FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2327438087> ?p ?o ?g. }

• W2327438087 abstract "We have measured the absolute double-differential cross sections (DDCS) for electron emission in ionization of He and Ne atoms under the impact of 6-MeV/u ${mathrm{C}}^{6+}$ ions. Data were collected between 1 and 500 eV for He, while for Ne this range was extended up to 1000 eV. The angular ranges covered in the experiment are ${30}^{ensuremath{circ}}$ to ${150}^{ensuremath{circ}}$ and ${20}^{ensuremath{circ}}$ to ${160}^{ensuremath{circ}}$ for He and Ne, respectively. The DDCS spectra are compared with the prior and the post forms of the state-of-the-art continuum-distorted-wave eikonal-initial-state model. Both the theoretical models show very good agreement with the energy and angular distributions of the DDCS in the case of He. For Ne, at low energies both are going together and matching very well with the data. In the high-energy region, at extreme forward and backward angles, although both the forms are underestimating the experimental data to some extent, the prior form shows much better agreement compared to the post form. This post-prior discrepancy is attributed to the influence of dynamic screening, on the ionized one, produced by the electrons remaining in the target. The single differential cross sections (SDCS) in emission angle $(frac{densuremath{sigma}}{d{ensuremath{Omega}}_{e}})$ and electron energy $(frac{densuremath{sigma}}{d{ensuremath{epsilon}}_{e}})$ are deduced by integrating the electron DDCS spectra. While excellent agreement is obtained for the $frac{densuremath{sigma}}{d{ensuremath{epsilon}}_{e}}$ spectrum, the $frac{densuremath{sigma}}{d{ensuremath{Omega}}_{e}}$ provides a further sensitive test to the adequacy of the theoretical model employed. The total cross section obtained from the SDCS spectra is about 11% higher than the prior model for He and about 6% lower for Ne. To get the quantitative picture of the two-center effect, the forward-backward angular asymmetry parameter has been deduced as a function of velocity of the ejected electrons. For both the targets, it is very well reproduced by both the forms of the theory. For the Ne target, $K$-LL Auger angular distribution has also been studied, which shows small asymmetry caused by multiple vacancies in the $L$ shell along with the $K$-shell vacancy." @default.
• W2327438087 created "2016-06-24" @default.
• W2327438087 creator A5002535567 @default.
• W2327438087 creator A5019734185 @default.
• W2327438087 creator A5022323541 @default.
• W2327438087 creator A5035083056 @default.
• W2327438087 creator A5049892737 @default.
• W2327438087 creator A5059165968 @default.
• W2327438087 date "2014-11-17" @default.
• W2327438087 modified "2023-10-14" @default.
• W2327438087 title "Energy and angular distribution of electrons in ionization of He and Ne by 6-MeV/u bare carbon ions: Comparison with continuum-distorted-wave eikonal-initial-state calculations in prior and post forms" @default.
• W2327438087 cites W1482386893 @default.
• W2327438087 cites W1624531027 @default.
• W2327438087 cites W1966269594 @default.
• W2327438087 cites W1967806128 @default.
• W2327438087 cites W1967958941 @default.
• W2327438087 cites W1970600082 @default.
• W2327438087 cites W1971955304 @default.
• W2327438087 cites W1972175771 @default.
• W2327438087 cites W1972685022 @default.
• W2327438087 cites W1974752746 @default.
• W2327438087 cites W1979452492 @default.
• W2327438087 cites W1981098317 @default.
• W2327438087 cites W1983775013 @default.
• W2327438087 cites W1984568778 @default.
• W2327438087 cites W1990325744 @default.
• W2327438087 cites W1990615114 @default.
• W2327438087 cites W1998793378 @default.
• W2327438087 cites W2000575092 @default.
• W2327438087 cites W2002215024 @default.
• W2327438087 cites W2004659757 @default.
• W2327438087 cites W2006509627 @default.
• W2327438087 cites W2008696840 @default.
• W2327438087 cites W2008697068 @default.
• W2327438087 cites W2009372152 @default.
• W2327438087 cites W2012159833 @default.
• W2327438087 cites W2013118472 @default.
• W2327438087 cites W2015621381 @default.
• W2327438087 cites W2016118608 @default.
• W2327438087 cites W2017932262 @default.
• W2327438087 cites W2022920847 @default.
• W2327438087 cites W2027821457 @default.
• W2327438087 cites W2032872731 @default.
• W2327438087 cites W2034882017 @default.
• W2327438087 cites W2036716899 @default.
• W2327438087 cites W2038204900 @default.
• W2327438087 cites W2043582455 @default.
• W2327438087 cites W2044358858 @default.
• W2327438087 cites W2052229300 @default.
• W2327438087 cites W2053067241 @default.
• W2327438087 cites W2060331159 @default.
• W2327438087 cites W2061268165 @default.
• W2327438087 cites W2071880086 @default.
• W2327438087 cites W2075355486 @default.
• W2327438087 cites W2078441433 @default.
• W2327438087 cites W2080299990 @default.
• W2327438087 cites W2080694416 @default.
• W2327438087 cites W2081177259 @default.
• W2327438087 cites W2082803617 @default.
• W2327438087 cites W2082887857 @default.
• W2327438087 cites W2083648588 @default.
• W2327438087 cites W2087170775 @default.
• W2327438087 cites W2087197902 @default.
• W2327438087 cites W2088163964 @default.
• W2327438087 cites W2088977362 @default.
• W2327438087 cites W2093874384 @default.
• W2327438087 cites W2095508566 @default.
• W2327438087 cites W2114267968 @default.
• W2327438087 cites W2313303368 @default.
• W2327438087 cites W2317063525 @default.
• W2327438087 cites W2326541206 @default.
• W2327438087 cites W2329671789 @default.
• W2327438087 cites W269770743 @default.
• W2327438087 cites W4211178441 @default.
• W2327438087 doi "https://doi.org/10.1103/physreva.90.052714" @default.
• W2327438087 hasPublicationYear "2014" @default.
• W2327438087 type Work @default.
• W2327438087 sameAs 2327438087 @default.
• W2327438087 citedByCount "15" @default.
• W2327438087 countsByYear W23274380872015 @default.
• W2327438087 countsByYear W23274380872017 @default.
• W2327438087 countsByYear W23274380872018 @default.
• W2327438087 countsByYear W23274380872019 @default.
• W2327438087 countsByYear W23274380872021 @default.
• W2327438087 countsByYear W23274380872022 @default.
• W2327438087 countsByYear W23274380872023 @default.
• W2327438087 crossrefType "journal-article" @default.
• W2327438087 hasAuthorship W2327438087A5002535567 @default.
• W2327438087 hasAuthorship W2327438087A5019734185 @default.
• W2327438087 hasAuthorship W2327438087A5022323541 @default.
• W2327438087 hasAuthorship W2327438087A5035083056 @default.
• W2327438087 hasAuthorship W2327438087A5049892737 @default.
• W2327438087 hasAuthorship W2327438087A5059165968 @default.
• W2327438087 hasBestOaLocation W23274380872 @default.
• W2327438087 hasConcept C121332964 @default.
• W2327438087 hasConcept C141595757 @default.
• W2327438087 hasConcept C145148216 @default.
• W2327438087 hasConcept C147120987 @default.
• W2327438087 hasConcept C184779094 @default.
• W2327438087 hasConcept C185544564 @default.

• next