/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Problem 10 Find the geodesics on the parabo... [FREE SOLUTION] | 91Ó°ÊÓ

91Ó°ÊÓ

Find the geodesics on the parabolic cylinder \(y=x^{2}\).

Short Answer

Expert verified
Geodesics largely follow u,z parameters curved in initial parametric input.

Step by step solution

01

Title - Parametrize the Surface

A good starting point is to parametrize the surface of the parabolic cylinder. Use the surface equation and a parameter. Let the parameters be: \( x = u \) \( y = u^2 \) \( z = v \)
02

Title - Find the Metric Tensor

Next, compute the metric tensor. Start by finding the partial derivatives of the parametric equations with respect to the parameters \(u\) and \(v\):\( \mathbf{r}_u = (1, 2u, 0) \)\( \mathbf{r}_v = (0, 0, 1) \)The metric tensor \(g_{ij}\) is then:\[ g_{ij} = \begin{pmatrix} \mathbf{r}_u \ \mathbf{r}_v \end{pmatrix} \begin{pmatrix} \mathbf{r}_u^T & \mathbf{r}_v^T \end{pmatrix} \]Computing the inner products:\[ g_{11} = \mathbf{r}_u \cdot \mathbf{r}_u = 1 + 4u^2, \ g_{12} = \mathbf{r}_u \cdot \mathbf{r}_v = 0, \ g_{22} = \mathbf{r}_v \cdot \mathbf{r}_v = 1 \]So, the metric tensor \(g_{ij}\) is:\[ g_{ij} = \begin{pmatrix} 1+4u^2 & 0 \ 0 & 1 \end{pmatrix} \]
03

Title - Write Down the Geodesic Equations

With the metric tensor known, write down the geodesic equations using the Christoffel symbols. The geodesic equations are:\[ \frac{d^2 u^k}{d \tau^2} + \Gamma_{ij}^k \frac{d u^i}{d \tau} \frac{d u^j}{d \tau} = 0 \]where the Christoffel symbols \( \Gamma_{ij}^k \) are calculated from the metric tensor. For the metric tensor \(g_{ij}\), Christoffel symbols can be computed, but in this specific case, it's easier to see the inherent symmetry and deduce these values directly.
04

Title - Solve the Geodesic Equations

Given the simplicity of the parameterization and metric, simpler geodesic paths occur when the complexity of curvature is bounded by parameters. This means lines parallel to the z-axis and slight curvatures due to \(u\). General solutions are combinations of connections on lines projected on z from the initial lines along the parabolic x,y relationship. Numerical methods might be required for more detail.
05

Title - Interpret the Physical Meaning

Translate the mathematical solutions into a physical and visual interpretation. Normally, the shortest path on the cylinder will follow the curves of the parabolic surface but projected, such paths simplify for lines along 'z', thus direct translation happens more simplified.

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with 91Ó°ÊÓ!

Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Parametric Surfaces
To understand geodesics, we start with the concept of parametric surfaces. This is a way to describe a surface using parameters and equations. For the parabolic cylinder, the surface is described by the equation \(y = x^2\). We use parameters \(u\) and \(v\) to express this surface as:
  • \( x = u \)
  • \( y = u^2 \)
  • \( z = v \)
This means any point on the surface can be described using these two variables. This method helps us simplify and break down complex surfaces into manageable pieces.
Metric Tensor
The metric tensor is a key concept in differential geometry as it helps measure distances on surfaces. Once we have our parametric equations, we find partial derivatives with respect to parameters (\(u\) and \(v\)). For the parabolic cylinder:
  • \(\mathbf{r}_u = (1, 2u, 0)\)
  • \(\mathbf{r}_v = (0, 0, 1)\)
The metric tensor \(g_{ij}\) is built using these partial derivatives. We compute inner products:
  • \( g_{11} = \mathbf{r}_u \cdot \mathbf{r}_u = 1 + 4u^2 \)
  • \( g_{12} = \mathbf{r}_u \cdot \mathbf{r}_v = 0 \)
  • \( g_{22} = \mathbf{r}_v \cdot \mathbf{r}_v = 1 \)

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

A uniform flexible chain of given length is suspended at given points \(\left(x_{1}, y_{1}\right)\) and \(\left(x_{2}, y_{2}\right) .\) Find the curve in which it hangs. Hint: It will hang so that its center of gravity is as low as possible.

A yo-yo (as shown) falls under gravity. Assume that it falls straight down, unwinding as it goes. Find the Lagrange equation of motion. Hints: The kinetic energy is the sum of the translational energy \(\frac{1}{2} m \dot{z}^{2}\) and the rotational energy \(\frac{1}{2} I \dot{\theta}^{2}\) where \(I\) is the moment of inertia. What is the relation between \(\dot{z}\) and \(\dot{\theta}\) ? Assume the yo-yo is a solid cylinder with inner radius \(a\) and outer radius \(b\).

In the brachistochrone problem, show that if the particle is given an initial velocity \(v_{0} \neq 0,\) the path of minimum time is still a cycloid.

A hoop of mass \(M\) and radius \(a\) rolls without slipping down an inclined plane of angle \(\alpha .\) Find the Lagrangian and the Lagrange equation of motion. Hint: The kinetic energy of a body which is both translating and rotating is a sum of two terms: the translational kinetic energy \(\frac{1}{2} M v^{2}\) where \(v\) is the velocity of the center of mass, and the rotational kinetic energy \(\frac{1}{2} I \omega^{2}\) where \(\omega\) is the angular velocity and \(I\) is the moment of inertia around the rotation axis through the center of mass.

Write the \(\theta\) Lagrange equation for a particle moving in a plane if \(V=V(r)\) (that is, a central force). Use the \(\theta\) equation to show that: (a) The angular momentum \(\mathbf{r} \times m \mathbf{v}\) is constant. (b) The vector \(\mathbf{r}\) sweeps out equal areas in equal times (Kepler's second law).

See all solutions

Recommended explanations on Combined Science Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.