Crystal detector

Types

The crystal detector consisted of an electrical contact between the surface of a semiconducting crystalline mineral and either a metal or another crystal. Since at the time they were developed no one knew how they worked, crystal detectors evolved by trial and error. The construction of the detector depended on the type of crystal used, as it was found different minerals varied in how much contact area and pressure on the crystal surface was needed to make a sensitive rectifying contact. Crystals that required a light pressure like galena are used with the wire cat whisker contact; silicon is used with a heavier point contact, while silicon carbide (carborundum) can tolerate the heaviest pressure. Another type uses two crystals of different minerals with their surfaces touching, the most common being the "Perikon" detector. Since the detector can only function when the contact is made at certain spots on the crystal surface, the contact point was almost always made adjustable. Below are the major categories of crystal detectors used during the early 20th century:

Cat whisker detector

Patented by Karl Ferdinand Braun and Greenleaf Whittier Pickard in 1906, this was the most common type of crystal detector, mainly used with galena but also other crystals. It consists of a pea-size piece of crystalline mineral in a metal holder, with its surface touched by a fine metal wire or needle (the "cat whisker"). The contact between the tip of the wire and the surface of the crystal forms a crude unstable point-contact metal–semiconductor junction, forming a Schottky barrier diode. The wire whisker is the anode, and the crystal is the cathode; current can flow from the wire into the crystal but not in the other direction.

Only certain sites on the crystal surface function as rectifying junctions. The device is very sensitive to the exact geometry and pressure of contact between wire and crystal, and the contact can be disrupted by the slightest vibration. Therefore, a usable point of contact has to be found by trial and error before each use. The wire is suspended from a moveable arm and dragged across the crystal face by the user until the device begins functioning. In a crystal radio, the user will tune the radio to a strong local station if possible and then adjust the cat whisker until the station or radio noise (a static hissing noise) was heard in the radio's earphones. This requires some skill and a lot of patience. An alternative method of adjustment is to use a battery-operated electromechanical buzzer connected to the radio's ground wire or inductively coupled to the tuning coil, to generate a test signal. The spark produced by the buzzer's contacts functions as a weak radio transmitter whose radio waves can be received by the detector, so when a rectifying spot had been found on the crystal the buzz can be heard in the earphones, at which time the buzzer is turned off.

The detector consists of two parts mounted next to each other on a flat nonconductive base: a crystalline mineral forming the semiconductor side of the junction, and a "cat whisker", a springy piece of thin metal wire, forming the metal side of the junction

Crystal

The most common crystal used was galena (lead sulfide, PbS), a widely occurring ore of lead. Varieties were sold under the names "Lenzite" and "Hertzite". Other crystalline minerals were also used, the more common ones being iron pyrite (iron sulfide, FeS₂, "fool's gold", also sold under the trade names "Pyron", "Ferron", and "Radiocite") molybdenite (molybdenum disulfide, MoS₂), and cerussite (lead carbonate, PbCO₃) Not all specimens of a crystal will function in a detector. Often several crystal pieces had to be tried to find an active one. Galena with good detecting properties is rare and has no reliable visual characteristics distinguishing it.

A rough pebble of detecting mineral about the size of a pea was mounted in a metal cup, which formed one side of the circuit. The electrical contact between the cup and the crystal has to be good, because it is important for this contact to not to act as a second rectifying junction, which will create two back-to-back diodes which prevents the device from conducting at all. To make good contact with the crystal, it is either clamped with setscrews or embedded in solder. Because the relatively high melting temperature of tin-lead solder could damage many crystals, a fusible alloy with a low melting point, well under 200 °F (93 °C), such as Wood's metal is used. One surface is left exposed to allow contact with the cat-whisker wire.

Cat whisker wire

Phosphor bronze wire of about 30 AWG (0.25 mm) diameter was commonly used as a cat whisker because it had the right amount of springiness. It was mounted on an adjustable arm with an insulated handle so that the entire exposed surface of the crystal could be probed from many directions to find the most sensitive spot. Cat whiskers in homemade detectors usually had a simple curved shape, but most professional cat whiskers had a coiled section in the middle that served as a spring. The crystal requires just the right gentle pressure by the wire; too much pressure causes the device to conduct in both directions. Precision detectors made for radiotelegraphy stations often used a metal needle instead of a "cat's whisker", mounted on a thumbscrew-operated leaf spring to adjust the pressure applied. Gold or silver needles were used with some crystals.

