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Origin of the elements
What is the origin of the oxygen we breathe, the hydrogen and oxygen (in form of water
H2O) in rivers and oceans, the carbon in all organic compounds, the silicon in electronic …
H2O) in rivers and oceans, the carbon in all organic compounds, the silicon in electronic …
Origin of the heaviest elements: The rapid neutron-capture process
The production of about half of the heavy elements found in nature is assigned to a specific
astrophysical nucleosynthesis process: the rapid neutron-capture process (r process) …
astrophysical nucleosynthesis process: the rapid neutron-capture process (r process) …
Supernova neutrinos: production, oscillations and detection
Neutrinos play a crucial role in the collapse and explosion of massive stars, governing the
infall dynamics of the stellar core, triggering and fueling the explosion and driving the …
infall dynamics of the stellar core, triggering and fueling the explosion and driving the …
Explosion mechanisms of core-collapse supernovae
HT Janka - Annual Review of Nuclear and Particle Science, 2012 - annualreviews.org
Supernova theory, numerical and analytic, has made remarkable progress in the past
decade. This progress was made possible by more sophisticated simulation tools, especially …
decade. This progress was made possible by more sophisticated simulation tools, especially …
Neutrinos from dense environments: Flavor mechanisms, theoretical approaches, observations, and new directions
MC Volpe - Reviews of Modern Physics, 2024 - APS
Neutrino masses and mixings produce vacuum oscillations, an established quantum
mechanical phenomenon. In matter, the Mikheev-Smirnov-Wolfenstein effect, due to …
mechanical phenomenon. In matter, the Mikheev-Smirnov-Wolfenstein effect, due to …
Mass ejection from the remnant of a binary neutron star merger: viscous-radiation hydrodynamics study
We perform long-term general relativistic neutrino radiation hydrodynamics simulations (in
axisymmetry) for a massive neutron star (MNS) surrounded by a torus, which is a canonical …
axisymmetry) for a massive neutron star (MNS) surrounded by a torus, which is a canonical …
Electromagnetic counterparts of compact object mergers powered by the radioactive decay of r-process nuclei
The most promising astrophysical sources of kHz gravitational waves (GWs) are the inspiral
and merger of binary neutron star (NS)/black hole systems. Maximizing the scientific return …
and merger of binary neutron star (NS)/black hole systems. Maximizing the scientific return …
The evolution and explosion of massive stars
Like all true stars, massive stars are gravitationally confined thermonuclear reactors whose
composition evolves as energy is lost to radiation and neutrinos. Unlike lower-mass stars …
composition evolves as energy is lost to radiation and neutrinos. Unlike lower-mass stars …
Red or blue? A potential kilonova imprint of the delay until black hole formation following a neutron star merger
Mergers of binary neutron stars usually result in the formation of a hypermassive neutron
star (HMNS). Whether and when this remnant collapses to a black hole (BH) depends …
star (HMNS). Whether and when this remnant collapses to a black hole (BH) depends …
Collapsars: Gamma-ray bursts and explosions in “failed supernovae”
Using a two-dimensional hydrodynamics code (PROMETHEUS), we explore the continued
evolution of rotating helium stars, M α≳ 10 M⊙, in which iron-core collapse does not …
evolution of rotating helium stars, M α≳ 10 M⊙, in which iron-core collapse does not …