J/A+A/687/A41         Atomic data in Hf, Os, and Au I-IV       (Ben Nasr+, 2024)

Comparative study of kilonova opacities for three elements of the sixth period (hafnium, osmium, and gold) from new atomic structure calculations in Hf I-IV, Os I-IV, and Au I-IV. Ben Nasr S., Carvajal Gallego H., Deprince J., Palmeri P., Quinet P. <Astron. Astrophys. 687, A41 (2024)> =2024A&A...687A..41B 2024A&A...687A..41B (SIMBAD/NED BibCode)
ADC_Keywords: Atomic physics ; Opacities Keywords: atomic data - atomic processes - opacity Abstract: It is now well established that a large amount of heavy (trans-iron) elements are produced during neutron star (NS) mergers. These elements can be detected in the spectra of the kilonova emitted from the post-merger ejected materials. Due to the high level densities that characterize the complex configurations belonging to heavy elements, thus giving rise to millions of absorption lines, the kilonova ejecta opacity is of significant importance. The elements that contribute the most to the latter are those with an unfilled nd subshell belonging to the fifth and the sixth rows of the periodic table, and those with an unfilled nf subshell belonging to the lanthanide and actinide groups. The aim of the present work is to make a new contribution to this field by performing large-scale atomic structure calculations in three specific sixth-row 5d elements, namely hafnium, osmium, and gold, in the first four charge stages (I-IV), and by computing the corresponding opacities, while focusing on the importance of the atomic models used. The pseudo-relativistic Hartree-Fock (HFR) method, including extended sets of interacting configurations, was used for the atomic structure and radiative parameter calculations, while the expansion formalism was used to estimate the opacities. Theoretical energy levels, wavelengths, and oscillator strengths were computed for millions of spectral lines in Hf I-IV, Os I-IV, and Au I-IV ions, the reliability of these parameters being assessed through detailed comparisons with previously published experimental and theoretical results. The newly obtained atomic data were then used to calculate expansion opacities for typical kilonova conditions expected one day after the NS merger; these are a density of rho=10-13g/cm3 and temperatures ranging from T=5000K to T=15000K. Some agreements and differences were found when comparing our results with available data, highlighting the importance of using sufficiently complete atomic models for the determination of opacities. Description: Pseudo-relativistic Hartree-Fock (HFR) oscillator strengths for experimentally observed radiative transitions in Hf I-IV, Os I-IV and Au I-IV ions and comparison with previously published data. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 56 118 Oscillator strengths (log gf) for experimentally observed lines in Hf I table3.dat 80 53 Oscillator strengths (log gf) for experimentally observed lines in Hf II table4.dat 56 46 Oscillator strengths (log gf) for experimentally observed lines in Hf III table5.dat 50 41 Oscillator strengths (log gf) for experimentally observed lines in Hf IV table6.dat 68 23 Oscillator strengths (log gf) for experimentally observed lines in Os I table7.dat 62 24 Oscillator strengths (log gf) for experimentally observed lines in Os II table8.dat 56 73 Oscillator strengths (log gf) for experimentally observed lines in Os III table9.dat 56 70 Oscillator strengths (log gf) for experimentally observed lines in Os IV table10.dat 60 65 Oscillator strengths (log gf) for experimentally observed lines in Au I table11.dat 68 51 Oscillator strengths (log gf) for experimentally observed lines in Au II table12.dat 62 74 Oscillator strengths (log gf) for experimentally observed lines in Au III table13.dat 62 44 Oscillator strengths (log gf) for experimentally observed lines in Au IV -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- Lev(even) Even level 18- 31 A14 --- Lev(odd) Odd level 37- 44 F8.3 0.1nm lambda(EXP) Experimental wavelength (1) 46- 50 F5.2 --- loggf(HFR) Weighted oscillator strength (2) 52- 56 F5.2 --- loggf(prev) ? Weighted oscillator strength (3) -------------------------------------------------------------------------------- Note (1): From Kramida et al., NIST Atomic Database, 2023, https://physics.nist.gov/asd Note (2): Computed in the present work Note (3): From Duquette et al., 1986, JQSRT 35, 281 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 14 A14 --- Lev(even) Even level 18- 32 A15 --- Lev(odd) Odd level 37- 44 F8.3 0.1nm lambda(EXP) Experimental wavelength (1) 46- 50 F5.2 --- loggf(HFR) Weigthed oscillator strength (2) 52- 56 F5.2 --- loggf(preva) ? Weighted oscillator strength (3) 58- 62 F5.2 --- loggf(prevb) ? Weighted oscillator strength (4) 64- 68 F5.2 --- loggf(prevc) ? Weighted oscillator strength (5) 70- 74 F5.2 --- loggf(prevd) ? Weighted oscillator strength (6) 76- 80 F5.2 --- loggf(preve) ? Weighted oscillator strength (7) -------------------------------------------------------------------------------- Note (1): From Kramida et al., NIST Atomic Database, 2023, https://physics.nist.gov/asd Note (2): Computed in the present work Note (3): From Lawler et al., 2007ApJS..169..120L 2007ApJS..169..120L Note (4): From Lundqvist et al., 2006A&A...450..407L 2006A&A...450..407L Note (5): From Bouazza et al., 2015, JQSRT 163, 39 Note (6): From Bouazza et al., 2015, JQSRT 163, 39 Note (7): From Den Hartog et al., 2021ApJS..255...27D 2021ApJS..255...27D -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- Lev(even) Even level 18- 28 A11 --- Lev(odd) Odd level 37- 44 F8.3 0.1nm lambda(EXP) Experimental wavelength (1) 46- 50 F5.2 --- loggf(HFR) Weighted oscillator strength (2) 52- 56 F5.2 --- loggf(prev) Weighted oscillator strength (1) -------------------------------------------------------------------------------- Note (1): From Malcheva et al., 2009MNRAS.396.2289M 2009MNRAS.396.2289M Note (2): Computed in the present work -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- Lev(even) Even level 18- 29 A12 --- Lev(odd) Odd level 38- 44 F7.3 0.1nm lambda(EXP) Experimental wavelength (1) 46- 50 F5.2 --- loggf(HFR) Weighted oscillator strength (2) -------------------------------------------------------------------------------- Note (1): From Sugar et al., 1974, JOSA 64, 1656 Note (2): Computed in the present work -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- Lev(even) Evel level 18- 32 A15 --- Lev(odd) Odd level 37- 44 F8.3 0.1nm lambda(EXP) Experimental wavelength (1) 46- 50 F5.2 --- loggf(HFR) Weighted oscillator strength (2) 52- 56 F5.2 --- loggf(preva) Weighted oscillator strength (1) 58- 62 F5.2 --- loggf(prevb) ? Weighted oscillator strength (3) 64- 68 F5.2 --- loggf(prevc) ? Weighted oscillator strength (4) -------------------------------------------------------------------------------- Note (1): From Quinet et al., 2006A&A...448.1207Q 2006A&A...448.1207Q Note (2): Computed in the present work Note (3): From Ivarsson et al., 2003A&A...409.1141I 2003A&A...409.1141I Note (4): From Kurucz, 1993, CD-ROM No 18 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table7.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 15 A15 --- Lev(even) Even level 18- 33 A16 --- Lev(odd) Odd level 37- 44 F8.3 0.1nm lambda(EXP) Experimental wavelength (1) 46- 50 F5.2 --- loggf(HFR) Weighted oscillator strength (2) 52- 56 F5.2 --- loggf(preva) Weighted oscillator strength (1) 58- 62 F5.2 --- loggf(prevb) Weighted oscillator strength (3) -------------------------------------------------------------------------------- Note (1): From Quinet et al., 2006A&A...448.1207Q 2006A&A...448.1207Q Note (2): Computed in the present work Note (3): From Ivarsson et al., 2004A&A...425..353I 2004A&A...425..353I -------------------------------------------------------------------------------- Byte-by-byte Description of file: table8.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- Lev(even) Even level 18- 31 A14 --- Lev(odd) Odd level 37- 44 F8.3 0.1nm lambda(EXP) Experimental wavelength (1) 46- 50 F5.2 --- loggf(HFR) Weighted oscillator strength (2) 52- 56 F5.2 --- loggf(prev) Weighted oscillator strength (3) -------------------------------------------------------------------------------- Note (1): From Kramida et al., NIST Atomic Database, 2023, https://physics.nist.gov/asd Note (2): Computed in the present work Note (3): From Azarov et al., 2018, ADNDT 121, 345 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table9.