Amherst College: Syllabus https://www.amherst.edu/ en Syllabus https://www.amherst.edu/academiclife/departments/courses/0809S/PHYS/PHYS-16-0809S/info/syllabus/node/85821 <span class="field field--name-title field--type-string field--label-hidden">Syllabus</span> <span class="field field--name-uid field--type-entity-reference field--label-hidden"><span>Nicholas C. Darnton (inactive)</span></span> <span class="field field--name-created field--type-created field--label-hidden"><time datetime="2009-01-06T22:00:08-05:00" title="Tuesday, January 6, 2009, at 10:00 PM" class="datetime">Tuesday, 1/6/2009, at 10:00 PM</time> </span> <div class="field field--name-body field--type-text-with-summary field--label-hidden field__item"><p>Physics 16 is an introduction to mechanics at the level of Newton's laws of motion.&nbsp; We will present Newton's laws within the first three weeks of the course and apply them to standard phenomena of introductory mechanics:&nbsp; pulleys, ropes, springs, levers, friction and inclined planes.&nbsp; We will develop concepts and techniques to solve more challenging mechanics problems;&nbsp; chief among these techniques are the conservation laws of energy, momentum, and angular momentum.&nbsp; We will learn when these quantities are conserved and how to use conservation laws to simplify mechanics problems.</p><p>Many of the concepts introduced in Physics 16 will be important in other contexts; an understanding of energy, power, force, work and momentum is critical to every subsequent physics course, to chemistry, geology, and astronomy, and to small-scale (molecular) and large-scale biology (ecology).</p><p>Newton's laws are most easily understood using calculus, and we will frequently refer to concepts, such as derivatives and integrals, from calculus.&nbsp; An understanding of calculus is important, and a solid grasp of trigonometry is critical.&nbsp; However, this is not a math class: we will distinguish between physics (writing down a self-consistent set of equations that uniquely define the important properties of a system) and math (solving those equations); the former is important, while the latter is a chore.&nbsp; We will discuss the difference between a mathematical solution and the physically allowed portions of that solution.&nbsp;</p><p>The methods we develop could, in principle, be used to solve very complex problems, but the math becomes prohibitively tedious and time-consuming.&nbsp; Most problems we encounter will involve, at worst, piecewise constant acceleration.&nbsp; At the end of the course we will encounter situations requiring non-constant accelerations: periodic motion of a mass and of a wave.&nbsp; Time permitting, we will see how Kepler's laws of planetary motion&nbsp; – the culmination of centuries of inquiry – are nothing more than a special case of Newton's laws with a particular force field.</p><p>The lecture portion of the course will focus primarily on problem solving.&nbsp; Exams will be effectively small, timed problem sets.&nbsp; The lab portion will apply the concepts from lecture to real situations, where dropped factors of two will become blindingly obvious.&nbsp; We will discuss measurement error and develop error propagation. &nbsp;</p></div> Wed, 07 Jan 2009 03:00:08 +0000 ndarnton 85821 at https://www.amherst.edu