Carborundum detector

Invented in 1906 by Henry H. C. Dunwoody, this consists of a piece of silicon carbide (SiC, then known by the trade name carborundum), either clamped between two flat metal contacts, or mounted in fusible alloy in a metal cup with a contact consisting of a hardened steel point pressed firmly against it with a spring. Carborundum, an artificial product of electric furnaces produced in 1893, requires a heavier pressure than the cat whisker contact. The carborundum detector was popular because its sturdy contact did not require readjustment each time it was used, like the delicate cat whisker devices. Some carborundum detectors were adjusted at the factory and then sealed and did not require adjustment by the user. It is not sensitive to vibration and so was used in shipboard wireless stations where the ship was rocked by waves, and military stations where vibration from gunfire could be expected. Another advantage is that it is tolerant of high currents, and cannot be "burned out" by atmospheric electricity from the antenna. Therefore, it was the most common type used in commercial radiotelegraphy stations.

Silicon carbide is a semiconductor with a wide band gap of 3 eV, so to make the detector more sensitive a forward bias voltage of around a volt was usually applied across the junction by a battery and potentiometer. The voltage is adjusted with the potentiometer until the sound was loudest in the earphone. The bias moves the operating point to the curved "knee" of the device's current–voltage curve, which produces the largest rectified current.

Silicon detector

Patented and first manufactured in 1906 by Pickard, this was the first type of crystal detector to be commercially produced. Silicon required more pressure than the cat whisker contact, although not as much as carborundum. A flat piece of silicon was embedded in fusible alloy in a metal cup, and a metal point, usually brass or gold, was pressed against it with a spring. The surface of the silicon was usually ground flat and polished. Silicon was also used with antimony and arsenic contacts. The silicon detector was popular because it had much the same advantages as carborundum; its firm contact could not be jarred loose by vibration and it did not require a bias battery, so it saw wide use in commercial and military radiotelegraphy stations.

Crystal-to-crystal detectors

Another category was detectors which used two different crystals with their surfaces touching, forming a crystal-to-crystal contact. The "Perikon" detector, invented 1908 by Pickard was the most common. Perikon stood for "PERfect pIcKard cONtact". It consisted of two crystals in metal holders, mounted face to face. One crystal was zincite (zinc oxide, ZnO), the other was a copper iron sulfide, either bornite (Cu₅FeS₄) or chalcopyrite (CuFeS₂). In Pickard's commercial detector (see picture), multiple zincite crystals were mounted in a fusible alloy in a round cup (on right), while the chalcopyrite crystal was mounted in a cup on an adjustable arm facing it (on left). The chalcopyrite crystal was moved forward until it touched the surface of one of the zincite crystals. When a sensitive spot was located, the arm was locked in place with the setscrew. Multiple zincite pieces were provided because the fragile zincite crystal could be damaged by excessive currents and tended to "burn out" due to atmospheric electricity from the wire antenna or currents leaking into the receiver from the powerful spark transmitters used at the time. This detector was also sometimes used with a small forward bias voltage of around 0.2V from a battery to make it more sensitive.

Although the zincite-chalcopyrite "Perikon" was the most widely used crystal-to-crystal detector, other crystal pairs were also used. Zincite was used with carbon, galena, and tellurium. Silicon was used with arsenic, antimony and tellurium crystals.

History

During the first three decades of radio, from 1888 to 1918, called the wireless telegraphy or "spark" era, primitive radio transmitters called spark gap transmitters were used, which generated radio waves by an electric spark. These transmitters were unable to produce the continuous sinusoidal waves which are used to transmit audio (sound) in modern AM or FM radio transmission. Instead spark gap transmitters transmitted information by wireless telegraphy; the user turned the transmitter on and off rapidly by tapping on a telegraph key, producing pulses of radio waves which spelled out text messages in Morse code. Therefore, the radio receivers of this era did not have to demodulate the radio wave, extract an audio signal from it as modern receivers do, they merely had to detect the presence or absence of the radio waves, to make a sound in the earphone when the radio wave was present to represent the "dots" and "dashes" of Morse code. The device which did this was called a detector. The crystal detector was the most successful of many detector devices invented during this era.

