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Maser

A maser is a device that produces coherent electromagnetic waves (microwaves), through amplification by stimulated emission. The term is an acronym for microwave amplification by stimulated emission of radiation. First suggested by Joseph Weber, The first maser was built by Charles H. Townes, James P. Gordon, and Herbert J. Zeiger at Columbia University in 1953. Townes, Nikolay Basov and Alexander Prokhorov were awarded the 1964 Nobel Prize in Physics for theoretical work leading to the maser. Masers are also used as the timekeeping device in atomic clocks, and as extremely low-noise microwave amplifiers in radio telescopes and deep-space spacecraft communication ground stations.

First prototype ammonia maser in front of its inventor Charles H. Townes. The ammonia nozzle is at left in the box, the four brass rods at center are the quadrupole state selector, and the resonant cavity is at right. The 24 GHz microwaves exit through the vertical waveguide Townes is adjusting. At bottom are the vacuum pumps.
A hydrogen radio frequency discharge, the first element inside a hydrogen maser (see description below)

Modern masers can be designed to generate electromagnetic waves at not only microwave frequencies but also radio and infrared frequencies. For this reason, Townes suggested replacing "microwave" with "molecular" as the first word in the acronym "maser".[1]

The laser works by the same principle as the maser but produces higher frequency coherent radiation at visible wavelengths. The maser was the precursor to the laser, inspiring theoretical work by Townes and Arthur Leonard Schawlow that led to the invention of the laser in 1960 by Theodore Maiman. When the coherent optical oscillator was first imagined in 1957, it was originally called the "optical maser". This was ultimately changed to laser, for "light amplification by stimulated emission of radiation". Gordon Gould is credited with creating this acronym in 1957.

History edit

The theoretical principles governing the operation of a maser were first described by Joseph Weber of the University of Maryland, College Park at the Electron Tube Research Conference in June 1952 in Ottawa,[2] with a summary published in the June 1953 Transactions of the Institute of Radio Engineers Professional Group on Electron Devices,[3] and simultaneously by Nikolay Basov and Alexander Prokhorov from Lebedev Institute of Physics, at an All-Union Conference on Radio-Spectroscopy held by the USSR Academy of Sciences in May 1952, subsequently published in October 1954.

Independently, Charles Hard Townes, James P. Gordon, and H. J. Zeiger built the first ammonia maser at Columbia University in 1953. This device used stimulated emission in a stream of energized ammonia molecules to produce amplification of microwaves at a frequency of about 24.0 gigahertz.[4] Townes later worked with Arthur L. Schawlow to describe the principle of the optical maser, or laser,[5] of which Theodore H. Maiman created the first working model in 1960.

For their research in the field of stimulated emission, Townes, Basov and Prokhorov were awarded the Nobel Prize in Physics in 1964.[6]

Technology edit

The maser is based on the principle of stimulated emission proposed by Albert Einstein in 1917. When atoms have been induced into an excited energy state, they can amplify radiation at a frequency particular to the element or molecule used as the masing medium (similar to what occurs in the lasing medium in a laser).

By putting such an amplifying medium in a resonant cavity, feedback is created that can produce coherent radiation.

Some common types edit

21st-century developments edit

In 2012, a research team from the National Physical Laboratory and Imperial College London developed a solid-state maser that operated at room temperature by using optically pumped, pentacene-doped p-Terphenyl as the amplifier medium.[8][9][10] It produced pulses of maser emission lasting for a few hundred microseconds.

In 2018, a research team from Imperial College London and University College London demonstrated continuous-wave maser oscillation using synthetic diamonds containing nitrogen-vacancy defects.[11][12]

Uses edit

Masers serve as high precision frequency references. These "atomic frequency standards" are one of the many forms of atomic clocks. Masers were also used as low-noise microwave amplifiers in radio telescopes, though these have largely been replaced by amplifiers based on FETs.[13]

