Daniel Kresse
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View article: Evidence of polar and ultralow supernova kicks from the orbits of Be X-ray binaries
Evidence of polar and ultralow supernova kicks from the orbits of Be X-ray binaries Open
Supernovae, the explosive deaths of massive stars, create heavy elements and form black holes and neutron stars. These compact objects often receive a velocity at formation, a "kick" whose physical origin remains debated. We investigate ki…
View article: Interplay between neutrino kicks and hydrodynamic kicks of neutron stars and black holes
Interplay between neutrino kicks and hydrodynamic kicks of neutron stars and black holes Open
Neutron stars (NSs) are observed with high space velocities and elliptical orbits in binaries. The magnitude of these effects points to natal kicks that originate from asymmetries during the supernova (SN) explosions. Using a growing set o…
View article: Constraints on Neutrino Natal Kicks from Black-Hole Binary VFTS 243
Constraints on Neutrino Natal Kicks from Black-Hole Binary VFTS 243 Open
The recently reported observation of VFTS 243 is the first example of a massive black-hole binary system with negligible binary interaction following black-hole formation. The black-hole mass (≈10M⊙) and near-circular orbit (e≈0.02) of VFT…
View article: Interplay Between Neutrino Kicks and HydrodynamicKicks of Neutron Stars and Black Holes
Interplay Between Neutrino Kicks and HydrodynamicKicks of Neutron Stars and Black Holes Open
Neutron stars (NSs) are observed with high space velocities and elliptical orbits in binaries. The magnitude of these effects points to natal kicks that originate from asymmetries during the supernova (SN) explosions. Using a growing set o…
View article: Interplay Between Neutrino Kicks and Hydrodynamic Kicks of Neutron Stars and Black Holes
Interplay Between Neutrino Kicks and Hydrodynamic Kicks of Neutron Stars and Black Holes Open
Neutron stars (NSs) are observed with high space velocities and elliptical orbits in binaries. The magnitude of these effects points to natal kicks that originate from asymmetries during the supernova (SN) explosions. Using a growing set o…
View article: Production of <sup>44</sup>Ti and Iron-group Nuclei in the Ejecta of 3D Neutrino-driven Supernovae
Production of <sup>44</sup>Ti and Iron-group Nuclei in the Ejecta of 3D Neutrino-driven Supernovae Open
The radioactive isotopes 44 Ti and 56 Ni are important products of explosive nucleosynthesis, which play a key role in supernova (SN) diagnostics and have been detected in several nearby young SN remnants. However, most SN models based on …
View article: Constraints on neutrino natal kicks from black-hole binary VFTS 243
Constraints on neutrino natal kicks from black-hole binary VFTS 243 Open
The recently reported observation of VFTS 243 is the first example of a massive black-hole binary system with negligible binary interaction following black-hole formation. The black-hole mass ($\approx 10\ M_{\odot}$) and near-circular orb…
View article: Production of 44Ti and iron-group nuclei in the ejecta of 3D neutrino-driven supernovae
Production of 44Ti and iron-group nuclei in the ejecta of 3D neutrino-driven supernovae Open
The radioactive isotopes of 44Ti and 56Ni are important products of explosive nucleosynthesis, which play a key role for supernova (SN) diagnostics and were detected in several nearby young SN remnants. However, most SN models based on non…
View article: Low-luminosity type IIP supermnovae: SN 2005cs and SN 2020cxd as very low-energy iron core-collapse explosions
Low-luminosity type IIP supermnovae: SN 2005cs and SN 2020cxd as very low-energy iron core-collapse explosions Open
SN 2020cxd is a representative of the family of low-energy, underluminous Type IIP supernovae (SNe), whose observations and analysis were recently reported by Yang et al. (2021). Here, we re-evaluate the observational data for the diagnost…
View article: Detecting the diffuse supernova neutrino background in the future water-based liquid scintillator detector Theia
Detecting the diffuse supernova neutrino background in the future water-based liquid scintillator detector Theia Open
A large-scale neutrino observatory based on Water-based Liquid Scintillator\n(WbLS) will be excellently suited for a measurement of the Diffuse Supernova\nNeutrino Background (DSNB). The WbLS technique offers high signal efficiency\nand ef…
View article: Three-dimensional models of core-collapse supernovae from low-mass progenitors with implications for Crab
Three-dimensional models of core-collapse supernovae from low-mass progenitors with implications for Crab Open
We present 3D full-sphere supernova simulations of non-rotating low-mass (∼9 M⊙) progenitors, covering the entire evolution from core collapse through bounce and shock revival, through shock breakout from the stellar surface, until fallbac…
View article: Neutrino emission characteristics of black hole formation in three-dimensional simulations of stellar collapse
Neutrino emission characteristics of black hole formation in three-dimensional simulations of stellar collapse Open
Neutrinos are unique probes of core-collapse supernova dynamics, especially\nin the case of black hole (BH) forming stellar collapses, where the\nelectromagnetic emission may be faint or absent. By investigating two 3D\nhydrodynamical simu…