Warning: foreach() argument must be of type array|object, bool given in /var/www/html/web/app/themes/studypress-core-theme/template-parts/header/mobile-offcanvas.php on line 20

The following are the values and standard errors of a physical quantity \(f(\theta)\) measured at various values of \(\theta\) (in which there is negligible error): \(\begin{array}{lcccc}\theta & 0 & \pi / 6 & \pi / 4 & \pi / 3 \\ f(\theta) & 3.72 \pm 0.2 & 1.98 \pm 0.1 & -0.06 \pm 0.1 & -2.05 \pm 0.1 \\ \theta & \pi / 2 & 2 \pi / 3 & 3 \pi / 4 & \pi \\ f(\theta) & -2.83 \pm 0.2 & 1.15 \pm 0.1 & 3.99 \pm 0.2 & 9.71 \pm 0.4\end{array}\) Theory suggests that \(f\) should be of the form \(a_{1}+a_{2} \cos \theta+a_{3} \cos 2 \theta\). Show that the normal equations for the coefficients \(a_{i}\) are $$ \begin{aligned} 481.3 a_{1}+158.4 a_{2}-43.8 a_{3} &=284.7 \\ 158.4 a_{1}+218.8 a_{2}+62.1 a_{3} &=-31.1 \\ -43.8 a_{1}+62.1 a_{2}+131.3 a_{3} &=368.4 \end{aligned} $$ (a) If you have matrix inversion routines available on a computer, determine the best values and variances for the coefficients \(a_{i}\) and the correlation between the coefficients \(a_{1}\) and \(a_{2}\). (b) If you have only a calculator available, solve for the values using GaussSeidel iteration starting from the approximate solution \(a_{1}=2, a_{2}=-2, a_{3}=\) 4.

Short Answer

Expert verified
Use matrix inversion to find \( a_1, a_2, a_3 \). Alternatively, apply Gauss-Seidel starting from \( a_1 = 2, a_2 = -2, a_3 = 4 \).

Step by step solution

01

Write Down the Given Values

The values of \( f(\theta) \) and their errors are given for various \( \theta \) values. Write these values in a tabular format for easy reference.
02

Formulate the Function Model

According to the theory, \(f(\theta) = a_1 + a_2 \cos \theta + a_3 \cos 2\theta \). Substitute the given \( \theta \) values into this function.
03

Set Up the Normal Equations

Use the method of least squares to derive the normal equations. The given normal equations are already provided: \[481.3 a_{1}+158.4 a_{2}-43.8 a_{3} =284.7 \ 158.4 a_{1}+218.8 a_{2}+62.1 a_{3} =-31.1 \ -43.8 a_{1}+62.1 a_{2}+131.3 a_{3}=368.4\]
04

Matrix Form Representation

Represent the normal equations in matrix form: \[ \begin{pmatrix} 481.3 & 158.4 & -43.8 \ 158.4 & 218.8 & 62.1 \ -43.8 & 62.1 & 131.3 \end{pmatrix} \begin{pmatrix} a_1 \ a_2 \ a_3 \end{pmatrix} = \begin{pmatrix} 284.7 \ -31.1 \ 368.4 \end{pmatrix} \]
05

Solve Using Matrix Inversion (Part a)

Use a computer with matrix inversion routines to solve the matrix equation: \( \mathbf{A} \mathbf{x} = \mathbf{b} \). Calculate \( \mathbf{x} = \mathbf{A}^{-1} \mathbf{b} \) to determine the best values for \( a_1, a_2, \text{ and } a_3 \). Find the variances and correlation between the coefficients.
06

Gauss-Seidel Iteration (Part b)

Start with the approximate solution: \(a_1 = 2, a_2 = -2, a_3 = 4\). Use Gauss-Seidel iteration to update the values iteratively. Update each coefficient using the others' current values until the values converge.

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 Vaia!

