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Mathematical Models and Computer Simulations

Erschienen in:

01.08.2022

Simulation of SN2009ip Bolometric Light Curves

verfasst von: E. Urvachev, S. Glazyrin

Erschienen in: Mathematical Models and Computer Simulations | Ausgabe 4/2022

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Abstract

The direct method for determining cosmological distances uses observations at the growth stage of the luminosity of superluminous supernovae, whose light curve can be explained by the interaction of a shock wave with dense circumstellar matter. The method is based on the assumption of spherical symmetry of the dense thin layer formed in the system, which can be unstable in a multidimensional model. In this paper, we consider the simulation of the supernova SN2009ip, which has been successfully applied for the direct method, using the radiation-hydrodynamics code, FRONT. It is shown that the current implementation of the code correctly reproduces the bolometric light curve and the dynamics of the dense shell’s motion in a simplified SN2009ip model. It is also shown that in the formulation under consideration, the shell remains spherically symmetric at least during the growth period of the light curve.

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D. Branch and G. A. Tammann, “Type Ia supernovae as standard candles,” Annu. Rev. Astron. Astrophys. 30, 359–389 (1992). https://doi.org/10.1146/annurev.aa.30.090192.002043CrossRef

S. Blinnikov, M. Potashov, P. Baklanov, and A. Dolgov, “Direct determination of the Hubble parameter using type IIn supernovae,” JETP Lett. 96 (3), 153–157 (2012). https://doi.org/10.1134/S0021364012150039CrossRef

P. V. Baklanov, S. I. Blinnikov, M. Sh. Potashov, and A. D. Dolgov, “Study of supernovae important for cosmology,” JETP Lett. 98 (7), 432–439 (2013). https://doi.org/10.1134/S0021364013200034CrossRef

E. K. Grasberg and D. K. Nadezhin, “Type II supernovae—Two successive explosions?” Sov. Astron. Lett. 12 (1), 68–70 (1986).

N. N. Chugai, S. I. Blinnikov, R. J. Cumming, P. Lundqvist, A. Bragaglia, A. V. Filippenko, D. C. Leonard, T. Matheson, and J. Sollerman, “The Type IIn supernova 1994W: evidence for the explosive ejection of a circumstellar envelope,” Mon. Not. R. Astron. Soc. 352 (4), 1213–1231 (2004). https://doi.org/10.1111/j.1365-2966.2004.08011.xCrossRef

S. E. Woosley, S. Blinnikov, and A. Heger, “Pulsational pair instability as an explanation for the most luminous supernovae,” Nature 450 (7168), 390–392 (2007). https://doi.org/10.1038/nature06333CrossRef

R. A. Chevalier and C. M. Irwin, “Shock breakout in dense mass loss: luminous supernovae,” Astrophys. J. Lett. 729 (1), L6 (2011). https://doi.org/10.1088/2041-8205/729/1/L6CrossRef

E. Sorokina, S. Blinnikov, K. Nomoto, R. Quimby, and A. Tolstov, “Type I superluminous supernovae as explosions inside non-hydrogen circumstellar envelopes,” Astrophys. J. 829 (1), 17 (2016). https://doi.org/10.3847/0004-637X/829/1/17CrossRef

T. J. Moriya, E. I. Sorokina, and R. A. Chevalier, “Superluminous supernovae,” Space Sci. Rev. 214 (2), 59 (2018). https://doi.org/10.1007/s11214-018-0493-6CrossRef

10.

R. Chevalier and J. M. Blondin, “Hydrodynamic instabilities in supernova remnants: Early radiative cooling,” Astrophys. J. 444, 312–317 (1995). https://doi.org/10.1086/175606CrossRef

11.

D. A. Badjin, S. I. Glazyrin, K. V. Manukovskiy, and S. I. Blinnikov, “On physical and numerical instabilities arising in simulations of non-stationary radiatively cooling shocks,” Mon. Not. R. Astron. Soc. 459 (2), 2188–2211 (2016). https://doi.org/10.1093/mnras/stw790CrossRef

12.

D. A. Badjin and S. I. Glazyrin, “Physical and numerical instabilities of radiatively cooling shocks in turbulent magnetized media,” Mon. Not. R. Astron. Soc. 507 (1), 1492–1512 (2021). https://doi.org/10.1093/mnras/stab2318CrossRef

13.

S. I. Glazyrin, “Investigation of burning in type Ia supernovae,” Astron. Lett. 39 (4), 221–226 (2013). https://doi.org/10.1134/S1063773713040026CrossRef

14.

E. Urvachev, D. Shidlovski, N. Tominaga, S. Glazyrin, and S. Blinnikov, “The simulation of superluminous supernovae using the M1 approach for radiation transfer,” Astrophys. J. Suppl. Ser. 256 (1), 8 (2021). https://doi.org/10.3847/1538-4365/ac0972CrossRef

15.

M. Potashov, S. Blinnikov, P. Baklanov, and A. Dolgov, “Direct distance measurements to SN 2009ip,” Mon. Not. R. Astron. Soc.: Lett. 431 (1), L98–L101 (2013). https://doi.org/10.1093/mnrasl/slt016CrossRef

16.

