Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7509
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dc.contributor.authorChaudhuri, S. K-
dc.contributor.authorMukherjee, P. K-
dc.contributor.authorChaudhuri, R. K-
dc.contributor.authorChattopadhyay, S-
dc.date.accessioned2020-11-27T12:55:47Z-
dc.date.available2020-11-27T12:55:47Z-
dc.date.issued2018-04-
dc.identifier.citationPhysics of Plasmas, Vol. 25, No. 4, 042705en_US
dc.identifier.issn1070-664X-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/7509-
dc.descriptionRestricted Access © American Institute of Physics https://doi.org/10.1063/1.5011791en_US
dc.description.abstractThe equation of motion coupled cluster methodology within relativistic framework has been applied to analyze the electron correlation effects on the low lying dipole allowed excited states of Ne and Al3þ under classical and quantum plasma environments. The effect of confinement due to classical plasma has been incorporated through screened Coulomb potential, while that of quantum plasma has been treated by exponential cosine screened Coulomb potential. The confined structural properties investigated are the depression of ionization potential, low lying excitation energies (dipole allowed), oscillator strengths, transition probabilities, and frequency dependent polarizabilities under systematic variation of the plasma-atom coupling strength determined through the screening parameter. Specific atomic systems are chosen for their astrophysical importance and availability of experimental data related to laboratory plasma with special reference to Al3þ ion. Here, we consider 1s22s22p6ð1S0Þ ! 1s22s22p5 ns=nd ð1P1Þ ðn ¼ 3; 4Þ dipole allowed transitions of Ne and Al3þ. Results for the free (isolated) atomic systems agree well with those available in the literature. Spectroscopic properties under confinement show systematic and interesting pattern with respect to plasma screening parameter.en_US
dc.language.isoenen_US
dc.titleEquation of motion approach for describing allowed transitions in Ne and Al3+ under classical and quantum plasmasen_US
dc.typeArticleen_US
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