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Continuum Hard-Photon K-Shell Yields From Z-Pinch Implosions: Present Status and Scaling to Higher Currents
The use of the recombination continuum for X-ray radiation production in Z-pinches is discussed as an option for generating high yields in the warm photon energy range, \hslash \omega \gt 10 keV. The free-bound direct-recombination continuum emission is an inherently weaker radiation production me...
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Published in: | IEEE transactions on plasma science 2024-06, Vol.52 (6), p.2094-2116 |
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creator | Velikovich, Alexander L. Ouart, Nicholas D. Dasgupta, Arati Giuliani, John L. Tangri, Varun Harvey-Thompson, Adam J. Schaeuble, Marc-Andre Schwarz, Jens Myers, Clayton E. Ampleford, David J. Vesey, Roger A. Jones, Brent |
description | The use of the recombination continuum for X-ray radiation production in Z-pinches is discussed as an option for generating high yields in the warm photon energy range, \hslash \omega \gt 10 keV. The free-bound direct-recombination continuum emission is an inherently weaker radiation production mechanism than the resonant-line emission. However, it is challenging, if at all possible, to heat stagnated Z-pinch plasmas with atomic numbers Z_{A} \gt 36 to temperatures above ~10 keV needed for efficient K-shell line emission in the warm photon energy range. As the atomic number of the load material increases from Z_{A} = 18 (argon) to Z_{A} = 26 and 29 (iron and copper, respectively), the scaling parameter determining the ratio of the recombination continuum to hydrogen-like line K-shell yield increases by a factor of 2-3. This indicates a possibility of using wire-array Z-pinch implosions on next-generation pulsed-power facilities (NGPPs) to produce significant continuum yields in warm photons. Such an option is feasible, provided that stripping substantial fractions of iron and copper ions at stagnation to an H-like state can be demonstrated. We analyze K-shell continuum yields measured in recent Z experiments with argon double-shell gas-puff and stainless-steel nested wire-array loads, with a view of scaling present-day results to higher driver currents. |
doi_str_mv | 10.1109/TPS.2024.3428372 |
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The free-bound direct-recombination continuum emission is an inherently weaker radiation production mechanism than the resonant-line emission. However, it is challenging, if at all possible, to heat stagnated Z-pinch plasmas with atomic numbers <inline-formula> <tex-math notation="LaTeX">Z_{A} \gt 36 </tex-math></inline-formula> to temperatures above ~10 keV needed for efficient K-shell line emission in the warm photon energy range. As the atomic number of the load material increases from <inline-formula> <tex-math notation="LaTeX">Z_{A} = 18 </tex-math></inline-formula> (argon) to <inline-formula> <tex-math notation="LaTeX">Z_{A} = 26 </tex-math></inline-formula> and 29 (iron and copper, respectively), the scaling parameter determining the ratio of the recombination continuum to hydrogen-like line K-shell yield increases by a factor of 2-3. This indicates a possibility of using wire-array Z-pinch implosions on next-generation pulsed-power facilities (NGPPs) to produce significant continuum yields in warm photons. Such an option is feasible, provided that stripping substantial fractions of iron and copper ions at stagnation to an H-like state can be demonstrated. We analyze K-shell continuum yields measured in recent Z experiments with argon double-shell gas-puff and stainless-steel nested wire-array loads, with a view of scaling present-day results to higher driver currents.]]