Work toward experimental evidence of hard x-ray photoionization in highly charged krypton.
- X-Ray Science Division
Ions of almost any charge state can be produced through electron-impact ionization. Here we describe our first experiments designed to photoionize these highly charged ions with hard x-rays by pairing an electron and photon beam. A spectral line at 12.7(1) keV with an intensity corroborated by theory may be the first evidence of hard x-ray photoionization of a highly charged ion.
- Research Organization:
- Argonne National Lab. (ANL), Argonne, IL (United States)
- Sponsoring Organization:
- National Aeronautics and Space Administration (NASA); USDOE Office of Science (SC)
- DOE Contract Number:
- DE-AC02-06CH11357
- OSTI ID:
- 1029882
- Report Number(s):
- ANL/XSD/CP-71551; TRN: US1105843
- Resource Relation:
- Conference: 21st Int. Conf. on Application of Accelerators in Research and Industry:; Aug. 8, 2010 - Aug. 13, 2010; Fort Worth, TX
- Country of Publication:
- United States
- Language:
- ENGLISH
Similar Records
Work Towards Experimental Evidence Of Hard X-Ray Photoionization In Highly Charged Krypton
EVIDENCE FOR ULTRA-FAST OUTFLOWS IN RADIO-QUIET ACTIVE GALACTIC NUCLEI. II. DETAILED PHOTOIONIZATION MODELING OF Fe K-SHELL ABSORPTION LINES
EVIDENCE FOR THE FULL HARD X-RAY SPECTRAL SIGNATURE OF NONUNIFORM IONIZATION IN A SOLAR FLARE
Journal Article
·
Wed Jun 01 00:00:00 EDT 2011
· AIP Conference Proceedings
·
OSTI ID:1029882
+9 more
EVIDENCE FOR ULTRA-FAST OUTFLOWS IN RADIO-QUIET ACTIVE GALACTIC NUCLEI. II. DETAILED PHOTOIONIZATION MODELING OF Fe K-SHELL ABSORPTION LINES
Journal Article
·
Sun Nov 20 00:00:00 EST 2011
· Astrophysical Journal
·
OSTI ID:1029882
+3 more
EVIDENCE FOR THE FULL HARD X-RAY SPECTRAL SIGNATURE OF NONUNIFORM IONIZATION IN A SOLAR FLARE
Journal Article
·
Wed Apr 20 00:00:00 EDT 2011
· Astrophysical Journal
·
OSTI ID:1029882