The crystal detector evolved from an earlier device, the first primitive radio wave detector, called a coherer, developed in 1890 by Édouard Branly and used in the first radio receivers in 1894–96 by Marconi and Oliver Lodge. Made in many forms, the coherer consisted of a high resistance electrical contact, composed of conductors touching with a thin resistive surface film, usually oxidation, between them. Radio waves changed the resistance of the contact, causing it to conduct a DC current. The most common form consisted of a glass tube with electrodes at each end, containing loose metal filings in contact with the electrodes. Before a radio wave was applied, this device had a high electrical resistance, in the megohm range. When a radio wave from the antenna was applied across the electrodes it caused the filings to "cohere" or clump together and the coherer's resistance fell, causing a DC current from a battery to pass through it, which rang a bell or produced a mark on a paper tape representing the "dots" and "dashes" of Morse code. Most coherers had to be tapped mechanically between each pulse of radio waves to return them to a nonconductive state.

The coherer was a very poor detector, motivating much research to find better detectors. It worked by complicated thin film surface effects, so scientists of the time did not understand how it worked, except for a vague idea that radio wave detection depended on some mysterious property of "imperfect" electrical contacts. Researchers investigating the effect of radio waves on various types of "imperfect" contacts to develop better coherers, invented crystal detectors.

Braun's experiments

The "unilateral conduction" of crystals was discovered by Karl Ferdinand Braun, a German physicist, in 1874 at the University of Würzburg. He studied copper pyrite (Cu₅FeS₄), iron pyrite (iron sulfide, FeS₂), galena (PbS) and copper antimony sulfide (Cu₃SbS₄). This was before radio waves had been discovered, and Braun did not apply these devices practically but was interested in the nonlinear current–voltage characteristic that these sulfides exhibited. Braun's method of making contact with the crystal may have been crucial to his results: he placed the sample on a circle of wire, then touched it with the end of a slender silver wire, a "cat's whisker" contact. Graphing the current as a function of voltage across a contact, he found the result was a line that was flat for current in one direction but curved upward for current in the other direction, instead of a straight line, showing that these substances did not obey Ohm's law. Due to this characteristic, some crystals had up to twice as much resistance to current in one direction as they did to current in the other. In 1877 and 1878 he reported further experiments with psilomelane, (Ba,H
₂O)
₂Mn
₅O
₁₀. Braun did investigations which ruled out several possible causes of asymmetric conduction, such as electrolytic action and some types of thermoelectric effects.

Thirty years after these discoveries, in 1899 Braun began experimenting with his crystalline contacts as radio wave detectors. However they were not usable at that time because crystal detectors were not compatible with the paper tape siphon recorder, the standard output device used by coherer receivers.

Bose's experiments

Jagadish Chandra Bose first used crystals for radio wave detection in his 60 GHz microwave optics experiments at the University of Calcutta from 1894 to 1900. Like other scientists since Hertz, Bose was investigating the similarity between radio waves and light by duplicating classic optics experiments with radio waves. For a receiver he first used a coherer consisting of a steel spring pressing against a metal surface with a current passing through it. Dissatisfied with this detector, around 1897 Bose measured the change in resistivity of dozens of metals and metal compounds exposed to microwaves. He experimented with many substances as contact detectors, focusing on galena.

His detectors consisted of a small galena crystal with a metal point contact pressed against it with a thumbscrew, mounted inside a closed waveguide ending in a horn antenna to collect the microwaves. Bose passed a current from a battery through the crystal, and used a galvanometer to measure it. When microwaves struck the crystal the galvanometer registered a drop in resistance of the detector. Thomas Lee has pointed out that this detector did not function as a rectifier like later crystal detectors, but as a thermal detector called a bolometer. At the time scientists thought that radio wave detectors functioned by some mechanism analogous to the way the eye detected light, and Bose found his detector was also sensitive to visible light and ultraviolet, leading him to call it an artificial retina. He patented the detector 30 September 1901. This is often considered the first patent on a semiconductor device.