></description><identifier>ISSN: 0093-3813</identifier><identifier>EISSN: 1939-9375</identifier><identifier>DOI: 10.1109/TPS.2024.3428372</identifier><identifier>CODEN: ITPSBD</identifier><language>eng</language><publisher>IEEE</publisher><subject>Atomic measurements ; Electrons ; Ions ; K-shell radiation ; plasma pinch ; Plasma temperature ; Plasmas ; Radiative recombination ; recombination continuum ; Temperature measurement ; X-ray production ; Z pulsed-power facility</subject><ispartof>IEEE transactions on plasma science, 2024-06, Vol.52 (6), p.2094-2116</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c189t-ecd1b4796b57270d27458a42316db1235fc844879e5ba23dc86e1ee4e56250413</cites><orcidid>0000-0002-2782-6246 ; 0000-0003-1977-7779 ; 0000-0003-4539-8406 ; 0000-0002-3742-2421 ; 0000-0001-7684-6932 ; 0000-0003-0459-0119</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://ieeexplore.ieee.org/document/10609758$$EHTML$$P50$$Gieee$$H</linktohtml><link.rule.ids>314,780,784,27922,27923,54794</link.rule.ids></links><search><creatorcontrib>Velikovich, Alexander L.</creatorcontrib><creatorcontrib>Ouart, Nicholas D.</creatorcontrib><creatorcontrib>Dasgupta, Arati</creatorcontrib><creatorcontrib>Giuliani, John L.</creatorcontrib><creatorcontrib>Tangri, Varun</creatorcontrib><creatorcontrib>Harvey-Thompson, Adam J.</creatorcontrib><creatorcontrib>Schaeuble, Marc-Andre</creatorcontrib><creatorcontrib>Schwarz, Jens</creatorcontrib><creatorcontrib>Myers, Clayton E.</creatorcontrib><creatorcontrib>Ampleford, David J.</creatorcontrib><creatorcontrib>Vesey, Roger A.</creatorcontrib><creatorcontrib>Jones, Brent</creatorcontrib><title>Continuum Hard-Photon K-Shell Yields From Z-Pinch Implosions: Present Status and Scaling to Higher Currents</title><title>IEEE transactions on plasma science</title><addtitle>TPS</addtitle><description><![CDATA[The use of the recombination continuum for X-ray radiation production in Z-pinches is discussed as an option for generating high yields in the warm photon energy range, <inline-formula> <tex-math notation="LaTeX">\hslash \omega \gt 10 </tex-math></inline-formula> keV. The free-bound direct-recombination continuum emission is an inherently weaker radiation production mechanism than the resonant-line emission. However, it is challenging, if at all possible, to heat stagnated Z-pinch plasmas with atomic numbers <inline-formula> <tex-math notation="LaTeX">Z_{A} \gt 36 </tex-math></inline-formula> to temperatures above ~10 keV needed for efficient K-shell line emission in the warm photon energy range. As the atomic number of the load material increases from <inline-formula> <tex-math notation="LaTeX">Z_{A} = 18 </tex-math></inline-formula> (argon) to <inline-formula> <tex-math notation="LaTeX">Z_{A} = 26 </tex-math></inline-formula> and 29 (iron and copper, respectively), the scaling parameter determining the ratio of the recombination continuum to hydrogen-like line K-shell yield increases by a factor of 2-3. This indicates a possibility of using wire-array Z-pinch implosions on next-generation pulsed-power facilities (NGPPs) to produce significant continuum yields in warm photons. Such an option is feasible, provided that stripping substantial fractions of iron and copper ions at stagnation to an H-like state can be demonstrated. We analyze K-shell continuum yields measured in recent Z experiments with argon double-shell gas-puff and stainless-steel nested wire-array loads, with a view of scaling present-day results to higher driver currents.]]