N. M. H. Vaytet, E. Audit, B. Dubroca, and F. Delahaye, “A numerical model for multigroup radiation hydrodynamics,” J. Quant. Spectrosc. Radiat. Transfer 112 (8), 1323–1335 (2011). https://doi.org/10.1016/j.jqsrt.2011.01.027CrossRef

17.

M. A. Skinner, J. C. Dolence, A. Burrows, D. Radice, and D. Vartanyan, “Fornax: A flexible code for multiphysics astrophysical simulations,” Astrophys. J. Suppl. Ser. 241 (1), 7 (2019). https://doi.org/10.3847/1538-4365/ab007fCrossRef

18.

M. González, E. Audit, and P. Huynh, “HERACLES: a three-dimensional radiation hydrodynamics code,” Astron. Astrophys. 464 (2), 429–435 (2007). https://doi.org/10.1051/0004-6361:20065486CrossRef

19.

M. R. Krumholz, R. I. Klein, and C. F. McKee, “Radiation-hydrodynamic simulations of collapse and fragmentation in massive protostellar cores,” Astrophys. J. 656 (2), 959–979 (2007). https://doi.org/10.1086/510664CrossRef

20.

C. D. Levermore, “Relating Eddington factors to flux limiters,” J. Quant. Spectrosc. Radiat. Transfer 31 (2), 149–160 (1984). https://doi.org/10.1016/0022-4073(84)90112-2CrossRef

21.

B. Dubroca and J.-L. Feugeas, “Etude théorique et numérique d’une hiérarchie de modèles aux moments pour le transfert radiatif,” C. R. Acad. Sci., Ser. I: Math. 329 (10), 915–920 (1999). https://doi.org/10.1016/S0764-4442(00)87499-6CrossRefMATH

22.

O. Just, M. Obergaulinger, and H.-T. Janka, “A new multidimensional, energy-dependent two-moment transport code for neutrino-hydrodynamics,” Mon. Not. R. Astron. Soc. 453 (4), 3386–3413 (2015). https://doi.org/10.1093/mnras/stv1892CrossRef

23.

D. Mihalas and B. Weibel-Mihalas, Foundations of Radiation Hydrodynamics (Oxford Univ. Press, New York, 1984).MATH

24.

E. F. Toro, Riemann Solvers and Numerical Methods for Fluid Dynamics: A Practical Introduction (Springer, New York, 2013).

25.

M. A. Skinner and E. C. Ostriker, “A two-moment radiation hydrodynamics module in Athena using a time-explicit Godunov method,” Astrophys. J. Suppl. Ser. 206 (2), 21 (2013). https://doi.org/10.1088/0067-0049/206/2/21CrossRef

26.

S. I. Blinnikov, R. Eastman, O. S. Bartunov, V. A. Popolitov, and S. E. Woosley, “A comparative modeling of supernova 1993J,” Astrophys. J. 496 (1), 454–472 (1998). https://doi.org/10.1086/305375CrossRef

27.

N. Roth and D. Kasen, “Monte Carlo radiation-hydrodynamics with implicit methods,” Astrophys. J. Suppl. Ser. 217 (1), 9 (2015). https://doi.org/10.1088/0067-0049/217/1/9CrossRef

28a.

I. Hubeny and A. Burrows, “A new algorithm for 2-D transport for astrophysical simulations: I. General formulation and tests for the 1-D spherical case,” arXiv preprint arXiv:astro-ph/0609049 (2006);

28b.

Astrophys. J. 659 (2), 1458–1487 (2007). https://doi.org/10.1086/512179

29.

J. M. Ferguson, J. E. Morel, and R. Lowrie, “The equilibrium-diffusion limit for radiation hydrodynamics,” J. Quant. Spectrosc. Radiat. Transfer 202, 176–186 (2017). https://doi.org/10.1016/j.jqsrt.2017.07.031CrossRef

30.

W. Zhang, L. Howell, A. Almgren, A. Burrows, J. Dolence, and J. Bell, “CASTRO: a new compressible astrophysical solver. III. Multigroup radiation hydrodynamics,” Astrophys. J. Suppl. Ser. 204 (1), 7 (2013). https://doi.org/10.1088/0067-0049/204/1/7CrossRef

31.

R. Teyssier, “Grid-based hydrodynamics in astrophysical fluid flows,” Annu. Rev. Astron. Astrophys. 53, 325–364 (2015). https://doi.org/10.1146/annurev-astro-082214-122309CrossRef

32.

S. I. Blinnikov, F. K. Röpke, E. I. Sorokina1, M. Gieseler, M. Reinecke, C. Travaglio, W. Hillerbrandt, and M. Stritzinger, “Theoretical light curves for deflagration models of type Ia supernova,” Astron. Astrophys. 453 (1), 229–240 (2006). https://doi.org/10.1051/0004-6361:20054594CrossRef

Titel: Simulation of SN2009ip Bolometric Light Curves
verfasst von: E. Urvachev
S. Glazyrin
Publikationsdatum: 01.08.2022
Verlag: Pleiades Publishing
Erschienen in: Mathematical Models and Computer Simulations / Ausgabe 4/2022
Print ISSN: 2070-0482
Elektronische ISSN: 2070-0490
DOI: https://doi.org/10.1134/S2070048222040135

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