Pickard: Discovery of rectification

Greenleaf Whittier Pickard, an engineer with the American Wireless Telephone and Telegraph Co. invented the rectifying contact detector, discovering rectification of radio waves in 1902 while experimenting with a coherer detector consisting of a steel needle resting across two carbon blocks. On 29 May 1902 he was operating this device, listening to a radiotelegraphy station. Coherers required an external current source to operate, so he had the coherer and telephone earphone connected in series with a 3 cell battery to provide power to operate the earphone. Annoyed by background "frying" noise caused by the current through the carbon, he reached over to cut two of the battery cells out of the circuit to reduce the current

The frying ceased, and the signals, though much weakened, became materially clearer through being freed of their background of microphonic noise. Glancing over at my circuit, I discovered to my great surprise that instead of cutting out two of the cells I had cut out all three; so, therefore, the telephone diaphragm was being operated solely by the energy of the receiver signals. A contact detector operating without local battery seemed so contrary to all my previous experience that ... I resolved at once to thoroughly investigate the phenomenon.

The generation of an audio signal without a DC bias battery made Pickard realize the device was acting as a rectifier. Pickard began to experiment and found an oxidized steel surface worked better, so he tried magnetite (Fe₃O₄). On 16 October 1902 he received a radio station using magnetite touched by a copper wire, the first reception by a crystal detector.

During the next seven years, Pickard conducted an exhaustive search to find which substances formed the most sensitive detecting contacts, eventually testing thousands of minerals, and discovered about 250 rectifying crystals. In 1906 he obtained a sample of fused silicon, an artificial product recently synthesized in electric furnaces, and it outperformed all other substances. He patented the silicon detector 30 August 1906. In 1907 he formed a company to manufacture his detectors, Wireless Specialty Products Co., and the silicon detector was the first crystal detector to be sold commercially. Pickard went on to produce other detectors using the crystals he had discovered; the more popular being the iron pyrite "Pyron" detector and the zincite–chalcopyrite crystal-to-crystal "Perikon" detector in 1908, which stood for "PERfect pIcKard cONtact".

Crystal detectors become popular

Around 1906 it was recognised by radio researchers that mineral crystals could be a better detector than the coherer, crystal radios began to be made, and many new crystal detectors were invented. Part of the reason for this interest was that coherer receivers had switched from using paper tape recorders (siphon recorders) as an output device, which were incompatible with crystal detectors, to earphones, which could use the crystal's output current.

On 23 March 1906 Henry Harrison Chase Dunwoody, a retired general in the U.S. Army Signal Corps, patented the silicon carbide (carborundum) detector, using another recent product of electric furnaces. The semiconductor silicon carbide has a wide band gap and Pickard discovered the detector's sensitivity could be increased by applying a forward bias, a DC potential of around a volt from a battery and potentiometer, to it.

Braun began to experiment with crystals as radio detectors in 1899 and in 1906 patented a galena cat whisker detector in Germany. In 1906 L. W. Austin invented a silicon–tellurium detector, in 1907 Pickard invented the molybdenite detector, and in 1911 Thompson H. Lyon invented the cerussite detector. In Germany a tellurium-carbon detector became popular, called "the Bronc cell". In 1908 Wichi Torikata at Tokyo Imperial University investigated 200 minerals and found cassiterite (tin oxide), pyrolusite (manganese dioxide), zincite, galena, and pyrite were sensitive, and subsequently tested all the mineral samples at the Mineral College and found 34 rectifying minerals. He patented a mineral detector in 1908. Lee De Forest, George Washington Pierce, and William Henry Eccles also studied mineral detectors.

The fine wire catwhisker contact invented early in the detector's history was patented in 1911 by Pickard

Use during the wireless telegraphy era

Guglielmo Marconi developed the first practical wireless telegraphy transmitters and receivers in 1896, and radio began to be used for communication around 1899. The coherer was used as detector for the first 10 years, until around 1906. During the wireless telegraphy era prior to 1920, there was virtually no broadcasting; radio served as a point-to-point text messaging service. Until the triode vacuum tube began to be used around World War I, radio receivers had no amplification and were powered only by the radio waves picked up by their antennae. Long-distance radio communication depended on high power transmitters (up to 1 megawatt), huge wire antennas, and a receiver with a sensitive detector.

