Finite temperature dense matter studies on next-generation light sources

Richard W. Lee; Stephen J. Moon; Hyun-Kyung Chung; Wojciech Rozmus; Hector A. Baldis; Gianluca Gregori; Robert C. Cauble; Otto L. Landen; Justin S. Wark; Andrew Ng; Steven J. Rose; Ciaran L. Lewis; Dave Riley; Jean-Claude Gauthier; Patrick Audebert

doi:10.1364/JOSAB.20.000770

Journal of the Optical Society of America B
Vol. 20,
Issue 4,
pp. 770-778
(2003)
•https://doi.org/10.1364/JOSAB.20.000770

Finite temperature dense matter studies on next-generation light sources

Richard W. Lee, Stephen J. Moon, Hyun-Kyung Chung, Wojciech Rozmus, Hector A. Baldis, Gianluca Gregori, Robert C. Cauble, Otto L. Landen, Justin S. Wark, Andrew Ng, Steven J. Rose, Ciaran L. Lewis, Dave Riley, Jean-Claude Gauthier, and Patrick Audebert

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Richard W. Lee, Stephen J. Moon, Hyun-Kyung Chung, Wojciech Rozmus, Hector A. Baldis, Gianluca Gregori, Robert C. Cauble, Otto L. Landen, Justin S. Wark, Andrew Ng, Steven J. Rose, Ciaran L. Lewis, Dave Riley, Jean-Claude Gauthier, and Patrick Audebert, "Finite temperature dense matter studies on next-generation light sources," J. Opt. Soc. Am. B 20, 770-778 (2003)

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Abstract

The construction of short-pulse tunable soft x-ray free electron laser sources based on the self-amplified spontaneous emission process will provide a major advance in capability for dense plasma-related and warm dense matter (WDM) research. The sources will provide $10^{13} photons$ in a 200-fs duration pulse that is tunable from approximately 6 to 100 nm. Here we discuss only two of the many applications made possible for WDM that has been severely hampered by the fact that laser-based methods have been unavailable because visible light will not propagate at electron densities of $n_{e} \geq 10^{22} {cm}^{- 3} .$ The next-generation light sources will remove these restrictions.

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$λ_{probe}$ (μm)	$n_{e} / 10^{21} {cm}^{- 3}$	1 ps	2 ps	3 ps	4 ps	5 ps
1	1	2.85	6.27	7.16	7.54	7.74
1/2	4	2.80	5.98	6.69	6.90	6.92
1/3	9	2.74	5.49	5.90	5.83	5.56

$T_{e}$ (eV)	$Log n_{e}$ (cm^-3 )	$λ_{laser}$ (Å)	Number of Particles/Debye Sphere^a	Γ^b	α^c	$L_{abs}$ ^d (μm)	Length^e (μm)	Fraction^f Scattered (#)
1	19	190	0.54	0.5	1.0	$5.00 \times 10^{5}$	5000	$1.22 \times 10^{- 6}$
1	20	190	0.17	1.08	2.0	$1.90 \times 10^{4}$	5000	$1.31 \times 10^{- 6}$
2	21	190	1.50	1.16	4.6	$3.47 \times 10^{2}$	500	$2.83 \times 10^{- 8}$
50	23	147	1.90	0.22	7.1	$1.84 \times 10^{0}$	10	$3.04 \times 10^{- 9}$
1	19	60	0.54	0.5	0.2	$5.00 \times 10^{6}$	5000	$1.68 \times 10^{- 6}$
1	20	60	0.17	1.08	0.6	$1.09 \times 10^{5}$	5000	$1.12 \times 10^{- 5}$
2	21	60	0.15	1.16	1.4	$4.50 \times 10^{3}$	500	$4.07 \times 10^{- 6}$
10	22	60	0.54	0.5	2.0	$1.58 \times 10^{2}$	500	$1.43 \times 10^{- 6}$
10	23	60	0.17	0.67	6.5	$3.45 \times 10^{0}$	10	$2.12 \times 10^{- 9}$
100	22	60	17.0	0.03	0.6	$1.90 \times 10^{3}$	10	$2.46 \times 10^{- 6}$
100	23	60	5.37	0.07	2.0	$2.40 \times 10^{1}$	10	$4.47 \times 10^{- 6}$

$λ_{probe}$ (μm)	$n_{e} / 10^{21} {cm}^{- 3}$	1 ps	2 ps	3 ps	4 ps	5 ps
1	1	2.85	6.27	7.16	7.54	7.74
1/2	4	2.80	5.98	6.69	6.90	6.92
1/3	9	2.74	5.49	5.90	5.83	5.56

$T_{e}$ (eV)	$Log n_{e}$ (cm^-3 )	$λ_{laser}$ (Å)	Number of Particles/Debye Sphere^a	Γ^b	α^c	$L_{abs}$ ^d (μm)	Length^e (μm)	Fraction^f Scattered (#)
1	19	190	0.54	0.5	1.0	$5.00 \times 10^{5}$	5000	$1.22 \times 10^{- 6}$
1	20	190	0.17	1.08	2.0	$1.90 \times 10^{4}$	5000	$1.31 \times 10^{- 6}$
2	21	190	1.50	1.16	4.6	$3.47 \times 10^{2}$	500	$2.83 \times 10^{- 8}$
50	23	147	1.90	0.22	7.1	$1.84 \times 10^{0}$	10	$3.04 \times 10^{- 9}$
1	19	60	0.54	0.5	0.2	$5.00 \times 10^{6}$	5000	$1.68 \times 10^{- 6}$
1	20	60	0.17	1.08	0.6	$1.09 \times 10^{5}$	5000	$1.12 \times 10^{- 5}$
2	21	60	0.15	1.16	1.4	$4.50 \times 10^{3}$	500	$4.07 \times 10^{- 6}$
10	22	60	0.54	0.5	2.0	$1.58 \times 10^{2}$	500	$1.43 \times 10^{- 6}$
10	23	60	0.17	0.67	6.5	$3.45 \times 10^{0}$	10	$2.12 \times 10^{- 9}$
100	22	60	17.0	0.03	0.6	$1.90 \times 10^{3}$	10	$2.46 \times 10^{- 6}$
100	23	60	5.37	0.07	2.0	$2.40 \times 10^{1}$	10	$4.47 \times 10^{- 6}$

Abstract

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Tables (2)

Equations (7)

Journal of the Optical Society of America B