During the early 1960s, the Jet Propulsion Laboratory developed a maser to provide ultra-low-noise amplification of S-band microwave signals received from deep space probes.[14] This maser used deeply refrigerated helium to chill the amplifier down to a temperature of 4 kelvin. Amplification was achieved by exciting a ruby comb with a 12.0 gigahertz klystron. In the early years, it took days to chill and remove the impurities from the hydrogen lines. Refrigeration was a two-stage process with a large Linde unit on the ground, and a crosshead compressor within the antenna. The final injection was at 21 MPa (3,000 psi) through a 150 μm (0.006 in) micrometer-adjustable entry to the chamber. The whole system noise temperature looking at cold sky (2.7 kelvin in the microwave band) was 17 kelvin; this gave such a low noise figure that the Mariner IV space probe could send still pictures from Mars back to the Earth even though the output power of its radio transmitter was only 15 watts, and hence the total signal power received was only −169 decibels with respect to a milliwatt (dBm).

Hydrogen maser edit

 
A hydrogen maser.

The hydrogen maser is used as an atomic frequency standard. Together with other kinds of atomic clocks, these help make up the International Atomic Time standard ("Temps Atomique International" or "TAI" in French). This is the international time scale coordinated by the International Bureau of Weights and Measures. Norman Ramsey and his colleagues first conceived of the maser as a timing standard. More recent masers are practically identical to their original design. Maser oscillations rely on the stimulated emission between two hyperfine energy levels of atomic hydrogen.

Here is a brief description of how they work:

  • First, a beam of atomic hydrogen is produced. This is done by submitting the gas at low pressure to a high-frequency radio wave 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 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 Q factor (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 tuned to the frequency of the hyperfine energy transition of hydrogen: 1,420,405,752 hertz.[15]
  • A small fraction of the signal in the microwave cavity is coupled into a coaxial cable and then sent to a coherent radio receiver.
  • The microwave signal coming out of the maser is very weak, a few picowatts. The frequency of the signal is fixed and 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 edit

Maser-like stimulated emission has also been observed in nature from interstellar space, and it is frequently called "superradiant emission" to distinguish it from laboratory masers. Such emission is observed from molecules such as water (H2O), hydroxyl radicals (•OH), methanol (CH3OH), formaldehyde (HCHO), silicon monoxide (SiO), and carbodiimide (HNCNH).[16] Water molecules in star-forming regions can undergo a population inversion and emit radiation at about 22.0 GHz, creating the brightest spectral line in the radio universe. Some water masers also emit radiation from a rotational transition at a frequency of 96 GHz.[17][18]

Extremely powerful masers, associated with active galactic nuclei, are known as megamasers and are up to a million times more powerful than stellar masers.

Terminology edit

The meaning of the term maser has changed slightly since its introduction. Initially the acronym was universally given as "microwave amplification by stimulated emission of radiation", which described devices which emitted in the microwave region of the electromagnetic spectrum.

The principle and concept of stimulated emission has since been extended to more devices and frequencies. Thus, the original acronym is sometimes modified, as suggested by Charles H. Townes,[1] to "molecular amplification by stimulated emission of radiation." Some have asserted that Townes's efforts to extend the acronym in this way were primarily motivated by the desire to increase the importance of his invention, and his reputation in the scientific community.[19]

When the laser was developed, Townes and 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.[20] 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, regardless of whether they emit microwaves or other frequencies.

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 (RF masers). Most of these terms never caught on, however, and all have now become (apart from in science fiction) obsolete except for maser and laser.[citation needed]

