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The Astrophysical Journal, ISSN 0004-637X, 01/2010, Volume 708, Issue 2, pp. 1025 - 1031
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 10/2006, Volume 649, Issue 2 I, pp. 939 - 953
We undertake a theoretical study of the near-infrared (NIR) light curves of Type Ia supernovae (SNe Ia). In these bands, the light curves are distinguished by... 
Supernovae: general | Radiative transfer | LUMINOSITY | HUBBLE DIAGRAM | radiative transfer | OPACITY | EXPLOSION | supernovae : general | SN 1994D | PHOTOMETRY | ASTRONOMY & ASTROPHYSICS | DETONATION | SIMULATIONS | SPECTRA | WHITE-DWARF MODELS
Journal Article
Nature, ISSN 0028-0836, 10/2013, Volume 502, Issue 7471, pp. 310 - 312
The origin of ordinary supernovae has been agreed on for decades; the most common events occur when a moderately massive star (one of around 10-20 solar... 
Magnitudes | Spectra | Supernovae | Observations | Stars | Neutron stars | Astrophysics | Chemical elements | Stars & galaxies
Journal Article
Nature, ISSN 0028-0836, 11/2017, Volume 551, Issue 7679, pp. 210 - 213
Journal Article
Nature, ISSN 0028-0836, 07/2010, Volume 466, Issue 7302, pp. 37 - 38
[...] at least now, observations and theory both suggest that much of the common variation is due to asymmetry17. Because supernovae are randomly oriented with... 
Explosions | Supernovae | Asymmetry | Stars & galaxies | Astronomy
Journal Article
Nature, ISSN 0028-0836, 2013, Volume 502, Issue 7471, pp. 310 - 312
Journal Article
Astrophysical Journal, Supplement Series, ISSN 0067-0049, 03/2015, Volume 217, Issue 1
We explore the application of Monte Carlo transport methods to solving coupled radiation-hydrodynamics (RHD) problems. We use a time-dependent,... 
RADIANT HEAT TRANSFER | TENSORS | MONTE CARLO METHOD | RADIATIVE COOLING | HYDRODYNAMICS | LAGRANGIAN FUNCTION | RELATIVISTIC RANGE | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | ASTROPHYSICS | FREQUENCY DEPENDENCE | RADIATION PRESSURE | TIME DEPENDENCE | RADIATION TRANSPORT | SCATTERING
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 01/2018, Volume 852, Issue 2, p. L33
There are two classes of viable progenitors for normal Type Ia supernovae (SNe Ia): systems in which a white dwarf explodes at the Chandrasekhar mass (M-ch),... 
supernovae: general | ACCRETING WHITE-DWARFS | PROGENITORS | EVOLUTION | ASTRONOMY & ASTROPHYSICS | BINARIES | OPACITY | EXPLOSION | SYSTEMS | LIGHT CURVES | PHYSICS | DETONATIONS | Physics - High Energy Astrophysical Phenomena
Journal Article