### Section Learning Objectives

By the end of this section, you will be able to do the following:

- Describe the Compton effect
- Calculate the momentum of a photon
- Explain how photon momentum is used in solar sails
- Explain the particle-wave duality of light

### Teacher Support

#### Teacher Support

The learning objectives in this section will help your students master the following standards:

- (3) Scientific processes. The student uses critical thinking, scientific reasoning, and problem solving to make informed decisions within and outside the classroom. The student is expected to:
- (D) explain the impacts of the scientific contributions of a variety of historical and contemporary scientists on scientific thought and society.

- (8) Science concepts. The student knows simple examples of atomic, nuclear, and quantum phenomena. The student is expected to:
- (A) describe the photoelectric effect and the dual nature of light.

### Section Key Terms

Compton effect | particle-wave duality | photon momentum |

### Photon Momentum

### Teacher Support

#### Teacher Support

Have students read the section heading. Ask them whether photons demonstrate momentum. They should answer yes, based on the photoelectric effect. Ask them what equation they would use to calculate this momentum. Push them on the idea that the momentum equation relies on mass, while photons are massless particles.

Do photons abide by the fundamental properties of physics? Can packets of electromagnetic energy possibly follow the same rules as a ping-pong ball or an electron? Although strange to consider, the answer to both questions is yes.

Despite the odd nature of photons, scientists prior to Einstein had long suspected that the fundamental particle of electromagnetic radiation shared properties with our more macroscopic particles. This is no clearer than when considering the photoelectric effect, where photons knock electrons out of a substance. While it is strange to think of a massless particle exhibiting momentum, it is now a well-established fact within the scientific community. Figure 21.10 shows macroscopic evidence of photon momentum.

Figure 21.10 shows a comet with two prominent tails. Comet tails are composed of gases and dust evaporated from the body of the comet and ionized gas. What most people do not know about the tails is that they always point *away *from the Sun rather than trailing behind the comet. This can be seen in the diagram.

Why would this be the case? The evidence indicates that the dust particles of the comet are forced away from the Sun when photons strike them. Evidently, photons carry momentum in the direction of their motion away from the Sun, and some of this momentum is transferred to dust particles in collisions. The blue tail is caused by the solar wind, a stream of plasma consisting primarily of protons and electrons evaporating from the corona of the Sun.

### Momentum, The Compton Effect, and Solar Sails

Momentum is conserved in quantum mechanics, just as it is in relativity and classical physics. Some of the earliest direct experimental evidence of this came from the scattering of X-ray photons by electrons in substances, a phenomenon discovered by American physicist Arthur H. Compton (1892–1962). Around 1923, Compton observed that X-rays reflecting from materials had decreased energy and correctly interpreted this as being due to the scattering of the X-ray photons by electrons. This phenomenon could be handled as a collision between two particles—a photon and an electron at rest in the material. After careful observation, it was found that both energy and momentum were conserved in the collision. See Figure 21.11. For the discovery of this conserved scattering, now known as the Compton effect, Arthur Compton was awarded the Nobel Prize in 1929.

Shortly after the discovery of Compton scattering, the value of the photon momentum, $p=\frac{h}{\lambda},$

was determined by Louis de Broglie. In this equation, called the de Broglie relation, *h *represents Planck’s constant and *λ *is the photon wavelength.

### Teacher Support

#### Teacher Support

[BL][OL]Can students think of an equivalent macroscopic event that models both momentum and energy? Discuss the difficulties in modeling this on the particle scale.

[AL]Have the students determine what information would need to be measured in order to show that both quantum energy and momentum were conserved. Additionally, the students could create a set of data that would fulfill the energy and momentum conservation equations used in Figure 21.11.

We can see that photon momentum is small, since $p=h/\lambda .$ and *h *is very small. It is for this reason that we do not ordinarily observe photon momentum. Our mirrors do not recoil when light reflects from them, except perhaps in cartoons. Compton saw the effects of photon momentum because he was observing X-rays, which have a small wavelength and a relatively large momentum, interacting with the lightest of particles, the electron.

### Worked Example

#### Electron and Photon Momentum Compared

(a) Calculate the momentum of a visible photon that has a wavelength of 500 nm. (b) Find the velocity of an electron having the same momentum. (c) What is the energy of the electron, and how does it compare with the energy of the photon?

### Strategy

Finding the photon momentum is a straightforward application of its definition: $p=h/\lambda .$ If we find the photon momentum is small, we can assume that an electron with the same momentum will be nonrelativistic, making it easy to find its velocity and kinetic energy from the classical formulas.

Photon momentum is given by the de Broglie relation.

Entering the given photon wavelength yields

Since this momentum is indeed small, we will use the classical expression $p=mv$ to find the velocity of an electron with this momentum. Solving for *v *and using the known value for the mass of an electron gives

The electron has kinetic energy, which is classically given by

Thus,

Converting this to eV by multiplying by $\frac{\left(1\phantom{\rule{0.3em}{0ex}}\text{eV}\right)}{\left(1.602\phantom{\rule{0.25em}{0ex}}\times \phantom{\rule{0.25em}{0ex}}{10}^{\u201319}\text{J}\right)}\text{}$ yields

The photon energy *E* is

which is about five orders of magnitude greater.

