Measurement of n-resolved State-Selective Charge Exchange in Ne(8,9)+ Collision with He and H2
arXiv:2105.04438 · doi:10.3847/1538-4365/abd020
Abstract
Charge exchange between highly charged ions and neutral atoms and molecules has been considered as one of the important mechanisms controlling soft X ray emissions in many astrophysical objects and environments. However, for modeling charge exchange soft X ray emission, the data of n and l resolved state selective capture cross sections are often obtained by empirical and semiclassical theory calculations. With a newly built cold target recoil ion momentum spectroscopy (COLTRIMS) apparatus, we perform a series of measurements of the charge exchange of Ne(8,9)+ ions with He and H2 for collision energy ranging from 1 to 24.75 keV/u. n resolved state selective capture cross-sections are reported. By comparing the measured state selective capture cross sections to those calculated by the multichannel Landau Zener method (MCLZ), it is found that MCLZ calculations are in good agreement with the measurement for the dominant n capture for He target. Furthermore, by using nl resolved cross sections calculated by MCLZ and applying l distributions commonly used in the astrophysical literature to experimentally derived n resolved cross sections, we calculate the soft X ray emissions in the charge exchange between 4 keV/u Ne8+ and He by considering the radiative cascade from the excited Ne7+ ions. Reasonable agreement is found in comparison to the measurement for even and separable models, and MCLZ calculations give results in a better agreement.
References in corpus (21)
- An unidentified line in X-ray spectra of the Andromeda galaxy and Perseus galaxy cluster
- Updated Atomic Data and Calculations for X-ray Spectroscopy
- The Baryon Census in a Multiphase Intergalactic Medium: 30% of the Baryons May Still Be Missing
- The Quiescent Intracluster Medium in the Core of the Perseus Cluster
- A High Spectral Resolution Observation of the Soft X-ray Diffuse Background with Thermal Detectors
- Observations of the MIssing Baryons in the warm-hot intergalactic medium
- The energy source of the filaments around the giant galaxy NGC1275
- A study of Jupiter's aurorae with XMM-Newton
- A novel scenario for the possible X-ray line feature at ~3.5 keV: Charge exchange with bare sulfur ions
- Possible Charge-Exchange X-Ray Emission in the Cygnus Loop Detected with Suzaku
- Resolving the Origin of the Diffuse Soft X-ray Background
- Plasma code for astrophysical charge exchange emission at X-ray wavelengths
- The solar wind charge-transfer X-ray emission in the 1/4 keV energy range: inferences on Local Bubble hot gas at low Z
- Charge Exchange X-ray Emission of Nearby Star-forming Galaxies
- Charge Exchange Induced X-ray Emission of Fe XXV and Fe XXVI via a Streamlined Model
- Laboratory Measurements of the K-shell transition energies in L-shell ions of Si and S
- Measurement of n-resolved State-Selective Charge Exchange in Ne(8,9)+ Collision with He and H2
- X-ray emission measurements following charge exchange between C and H
- Ne X X-ray Emission due to Charge Exchange in M82
- Suzaku Metal Abundance Patterns in the Outflow Region of M82 and the Importance of Charge Exchange
- High-resolution Charge Exchange Spectra with L-shell Nickel Show Striking Differences from Models