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Prof. Ming-chung CHU
Department of Physics, The Chinese University of Hong Kong

 

Imagine that one day you receive a gift. The catch is that you have to guess what it is without opening the wrapped box. How can you know what it is? Perhaps you will shake the box and guess the content by sensing its weight and shape. That is of course unreliable. Or you may watch the box under a lamp, hoping that part of the light will pass through it to produce a shadow of its content. An idea pops up: how about going to the airport and asking the security guards there to use their X-ray machine to examine your gift. That’s a good idea. However, all you find out is that there is a smaller box inside, made of thick plates of lead. You still cannot see what’s inside the smaller box even with the X-rays. So, what should you do?

Rest assured that you are not alone. Physicists who study the ultimate structure of matter face the same problem. With many years of work, they have already learned of many levels of structures in matter, but the quest to uncover the ultimate structure of matter is far from over. One technique that has helped physicists tremendously is really the same as your idea of shining X-rays through your gift box. This technique is called the collision experiment.

Through a series of collision experiments conducted between 1909 and 1914, the New Zealand physicist Ernest Rutherford and his students Hans Geiger and Ernest Marsden have not only made a breakthrough in atomic physics, but also set up a paradigm in modern experimental particle physics. Rutherford shot a beam of a-particles1 at a speed of about 20,000 km/s at a thin gold foil (Fig. 1). As he expected, most a-particles passed through the foil, with only slight changes in their velocities. However, to his surprise, a small fraction of a-particles suffered large deflections – some even rebounded backward! While most of the a-particles were passing straight through the gold foil as if they met no obstacles, a few crashed on very hard objects, resulting in back scattering. In Rutherford’s own words, "It was as if you fired a 15-inch shell at a piece of tissue paper and it came back and hit you."2. He concluded that most of the mass inside an atom were concentrated in a tiny space called the atomic nucleus. Furthermore, Rutherford deduced from the data that the diameter of an atomic nucleus is approximately m, which is merely one a hundred thousandth of an atom’s diameter. The atomic nuclei carry positive electric charges, and they therefore repel a-particles. Most of the space inside an atom is occupied by electrons, which are negatively charged. This atomic model of Rutherford proves to be generally correct. It reveals that atoms, which were previously thought to be the fundamental and indestructible, also have their own structures.


(Fig. 1 Rutherford’s collision experiment: colliding a-particles with a gold foil.)

Rutherford's experiment tells us not only the existence of the atomic nucleus, but also its mass. Assuming the conservation of momentum and energy, Rutherford calculated from his data that the masses of various atomic nuclei were all nearly integral multiples of the proton mass. The multiple is called the mass number and is approximately two times the atomic number3 of the element. He therefore speculated that an atomic nucleus was made up of roughly the same number of protons and another kind of particles called the neutron4, which was similar to the proton in mass but electrically neutral. How could one test this conjecture?

James Chadwick, another one of Rutherford’s students, eventually discovered the neutron in 1932. Chadwick again did a collision experiment, but this time he used two collisions instead of one. It is difficult to detect neutrons, because they have zero electric charge and high penetrability. Chadwick's method was to modify Rutherford's experiment mentioned above (Fig. 1) by adding an "air cushion" behind the foil, as shown in Fig. 2. The a-particles he used were energetic enough that they could break up the atomic nuclei in the beryllium foil to eject protons or neutrons (collectively known as nucleons). Rutherford had earlier discovered that protons could be released by colliding atoms with a-particles5, which proved that there were protons inside atomic nuclei. These protons were readily absorbed by the foil or air. Chadwick's idea was to intercept the ejected neutrons by the extra "air cushion" made of nitrogen gas. The neutrons might hit some nitrogen nuclei and expel them from the "air cushion". Being positively charged, these nitrogen nuclei were easily detectable.


(Fig. 2 Chadwick’s collision experiment: to prove the existence of neutrons using Nitrogen nuclei in secondary collisions.
)

Two fundamentally important concepts are involved in Rutherford's and Chadwick's experiments. First, nuclei are tiny and their diameters are far smaller than the wavelength of visible light. It is therefore impossible to 'see' their structures with optical microscopes. Chadwick's method was to bombard the atomic nuclei with high energy 'bullets' so as to break them up, and then he could infer the "contents" of atomic nuclei from the remnants. Just for fun, let us call this "the blast-it-up paradigm". Now you probably know how to deal with your gift box. Secondly, often it is not so easy to detect some particles such as the neutron directly. Chadwick therefore applied an indirect method; he introduced an additional element – the nitrogen nuclei – to 'catch' the neutrons. He could then not only prove the existence of the neutron, but also study its properties through its collisions with the nitrogen nuclei. This technique is frequently applied in modern physics. For example, two of the 2002 Nobel Physics Laureates applied this technique to construct neutrino5 telescopes successfully and made important discoveries in neutrino astrophysics.

Incidentally, Rutherford not only set up the "blast-it-up paradigm", but also made an unprecedented achievement. He was the first person ever to succeed in transforming one element into another6. It was a historic event in the development of science, technology, and civilization.