Around 1907 crystal detectors replaced the coherer and electrolytic detector to become the most widely used form of radio detector. Until the triode vacuum tube began to be used during World War I, crystals were the best radio reception technology, used in sophisticated receivers in wireless telegraphy stations, as well as in homemade crystal radios. In transoceanic radiotelegraphy stations elaborate inductively coupled crystal receivers fed by mile long wire antennas were used to receive transatlantic telegram traffic.

Much research went into finding better detectors and many types of crystals were tried. The goal of researchers was to find rectifying crystals that were less fragile and sensitive to vibration than galena and pyrite. Another desired property was tolerance of high currents; many crystals would become insensitive when subjected to discharges of atmospheric electricity from the outdoor wire antenna, or current from the powerful spark transmitter leaking into the receiver. Carborundum proved to be the best of these; it could rectify when clamped firmly between flat contacts. Therefore, carborundum detectors were used in shipboard wireless stations where waves caused the floor to rock, and military stations where gunfire was expected.

In 1907–1909, George Washington Pierce at Harvard conducted research into how crystal detectors worked. Using an oscilloscope made with Braun's new cathode ray tube, he produced the first pictures of the waveforms in a working detector, proving that it did rectify the radio wave. During this era, before modern solid-state physics, most scientists believed that crystal detectors operated by some thermoelectric effect. Although Pierce did not discover the mechanism by which it worked, he did prove that the existing theories were wrong; his oscilloscope waveforms showed there was no phase delay between the voltage and current in the detector, ruling out thermal mechanisms. Pierce originated the name crystal rectifier.

Between about 1905 and 1915 new types of radio transmitters were developed which produced continuous sinusoidal waves: the arc converter (Poulsen arc) and the Alexanderson alternator. These slowly replaced the old damped wave spark transmitters. Besides having a longer transmission range, these transmitters could be modulated with an audio signal to transmit sound by amplitude modulation (AM). It was found that, unlike the coherer, the rectifying action of the crystal detector allowed it to demodulate an AM radio signal, producing audio (sound). Although other detectors used at the time, the electrolytic detector, Fleming valve and the triode could also rectify AM signals, crystals were the simplest, cheapest AM detector. As more and more radio stations began experimenting with transmitting sound after World War I, a growing community of radio listeners built or bought crystal radios to listen to them. Use continued to grow until the 1920s when vacuum tube radios replaced them.

Crystodyne: negative resistance diodes

Some semiconductor diodes have a property called negative resistance which means the current through them decreases as the voltage increases over a part of their I–V curve. This allows a diode, normally a passive device, to function as an amplifier or oscillator. For example, when connected to a resonant circuit and biased with a DC voltage, the negative resistance of the diode can cancel the positive resistance of the circuit, creating a circuit with zero AC resistance, in which spontaneous oscillating currents arise. This property was first observed in crystal detectors around 1909 by William Henry Eccles and Pickard. They noticed that when their detectors were biased with a DC voltage to improve their sensitivity, they would sometimes break into spontaneous oscillations. However these researchers just published brief accounts and did not pursue the effect.

The first person to exploit negative resistance practically was self-taught Russian physicist Oleg Losev, who devoted his career to the study of crystal detectors. In 1922 working at the new Nizhny Novgorod Radio Laboratory he discovered negative resistance in biased zincite (zinc oxide) point contact junctions. He realized that amplifying crystals could be an alternative to the fragile, expensive, energy-wasting vacuum tube. He used biased negative resistance crystal junctions to build solid-state amplifiers, oscillators, and amplifying and regenerative radio receivers, 25 years before the invention of the transistor. Later he even built a superheterodyne receiver. However his achievements were overlooked because of the success of vacuum tubes. His technology was dubbed "Crystodyne" by science publisher Hugo Gernsback one of the few people in the West who paid attention to it. After ten years he abandoned research into this technology and it was forgotten.