See also edit

References edit

  1. ^ a b Townes, Charles H. (1964-12-11). "Production of coherent radiation by atoms and molecules - Nobel Lecture" (PDF). The Nobel Prize. p. 63. (pdf) from the original on 2020-08-27. Retrieved 2020-08-27. We called this general type of system the maser, an acronym for microwave amplification by stimulated emission of radiation. The idea has been successfully extended to such a variety of devices and frequencies that it is probably well to generalize the name - perhaps to mean molecular amplification by stimulated emission of radiation.
  2. ^ American Institute of Physics Oral History Interview with Weber
  3. ^ Mario Bertolotti (2004). The History of the Laser. CRC Press. p. 180. ISBN 978-1420033403.
  4. ^ Gordon, J. P.; Zeiger, H. J.; Townes, C. H. (1955). "The Maser—New Type of Microwave Amplifier, Frequency Standard, and Spectrometer". Phys. Rev. 99 (4): 1264. Bibcode:1955PhRv...99.1264G. doi:10.1103/PhysRev.99.1264.
  5. ^ Schawlow, A.L.; Townes, C.H. (15 December 1958). "Infrared and Optical Masers". Physical Review. 112 (6): 1940–1949. Bibcode:1958PhRv..112.1940S. doi:10.1103/PhysRev.112.1940.
  6. ^ "The Nobel Prize in Physics 1964". NobelPrize.org. Retrieved 2020-08-27.
  7. ^ , Harvard University, Department of Physics
  8. ^ Brumfiel, G. (2012). "Microwave laser fulfills 60 years of promise". Nature. doi:10.1038/nature.2012.11199. S2CID 124247048.
  9. ^ Palmer, Jason (16 August 2012). . BBC News. Archived from the original on July 29, 2016. Retrieved 23 August 2012.
  10. ^ Microwave Laser Fulfills 60 Years of Promise
  11. ^ Liu, Ren-Bao (March 2018). "A diamond age of masers". Nature. 555 (7697): 447–449. Bibcode:2018Natur.555..447L. doi:10.1038/d41586-018-03215-3. PMID 29565370.
  12. ^ Scientists use diamond in world's first continuous room-temperature solid-state maser, phys.org
  13. ^ "Low Noise Amplifiers – Pushing the limits of low noise". National Radio Astronomy Observatory (NRAO).
  14. ^ Macgregor S. Reid, ed. (2008). "Low-Noise Systems in the Deep Space Network" (PDF). JPL.
  15. ^ "Time and Frequency From A to Z: H". NIST. 12 May 2010.
  16. ^ McGuire, Brett A.; Loomis, Ryan A.; Charness, Cameron M.; Corby, Joanna F.; Blake, Geoffrey A.; Hollis, Jan M.; Lovas, Frank J.; Jewell, Philip R.; Remijan, Anthony J. (2012-10-20). "Interstellar Carbodiimide (HNCNH): A New Astronomical Detection from the GBT Primos Survey Via Maser Emission Features". The Astrophysical Journal. 758 (2): L33. arXiv:1209.1590. Bibcode:2012ApJ...758L..33M. doi:10.1088/2041-8205/758/2/L33. ISSN 2041-8205. S2CID 26146516.
  17. ^ Neufeld, David A.; Melnick, Gary J. (1991). "Excitation of Millimeter and Submillimeter Water Masers in Warm Astrophysical Gas". Atoms, Ions and Molecules: New Results in Spectral Line Astrophysics, ASP Conference Series (ASP: San Francisco). 16: 163. Bibcode:1991ASPC...16..163N.
  18. ^ Tennyson, Jonathan; et al. (March 2013). "IUPAC critical evaluation of the rotational–vibrational spectra of water vapor, Part III: Energy levels and transition wavenumbers for H216O". Journal of Quantitative Spectroscopy and Radiative Transfer. 117: 29–58. Bibcode:2013JQSRT.117...29T. doi:10.1016/j.jqsrt.2012.10.002. hdl:10831/91303.
  19. ^ Taylor, Nick (2000). LASER: The inventor, the Nobel laureate, and the thirty-year patent war. New York: Simon & Schuster. ISBN 978-0-684-83515-0.
  20. ^ Taylor, Nick (2000). LASER: The inventor, the Nobel laureate, and the thirty-year patent war. New York: Simon & Schuster. pp. 66–70. ISBN 978-0-684-83515-0.

Further reading edit

  • J.R. Singer, Masers, John Whiley and Sons Inc., 1959.
  • J. Vanier, C. Audoin, The Quantum Physics of Atomic Frequency Standards, Adam Hilger, Bristol, 1989.