Even in huge numbers, the total momentum that photons carry is small. An electron that carries the same momentum as a 500-nm photon will have a 1,460 m/s velocity, which is clearly nonrelativistic. This is borne out by the experimental observation that it takes far less energy to give an electron the same momentum as a photon. That said, for high-energy photons interacting with small masses, photon momentum may be significant. Even on a large scale, photon momentum can have an effect if there are enough of them and if there is nothing to prevent the slow recoil of matter. Comet tails are one example, but there are also proposals to build space sails that use huge low-mass mirrors (made of aluminized Mylar) to reflect sunlight. In the vacuum of space, the mirrors would gradually recoil and could actually accelerate spacecraft within the solar system. See the following figure.

### Tips For Success

When determining energies in particle physics, it is more sensible to use the unit eV instead of Joules. Using eV will help you to recognize differences in magnitude more easily and will make calculations simpler. Also, eV is used by scientists to describe the binding energy of particles and their rest mass, so using eV will eliminate the need to convert energy quantities. Finally, eV is a convenient unit when linking electromagnetic forces to particle physics, as one eV is the amount energy given to an electron when placed in a field of 1-V potential difference.

### Practice Problems

Find the momentum of a 4.00-cm wavelength microwave photon.

- 0.83 × 10
^{−32}kg ⋅ m/s - 1.66 × 10
^{−34}kg ⋅ m/s - 0.83 × 10
^{−34}kg ⋅ m/s - 1.66 × 10
^{-32}kg ⋅ m/s

Calculate the wavelength of a photon that has the same momentum of a proton moving at 1.00 percent of the speed of light.

- 2.43 × 10
^{−10}m - 2.43 × 10
^{−12}m - 1.32 × 10
^{−15}m - 1.32 × 10
^{−13}m

### Links To Physics

#### LightSail-1 Project

*“Provide ships or sails adapted to the heavenly breezes, and there will be some who will brave even that void.”*

*— Johannes Kepler (in a letter to Galileo Galilei in 1608)*

Traversing the Solar System using nothing but the Sun’s power has long been a fantasy of scientists and science fiction writers alike. Though physicists like Compton, Einstein, and Planck all provided evidence of light’s propulsive capacity, it is only recently that the technology has become available to truly put these visions into motion. In 2016, by sending a lightweight satellite into space, the LightSail-1 project is designed to do just that.

A citizen-funded project headed by the Planetary Society, the 5.45-million-dollar LightSail-1 project is set to launch two crafts into orbit around the Earth. Each craft is equipped with a 32-square-meter solar sail prepared to unfurl once a rocket has launched it to an appropriate altitude. The sails are made of large mirrors, each a quarter of the thickness of a trash bag, which will receive an impulse from the Sun’s reflecting photons. Each time the Sun’s photon strikes the craft’s reflective surface and bounces off, it will provide a momentum to the sail much greater than if the photon were simply absorbed.

Attached to three tiny satellites called CubeSats, whose combined volume is no larger than a loaf of bread, the received momentum from the Sun’s photons should be enough to record a substantial increase in orbital speed. The intent of the LightSail-1 mission is to prove that the technology behind photon momentum travel is sound and can be done cheaply. A test flight in May 2015 showed that the craft’s Mylar sails could unfurl on command. With another successful result in 2016, the Planetary Society will be planning future versions of the craft with the hopes of eventually achieving interplanetary satellite travel. Though a few centuries premature, Kepler’s fantastic vision may not be that far away.

### Particle-Wave Duality

### Teacher Support

#### Teacher Support

Prior to this section, have the students create a chart of observations with columns that show that light is like a wave and light is like a particle. Reinforce that light is simply fulfilling both models and that we do not have a perfect model to describe its properties. Light does not *choose* when to be like a particle and when to be like a wave.

We have long known that EM radiation is like a wave, capable of interference and diffraction. We now see that light can also be modeled as particles—massless photons of discrete energy and momentum. We call this twofold nature the particle-wave duality, meaning that EM radiation has properties of both particles and waves. This may seem contradictory, since we ordinarily deal with large objects that never act like both waves and particles. An ocean wave, for example, looks nothing like a grain of sand. However, this so-called duality is simply a term for properties of the photon analogous to phenomena we can observe directly, on a macroscopic scale. See Figure 21.14. If this term seems strange, it is because we do not ordinarily observe details on the quantum level directly, and our observations yield either particle-like *or *wave-like properties, but never both simultaneously.

Since we have a particle-wave duality for photons, and since we have seen connections between photons and matter in that both have momentum, it is reasonable to ask whether there is a particle-wave duality for matter as well. If the EM radiation we once thought to be a pure wave has particle properties, is it possible that matter has wave properties? The answer, strangely, is yes. The consequences of this are tremendous, as particle-wave duality has been a constant source of scientific wonder during the twentieth and twenty-first centuries.

### Check Your Understanding

What fundamental physics properties were found to be conserved in Compton scattering?

- energy and wavelength
- energy and momentum
- mass and energy
- energy and angle

Why do classical or relativistic momentum equations not work in explaining the conservation of momentum that occurs in Compton scattering?

- because neither classical nor relativistic momentum equations utilize mass as a variable in their equations
- because relativistic momentum equations utilize mass as a variable in their formulas but classical momentum equations do not
- because classical momentum equations utilize mass as a variable in their formulas but relativistic momentum equations do not
- because both classical and relativistic momentum equations utilize mass as a variable in their formulas

True or false—It is possible to propel a solar sail craft using just particles within the solar wind.

- true
- false

True or false—Photon momentum more directly supports the wave model of light.

- false
- true

True or false—wave-particle duality exists for objects on the macroscopic scale.

- false
- true

What type of electromagnetic radiation was used in Compton scattering?

- visible light
- ultraviolet radiation
- radio waves
- X-rays