Forces


Introduction

We have been negligent to dive deeper into forces, despite introducing it briefly in the previous chapter. As a refresher, forces are simply a push or pull that may change motion. Again, they are not directly responsible for maintaining or causing motion, like we discussed in the previous lesson.

The Four Fundamental Forces

  • Gravitational Force: This is a force that arises due to gravity. It is one of the forces that will be important to us. Gravity is a long-range force, since it requires bodies to have quite large masses in order to take any effect. There is a specific equation we can use to calculate it, but that comes later on. particle theorized to be the vector particle for the gravitational interaction is the graviton.

  • Electromagnetic Forces: Virtually all the forces that we experience and see in the world fall under this category (e.g. friction, air resistance, etc.). If you know chemistry, you know there are electrons around the nucleus of the atom. All these forces are caused by repulsion of the electrons in objects when they come into “contact” with another. Again, this isn’t important for our purposes. Electromagnetic forces can actually be short-range or long-range, but for right now, most of them will be short-range, specifically in the form of contact forces, so we’ll treat them that way. The photon is the particle responsible for the electromagnetic interaction.

  • Strong Forces: Not of too particular interest to us. It only happens at an atomic scale, and it is primarily responsible for holding the nucleus of an atom together. This is a short-range force, since it only happens within and between protons and neutrons (protons and neutrons are actually a composite of three quarks bound by the strong force). You can think of it this way—it only acts at distances of one femtometer ($10^{-15}~\textrm m$). Its vector particle is the gluon, and unlike the photon it has mass and contributes most of the mass of the proton and neutron.

  • Weak Forces: This force also doesn’t show up until much later. It is the force that is behind nuclear fission and radioactive decay. Interestingly, it discriminates between left-handed (left-spimming) and right-handed particles. It is also a short-range atomic-level force, but unlike the strong force we can see it in action (for instance, in radioactive decay, which has very real consequences!) .It is interesting to note, however, that this force and the electromagnetic force become one at very high temperatures. The vector particles of this force are the $W+$, $W-$, and $Z$ bosons.

You don’t need to remember any of this particle exchange stuff for the actual lesson, but Eric finds it interesting, so it’s included in here. (Note from Eric: Edward just doesn’t understand it—at least not yet). The bolded parts are what are actually important for you to remember for our lesson, and just remember that all four of these forces are the four fundamental forces in nature.

IMPORTANT!! If a force does not fall under the category of any of those four forces, it does not exist (Note from Eric: sort of, but that will be taught later)!

The Gravitational Force

Firstly, there’s the gravitational force, but remember, that’s long range force. It is the primary long range interaction we will be dealing with in Newtonian mechanics. It is denoted as $F_G$ or $F_g$. Let’s start by considering an object in free fall, where the gravitational force is the only force acting on it, assuming no air resistance. Remember from kinematics that a body undergoing free-fall has acceleration equal to $g$, which is equal to $9.81~\textrm m /\textrm s$. $g$ is also sometimes called the gravitational field strength, and its units may also be denoted as $\textrm N /\textrm{kg}$. Thus, by Newton’s second law, the net force, or sum of all forces is equal to just $F_g$. But $F_g=ma$, and since we know the magnitude of acceleration to be $g$, $F_g=mg$. This is one of the primary forces that you will be dealing with.

Electromagnetic Forces

The following are all contact forces, meaning direct contact is required for them. Since these don’t look like gravitational forces, what must they be? Electromagnetic forces.

The normal force is the contact force exerted by a surface perpendicular to itself. It is denoted by $F_n$ or $F_N$. On a flat tabletop, the normal force acting on an object will always be upwards, but if you will note, on a surface that is tilted at an angle, the normal force points perpendicularly to the surface, so it is not perfectly upwards in that case. There is no particular equation that we use to calculate the normal force, it is pretty much always calculated from other forces acting on the body.

Tension forces are stretch forces transmitted along rope or similar materials. They are denoted by $F_T$ or sometimes just $T$ (though this letter is used to represent other quantities as well). We will assume that all the strings we work with are massless and inflexible (actually, in physics, a string literally implies masslessness, while using the word “rope” implies that there is mass). The reason for this is because massless means the tension is equally distributed throughout the entire string, and inflexible means the length of the string always remains constant (no stretching). Again, there is no specific equation to calculate the tension in a string, you will usually use other known values to calculate it in specific scenarios.