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- Lev(even) Even level 18- 32 A15 --- Lev(odd) Odd level 38- 44 F7.3 0.1nm lambda(EXP) Experimental wavelength (1) 46- 50 F5.2 --- logf(HFR) Weighted oscillator strength (2) 52- 56 F5.2 --- loggf(prev) Weighted oscillator strength (1) -------------------------------------------------------------------------------- Note (1): From Ryabtsev et al., 1998, Phys. Scr. 57, 82 Note (2): Computed in the present work -------------------------------------------------------------------------------- Byte-by-byte Description of file: table10.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 A16 --- Lev(even) Even level 18- 33 A16 --- Lev(odd) Odd level 37- 44 F8.3 0.1nm lambda(EXP) Experimental wavelength (1) 46- 50 F5.2 --- logf(HFR) Weighted oscillator strength (2) 52- 56 F5.2 --- loggf(prev) ? Weighted oscillator strength 58- 60 A3 --- r_loggf(prev) Reference of previously published data (3) -------------------------------------------------------------------------------- Note (1): From Kramida et al., NIST Atomic Database, 2023, https://physics.nist.gov/asd Note (2): Computed in the present work Note (3): References as follows: (c) = Kramida et al., NIST Atomic Database, 2023, https://physics.nist.gov/asd (d) = McCann et al., 2022MNRAS.509.4723M 2022MNRAS.509.4723M (e) = Zhang et al., 2018, J. Phys. B 51, 205001 (f) = Hannaford et al., 1981 J. Phys. B 14, 2321 (g) = Corliss et al., 1981 NBS Monograph 53 (h) = Gaarde et al., 1994 Phys. Rev. A 50, 209 (i) = Fivet et al., 2007 J. Elec. Spectr. Rel. Phen. 250 (j) = Desclaux et al., 1994 J. Phys. B 8, 1177 (k) = Migdalek and Baylis, 1979 JQSRT 22, 113 (l) = Migdalek and Garmulewicz, 2000 J. Phys. B 33, 1735 (m) = Safronova and Johnson, 2004 Phys. Rev. A 69, 052511 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table11.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- Lev(even) Even level 18- 29 A12 --- Lev(odd) Odd level 37- 44 F8.3 0.1nm lambda(EXP) Experimental wavelength (1) 46- 50 F5.2 --- loggf(HFR) Weighted oscillator strength (2) 52- 56 F5.2 --- loggf(preva) ? Weighted oscillator strength (1) 58- 62 F5.2 --- loggf(prevb) ? Weighted oscillator strength (3) 64- 68 F5.2 --- loggf(prevc) ? Weighted oscillator strength (4) -------------------------------------------------------------------------------- Note (1): From Zhang et al., 2002, J. Phys. B 35, 483 Note (2): Computed in the present work Note (3): From McCann et al., 2022MNRAS.509.4723M 2022MNRAS.509.4723M Note (4): From Biemont et al., 2007MNRAS.380.1581B 2007MNRAS.380.1581B -------------------------------------------------------------------------------- Byte-by-byte Description of file: table12.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 A16 --- Lev(even) Even level 18- 34 A17 --- Lev(odd) Odd level 37- 44 F8.3 0.1nm lambda(EXP) Experimental wavelength (1) 46- 50 F5.2 --- loggf(HFR) Weighted oscillator strength (2) 52- 56 F5.2 --- loggf(preva) Weighted oscillator strength (1) 58- 62 F5.2 --- loggf(prevb) ? Weighted oscillator strength (3) -------------------------------------------------------------------------------- Note (1): From Zainab and Tauheed, 2019, JQSRT 237, 106614 Note (2): Computed in the present work Note (3): From Enzonga Yoca et al., 2008, Phys. Scr. 78, 025303 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table13.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 A16 --- Lev(even) Even level 18- 34 A17 --- Lev(odd) Odd level 37- 44 F8.3 0.1nm lambda(EXP) Experimental wavelength (1) 46- 50 F5.2 --- loggf(HFR) Weighted oscillator strength (2) 52- 56 F5.2 --- loggf(preva) Weighted oscillator strength (1) 58- 62 F5.2 --- loggf(prevb) ? Weighted oscillator strength (3) -------------------------------------------------------------------------------- Note (1): From Wyart et al., 1994, Phys. Scr. 50, 672 Note (2): Computed in the present work Note (3): Reference not precised by the authors -------------------------------------------------------------------------------- Acknowledgements: Pascal Quinet, pascal.quinet(at)umons.ac.be
(End) Patricia Vannier [CDS] 20-Jun-2024
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line