></description><subject>Atomic measurements</subject><subject>Electrons</subject><subject>Ions</subject><subject>K-shell radiation</subject><subject>plasma pinch</subject><subject>Plasma temperature</subject><subject>Plasmas</subject><subject>Radiative recombination</subject><subject>recombination continuum</subject><subject>Temperature measurement</subject><subject>X-ray production</subject><subject>Z pulsed-power facility</subject><issn>0093-3813</issn><issn>1939-9375</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><recordid>eNpNkLtOwzAARS0EEqWwMzD4B1z8jG02VFFaUYlIKQMskZO4jSGxKzsZ-HtatQPTXc65wwHgnuAZIVg_bvJiRjHlM8apYpJegAnRTCPNpLgEE4w1Q0wRdg1uUvrGmHCB6QT8zIMfnB_HHi5NbFDehiF4-IaK1nYd_HS2axJcxNDDL5Q7X7dw1e-7kFzw6Qnm0SbrB1gMZhgTNL6BRW0653dwCHDpdq2NcD7GeIDSLbjami7Zu_NOwcfiZTNfovX762r-vEY1UXpAtm5IxaXOKiGpxA2VXCjDKSNZUxHKxLZWnCupragMZU2tMkus5VZkVGBO2BTg028dQ0rRbst9dL2JvyXB5TFWeYhVHmOV51gH5eGkOGvtPzzDWgrF_gDH4WW-</recordid><startdate>202406</startdate><enddate>202406</enddate><creator>Velikovich, Alexander L.</creator><creator>Ouart, Nicholas D.</creator><creator>Dasgupta, Arati</creator><creator>Giuliani, John L.</creator><creator>Tangri, Varun</creator><creator>Harvey-Thompson, Adam J.</creator><creator>Schaeuble, Marc-Andre</creator><creator>Schwarz, Jens</creator><creator>Myers, Clayton E.</creator><creator>Ampleford, David J.</creator><creator>Vesey, Roger A.</creator><creator>Jones, Brent</creator><general>IEEE</general><scope>97E</scope><scope>RIA</scope><scope>RIE</scope><scope>AAYXX</scope><scope>CITATION</scope><orcidid>https://orcid.org/0000-0002-2782-6246</orcidid><orcidid>https://orcid.org/0000-0003-1977-7779</orcidid><orcidid>https://orcid.org/0000-0003-4539-8406</orcidid><orcidid>https://orcid.org/0000-0002-3742-2421</orcidid><orcidid>https://orcid.org/0000-0001-7684-6932</orcidid><orcidid>https://orcid.org/0000-0003-0459-0119</orcidid></search><sort><creationdate>202406</creationdate><title>Continuum Hard-Photon K-Shell Yields From Z-Pinch Implosions: Present Status and Scaling to Higher Currents</title><author>Velikovich, Alexander L. ; 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The free-bound direct-recombination continuum emission is an inherently weaker radiation production mechanism than the resonant-line emission. However, it is challenging, if at all possible, to heat stagnated Z-pinch plasmas with atomic numbers <inline-formula> <tex-math notation="LaTeX">Z_{A} \gt 36 </tex-math></inline-formula> to temperatures above ~10 keV needed for efficient K-shell line emission in the warm photon energy range. As the atomic number of the load material increases from <inline-formula> <tex-math notation="LaTeX">Z_{A} = 18 </tex-math></inline-formula> (argon) to <inline-formula> <tex-math notation="LaTeX">Z_{A} = 26 </tex-math></inline-formula> and 29 (iron and copper, respectively), the scaling parameter determining the ratio of the recombination continuum to hydrogen-like line K-shell yield increases by a factor of 2-3. This indicates a possibility of using wire-array Z-pinch implosions on next-generation pulsed-power facilities (NGPPs) to produce significant continuum yields in warm photons. Such an option is feasible, provided that stripping substantial fractions of iron and copper ions at stagnation to an H-like state can be demonstrated. We analyze K-shell continuum yields measured in recent Z experiments with argon double-shell gas-puff and stainless-steel nested wire-array loads, with a view of scaling present-day results to higher driver currents.]]></abstract><pub>IEEE</pub><doi>10.1109/TPS.2024.3428372</doi><tpages>23</tpages><orcidid>https://orcid.org/0000-0002-2782-6246</orcidid><orcidid>https://orcid.org/0000-0003-1977-7779</orcidid><orcidid>https://orcid.org/0000-0003-4539-8406</orcidid><orcidid>https://orcid.org/0000-0002-3742-2421</orcidid><orcidid>https://orcid.org/0000-0001-7684-6932</orcidid><orcidid>https://orcid.org/0000-0003-0459-0119</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Atomic measurements Electrons Ions K-shell radiation plasma pinch Plasma temperature Plasmas Radiative recombination recombination continuum Temperature measurement X-ray production Z pulsed-power facility |
title | Continuum Hard-Photon K-Shell Yields From Z-Pinch Implosions: Present Status and Scaling to Higher Currents |
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