The last of these forces is called the frictional force, which is discussed upon in the next page. Remember that all these forces are not "new" fundamental forces, they are simply types of forces that fall under the categorization of electromagnetic forces!! For the rest of mechanics, if we introduce a force, and you know for sure its not gravity, then it is obviously an electromagnetic force, since it is not strong nor weak (we aren't dealing with those two remember).

The Frictional Force


Note: Even though the title says "The Frictional Force", it's NOT a new "type" of force. Remember that frictional forces fall under the Electromagnetic forces category.

Frictional forces are contact forces exerted parallel to a surface. They are denoted by $F_f$ or sometimes simply $f$ (though, again, this is a letter used by other quantities as well). Friction is really quite a complex force resulting from microscopic interactions between the irregularities between surfaces. Even things that seem very smooth have many ridges and bumps at a microscopic level. Friction between surfaces is proportional to the normal force and a dimensionless constant known as the coefficient of friction, which varies between surfaces and for different modes of motion.

In general, there are two types of frictional forces: static and kinetic. Static friction acts when an object is still at rest relative to the surface it rests on. Kinetic friction acts when an object is in motion relative to the surface it rests on.

The coefficient of static friction is denoted as $\mu_s$ and kinetic friction $\mu_k$. Static friction is also sometimes written as $\mu_s^{MAX}$, and you will see why in a second. If both are equal, usually just $\mu$ is used for simplicity. The friction force is equal to $\mu \cdot F_N$ and is usually oppositely directed to any net applied force, but this doesn’t always hold true. The more general rule is that friction always opposes relative motion between two surfaces. This will become more prevalent later on when we teach free-body diagrams.

One really important concept that we recognize and clear out of the way for friction is how the frictional force actually works. Static friction is actually a force that will automatically adjust itself to match the applied force. However, there is a certain maximum for this. That's what $\mu_s$ is here for. The magnitude of the frictional force will always be $≤\mu_s F_N$, and so when you exceed that value, the frictional force turns into the kinetic frictional force, which is always constant value of $\mu_k \cdot F_N$. This means that the coefficient of static friction must be greater than the coefficient of kinetic friction!!

There's no doubt you've definitely tried to push something across a floor at some point in your life. You'll notice that it is actually harder to get the box moving at first, but once it is moving, it becomes a bit smoother sailing from there. What we just explained, if you think about it, perfectly matches up with this intuition!

A graph here to show what we mean:

Figure 1: A graph that shows the magnitude of frictional force over time, in accordance with the applied force.


You are probably wondering, is it possible for $\mu_k$ instead to be greater than $\mu_s$? Let's take a closer look. Remember, once we apply a force $F$ that less than or equal to $\mu_s F_N$, the object will not move because the static friction can counteract this force. However, once the force exceeds the value of $\mu_s F_N$, the object will begin to slide. That is the standard for how friction operates.

When it begins sliding, it switches to kinetic friction, $\mu_k F_N$. Now if $\mu_k$ is greater than $\mu_s$, then the magnitude of the kinetic frictional force will automatically be greater than the static frictional force, which means as soon as it switches to kinetic friction, the block will not move. But that contradicts our earlier statement of it will begin to slide when the applied force exceeds $\mu_s F_N$ in magnitude. So thus, the statement that $\mu_s≥\mu_k$ must hold.

Conclusion

So far, these are all the forces you will encounter. This chapter was not particularly problem-heavy, but more on concepts. There are most definitely more forces that we will add to our collection as we progress. As for you calculus students, we know you're itching to pull our your calculus tools. Unfortunately, this isn't your chapter just yet. Calculus will begin to play a more important role with the chapters to come! Remember, all these forces are not “new” types of forces, they all will fall under the category of one of the four fundamental forces in nature. We stress this importance because it's crucial that you realize the difference. In your journey through Newtonian mechanics, for the most part, if the force not is gravitational, then it must be electromagnetic.

But simply knowing these forces is not enough. You will learn how to use this knowledge to solve problems and draw free-body diagrams, which is arguably one of the most important things you will ever learn in mechanics.