The negative resistance diode was rediscovered with the invention of the tunnel diode in 1957, for which Leo Esaki won the 1973 Nobel Prize in Physics. Today, negative resistance diodes such as the Gunn diode and IMPATT diode are widely used as microwave oscillators in such devices as radar speed guns and garage door openers.

Discovery of the light emitting diode (LED)

In 1907 British Marconi engineer Henry Joseph Round noticed that when direct current was passed through a silicon carbide (carborundum) point contact junction, a spot of greenish, bluish, or yellowish light was given off at the contact point. Round had constructed a light emitting diode (LED). However he just published a brief two paragraph note about it and did no further research.

While investigating crystal detectors in the mid-1920s at Nizhny Novgorod, Oleg Losev independently discovered that biased carborundum and zincite junctions emitted light. Losev was the first to analyze this device, investigate the source of the light, propose a theory of how it worked, and envision practical applications. He published his experiments in 1927 in a Russian journal, and the 16 papers he published on LEDs between 1924 and 1930 constitute a comprehensive study of this device. Losev did extensive research into the mechanism of light emission. He measured rates of evaporation of benzine from the crystal surface and found it was not accelerated when light was emitted, concluding that the luminescence was a "cold" light not caused by thermal effects. He theorized correctly that the explanation of the light emission was in the new science of quantum mechanics, speculating that it was the inverse of the photoelectric effect discovered by Albert Einstein in 1905. He wrote to Einstein about it, but did not receive a reply. Losev designed practical carborundum electroluminescent lights, but found no one interested in commercially producing these weak light sources.

Losev died in World War II. Due partly to the fact that his papers were published in Russian and German, and partly to his lack of reputation (his upper class birth barred him from a college education or career advancement in Soviet society, so he never held an official position higher than technician) his work is not well known in the West.

Use during the broadcast era

In the 1920s, the amplifying triode vacuum tube, invented in 1907 by Lee De Forest, replaced earlier technology in both radio transmitters and receivers. AM radio broadcasting spontaneously arose around 1920, and radio listening exploded to become a hugely popular pastime. The initial listening audience for the new broadcasting stations was largely owners of crystal radios, because many consumers couldn't afford the new tube radios. But lacking amplification, crystal radios had to be listened to with earphones, and could only receive nearby local stations. The amplifying vacuum tube radios which began to be mass-produced in 1921 had greater reception range, did not require the fussy adjustment of a cat whisker, and produced enough audio output power to drive loudspeakers, allowing the entire family to listen comfortably together, or dance to Jazz Age music.

So during the 1920s vacuum tube receivers replaced crystal radios in all except poor households. Commercial and military wireless telegraphy stations had already switched to more sensitive vacuum tube receivers. Vacuum tubes put an end to crystal detector development. The temperamental, unreliable action of the crystal detector had always been a barrier to its acceptance as a standard component in commercial radio equipment and was one reason for its rapid replacement. Frederick Seitz, an early semiconductor researcher, wrote:

Such variability, bordering on what seemed the mystical, plagued the early history of crystal detectors and caused many of the vacuum tube experts of a later generation to regard the art of crystal rectification as being close to disreputable.

The crystal radio became a cheap alternative receiver used in emergencies and by people who could not afford tube radios: teenagers, the poor, and those in developing countries. Building a crystal set remained a popular educational project to introduce people to radio, used by organizations like the Boy Scouts. The galena detector, the most widely used type among amateurs, became virtually the only detector used in crystal radios from this point on. The carborundum junction saw some use as a detector in early vacuum tube radios because it was more sensitive than the triode grid-leak detector. Crystal radios were kept as emergency backup radios on ships. During World War II in Nazi-occupied Europe the radio saw use as an easily constructed, easily concealed clandestine radio by Resistance groups. After World War II, the development of modern semiconductor diodes finally made the galena cat whisker detector obsolete.

