Results 111 to 120 of about 622,972 (290)
Nuclear input for core-collapse models
Nuclear Physics A, 2006 37 pages, 11 figures, for special issue of Nucl.
Martinez-Pinedo, Gabriel +2 more
openaire +3 more sources
3D‐Printed Porous Hydroxyapatite Formed via Enzymatic Mineralization
Advanced Functional Materials, EarlyView.Bone combines lightness, strength, and the ability to heal, inspiring new materials design. This work introduces a room‐temperature, enzyme‐mediated 3D printing method to create porous hydroxyapatite scaffolds. The process avoids energy‐intensive sintering, preserves bioactivity, and allows control over porosity and mineralization.
Francesca Bono +6 more
wiley +1 more source
Constraining the Pulsar 3D Velocity Distribution: The Impact of Spin–Velocity Alignment
The Astrophysical JournalQuantifying the natal kick distribution of pulsars is essential for understanding supernova physics and binary evolution, yet measurements are historically limited by the lack of radial velocity data.
Zheng Li +4 more
doaj +1 more source
Diffuse neutrino background from past core collapse supernovae. [PDF]
Proc Jpn Acad Ser B Phys Biol Sci, 2023 Ando S, Ekanger N, Horiuchi S, Koshio Y.
europepmc +1 more source
, 2014 We present a novel mechanism to enhance the mass-loss rates of massive stars shortly before their explosion. The neutrino luminosities of the stellar core of massive stars become larger as they get closer to the time of the core collapse.
Moriya, Takashi J.
core +1 more source
Quasi‐Static to Supersonic Energy Absorption of Nanoarchitected Tubulanes and Schwarzites
Advanced Functional Materials, EarlyView.Nanoarchitected energy‐absorptive Tubulanes exhibit record energy absorption under quasi‐static conditions and exceptional inelastic energy dissipation under 750 m s−1 ballistics impact, with high performance spanning strain rates of 12 orders of magnitude.
Peter Serles +16 more
wiley +1 more source
The role of the hadron-quark phase transition in core-collapse supernovae. [PDF]
Mon Not R Astron Soc, 2022 Jakobus P +5 more
europepmc +1 more source
Starless Cloud Core L1517B in Envelope Expansion with Core Collapse
, 2011 Various spectral emission lines from star-forming molecular cloud core L1517B manifest red asymmetric double-peaked profiles with stronger red peaks and weaker blue peaks, in contrast to the oft-observed blue-skewed molecular spectral line profiles with ...
Aguti +37 more
core +1 more source
Magnetorotational iron core collapse
The Astrophysical Journal, 1984 During its final evolutionary stages, a massive star, as considered in current astrophysical theory, undergoes rapid collapse, thereby triggering a sequence of a catastrophic event which results in a Type II supernova explosion. A remnant neutron star or a black hole is left after the explosion.
openaire +1 more source
Advanced Functional Materials, EarlyView.A Cu‐based crystal‐glass composite with high‐density twins is identified by a fast screening technique using combinatorial sputtering together with XRD and nanoindentation mapping. This bamboo‐like structure demonstrates homogenous plastic flow and retains high strength during in situ high temperature tests, up to 1 GPa at 550°C, owing to those ...
Chunhua Tian +10 more
wiley +1 more source