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Sebastian T. Ohlmann

Identifiers

  • name variant Sebastian T. Ohlmann 0.60 · backfill

Papers (18)

  1. Optimizing Distributed Tensor Contractions using Node-Aware Processor Grids cs.DC · 2023 · author #3
  2. Collisions of red giants in galactic nuclei astro-ph.HE · 2023 · author #4
  3. Gravitational wave emission from dynamical stellar interactions astro-ph.HE · 2023 · author #4
  4. From 3D hydrodynamic simulations of common-envelope interaction to gravitational-wave mergers astro-ph.SR · 2021 · author #4
  5. Octopus, a computational framework for exploring light-driven phenomena and quantum dynamics in extended and finite systems physics.comp-ph · 2019 · author #25
  6. How mergers magnetise massive stars astro-ph.SR · 2019 · author #2
  7. Hydrodynamical moving-mesh simulations of the tidal disruption of stars by supermassive black holes astro-ph.HE · 2019 · author #3
  8. Simulating the observed diversity of Type Ia supernovae - Introducing a model data base astro-ph.HE · 2017 · author #2
  9. Constructing stable 3D hydrodynamical models of giant stars astro-ph.SR · 2016 · author #1
  10. Neutrinos from type Ia supernovae: The gravitationally confined detonation scenario astro-ph.HE · 2016 · author #3
  11. Magnetic Field Amplification During the Common Envelope Phase astro-ph.SR · 2016 · author #1
  12. Three-dimensional simulations of gravitationally confined detonations compared to observations of SN 1991T astro-ph.SR · 2016 · author #3
  13. Hydrodynamic moving-mesh simulations of the common envelope phase in binary stellar systems astro-ph.SR · 2015 · author #1
  14. Neutrino and gravitational wave signal of a delayed-detonation model of Type Ia supernovae astro-ph.SR · 2015 · author #5
  15. Type Ia supernovae from exploding oxygen-neon white dwarfs astro-ph.SR · 2015 · author #5
  16. Improving the convergence properties of the moving-mesh code AREPO astro-ph.GA · 2015 · author #6
  17. The origin of the cosmic gamma-ray background in the MeV range astro-ph.HE · 2015 · author #7
  18. The white dwarf's carbon fraction as a secondary parameter of Type Ia supernovae astro-ph.SR · 2014 · author #1

Mentions

  • 2307.07338 #4 · arxiv_oai · confidence 0.70 Sebastian T. Ohlmann
  • 2307.08829 #3 · arxiv_oai · confidence 0.70 Sebastian T. Ohlmann
  • 2303.05519 #4 · arxiv_oai · confidence 0.70 Sebastian T. Ohlmann
  • 2111.12112 #4 · arxiv_oai · confidence 0.70 Sebastian T. Ohlmann
  • 1912.07921 #25 · arxiv_oai · confidence 0.70 Sebastian T. Ohlmann
  • 1910.14058 #2 · arxiv_oai · confidence 0.70 Sebastian T. Ohlmann
  • 1902.08202 #3 · arxiv_oai · confidence 0.70 Sebastian T. Ohlmann
  • 1706.09879 #2 · arxiv_oai · confidence 0.70 Sebastian T. Ohlmann
  • 1609.07403 #3 · arxiv_oai · confidence 0.70 Sebastian T. Ohlmann
  • 1612.00008 #1 · arxiv_oai · confidence 0.70 Sebastian T. Ohlmann
  • 1606.00089 #3 · arxiv_oai · confidence 0.70 Sebastian T. Ohlmann
  • 1607.05996 #1 · arxiv_oai · confidence 0.70 Sebastian T. Ohlmann
  • 1502.06116 #7 · arxiv_oai · confidence 0.70 Sebastian T. Ohlmann
  • 1511.02542 #5 · arxiv_oai · confidence 0.70 Sebastian T. Ohlmann
  • 1512.04529 #1 · arxiv_oai · confidence 0.70 Sebastian T. Ohlmann
  • 1503.00562 #6 · arxiv_oai · confidence 0.70 Sebastian T. Ohlmann
  • 1506.05809 #5 · arxiv_oai · confidence 0.70 Sebastian T. Ohlmann
  • 1409.2866 #1 · arxiv_oai · confidence 0.70 Sebastian T. Ohlmann
  • 1511.02542 #5 · backfill · confidence 0.70 Sebastian T. Ohlmann
  • 1506.05809 #5 · backfill · confidence 0.70 Sebastian T. Ohlmann
  • 1503.00562 #6 · backfill · confidence 0.70 Sebastian T. Ohlmann
  • 1502.06116 #7 · backfill · confidence 0.70 Sebastian T. Ohlmann
  • 1409.2866 #1 · backfill · confidence 0.70 Sebastian T. Ohlmann

Frequent Coauthors