J/A+A/678/A170      Effective collision strengths for Ni III    (Blondin+, 2023)

Nebular spectra from Type Ia supernova explosion models compared to JWST observations of SN 2021aefx. Blondin S., Dessart L., Hillier D.J., Ramsbottom C.A., Storey P.J. <Astron. Astrophys. 678, A170 (2023)> =2023A&A...678A.170B 2023A&A...678A.170B (SIMBAD/NED BibCode)
ADC_Keywords: Atomic physics ; Excitation rates ; Models, atmosphere Keywords: supernovae: general - radiative transfer - atomic data - line: identification - supernovae: individual: SN 2021aefx Abstract: Recent JWST observations of the Type Ia supernova (SN Ia) 2021aefx in the nebular phase have paved the way for late-time studies covering the full optical to mid-infrared (MIR) wavelength range, and with it the hope to better constrain SN Ia explosion mechanisms. We investigate whether public SN Ia models covering a broad range of progenitor scenarios and explosion mechanisms (Chandrasekhar-mass, or MCh, delayed detonations, pulsationally assisted gravitationally-confined detonations, sub-MCh double detonations, and violent mergers) can reproduce the full optical-MIR spectrum of SN 2021aefx at ∼270 days post explosion. Methods. We consider spherically-averaged 3D models available from the Heidelberg Supernova Model Archive with a 56Ni yield in the range 0.5-0.8M. We perform 1D steady-state non-local thermodynamic equilibrium simulations with the radiative-transfer code CMFGEN, and compare the predicted spectra to SN 2021aefx. The models can explain the main features of SN 2021aefx over the full wavelength range. However, no single model, or mechanism, emerges as a preferred match, and the predicted spectra are similar to one another despite the very different explosion mechanisms. We discuss possible causes for the mismatch of the models, including ejecta asymmetries and ionisation effects. Our new calculations of the collisional strengths for NiIII have a major impact on the two prominent lines at 7.35um and 11.00um, and highlight the need for more accurate collisional data for forbidden transitions. Using updated atomic data, we identify a strong feature due to [CaIV] 3.21um, attributed to [NiI] in previous studies. We also provide a tentative identification of a forbidden line due to [NeII] 12.81um, whose peaked profile suggests that neon is mixed inwards during the explosion, as predicted for instance in violent merger models. Contrary to previous claims, we show that the [ArIII] 8.99um line can be broader in sub-MCh models compared to near-MCh models. Last, the total flux in lines of Ni is found to correlate strongly with the stable nickel yield, although ionisation effects can bias the inferred abundance. Our models suggest that key physical ingredients are missing from either the explosion models, or the radiative-transfer post-processing, or both. Nonetheless, they also show the potential of the near- and mid-infrared to uncover new spectroscopic diagnostics of SN Ia explosion mechanisms. Description: We carried out calculations of collisional cross-sections for electron-impact excitation of NiIII. We report transition probabilities (Aul) and effective collision strengths (Υlu) in the temperature range 1000-100000K. Entries for transitions among the lowest eight levels for temperatures ≤40000K were computed following the methods outlined in Storey et al. (2016MNRAS.456.1974S 2016MNRAS.456.1974S, Cat. VI/148). All other entries are based on Ramsbottom et al. (2007A&A...475..765R 2007A&A...475..765R, Cat. J/A+A/475/765); in this latter approach, transition probabilities less than 10-10s-1 are deemed too small to be significant and we set these to an arbitrarily small value 10-30s-1. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablef1.dat 20 43 Level indexing for NiIII used in tablef2.dat tablef2.dat 185 903 Transition probabilities and collision strengths -------------------------------------------------------------------------------- See also: VI/148 : Collision Strengths for [Co II] Forbidden Lines - SS4 (Storey+, 2016) J/A+A/475/765 : Fine structure forbidden lines in FeII (Ramsbottom+, 2007) Byte-by-byte Description of file: tablef1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Index [1/43] Level index 4- 20 A17 --- Level Level name -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablef2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- l [1/42] Lower level index 4- 5 I2 --- u [2/43] Upper level index 7- 14 E8.3 s-1 Aul Transition probability (Einstein A value) 16- 23 E8.3 --- ups1.0e3 Effective collision strength at T=1.0e+3K 25- 32 E8.3 --- ups1.5e3 Effective collision strength at T=1.5e+3K 34- 41 E8.3 --- ups1.8e3 Effective collision strength at T=1.8e+3K 43- 50 E8.3 --- ups2.0e3 Effective collision strength at T=2.0e+3K 52- 59 E8.3 --- ups2.5e3 Effective collision strength at T=2.5e+3K 61- 68 E8.3 --- ups5.0e3 Effective collision strength at T=5.0e+3K 70- 77 E8.3 --- ups7.5e3 Effective collision strength at T=7.5e+3K 79- 86 E8.3 --- ups1.0e4 Effective collision strength at T=1.0e+4K 88- 95 E8.3 --- ups1.5e4 Effective collision strength at T=1.5e+4K 97-104 E8.3 --- ups1.8e4 Effective collision strength at T=1.8e+4K 106-113 E8.3 --- ups2.0e4 Effective collision strength at T=2.0e+4K 115-122 E8.3 --- ups3.0e4 Effective collision strength at T=3.0e+4K 124-131 E8.3 --- ups4.0e4 Effective collision strength at T=4.0e+4K 133-140 E8.3 --- ups5.0e4 Effective collision strength at T=5.0e+4K 142-149 E8.3 --- ups6.0e4 Effective collision strength at T=6.0e+4K 151-158 E8.3 --- ups7.0e4 Effective collision strength at T=7.0e+4K 160-167 E8.3 --- ups8.0e4 Effective collision strength at T=8.0e+4K 169-176 E8.3 --- ups9.0e4 Effective collision strength at T=9.0e+4K 178-185 E8.3 --- ups1.0e5 Effective collision strength at T=1.0e+5K -------------------------------------------------------------------------------- Acknowledgements: Stephane Blondim, stephane.blondin(at)lam.fr
(End) Patricia Vannier [CDS] 29-Aug-2023
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