| Summary: | In this work, a krypton gas impurity seeding experiment was conducted in a Large Helical Device. Emission lines from the Na-like Kr ion in the extreme ultraviolet wavelength region, such as 22.00 nm, 17.89 nm, 16.51 nm, 15.99 nm, and 14.08 nm, respective to <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mn>2</mn><msup><mi mathvariant="normal">p</mi><mn>6</mn></msup><mn>3</mn><mi mathvariant="normal">p</mi><mrow><msup><mo>(</mo><mn>2</mn></msup><msubsup><mi mathvariant="normal">P</mi><mrow><mn>1</mn><mo>/</mo><mn>2</mn></mrow><mi mathvariant="normal">o</mi></msubsup><mo>)</mo></mrow><mo>−</mo><mn>2</mn><msup><mi mathvariant="normal">p</mi><mn>6</mn></msup><mn>3</mn><mi mathvariant="normal">s</mi><mrow><msup><mo>(</mo><mn>2</mn></msup><msub><mi mathvariant="normal">S</mi><mrow><mn>1</mn><mo>/</mo><mn>2</mn></mrow></msub><mo>)</mo></mrow></mrow></semantics></math></inline-formula>, <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mn>2</mn><msup><mi mathvariant="normal">p</mi><mn>6</mn></msup><mn>3</mn><mi mathvariant="normal">p</mi><mrow><msup><mo>(</mo><mn>2</mn></msup><msubsup><mi mathvariant="normal">P</mi><mrow><mn>3</mn><mo>/</mo><mn>2</mn></mrow><mi mathvariant="normal">o</mi></msubsup><mo>)</mo></mrow><mo>−</mo><mn>2</mn><msup><mi mathvariant="normal">p</mi><mn>6</mn></msup><mn>3</mn><mi mathvariant="normal">s</mi><mrow><msup><mo>(</mo><mn>2</mn></msup><msub><mi mathvariant="normal">S</mi><mrow><mn>1</mn><mo>/</mo><mn>2</mn></mrow></msub><mo>)</mo></mrow></mrow></semantics></math></inline-formula>, <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mn>2</mn><msup><mi mathvariant="normal">p</mi><mn>6</mn></msup><mn>3</mn><mi mathvariant="normal">d</mi><mrow><msup><mo>(</mo><mn>2</mn></msup><msub><mi mathvariant="normal">D</mi><mrow><mn>3</mn><mo>/</mo><mn>2</mn></mrow></msub><mo>)</mo></mrow><mo>−</mo><mn>2</mn><msup><mi mathvariant="normal">p</mi><mn>6</mn></msup><mn>3</mn><mi mathvariant="normal">p</mi><mrow><msup><mo>(</mo><mn>2</mn></msup><msubsup><mi mathvariant="normal">P</mi><mrow><mn>3</mn><mo>/</mo><mn>2</mn></mrow><mi mathvariant="normal">o</mi></msubsup><mo>)</mo></mrow></mrow></semantics></math></inline-formula>, <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mn>2</mn><msup><mi mathvariant="normal">p</mi><mn>6</mn></msup><mn>3</mn><mi mathvariant="normal">d</mi><mrow><msup><mo>(</mo><mn>2</mn></msup><msub><mi mathvariant="normal">D</mi><mrow><mn>5</mn><mo>/</mo><mn>2</mn></mrow></msub><mo>)</mo></mrow><mo>−</mo><mn>2</mn><msup><mi mathvariant="normal">p</mi><mn>6</mn></msup><mn>3</mn><mi mathvariant="normal">p</mi><mrow><msup><mo>(</mo><mn>2</mn></msup><msubsup><mi mathvariant="normal">P</mi><mrow><mn>3</mn><mo>/</mo><mn>2</mn></mrow><mi mathvariant="normal">o</mi></msubsup><mo>)</mo></mrow></mrow></semantics></math></inline-formula>, and <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mn>2</mn><msup><mi mathvariant="normal">p</mi><mn>6</mn></msup><mn>3</mn><mi mathvariant="normal">d</mi><mrow><msup><mo>(</mo><mn>2</mn></msup><msub><mi mathvariant="normal">D</mi><mrow><mn>3</mn><mo>/</mo><mn>2</mn></mrow></msub><mo>)</mo></mrow><mo>−</mo><mn>2</mn><msup><mi mathvariant="normal">p</mi><mn>6</mn></msup><mn>3</mn><mi mathvariant="normal">p</mi><mrow><msup><mo>(</mo><mn>2</mn></msup><msubsup><mi mathvariant="normal">P</mi><mrow><mn>1</mn><mo>/</mo><mn>2</mn></mrow><mi mathvariant="normal">o</mi></msubsup><mo>)</mo></mrow></mrow></semantics></math></inline-formula> transitions, are observed. In order to generate a theoretical synthetic spectrum, an extensive calculation concerning the excitation of the <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msup><mi>Kr</mi><mrow><mn>25</mn><mo>+</mo></mrow></msup></semantics></math></inline-formula> ion through electron impact was performed for the development of a suitable plasma model. For this, the relativistic multiconfiguration Dirac–Hartree–Fock method was employed along with its extension to the relativistic configuration interaction method to compute the relativistic bound-state wave functions and excitation energies of the fine structure levels using the General Relativistic Atomic Structure Package-2018. In addition, another set of calculations was carried out utilizing the relativistic many-body perturbation theory and relativistic configuration interaction methods integrated within the Flexible Atomic Code. To investigate the reliability of our findings, the results of excitation energies, transition probabilities, and weighted oscillator strengths of different dipole-allowed transitions obtained from these different methods are presented and compared with the available data. Further, the detailed electron impact excitation cross-sections and their respective rate coefficients are obtained for various fine structure resolved transitions using the fully relativistic distorted wave method. Rate coefficients, calculated using the Flexible Atomic Code for population and de-population kinetic processes, are integrated into the collisional-radiative plasma model to generate a theoretical spectrum. Further, the emission lines observed from the <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msup><mi>Kr</mi><mrow><mn>25</mn><mo>+</mo></mrow></msup></semantics></math></inline-formula> ion in the impurity seeding experiment were compared with the present plasma model spectrum, demonstrating a noteworthy overall agreement between the measurement and the theoretical synthetic spectrum.
|
|---|