Zobrazeno 1 - 10
of 6 640
pro vyhledávání: '"Eissner, A"'
Autor:
Anand K. Bhatia, Anthony E. Lynas-Gray, Claudio Mendoza, Sultana Nahar, Harry Nussbaumer, Anil K. Pradhan, Anthony M. Seaton, Günter Wunner, Claude J. Zeippen
Publikováno v:
Atoms, Vol 11, Iss 3, p 59 (2023)
Werner Eissner (Figure 1), a pioneer in computational atomic physics, was born on 16 October 1930 in the city of Görlitz, Germany, to Bernhard and Frieda (née Eckert) Eissner [...]
Externí odkaz:
https://doaj.org/article/4d2d779ede6a4a35baacf2572ae8b46b
Publikováno v:
Industrial Arene Chemistry. :1463-1478
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7445716a09038ae67bf83048ac98a76a
https://doi.org/10.1002/9783527827992.ch49
https://doi.org/10.1002/9783527827992.ch49
Autor:
Bhatia, Anand K., Lynas-Gray, Anthony E., Mendoza, Claudio, Nahar, Sultana, Nussbaumer, Harry, Pradhan, Anil K., Seaton, Anthony M., Wunner, Günter, Zeippen, Claude J.
Publikováno v:
Atoms (2218-2004); Mar2023, Vol. 11 Issue 3, p59, 6p
Autor:
Gierl, Martin
Publikováno v:
Zeitschrift für Historische Forschung, 2018 Jan 01. 45(2), 416-418.
Externí odkaz:
https://www.jstor.org/stable/26648053
Autor:
Bhatia, Anand K., Lynas-Gray, Anthony E., Mendoza, Claudio, Nahar, Sultana, Nussbaumer, Harry, Pradhan, Anil K., Seaton, Anthony M., Wunner, Günter, Zeippen, Claude J.
Publikováno v:
Atoms, 11 (3)
ISSN:2218-2004
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dfb4233f311eb7ff70c5aab7bc123a57
An extended version of the R-matrix methodology is presented for calculation of radiative parameters for improved plasma opacities. Contrast and comparisons with existing methods primarily relying on the Distorted Wave (DW) approximation are discusse
Externí odkaz:
http://arxiv.org/abs/2308.14882
To investigate the completeness of coupled channel (CC) Breit-Pauli R-Matrix (BPRM) calculations for opacities, we employ the relativistic distorted wave (RDW) method to complement (``top-up'') and compare the BPRM photoionization cross sections for
Externí odkaz:
http://arxiv.org/abs/2308.14880
Iron is the dominant heavy element that plays an important role in radiation transport in stellar interiors. Owing to its abundance and large number of bound levels and transitions, iron ions determine the opacity more than any other astrophysically
Externí odkaz:
http://arxiv.org/abs/2308.14854