External links edit

  • The Feynman Lectures on Physics Vol. III Ch. 9: The Ammonia Maser
  • arXiv.org search for "maser"
  • . Harvard-Smithsonian Center for Astrophysics. Archived from the original on 2006-10-10.
  • Bright Idea: The First Lasers 2014-04-24 at the Wayback Machine
  • Invention of the Maser and Laser, American Physical Society
  • , Bell Labs

maser, other, uses, disambiguation, maser, device, that, produces, coherent, electromagnetic, waves, microwaves, through, amplification, stimulated, emission, term, acronym, microwave, amplification, stimulated, emission, radiation, first, suggested, joseph, w. For other uses see Maser disambiguation A maser is a device that produces coherent electromagnetic waves microwaves through amplification by stimulated emission The term is an acronym for microwave amplification by stimulated emission of radiation First suggested by Joseph Weber The first maser was built by Charles H Townes James P Gordon and Herbert J Zeiger at Columbia University in 1953 Townes Nikolay Basov and Alexander Prokhorov were awarded the 1964 Nobel Prize in Physics for theoretical work leading to the maser Masers are also used as the timekeeping device in atomic clocks and as extremely low noise microwave amplifiers in radio telescopes and deep space spacecraft communication ground stations First prototype ammonia maser in front of its inventor Charles H Townes The ammonia nozzle is at left in the box the four brass rods at center are the quadrupole state selector and the resonant cavity is at right The 24 GHz microwaves exit through the vertical waveguide Townes is adjusting At bottom are the vacuum pumps A hydrogen radio frequency discharge the first element inside a hydrogen maser see description below Modern masers can be designed to generate electromagnetic waves at not only microwave frequencies but also radio and infrared frequencies For this reason Townes suggested replacing microwave with molecular as the first word in the acronym maser 1 The laser works by the same principle as the maser but produces higher frequency coherent radiation at visible wavelengths The maser was the precursor to the laser inspiring theoretical work by Townes and Arthur Leonard Schawlow that led to the invention of the laser in 1960 by Theodore Maiman When the coherent optical oscillator was first imagined in 1957 it was originally called the optical maser This was ultimately changed to laser for light amplification by stimulated emission of radiation Gordon Gould is credited with creating this acronym in 1957 Contents 1 History 2 Technology 2 1 Some common types 2 2 21st century developments 3 Uses 3 1 Hydrogen maser 4 Astrophysical masers 5 Terminology 6 See also 7 References 8 Further reading 9 External linksHistory editThe theoretical principles governing the operation of a maser were first described by Joseph Weber of the University of Maryland College Park at the Electron Tube Research Conference in June 1952 in Ottawa 2 with a summary published in the June 1953 Transactions of the Institute of Radio Engineers Professional Group on Electron Devices 3 and simultaneously by Nikolay Basov and Alexander Prokhorov from Lebedev Institute of Physics at an All Union Conference on Radio Spectroscopy held by the USSR Academy of Sciences in May 1952 subsequently published in October 1954 Independently Charles Hard Townes James P Gordon and H J Zeiger built the first ammonia maser at Columbia University in 1953 This device used stimulated emission in a stream of energized ammonia molecules to produce amplification of microwaves at a frequency of about 24 0 gigahertz 4 Townes later worked with Arthur L Schawlow to describe the principle of the optical maser or laser 5 of which Theodore H Maiman created the first working model in 1960 For their research in the field of stimulated emission Townes Basov and Prokhorov were awarded the Nobel Prize in Physics in 1964 6 Technology editThe maser is based on the principle of stimulated emission proposed by Albert Einstein in 1917 When atoms have been induced into an excited energy state they can amplify radiation at a frequency particular to the element or molecule used as the masing medium similar to what occurs in the lasing medium in a laser By putting such an amplifying medium in a resonant cavity feedback is created that can produce coherent radiation Some common types edit Atomic beam masers Ammonia maser Free electron maser Hydrogen maser Gas masers Rubidium maser Liquid dye and chemical laser Solid state masers Ruby maser Whispering gallery modes iron sapphire maser Dual noble gas maser The dual noble gas of a masing medium which is