PROGRESS TOWARDS DEMONSTRATION OF SHORTER WAVELENGTH SOFT X-RAY AMPLIFIERS PUMPED BY THE NOVA LASER.

C. Keane; D. Eder; R. London; B. J. MacGowan; Dennis L Matthews; S. Maxon; M. Rosen; D. Whelan

PROGRESS TOWARDS DEMONSTRATION OF SHORTER WAVELENGTH SOFT X-RAY AMPLIFIERS PUMPED BY THE NOVA LASER.

C. Keane, D. Eder, R. London, B. J. MacGowan, Dennis L Matthews, S. Maxon, M. Rosen, D. Whelan

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

Experiments and theoretical modeling are reported that demonstrate significant gain-length products at wavelengths below the carbon K-edge at 44angstrom. Two different schemes have been examined. The first is collisional excitation of Ni-like ions, which is an analog of the 3s-3p Ne-like lasing schemes demonstrated in selenium (Z equals 34) through molybdenum (Z equals 42). Three-body recombination schemes in H-like and Li-like ions are also currently being examined as a means of producing gain at shorter wavelengths.

Original language	English (US)
Title of host publication	Unknown Host Publication Title
Place of Publication	New York, NY, USA
Publisher	IEEE
Pages	67-68
Number of pages	2
State	Published - 1987
Externally published	Yes

ASJC Scopus subject areas

Engineering(all)

Cite this

@inproceedings{77ae330c26fc45cfb56c1e03242ac275,

title = "PROGRESS TOWARDS DEMONSTRATION OF SHORTER WAVELENGTH SOFT X-RAY AMPLIFIERS PUMPED BY THE NOVA LASER.",

abstract = "Experiments and theoretical modeling are reported that demonstrate significant gain-length products at wavelengths below the carbon K-edge at 44angstrom. Two different schemes have been examined. The first is collisional excitation of Ni-like ions, which is an analog of the 3s-3p Ne-like lasing schemes demonstrated in selenium (Z equals 34) through molybdenum (Z equals 42). Three-body recombination schemes in H-like and Li-like ions are also currently being examined as a means of producing gain at shorter wavelengths.",

author = "C. Keane and D. Eder and R. London and MacGowan, {B. J.} and Matthews, {Dennis L} and S. Maxon and M. Rosen and D. Whelan",

year = "1987",

language = "English (US)",

pages = "67--68",

booktitle = "Unknown Host Publication Title",

publisher = "IEEE",

}

TY - GEN

T1 - PROGRESS TOWARDS DEMONSTRATION OF SHORTER WAVELENGTH SOFT X-RAY AMPLIFIERS PUMPED BY THE NOVA LASER.

AU - Keane, C.

AU - Eder, D.

AU - London, R.

AU - MacGowan, B. J.

AU - Matthews, Dennis L

AU - Maxon, S.

AU - Rosen, M.

AU - Whelan, D.

PY - 1987

Y1 - 1987

N2 - Experiments and theoretical modeling are reported that demonstrate significant gain-length products at wavelengths below the carbon K-edge at 44angstrom. Two different schemes have been examined. The first is collisional excitation of Ni-like ions, which is an analog of the 3s-3p Ne-like lasing schemes demonstrated in selenium (Z equals 34) through molybdenum (Z equals 42). Three-body recombination schemes in H-like and Li-like ions are also currently being examined as a means of producing gain at shorter wavelengths.

AB - Experiments and theoretical modeling are reported that demonstrate significant gain-length products at wavelengths below the carbon K-edge at 44angstrom. Two different schemes have been examined. The first is collisional excitation of Ni-like ions, which is an analog of the 3s-3p Ne-like lasing schemes demonstrated in selenium (Z equals 34) through molybdenum (Z equals 42). Three-body recombination schemes in H-like and Li-like ions are also currently being examined as a means of producing gain at shorter wavelengths.

UR - http://www.scopus.com/inward/record.url?scp=0023533415&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=0023533415&partnerID=8YFLogxK

M3 - Conference contribution

AN - SCOPUS:0023533415

SP - 67

EP - 68

BT - Unknown Host Publication Title

PB - IEEE

CY - New York, NY, USA

ER -

PROGRESS TOWARDS DEMONSTRATION OF SHORTER WAVELENGTH SOFT X-RAY AMPLIFIERS PUMPED BY THE NOVA LASER.

Abstract

ASJC Scopus subject areas

Other files and links

Fingerprint

Cite this