The absolute total cross sections for the charge exchange between highly charged ions15N7+, O7+, and atomic H have been measured with the ion-atom merged-beams apparatus at Oak Ridge National Laboratory. The collision energy range is from 1224 down to 2 eV u−1, which covers outflowing hot components of astrophysical charge exchange plasmas like stellar-wind and supernova remnants. Good agreement with the previous measurements and theory is found for the collision energies above 100 eV u−1, while below 100 eV u−1limited agreement is achieved with the available calculations. These cross-section data are useful for modeling X-ray emission resulting from the charge exchange at the interface of hot plasma interacting with ambient neutral gas.
- Home
- Search Results
- Page 1 of 1
Search for: All records
-
Total Resources3
- Resource Type
-
00030
- Availability
-
30
- Author / Contributor
- Filter by Author / Creator
-
-
Zhang, R. T. (3)
-
Andrianarijaona, V. M. (2)
-
Havener, C. C. (2)
-
Seely, D. G. (2)
-
Draganić, I. N. (1)
-
Feng, W. T. (1)
-
Fogle, M. (1)
-
Gao, Y. (1)
-
Guo, D. L. (1)
-
Ma, X. (1)
-
McCammon, D. (1)
-
Morgan, K. (1)
-
Schulz, M. (1)
-
Stancil, P. C. (1)
-
Wulf, D. (1)
-
Zhang, S. F. (1)
-
Zhao, D. M. (1)
-
Zhu, X. L. (1)
-
#Tyler Phillips, Kenneth E. (0)
-
#Willis, Ciara (0)
-
- Filter by Editor
-
-
& Spizer, S. M. (0)
-
& . Spizer, S. (0)
-
& Ahn, J. (0)
-
& Bateiha, S. (0)
-
& Bosch, N. (0)
-
& Brennan K. (0)
-
& Brennan, K. (0)
-
& Chen, B. (0)
-
& Chen, Bodong (0)
-
& Drown, S. (0)
-
& Ferretti, F. (0)
-
& Higgins, A. (0)
-
& J. Peters (0)
-
& Kali, Y. (0)
-
& Ruiz-Arias, P.M. (0)
-
& S. Spitzer (0)
-
& Spitzer, S. (0)
-
& Spitzer, S.M. (0)
-
(submitted - in Review for IEEE ICASSP-2024) (0)
-
- (0)
-
-
Have feedback or suggestions for a way to improve these results?
!
Note: When clicking on a Digital Object Identifier (DOI) number, you will be taken to an external site maintained by the publisher.
Some full text articles may not yet be available without a charge during the embargo (administrative interval).
What is a DOI Number?
Some links on this page may take you to non-federal websites. Their policies may differ from this site.
-
Abstract -
Gao, Y. ; Schulz, M. ; Guo, D. L. ; Zhang, S. F. ; Zhu, X. L. ; Zhang, R. T. ; Feng, W. T. ; Zhao, D. M. ; Ma, X. ( , Physical Review A)
-
Seely, D. G. ; Andrianarijaona, V. M. ; Wulf, D. ; Morgan, K. ; McCammon, D. ; Fogle, M. ; Stancil, P. C. ; Zhang, R. T. ; Havener, C. C. ( , Physical Review A)