activity
20232026
most citedPre-supernova evolution and final fate of stellar mergers and accretors of binary mass transfer

50 citations · 154 across the 16 of their papers we have counts for

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7 papers · 1 filter

astro-ph.HE2025

New gravitational-wave data support a bimodal black-hole mass distribution

R. Willcox, F. R. N. Schneider, E. Laplace +7

Detailed stellar evolution and supernova models yield a bimodal black-hole mass distribution with a narrow peak around 10 solar masses from stars within a narrow range of progenito…

astro-ph.HE2025★ 4 cited

Pulsations change the structures of massive stars before explosion: interpreting SN 2023ixf and SN 2024ggi

Eva Laplace, Vincent A. Bronner, Fabian R. N. Schneider +1

Massive red supergiants (RSGs) are known to become hydrodynamically unstable before they explode. Still, the vast majority of supernova (SN) models assume RSG progenitors in hydros…

astro-ph.HE2025★ 8 cited

Supernovae from stellar mergers and accretors of binary mass transfer: Implications for Type IIP, 1987A-like and interacting supernovae

F. R. N. Schneider, E. Laplace, Ph. Podsiadlowski

As most massive stars are born in binary and other multiple-star systems, many are expected to exchange mass with a companion star or merge with it during their lives. This means t…

astro-ph.HE2025

Supernova-induced binary-interaction-powered supernovae: a model for SN2022jli

Ryosuke Hirai, Philipp Podsiadlowski, Peter Hoeflich +4

We present 3D hydrodynamical modelling of supernova-induced binary-interaction-powered supernovae; a scenario proposed for the peculiar type Ic supernova SN2022jli. In this scenari…

astro-ph.HE2024★ 11 cited

Neutron star kicks plus rockets as a mechanism for forming wide low-eccentricity neutron star binaries

Ryosuke Hirai, Philipp Podsiadlowski, Alexander Heger +1

Recent neutron star surface observations corroborate a long-standing theory that neutron stars may be accelerated over extended periods after their birth. We analyze how these prol…

astro-ph.HE2023★ 12 cited

An upper limit on the spins of merging binary black holes formed through binary evolution

Pablo Marchant, Philipp Podsiadlowski, Ilya Mandel

As gravitational wave detectors improve, observations of black hole (BH) mergers will provide the joint distribution of their masses and spins. This will be a critical benchmark to…

astro-ph.HE2023★ 26 cited

Evolution and final fate of massive post-common-envelope binaries

Dandan Wei, Fabian R. N. Schneider, Philipp Podsiadlowski +3

Mergers of neutron stars (NSs) and black holes (BHs) are nowadays observed routinely thanks to gravitational-wave (GW) astronomy. In the isolated binary-evolution channel, a common…