Development of the theory of semiconductor rectification

Semiconductor devices like the crystal detector work by quantum mechanical principles; their operation cannot be explained by classical physics. The birth of quantum mechanics in the 1920s was the necessary foundation for the development of semiconductor physics in the 1930s, during which physicists arrived at an understanding of how the crystal detector worked. The German word halbleiter, translated into English as "semiconductor", was first used in 1911 to describe substances whose conductivity fell between conductors and insulators, such as the crystals in crystal detectors. Felix Bloch and Rudolf Peierls around 1930 applied quantum mechanics to create a theory of how electrons move through a crystal. In 1931, Alan Wilson created quantum band theory which explains the electrical conductivity of solids. Werner Heisenberg conceived the idea of a hole, a vacancy in a crystal lattice where an electron should be, which can move about the lattice like a positive particle; both electrons and holes conduct current in semiconductors.

A breakthrough came when it was realized that the rectifying action of crystalline semiconductors was not due to the crystal alone but to the presence of impurity atoms in the crystal lattice. In 1930 Bernhard Gudden and Wilson established that electrical conduction in semiconductors was due to trace impurities in the crystal. A "pure" semiconductor did not act as a semiconductor, but as an insulator (at low temperatures). The maddeningly variable activity of different pieces of crystal when used in a detector, and the presence of "active sites" on the surface, was due to natural variations in the concentration of these impurities throughout the crystal. Nobel Laureate Walter Brattain, coinventor of the transistor, noted:

At that time you could get a chunk of silicon... put a cat whisker down on one spot, and it would be very active and rectify very well in one direction. You moved it around a little bit-maybe a fraction, a thousandth of an inch-and you might find another active spot, but here it would rectify in the other direction.

The "metallurgical purity" chemicals used by scientists to make synthetic experimental detector crystals had about 1% impurities which were responsible for such inconsistent results. During the 1930s progressively better refining methods were developed, allowing scientists to create ultrapure semiconductor crystals into which they introduced precisely controlled amounts of trace elements (called doping). This for the first time created semiconductor junctions with reliable, repeatable characteristics, allowing scientists to test their theories, and later making manufacture of modern diodes possible.

The theory of rectification in a metal-semiconductor junction, the type used in a cat whisker detector, was developed in 1938 independently by Walter Schottky at Siemens & Halske research laboratory in Germany and Nevill Mott at Bristol University, UK. Mott received the 1977 Nobel Prize in Physics. In 1949 at Bell Labs William Shockley derived the Shockley diode equation which gives the nonlinear exponential current–voltage curve of a crystal detector, observed by scientists since Braun and Bose, which is responsible for rectification .

The first modern diodes

The development of microwave technology during the 1930s run up to World War II for use in military radar led to the resurrection of the point contact crystal detector. Microwave radar receivers required a nonlinear device that could act as a mixer, to mix the incoming microwave signal with a local oscillator signal, to shift the microwave signal down to a lower intermediate frequency (IF) at which it could be amplified. The vacuum tubes used as mixers at lower frequencies in superheterodyne receivers could not function at microwave frequencies due to excessive capacitance. In the mid-1930s George Southworth at Bell Labs, working on this problem, bought an old cat whisker detector and found it worked at microwave frequencies. Hans Hollmann in Germany made the same discovery. The MIT Radiation Laboratory launched a project to develop microwave detector diodes, focusing on silicon, which had the best detecting properties. By about 1942 point-contact silicon crystal detectors for radar receivers such as the 1N21 and 1N23 were being mass-produced, consisting of a slice of boron-doped silicon crystal with a tungsten wire point pressed firmly against it. The cat whisker contact did not require adjustment, and these were sealed units. A second parallel development program at Purdue University produced germanium diodes. Such point-contact diodes are still being manufactured, and may be considered the first modern diodes.

After the war, germanium diodes replaced galena cat whisker detectors in the few crystal radios being made. Germanium diodes are more sensitive than silicon diodes as detectors, because germanium has a lower forward voltage drop than silicon (0.4 vs 0.7 volts). Today a few galena cat whisker detectors are still being made, but only for antique replica crystal radios or devices for science education.

Introduced in 1946 by Sylvania, the 1N34 diode (followed later by the 1N34A) became one of the most widely deployed crystal detector diodes. The inexpensive, capable 1N34 was also capable of being used as a general-purpose diode.