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Law of Refraction

The law of refraction, which is generally known as Snell's law, governs the behaviour of light-rays as they propagate across a sharp interface between two transparent dielectric media.

Consider a light-ray incident on a plane interface between two transparent dielectric media, labelled 1 and 2, as shown in Fig. 57. The law of refraction states that the incident ray, the refracted ray, and the normal to the interface, all lie in the same plane. Furthermore,

\begin{displaymath}
n_1\,\sin\theta_1 = n_2\,\sin\theta_2,
\end{displaymath} (341)

where $\theta_1$ is the angle subtended between the incident ray and the normal to the interface, and $\theta_2$ is the angle subtended between the refracted ray and the normal to the interface. The quantities $n_1$ and $n_2$ are termed the refractive indices of media 1 and 2, respectively. Thus, the law of refraction predicts that a light-ray always deviates more towards the normal in the optically denser medium: i.e., the medium with the higher refractive index. Note that $n_2>n_1$ in the figure. The law of refraction also holds for non-planar interfaces, provided that the normal to the interface at any given point is understood to be the normal to the local tangent plane of the interface at that point.
Figure 57: The law of refraction.
\begin{figure}
\epsfysize =3in
\centerline{\epsffile{refract.eps}}
\end{figure}

By definition, the refractive index $n$ of a dielectric medium of dielectric constant $K$ is given by

\begin{displaymath}
n = \sqrt{K}.
\end{displaymath} (342)

Table 4 shows the refractive indices of some common materials (for yellow light of wavelength $\lambda =589$nm).

Table 4: Refractive indices of some common materials at $\lambda =589$ nm.
Material $n$
Air (STP) 1.00029
Water 1.33
Ice 1.31
Glass:  
  Light flint 1.58
  Heavy flint 1.65
  Heaviest flint 1.89
Diamond 2.42


The law of refraction follows directly from the fact that the speed $v$ with which light propagates through a dielectric medium is inversely proportional to the refractive index of the medium (see Sect. 11.3). In fact,

\begin{displaymath}
v =\frac{c}{n},
\end{displaymath} (343)

where $c$ is the speed of light in a vacuum. Consider two parallel light-rays, $a$ and $b$, incident at an angle $\theta_1$ with respect to the normal to the interface between two dielectric media, 1 and 2. Let the refractive indices of the two media be $n_1$ and $n_2$ respectively, with $n_2>n_1$. It is clear from Fig. 58 that ray $b$ must move from point $B$ to point $Q$, in medium 1, in the same time interval, ${\mit\Delta} t$, in which ray $a$ moves between points $A$ and $P$, in medium 2. Now, the speed of light in medium 1 is $v_1=c/n_1$, whereas the speed of light in medium 2 is $v_2=c/n_2$. It follows that the length $BQ$ is given by $v_1\,{\mit\Delta} t$, whereas the length $AP$ is given by $v_2\,{\mit\Delta} t$. By trigonometry,
\begin{displaymath}
\sin\theta_1 = \frac{BQ}{AQ} = \frac{v_1\,{\mit\Delta} t}{AQ},
\end{displaymath} (344)

and
\begin{displaymath}
\sin\theta_2 = \frac{AP}{AQ} = \frac{ v_2\,{\mit\Delta} t}{AQ}.
\end{displaymath} (345)

Hence,
\begin{displaymath}
\frac{\sin\theta_1}{\sin\theta_2} = \frac{v_1}{v_2} = \frac{n_2}{n_1},
\end{displaymath} (346)

which can be rearranged to give Snell's law. Note that the lines $AB$ and $PQ$ represent wave-fronts in media 1 and 2, respectively, and, therefore, cross rays $a$ and $b$ at right-angles.
Figure 58: Derivation of Snell's law.
\begin{figure}
\epsfysize =3.5in
\centerline{\epsffile{diagram.eps}}
\end{figure}

When light passes from one dielectric medium to another its velocity $v$ changes, but its frequency $f$ remains unchanged. Since, $v=f\,\lambda$ for all waves, where $\lambda$ is the wavelength, it follows that the wavelength of light must also change as it crosses an interface between two different media. Suppose that light propagates from medium 1 to medium 2. Let $n_1$ and $n_2$ be the refractive indices of the two media, respectively. The ratio of the wave-lengths in the two media is given by

\begin{displaymath}
\frac{\lambda_2}{\lambda_1} = \frac{v_2/f}{v_1/f} =
\frac{v_2}{v_1}=\frac{n_1}{n_2}.
\end{displaymath} (347)

Thus, as light moves from air to glass its wavelength decreases.


next up previous
Next: Total Internal Reflection Up: Geometric Optics Previous: Law of Reflection
Richard Fitzpatrick 2007-07-14