Maser

For other uses, see Maser (disambiguation).

A hydrogen radio frequency discharge, the first element inside a hydrogen maser (see description below)

A maser is a device that produces a highly intense, coherent beam of electromagnetic waves, particularly in the microwave region. Historically, the term came from the acronym "Microwave Amplification by Stimulated Emission of Radiation." Modern masers, however, emit over a broad portion of the electromagnetic spectrum. For this reason, Charles H. Townes has suggested replacing "microwave" with "molecular" in the acronym. When masers were developed to operate in the optical region, they were initially called optical masers, but it has become more common to refer to them as lasers, where "l" stands for "light."

Terminology

As noted above, maser was initially suggested as an acronym for "microwave amplification by stimulated emission of radiation," to describe devices that emitted in the microwave region of the electromagnetic spectrum. The principle of stimulated emission has since been extended to more devices and frequencies, and so Charles H. Townes suggested modifying the original acronym to "molecular amplification by stimulated emission of radiation."

When the laser was developed, Townes, Arthur Schawlow, and their colleagues at Bell Labs pushed the use of the term optical maser, but this was largely abandoned in favor of laser, coined by their rival Gordon Gould. In modern usage, devices that emit in the X-ray through infrared portions of the spectrum are typically called lasers, and devices that emit in the microwave region and below are commonly called masers.

Gould originally proposed distinct names for devices that emit in each portion of the spectrum, including grasers (gamma ray lasers), xasers (x-ray lasers), uvasers (ultraviolet lasers), lasers (visible lasers), irasers (infrared lasers), masers (microwave masers), and rasers (radio frequency masers). Most of these terms, except for maser and laser, never caught on and have become obsolete, apart from their use in science fiction.

History

Theoretically, reflecting principles previously discussed by Joseph Weber at the June 1952 conference of the Institute of Radio Engineers, the principle of the maser was described by Nikolay Basov and Alexander Prokhorov from Lebedev Institute of Physics at an All-Union Conference on Radio-Spectroscopy held by USSR Academy of Sciences in May 1952. They subsequently published their results in October 1954.

Independently, Charles H. Townes, J. P. Gordon, and H. J. Zeiger built the first maser at Columbia University in 1953. The device used stimulated emission in a stream of energized ammonia molecules to produce amplification of microwaves at a frequency of 24 gigahertz. Townes later worked with Arthur L. Schawlow to describe the principle of the optical maser, or laser, which Theodore H. Maiman first demonstrated in 1960. For their research in this field Townes, Basov, and Prokhorov were awarded the Nobel Prize in Physics in 1964.

Technology

The maser is based on the principle of stimulated emission proposed by Albert Einstein in 1917. When atoms have been put into an excited energy state, they can amplify radiation at the proper frequency. By putting such an amplifying medium in a resonant cavity, feedback is created that can produce coherent radiation.

Some common types of masers are noted below.

Atomic beam masers

• Ammonia maser
• Hydrogen maser

Gas masers

• Rubidium maser

Solid State masers

• Ruby maser

The dual noble gas maser is an example of a nonpolar medium in a maser.

Uses

Masers serve as high precision frequency references. These "atomic frequency standards" are one form of atomic clock. They are also used as electronic amplifiers in radio telescopes.

Hydrogen maser

A hydrogen maser.

Today, the most important type of maser is the hydrogen maser which is currently used as an atomic frequency standard. Together with other types of atomic clocks, they constitute the "Temps Atomique International" or TAI. This is the international time scale, which is coordinated by the Bureau International des Poids et Mesures, or BIPM.

It was Norman Ramsey and his colleagues who first realized this device. Today's masers are identical to the original design. The maser oscillation relies on stimulated emission between two hyperfine levels of atomic hydrogen. Here is a brief description of how it works:

• First, a beam of atomic hydrogen is produced. This is done by submitting the gas at low pressure to an RF discharge (see the picture on this page).

• The next step is "state selection"—in order to get some stimulated emission, it is necessary to create a population inversion of the atoms. This is done in a way that is very similar to the famous Stern-Gerlach experiment. After passing through an aperture and a magnetic field, many of the atoms in the beam are left in the upper energy level of the lasing transition. From this state, the atoms can decay to the lower state and emit some microwave radiation.

• A high quality factor microwave cavity confines the microwaves and reinjects them repeatedly into the atom beam. The stimulated emission amplifies the microwaves on each pass through the beam. This combination of amplification and feedback is what defines all oscillators. The resonant frequency of the microwave cavity is exactly tuned to the hyperfine structure of hydrogen: 1420 405 751.768 Hz.

• A small fraction of the signal in the microwave cavity is coupled into a coaxial cable and then sent to a coherent receiver.

• The microwave signal coming out of the maser is very weak (a few pW). The frequency of the signal is fixed but extremely stable. The coherent receiver is used to amplify the signal and change the frequency. This is done using a series of phase-locked loops and a high performance quartz oscillator.

Astrophysical masers

Stimulated microwave and radio wave emission is observed in astronomy, and this is usually called "masing," even in the absence of the resonant feedback that would be required for a true maser. Technically this form of stimulated emission is called superradiant emission, and it is closely associated with lasing and masing. Such emission is observed from molecules such as water (H₂O), hydroxyl radicals (OH), methanol (CH₃OH), formaldehyde (CH₂O), and silicon monoxide (SiO).

Maser-like stimulated emission also occurs in nature in interstellar space. Water molecules in star-forming regions can undergo a population inversion and emit radiation at 22 GHz, creating the brightest spectral line in the radio universe. Some water masers also emit radiation from a vibrational mode at 96 GHz.

See also

• Electromagnetic spectrum
• Laser
• Light
• Microwave
• Optics

References

ISBN links support NWE through referral fees

• Singer, J.R. 1959. Masers. New York, NY: Wiley.
• Vanier, J., C. Audoin. 1989. The Quantum Physics of Atomic Frequency Standards. Philadelphia, PA: A. Hilger. ISBN 9780852744338.
• Keating, Michael P. 2002. Geometric, Physical, and Visual Optics. Boston : Butterworth-Heinemann. ISBN 0750672625.

External links

• arXiv.org search for "maser". Retrieved June 19, 2008.
• Noble gas Maser. Retrieved June 19, 2008.

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