Key Concepts

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

Matrix Inversion
Matrix inversion is a fundamental concept in linear algebra. It involves finding a matrix, known as the inverse matrix, that, when multiplied by the original matrix, yields the identity matrix. This process is essential in solving systems of linear equations, particularly in the form \(\mathbf{A} \mathbf{x} = \mathbf{b}\).
To find the inverse of a matrix, several methods can be employed, including
  • Gaussian elimination
  • LU decomposition
  • Adjugate method.
These methods are particularly useful when dealing with complex systems that require precise solutions.
In the context of our exercise, matrix inversion helps determine the coefficients \(a_1, a_2, a_3\) by solving the matrix equation:
\ \mathbf{A} \mathbf{x} = \mathbf{b} \
Once the inverse matrix \ \mathbf{A}^{-1} \ is found, the coefficients can be computed using:
\ \mathbf{x} = \mathbf{A}^{-1} \mathbf{b} \
This method is efficient and accurate, especially when implemented through computational software.
Gauss-Seidel Iteration
The Gauss-Seidel iteration is an iterative method for solving a system of linear equations. This method is particularly useful when a quick approximation is needed, or computational resources are limited.
Here's how it works:
  • Start with an initial guess for the solution vector.
  • Iteratively update each variable using the most recent values of other variables.
  • Continue the process until the changes become negligibly small.
This approach is beneficial when solving our system of normal equations, especially when matrix inversion routines are unavailable. Starting with initial guesses (\(a_1 = 2, a_2 = -2, a_3 = 4\)), the Gauss-Seidel iteration can gradually refine the values until they converge to accurate solutions.
This method relies on updating each coefficient sequentially, improving the solution with each iteration.
Least Squares Method
The least squares method is a powerful statistical tool used to find the best-fitting curve or line through a set of data points. It minimizes the sum of the squares of the differences between observed values and the values provided by the model.
In our exercise, the least squares method is used to derive the normal equations for the coefficients \(a_1, a_2, a_3\). Given the theoretical model \(f(\theta) = a_1 + a_2 \cos\theta + a_3 \cos 2\theta\), we fit the model to the data points by minimizing the error.
The process involves:
  • Formulating the model equation.
  • Setting up the normal equations by equating partial derivatives of the error function to zero.
  • Solving the normal equations to find the optimal coefficients.
This method ensures that the model best represents the given data set with minimal discrepancies.
Correlation Coefficients
Correlation coefficients measure the strength and direction of the linear relationship between two variables. They range from -1 to 1, where:
  • -1 indicates a perfect negative correlation.
  • 0 indicates no correlation.
  • 1 indicates a perfect positive correlation.
In the context of our exercise, the correlation coefficient between coefficients (\(a_1\) and \(a_2\)) helps us understand the interdependence between these variables.
Using the coefficients found from the normal equations, calculating the correlation coefficient offers insights into how changes in one coefficient might influence the other. This is crucial for understanding the dynamics of our model and ensuring its accuracy and reliability.

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

The following are the values obtained by a class of 14 students when measuring a physical quantity \(x: 53.8,53.1,56.9,54.7,58.2,54.1,56.4,54.8,57.3,51.0,55.1\) \(55.0,54.2,56.6\) (a) Display these results as a histogram and state what you would give as the best value for \(x\). (b) Without calculation estimate how much reliance could be placed upon your answer to (a). (c) Databooks give the value of \(x\) as \(53.6\) with negligible error. Are the data obtained by the students in conflict with this?

According to a particular theory, two dimensionless quantities \(X\) and \(Y\) have equal values. Nine measurements of \(X\) gave values of \(22,11,19,19,14,27,8\), 24 and 18 , whilst seven measured values of \(Y\) were \(11,14,17,14,19,16\) and 14. Assuming that the measurements of both quantities are Gaussian distributed with a common variance, are they consistent with the theory? An alternative theory predicts that \(Y^{2}=\pi^{2} X\); is the data consistent with this proposal?

On a certain (testing) steeplechase course there are 12 fences to be jumped and any horse that falls is not allowed to continue in the race. In a season of racing a total of 500 horses started the course and the following numbers fell at each fence: \(\begin{array}{lrrrrrrrrrrrr}\text { Fence: } & 1 & 2 & 3 & 4 & 5 & 6 & 7 & 8 & 9 & 10 & 11 & 12 \\ \text { Falls: } & 62 & 75 & 49 & 29 & 33 & 25 & 30 & 17 & 19 & 11 & 15 & 12\end{array}\) Use this data to determine the overall probability of a horse falling at a fence, and test the hypothesis that it is the same for all horses and fences as follows. (a) draw up a table of the expected number of falls at each fence on the basis of the hypothesis; (b) consider for each fence \(i\) the standardised variable $$ z_{i}=\frac{\text { estimated falls }-\text { actual falls }}{\text { standard deviation of estimated falls }} $$ and use it in an appropriate \(\chi^{2}\) test; (c) show that the data indicates that the odds against all fences being equally testing are about 40 to \(1 .\) Identify the fences that are significantly easier or harder than the average.

A group of students uses a pendulum experiment to measure \(g\), the acceleration of free fall, and obtain the following values (in \(\mathrm{m} \mathrm{s}^{-2}\) ): \(9.80,9.84,9.72,9.74\) \(9.87,9.77,9.28,9.86,9.81,9.79,9.82 .\) What would you give as the best value and standard error for \(g\) as measured by the group?

A particle detector consisting of a shielded scintillator is being tested by placing it near a particle source of controlled intensity (by the use of absorbers). It might register counts even in the absence of particles from the source because of the cosmic ray background. The number of counts \(n\) registered in a fixed time interval as a function of the source strength \(s\) is given in the following table: $$ \begin{array}{llrrrrrr} \text { Source strength: } s & 0 & 1 & 2 & 3 & 4 & 5 & 6 \\ \text { Counts } n: & 6 & 11 & 20 & 42 & 44 & 62 & 61 \end{array} $$ At any given source strength the number of counts is expected to be Poisson distributed with mean $$ n=a+b s $$ where \(a\) and \(b\) are constants. Analyse the data for a fit to this relationship and obtain the best values for \(a\) and \(b\) together with their standard errors. (a) How well is the cosmic ray background determined? (b) What is the value of the correlation coefficient between \(a\) and \(b\) ? Is this consistent with what would happen if the cosmic ray background were imagined to be negligible? (c) Does the data fit the expected relationship well? Is there any evidence that the reported data 'is too good a fit'?

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.

Sign-up for free