ds} is the covariant derivative along the curve.
where Gamma_(jk)^(i)\Gamma^i_{jk} are the Christoffel symbols, (dx^(k))/(ds)\frac{dx^k}{ds} is the tangent vector to the curve, and (dB^(i))/(ds)\frac{dB^i}{ds} is the ordinary derivative of B^(i)B^i along the curve.
Thus, the parallel displacement condition becomes:
For parallel displacement, the term involving the Christoffel symbols vanishes because the Christoffel symbols only depend on the connection and are symmetric in their lower indices. Therefore:
Equation (2) shows that the antisymmetric combination (B^(l)B_(,j)^(i)-B^(i)B_(,j)^(l))(B^l B^i_{,j} – B^i B^l_{,j}), projected along the tangent vector (dx^(j))/(ds)\frac{dx^j}{ds}, must vanish for parallel displacement. This condition ensures that the change in B^(i)B^i along the curve is consistent with parallel transport.
Thus, the vector B^(i)B^i undergoes parallel displacement along the curve CC if and only if:
The inner product between two tensors A^(i_(1)cdotsi_(p))A^{i_1 \cdots i_p} and B_(i_(1)cdotsi_(p))B_{i_1 \cdots i_p} is a contraction over their common indices:
Since bar(C)=C\bar{C} = C, and T_(j_(1)cdotsj_(m))T_{j_1 \cdots j_m} is arbitrary, the coefficient of T_(j_(1)cdotsj_(m))T_{j_1 \cdots j_m} must match the transformation law for a tensor:
The transformation law for bar(S)^(i_(1)cdotsi_(m))\bar{S}^{i_1 \cdots i_m} matches that of a tensor of order mm. Therefore, S^(i_(1)cdotsi_(m))S^{i_1 \cdots i_m} is a tensor.
Thus, an entity whose inner product with an arbitrary tensor is a scalar is itself a tensor.
Question:-05
If the surface of a sphere is a two-dimensional Riemannian space, compute the Christoffel symbols.
Answer:
To compute the Christoffel symbols for the surface of a sphere, we begin by describing the sphere as a two-dimensional Riemannian manifold with a given metric. Let’s go step by step:
Step 1: Parametrize the Sphere
The sphere of radius RR can be parametrized in spherical coordinates (theta,phi)(\theta, \phi), where:
In Cartesian coordinates, the position vector of a point on the sphere is:
r=[[x],[y],[z]]=[[R sin theta cos phi],[R sin theta sin phi],[R cos theta]].\mathbf{r} = \begin{bmatrix} x \\ y \\ z \end{bmatrix} = \begin{bmatrix} R \sin\theta \cos\phi \\ R \sin\theta \sin\phi \\ R \cos\theta \end{bmatrix}.
Step 2: Metric of the Sphere
The metric tensor g_(ij)g_{ij} is derived from the arc length ds^(2)ds^2, which in spherical coordinates is:
Gamma_(phi phi)^(theta)=(1)/(2R^(2))*R^(2)*2sin theta cos theta=sin theta cos theta.\Gamma^\theta_{\phi\phi} = \frac{1}{2R^2} \cdot R^2 \cdot 2 \sin\theta \cos\theta = \sin\theta \cos\theta.
Gamma_(phi theta)^(phi)\Gamma^\phi_{\phi\theta} and Gamma_(theta phi)^(phi)\Gamma^\phi_{\theta\phi}:
These are symmetric (Gamma_(phi theta)^(phi)=Gamma_(theta phi)^(phi)\Gamma^\phi_{\phi\theta} = \Gamma^\phi_{\theta\phi}), so we compute one:
Gamma_(theta theta)^(phi)\Gamma^\phi_{\theta\theta}:
This component vanishes because g_(phi phi)g_{\phi\phi} does not depend on phi\phi.
Gamma_(theta theta)^(theta)\Gamma^\theta_{\theta\theta}:
This component vanishes because g_(theta theta)g_{\theta\theta} does not depend on theta\theta or phi\phi.
Summary of Non-Zero Christoffel Symbols
The non-zero Christoffel symbols for the surface of the sphere are:
Gamma_(phi phi)^(theta)=sin theta cos theta\Gamma^\theta_{\phi\phi} = \sin\theta \cos\theta,
k_(n)k_n is the normal curvature of the surface in a given direction.
k_(1)k_1 and k_(2)k_2 are the principal curvatures of the surface at the point.
theta\theta is the angle between the given direction and the direction of the first principal curvature (k_(1)k_1).
Proof of Meunier’s Theorem:
Step 1: Curvature of a Surface
At a given point pp on a surface, the normal curvaturek_(n)k_n in a direction specified by the unit tangent vector t\mathbf{t} is defined as the curvature of the curve obtained by intersecting the surface with the plane containing t\mathbf{t} and the normal vector N\mathbf{N}.
The shape operator (or Weingarten map) SS encodes the relationship between the normal curvature and the directions of interest. It is defined as:
where (:*,*:)\langle \cdot, \cdot \rangle denotes the dot product.
