activity
20182025
most citedNeutron Star Mergers Might not be the Only Source of r-Process Elements in the Milky Way

248 citations · 564 across the 16 of their papers we have counts for

collaborators

17 papers

astro-ph.HE2025★ 1 cited

Complete survey of r-process conditions: the (un-)robustness of the r-process(-es)

Jan Kuske, Almudena Arcones, Moritz Reichert

Heavy elements are synthesized by the r-process in neutron star mergers and potentially in rare supernovae linked to strong magnetic fields. Expensive hydrodynamic simulations of t…

astro-ph.SR2024★ 13 cited

Chemical Evolution of R-process Elements in Stars (CERES): IV. An observational run-up of the third r-process peak with Hf, Os, Ir, and Pt

Arthur Alencastro Puls, Jan Kuske, Camilla Juul Hansen +8

The third r-process peak (Os, Ir, Pt) is poorly understood due to observational challenges, with spectral lines located in the blue or near-ultraviolet region of stellar spectra. T…

astro-ph.SR2024★ 4 cited

Evolving massive stars to core collapse with GENEC: Extension of equation of state, opacities and effective nuclear network

Adam Griffiths, Miguel-Á Aloy, Raphael Hirschi +6

Stars with initial mass above roughly 8 solar masses will evolve to form a core made of iron group elements at which point no further exothermic nuclear reactions between charged n…

astro-ph.SR2024★ 2 cited

Do not forget the electrons: Extending moderately-sized nuclear networks for multidimensional hydrodynamic codes

Domingo García-Senz, Rubén M. Cabezón, Moritz Reichert +5

We present here an extended nuclear network, with 90 species, designed for being coupled with hydrodynamic simulations, which includes neutrons, protons, electrons, positrons, and…

astro-ph.HE2024

Nucleosynthesis in magnetorotational supernovae: impact of the magnetic field configuration

M. Reichert, M. Bugli, J. Guilet +3

The production of heavy elements is one of the main by-products of the explosive end of massive stars. A long sought goal is finding differentiated patterns in the nucleosynthesis…

astro-ph.IM2023★ 1 cited

The nuclear reaction network WinNet

M. Reichert, C. Winteler, O. Korobkin +13

We present the state-of-the-art single-zone nuclear reaction network WinNet that is capable of calculating the nucleosynthetic yields of a large variety of astrophysical environmen…

astro-ph.HE2023★ 4 cited

Nucleosynthesis in jet-driven and jet-associated supernovae

M. Obergaulinger, M. Reichert

In contrast to regular core-collapse supernovae, explosions of rapidly rotating massive stars can develop jets, fast collimated outflows directed along the rotational axis. Dependi…

astro-ph.HE2022★ 18 cited

Core-collapse supernova simulations with reduced nucleosynthesis networks

Gerard Navó, Moritz Reichert, Martin Obergaulinger +1

We present core-collapse supernova simulations including nuclear reaction networks that impact explosion dynamics and nucleosynthesis. The different composition treatment can lead…

astro-ph.GA2022★ 27 cited

Chemical Evolution of R-process Elements in Stars (CERES). I. Stellar parameters and chemical abundances from Na to Zr

Linda Lombardo, Piercarlo Bonifacio, Patrick François +10

Aims. The Chemical Evolution of R-process Elements in Stars (CERES) project aims to provide a homogeneous analysis of a sample of metal-poor stars ([Fe/H]<-1.5). We present the ste…

astro-ph.HE2022★ 75 cited

Magnetorotational supernovae: A nucleosynthetic analysis of sophisticated 3D models

Moritz Reichert, Martin Obergaulinger, Miguel-Angel Aloy +3

Magnetorotational supernovae are a rare type of core-collapse supernovae where the magnetic field and rotation play a central role in the dynamics of the explosion. We present the…

astro-ph.HE2021★ 21 cited

Post-explosion evolution of core-collapse supernovae

M. Witt, A. Psaltis, H. Yasin +6

We investigate the post-explosion phase in core-collapse supernovae with 2D hydrodynamical simulations and a simple neutrino treatment. The latter allows us to perform 46 simulatio…

astro-ph.GA2021★ 34 cited

Evolution of neutron capture elements in dwarf galaxies

Marta Molero, Donatella Romano, Moritz Reichert +6

We study the evolution of Eu and Ba abundances in local group dwarf spheroidal and ultra faint dwarf galaxies by means of detailed chemical evolution models and compare our results…

astro-ph.GA2021★ 23 cited

Extreme r-process enhanced stars at high metallicity in Fornax

M. Reichert, C. J. Hansen, A. Arcones

We present and discuss three extremely r-process enhanced stars located in the massive dwarf spheriodal galaxy Fornax. These stars are very unique with an extreme Eu enrichment ($1…

astro-ph.HE2020★ 66 cited

Nucleosynthesis in magneto-rotational supernovae

Moritz Reichert, Martin Obergaulinger, Marius Eichler +2

We present the nucleosynthesis of magneto-rotational supernovae (MR-SNe) including neutrino-driven and magneto-rotational-driven ejecta based, for the first time, on 2D simulations…

astro-ph.SR2020★ 2 cited

An empirical metallicity tracer in CEMP and C-normal stars

D. Singh, C. J. Hansen, J. S. Byrgesen +2

Deriving the metallicity, [Fe/H], in low-resolution spectra of carbon-enhanced metal-poor (CEMP) stars is a tedious task that, owing to the large number of line blends, often leads…

astro-ph.GA2018★ 25 cited

Unusual neutron-capture nucleosynthesis in a carbon-rich Galactic bulge star

A. Koch, M. Reichert, C. J. Hansen +4

Metal-poor stars in the Galactic halo often show strong enhancements in carbon and/or neutron-capture elements. However, the Galactic bulge is notable for its paucity of carbon-enh…

astro-ph.HE2018★ 248 cited

Neutron Star Mergers Might not be the Only Source of r-Process Elements in the Milky Way

Benoit Côté, Marius Eichler, Almudena Arcones +8

Probing the origin of r-process elements in the universe represents a multi-disciplinary challenge. We review the observational evidence that probe the properties of r-process site…