Abstract
The x-ray spectrum emitted by a gas jet irradiated at 1016 W/cm2 has been measured for laser wavelengths of 1.05 and 0.53 m. The flux of hard x rays (h>10 keV) emitted by a gas jet is less than 0.3% of that emitted by a glass target irradiated at the same intensity. This low flux implies that less than 0.1% of the incident energy is used to heat electrons to energies greater than 10 keV.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 256-260 |
| Number of pages | 5 |
| Journal | Physical Review Letters |
| Volume | 48 |
| Issue number | 4 |
| DOIs | |
| State | Published - 1982 |
| Externally published | Yes |
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ASJC Scopus subject areas
- Physics and Astronomy(all)
Cite this
Absence of fast electrons in laser-irradiated gas-jet targets. / Tarvin, J. A.; Mayer, F. J.; Slater, D. C.; Busch, Gar E.; Charatis, G.; Pattinson, T. R.; Schroeder, R. J.; Sullivan, D.; Matthews, Dennis L.
In: Physical Review Letters, Vol. 48, No. 4, 1982, p. 256-260.Research output: Contribution to journal › Article
}
TY - JOUR
T1 - Absence of fast electrons in laser-irradiated gas-jet targets
AU - Tarvin, J. A.
AU - Mayer, F. J.
AU - Slater, D. C.
AU - Busch, Gar E.
AU - Charatis, G.
AU - Pattinson, T. R.
AU - Schroeder, R. J.
AU - Sullivan, D.
AU - Matthews, Dennis L
PY - 1982
Y1 - 1982
N2 - The x-ray spectrum emitted by a gas jet irradiated at 1016 W/cm2 has been measured for laser wavelengths of 1.05 and 0.53 m. The flux of hard x rays (h>10 keV) emitted by a gas jet is less than 0.3% of that emitted by a glass target irradiated at the same intensity. This low flux implies that less than 0.1% of the incident energy is used to heat electrons to energies greater than 10 keV.
AB - The x-ray spectrum emitted by a gas jet irradiated at 1016 W/cm2 has been measured for laser wavelengths of 1.05 and 0.53 m. The flux of hard x rays (h>10 keV) emitted by a gas jet is less than 0.3% of that emitted by a glass target irradiated at the same intensity. This low flux implies that less than 0.1% of the incident energy is used to heat electrons to energies greater than 10 keV.
UR - http://www.scopus.com/inward/record.url?scp=3943092612&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=3943092612&partnerID=8YFLogxK
U2 - 10.1103/PhysRevLett.48.256
DO - 10.1103/PhysRevLett.48.256
M3 - Article
AN - SCOPUS:3943092612
VL - 48
SP - 256
EP - 260
JO - Physical Review Letters
JF - Physical Review Letters
SN - 0031-9007
IS - 4
ER -