Step 2: Principal Curvatures and Directions
The principal curvatures k_(1)k_1 and k_(2)k_2 are the eigenvalues of the shape operator SS, and the corresponding eigenvectors t_(1)\mathbf{t}_1 and t_(2)\mathbf{t}_2 are the principal directions. These directions are orthogonal:
Since t_(1)\mathbf{t}_1 and t_(2)\mathbf{t}_2 are unit vectors ((:t_(1),t_(1):)=1\langle \mathbf{t}_1, \mathbf{t}_1 \rangle = 1 and (:t_(2),t_(2):)=1\langle \mathbf{t}_2, \mathbf{t}_2 \rangle = 1), this simplifies to:
The normal curvature k_(n)k_n in a given direction is a weighted average of the principal curvatures k_(1)k_1 and k_(2)k_2.
The weights are cos^(2)theta\cos^2\theta and sin^(2)theta\sin^2\theta, which depend on how closely the direction aligns with the principal directions.
Question:-06(b)
Find the Geodesic curvature of the curve u=”constant”u = \text{constant} on the surface x=u cos thetax = u \cos \theta, y=u sin thetay = u \sin \theta, z=(1)/(2)au^(2)z = \frac{1}{2} a u^2
Answer:
To find the geodesic curvature of the curve u=”constant”u = \text{constant} on the given surface, we follow these steps:
Step 1: Understand the Surface and Curve
The surface is parameterized as:
x=u cos theta,quad y=u sin theta,quad z=(1)/(2)au^(2).x = u \cos \theta, \quad y = u \sin \theta, \quad z = \frac{1}{2} a u^2.
Here, uu and theta\theta are the surface parameters. The curve of interest is u=”constant”u = \text{constant}, so:
x=u_(0)cos theta,quad y=u_(0)sin theta,quad z=(1)/(2)au_(0)^(2),x = u_0 \cos \theta, \quad y = u_0 \sin \theta, \quad z = \frac{1}{2} a u_0^2,
where u_(0)u_0 is the fixed value of uu, and the curve is described only by the parameter theta\theta.
(a) Find the angle between two tangential directions on the surface in terms of direction ratios.
Answer:
To find the angle between two tangential directions on a surface in terms of their direction ratios, we use the concept of the first fundamental form of the surface.
where theta\theta and phi\phi are the angles made by the tangent and binormal vectors of a curve with fixed directions, kk is the curvature, and tau\tau is the torsion, we proceed as follows:
Step 1: Geometric Setup
Let the curve be parameterized by its arc length ss. The Frenet-Serret frame at any point consists of:
The tangent vectorT\mathbf{T},
The normal vectorN\mathbf{N},
The binormal vectorB\mathbf{B}.
These vectors satisfy the Frenet-Serret equations:
(dT)/(ds)=kN,\frac{d\mathbf{T}}{ds} = k \mathbf{N},
kk is the curvature, which measures the rate of change of T\mathbf{T} with respect to ss,
tau\tau is the torsion, which measures the rate of change of B\mathbf{B} with respect to ss.
Step 2: Angles with Fixed Directions
Suppose T\mathbf{T} (the tangent vector) makes an angle theta\theta with a fixed direction a\mathbf{a}, and B\mathbf{B} (the binormal vector) makes an angle phi\phi with the same fixed direction.
Let:
cos theta=T*a,quad cos phi=B*a.\cos\theta = \mathbf{T} \cdot \mathbf{a}, \quad \cos\phi = \mathbf{B} \cdot \mathbf{a}.
Differentiating these with respect to the arc length ss, we use the Frenet-Serret equations.
Step 3: Differentiating cos theta\cos\theta and cos phi\cos\phi
For cos theta=T*a\cos\theta = \mathbf{T} \cdot \mathbf{a}:
Substitute (dT)/(ds)=kN\frac{d\mathbf{T}}{ds} = k \mathbf{N}:
(d)/(ds)(cos theta)=k(N*a).\frac{d}{ds} (\cos\theta) = k (\mathbf{N} \cdot \mathbf{a}).
Let N*a=sin theta*cos psi\mathbf{N} \cdot \mathbf{a} = \sin\theta \cdot \cos\psi, where psi\psi is the angle between N\mathbf{N} and the projection of a\mathbf{a} onto the plane of T\mathbf{T} and N\mathbf{N}. Thus:
(d cos theta)/(ds)=k sin theta cos psi.\frac{d\cos\theta}{ds} = k \sin\theta \cos\psi.
For cos phi=B*a\cos\phi = \mathbf{B} \cdot \mathbf{a}:
(d cos phi)/(ds)=-tau sin theta cos psi.\frac{d\cos\phi}{ds} = -\tau \sin\theta \cos\psi.
Step 4: Relationship Between theta\theta and phi\phi
Using cos theta=T*a\cos\theta = \mathbf{T} \cdot \mathbf{a} and cos phi=B*a\cos\phi = \mathbf{B} \cdot \mathbf{a}, we differentiate with respect to ss and relate theta\theta and phi\phi:
(d cos theta)/(d cos phi)=(k)/( tau).\frac{d\cos\theta}{d\cos\phi} = \frac{k}{\tau}.
Switching to theta\theta and phi\phi themselves, the relationship becomes: