Course Objectives
At the completion of this course, students will be able to
1) calculate physical quantities such as work and energy.
2) calculate physical quantities such as work and energy.
3) obtain physical quantities such as angular momentum in planetary motion and other rotational motions.
Rubric
| Ideal Level of Achievement (Very Good) | Standard Level of Achievement (Good) | Unacceptable Level of Achievement (Fail) |
Evaluation 1 | Can calculate work and energy and obtain the motion of the particle. | Can calculate physical quantities such as work and energy. | Can't calculate physical quantities such as work and energy. |
Evaluation 2 | Can obtain a solution by using the conservation law for the collision problem of two particle. | Can calculate physical quantities such as work and energy. | Can't calculate physical quantities such as work and energy. |
Evaluation 3 | Can obtain rotational motion using the angular momentum conservation law, and so on. | Can obtain physical quantities such as angular momentum in planetary motion and other rotational motions. | Can't obtain physical quantities such as angular momentum in planetary motion and other rotational motions. |
Assigned Department Objectives
学習・教育到達度目標 A-5
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JABEE 1(2)(c)
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ディプロマポリシー 3
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Teaching Method
Outline:
Students will learn how to explain various phenomena based on a small number of basic physical laws.
The students will study the relation between work and energy in motion of 1 particles, the general theory of two-body problem, and collision problems, based on the knowledge of the lecture in applied physics I.
In addition, the momentum conservation law and the angular momentum conservation law will be studied, and the collision problems and the motion of the planet will be analyzed.
Style:
Lecture and exercises
Notice:
Students need to understand mathematics and physics that they have learned by the first semester of their third year.
Review the items that you cannot understand in advance.
Students are required to read the relevant part of the textbook on the day before the class, and to re-solve the exercises done in class or in the textbook after the class.
In this course, credit will be given for a score of 60 or more.
Students who receive less than 60 points may take a supplementary examination upon request. Students who receive credit for the examination will receive a grade of 60.
Characteristics of Class / Division in Learning
Course Plan
|
|
|
Theme |
Goals |
1st Semester |
1st Quarter |
1st |
Work and energy (I) |
Can calculate work in case of constant force.
|
2nd |
Work and energy (II) |
Can calculate work in case of force that chages strength.
|
3rd |
Work and energy (III) |
Can calculate the energy conservation law in two dimensional space.
|
4th |
Two-body problems |
Can construct equations of motion when 2 particles interact with each other, and derive the equation of motion of barycentric coordinates and relative coordinates.
|
5th |
Momentum and impulse |
Can derive the relationship between momentum variation and force product from the equation of motion.
|
6th |
Momentum conservation law and collision problems (I) |
Can derive the momentum conservation law when the external force is not working, and solve the one dimensional elastic collision problem.
|
7th |
Momentum conservation law and collision problems (II) |
Can solve the problems of one dimensional inelastic collision and two dimensional elastic collision.
|
8th |
Midterm exam |
|
2nd Quarter |
9th |
Answers to the midterm exam |
|
10th |
Outer product and angular momentum |
Can calculate the outer product of two vectors, and represent angular momentum and moment of force by using the outer product.
|
11th |
Central force and angular momentum conservation law (I) |
Can obtain the angular momentum conservation law from the equation of motion where the central force acts.
|
12th |
Central force and angular momentum conservation law (II) |
Can solve the problems of the angular momentum conservation law.
|
13th |
Universal gravitation and planetary motion(I) |
Can solve the Kepler-problem in the case of a circular motion.
|
14th |
Universal gravitation and planetary motion(II) |
Can calculate the potential energy of gravitational force.
|
15th |
Final exam |
|
16th |
Answers to the final exam |
|
Evaluation Method and Weight (%)
| Examination | Presentation | Mutual Evaluations between students | Behavior | Portfolio | Other | Total |
Subtotal | 100 | 0 | 0 | 0 | 0 | 0 | 100 |
Basic Ability | 100 | 0 | 0 | 0 | 0 | 0 | 100 |
Technical Ability | 0 | 0 | 0 | 0 | 0 | 0 | 0 |
Interdisciplinary Ability | 0 | 0 | 0 | 0 | 0 | 0 | 0 |