nonpolar 7 21st century developments edit In 2012 a research team from the National Physical Laboratory and Imperial College London developed a solid state maser that operated at room temperature by using optically pumped pentacene doped p Terphenyl as the amplifier medium 8 9 10 It produced pulses of maser emission lasting for a few hundred microseconds In 2018 a research team from Imperial College London and University College London demonstrated continuous wave maser oscillation using synthetic diamonds containing nitrogen vacancy defects 11 12 Uses editMasers serve as high precision frequency references These atomic frequency standards are one of the many forms of atomic clocks Masers were also used as low noise microwave amplifiers in radio telescopes though these have largely been replaced by amplifiers based on FETs 13 During the early 1960s the Jet Propulsion Laboratory developed a maser to provide ultra low noise amplification of S band microwave signals received from deep space probes 14 This maser used deeply refrigerated helium to chill the amplifier down to a temperature of 4 kelvin Amplification was achieved by exciting a ruby comb with a 12 0 gigahertz klystron In the early years it took days to chill and remove the impurities from the hydrogen lines Refrigeration was a two stage process with a large Linde unit on the ground and a crosshead compressor within the antenna The final injection was at 21 MPa 3 000 psi through a 150 mm 0 006 in micrometer adjustable entry to the chamber The whole system noise temperature looking at cold sky 2 7 kelvin in the microwave band was 17 kelvin this gave such a low noise figure that the Mariner IV space probe could send still pictures from Mars back to the Earth even though the output power of its radio transmitter was only 15 watts and hence the total signal power received was only 169 decibels with respect to a milliwatt dBm Hydrogen maser edit Main article Hydrogen maser nbsp A hydrogen maser The hydrogen maser is used as an atomic frequency standard Together with other kinds of atomic clocks these help make up the International Atomic Time standard Temps Atomique International or TAI in French This is the international time scale coordinated by the International Bureau of Weights and Measures Norman Ramsey and his colleagues first conceived of the maser as a timing standard More recent masers are practically identical to their original design Maser oscillations rely on the stimulated emission between two hyperfine energy levels of atomic hydrogen Here is a brief description of how they work First a beam of atomic hydrogen is produced This is done by submitting the gas at low pressure to a high frequency radio wave 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 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 Q factor 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 tuned to the frequency of the hyperfine energy transition of hydrogen 1 420 405 752 hertz 15 A small fraction of the signal in the microwave cavity is coupled into a coaxial cable and then sent to a coherent radio receiver The microwave signal coming out of the maser is very weak a few picowatts The frequency of the signal is fixed and 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 editMain article Astrophysical maser Maser like stimulated emission has also been observed in nature from interstellar space and it is frequently called superradiant emission to distinguish it from laboratory masers Such emission is observed from molecules such as water H2O hydroxyl radicals OH methanol CH3OH formaldehyde HCHO silicon monoxide SiO and carbodiimide HNCNH 16 Water molecules in star forming regions can undergo a population inversion and emit radiation at about 22 0 GHz creating the brightest spectral line in the radio universe Some water masers also emit radiation from a rotational transition at a frequency of 96 GHz 17 18 Extremely powerful masers associated with active galactic nuclei are known as megamasers and are up to a million times more powerful than stellar masers Terminology editThe meaning of the term maser has changed slightly since its introduction Initially the acronym was universally given as microwave amplification by stimulated emission of radiation which described devices which emitted in the microwave region of the electromagnetic spectrum The principle and concept of stimulated emission has since been extended to more devices and frequencies Thus the original acronym is sometimes modified as suggested by Charles H Townes 1 to molecular amplification by stimulated emission of radiation Some have asserted that Townes s efforts to extend the acronym