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SN 2019nyk: A rapidly declining Type II supernova with early interaction signatures
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Various challenges in numerical simulation of three-dimensional multi-physics and multi-material problems under extreme 条件
SN 2024ggi in NGC 3621: Rising Ionization in a Nearby, Circumstellar-material-interacting Type II Supernova
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Mapping a Lower Limit on the Mass Fraction of the Cold Neutral Medium Using Fourier-transformed H i 21 cm Emission Line Spectra: Application to the DRAO Deep Field from DHIGLS and the HI4PI Survey
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Late-end reionization with aton-he: towards constraints from Ly α emitters observed with JWST
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SN 2023ixf in Messier 101: Photo-ionization of Dense, Close-in Circumstellar Material in a Nearby Type II Supernova
W. V. Jacobson-Galán, L. Dessart, R. Margutti, R. Chornock, R. J. Foley, C. D. Kilpatrick, D. O. Jones, K. Taggart, C. R. Angus, S. Bhattacharjee, L. A. Braff, D. Brethauer, A. J. Burgasser, F. Cao, C. M. Carlile, K. C. Chambers, D. A. Coulter, E. Dominguez-Ruiz, C. B. Dickinson, T. de Boer, A. Gagliano, C. Gall, H. Gao, E. L. Gates, S. Gomez, et al. The Astrophysical Journal Letters 954(2) L42 (2023) https://doi.org/10.3847/2041-8213/acf2ec
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W. V. Jacobson-Galán, L. Dessart, D. O. Jones, R. Margutti, D. L. Coppejans, G. Dimitriadis, R. J. Foley, C. D. Kilpatrick, D. J. Matthews, S. Rest, G. Terreran, P. D. Aleo, K. Auchettl, P. K. Blanchard, D. A. Coulter, K. W. Davis, T. J. L. de Boer, L. DeMarchi, M. R. Drout, N. Earl, A. Gagliano, C. Gall, J. Hjorth, M. E. Huber, A. L. Ibik, et al. The Astrophysical Journal 924(1) 15 (2022) https://doi.org/10.3847/1538-4357/ac3f3a
VETTAM: a scheme for radiation hydrodynamics with adaptive mesh refinement using the variable Eddington tensor method
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Multigroup Radiation Magnetohydrodynamics Based on Discrete Ordinates including Compton Scattering
General Relativistic Radiation Magnetohydrodynamics Simulations of Black Hole Accretion Disks: Comparison of Methods Based on Variable Eddington Tensor and Based on M1 Closure
The Early Discovery of SN 2017ahn: Signatures of Persistent Interaction in a Fast-declining Type II Supernova
L. Tartaglia, D. J. Sand, J. H. Groh, S. Valenti, S. D. Wyatt, K. A. Bostroem, P. J. Brown, S. Yang, J. Burke, T.-W. Chen, S. Davis, F. Förster, L. Galbany, J. Haislip, D. Hiramatsu, G. Hosseinzadeh, D. A. Howell, E. Y. Hsiao, S. W. Jha, V. Kouprianov, H. Kuncarayakti, J. D. Lyman, C. McCully, M. M. Phillips, A. Rau, et al. The Astrophysical Journal 907(1) 52 (2021) https://doi.org/10.3847/1538-4357/abca8a
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Global 3D radiation hydrodynamic simulations of proto-Jupiter’s convective envelope
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The origins and impact of outflow from super-Eddington flow
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Simulating dust grain-radiation coupling on a moving mesh
Ryan McKinnon, Rahul Kannan, Mark Vogelsberger, et al. Monthly Notices of the Royal Astronomical Society 502(1) 1344 (2021) https://doi.org/10.1093/mnras/stab021
An Implicit Finite Volume Scheme to Solve the Time-dependent Radiation Transport Equation Based on Discrete Ordinates
Smoothed particle radiation hydrodynamics: two-moment method with local Eddington tensor closure
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Moving-mesh radiation-hydrodynamic simulations of wind-reprocessed transients
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Time-dependent radiation hydrodynamics on a moving mesh
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A Novel multidimensional Boltzmann neutrino transport scheme for core-collapse supernovae
arepo-rt: radiation hydrodynamics on a moving mesh
Rahul Kannan, Mark Vogelsberger, Federico Marinacci, et al. Monthly Notices of the Royal Astronomical Society 485(1) 117 (2019) https://doi.org/10.1093/mnras/stz287
CAFE-R: A Code That Solves the Special Relativistic Radiation Hydrodynamics Equations
Photoevaporation of Jeans-unstable molecular clumps
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A Radiative Transfer Module for Relativistic Magnetohydrodynamics in the PLUTO Code
Igor Kulikov, Igor Chernykh, Vitaly Vshivkov, et al. Communications in Computer and Information Science, Supercomputing 965 414 (2019) https://doi.org/10.1007/978-3-030-05807-4_35
Impact of the reduced speed of light approximation on the post-overlap neutral hydrogen fraction in numerical simulations of the epoch of reionization
Direct Collapse to Supermassive Black Hole Seeds with Radiative Transfer: Isolated Halos
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Super-luminous Type II supernovae powered by magnetars