in this way were primarily motivated by the desire to increase the importance of his invention and his reputation in the scientific community 19 When the laser was developed Townes and 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 20 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 regardless of whether they emit microwaves or other frequencies 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 RF masers Most of these terms never caught on however and all have now become apart from in science fiction obsolete except for maser and laser citation needed See also editList of laser types Laser X ray laser Gamma ray laser graser Sonic laser saser SpaserReferences edit a b Townes Charles H 1964 12 11 Production of coherent radiation by atoms and molecules Nobel Lecture PDF The Nobel Prize p 63 Archived pdf from the original on 2020 08 27 Retrieved 2020 08 27 We called this general type of system the maser an acronym for microwave amplification by stimulated emission of radiation The idea has been successfully extended to such a variety of devices and frequencies that it is probably well to generalize the name perhaps to mean molecular amplification by stimulated emission of radiation American Institute of Physics Oral History Interview with Weber Mario Bertolotti 2004 The History of the Laser CRC Press p 180 ISBN 978 1420033403 Gordon J P Zeiger H J Townes C H 1955 The Maser New Type of Microwave Amplifier Frequency Standard and Spectrometer Phys Rev 99 4 1264 Bibcode 1955PhRv 99 1264G doi 10 1103 PhysRev 99 1264 Schawlow A L Townes C H 15 December 1958 Infrared and Optical Masers Physical Review 112 6 1940 1949 Bibcode 1958PhRv 112 1940S doi 10 1103 PhysRev 112 1940 The Nobel Prize in Physics 1964 NobelPrize org Retrieved 2020 08 27 The Dual Noble Gas Maser Harvard University Department of Physics Brumfiel G 2012 Microwave laser fulfills 60 years of promise Nature doi 10 1038 nature 2012 11199 S2CID 124247048 Palmer Jason 16 August 2012 Maser source of microwave beams comes out of the cold BBC News Archived from the original on July 29 2016 Retrieved 23 August 2012 Microwave Laser Fulfills 60 Years of Promise Liu Ren Bao March 2018 A diamond age of masers Nature 555 7697 447 449 Bibcode 2018Natur 555 447L doi 10 1038 d41586 018 03215 3 PMID 29565370 Scientists use diamond in world s first continuous room temperature solid state maser phys org Low Noise Amplifiers Pushing the limits of low noise National Radio Astronomy Observatory NRAO Macgregor S Reid ed 2008 Low Noise Systems in the Deep Space Network PDF JPL Time and Frequency From A to Z H NIST 12 May 2010 McGuire Brett A Loomis Ryan A Charness Cameron M Corby Joanna F Blake Geoffrey A Hollis Jan M Lovas Frank J Jewell Philip R Remijan Anthony J 2012 10 20 Interstellar Carbodiimide HNCNH A New Astronomical Detection from the GBT Primos Survey Via Maser Emission Features The Astrophysical Journal 758 2 L33 arXiv 1209 1590 Bibcode 2012ApJ 758L 33M doi 10 1088 2041 8205 758 2 L33 ISSN 2041 8205 S2CID 26146516 Neufeld David A Melnick Gary J 1991 Excitation of Millimeter and Submillimeter Water Masers in Warm Astrophysical Gas Atoms Ions and Molecules New Results in Spectral Line Astrophysics ASP Conference Series ASP San Francisco 16 163 Bibcode 1991ASPC 16 163N Tennyson Jonathan et al March 2013 IUPAC critical evaluation of the rotational vibrational spectra of water vapor Part III Energy levels and transition wavenumbers for H216O Journal of Quantitative Spectroscopy and Radiative Transfer 117 29 58 Bibcode 2013JQSRT 117 29T doi 10 1016 j jqsrt 2012 10 002 hdl 10831 91303 Taylor Nick 2000 LASER The inventor the Nobel laureate and the thirty year patent war New York Simon amp Schuster ISBN 978 0 684 83515 0 Taylor Nick 2000 LASER The inventor the Nobel laureate and the thirty year patent war New York Simon amp Schuster pp 66 70 ISBN 978 0 684 83515 0 Further reading editJ R Singer Masers John Whiley and Sons Inc 1959 J Vanier C Audoin The Quantum Physics of Atomic Frequency Standards Adam Hilger Bristol 1989 External links edit nbsp Wikimedia Commons has media related to Masers The Feynman Lectures on Physics Vol III Ch 9 The Ammonia Maser arXiv org search for maser The Hydrogen Maser Clock Project Harvard Smithsonian Center for Astrophysics Archived from the original on 2006 10 10 Bright Idea The First Lasers Archived 2014 04 24 at the Wayback Machine Invention of the Maser and Laser American Physical Society Shawlow and Townes Invent the Laser Bell Labs Retrieved from https en wikipedia org w index php title Maser amp oldid 1203962656, wikipedia, wiki, book, books, library,

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