Results 81 to 90 of about 767 (211)
We build on the simplified spectral deferred corrections (SDC) coupling of hydrodynamics and reactions to handle the case of nuclear statistical equilibrium (NSE) and electron/positron captures/decays in the cores of massive stars.
Michael Zingale +4 more
doaj +1 more source
Consistency of cosmic-ray source abudances with explosive nucleosynthesis
A model was examined in which the cosmic ray abundances of elements from C to Fe are consistent with explosive nucleosynthesis. The observed abundance of cosmic rays near the earth, cosmic ray source abundance, and solar system abundance are discussed ...
Ramaty, R., Kozlovsky, B.
core
Under astrophysical conditions of extreme temperature and density, nuclear reactions can occur with rates that are comparable to a dynamical free-fall time, i.e. on the order of seconds.
Champagne, A.E., Wiescher, M.
core +1 more source
We have measured the Sm-147(n, alpha) cross section from 3 eV to 500 keV. These data were used to test nuclear statistical models which must be relied on to calculate the rates for as yet unmeasurable reactions occurring in explosive nucleosynthesis ...
Andrzejewski, J. +4 more
core +1 more source
Kilonova Emissions from Neutron Star Merger Remnants: Implications for the Nuclear Equation of State
Multimessenger observations of binary neutron star mergers can provide valuable information on the nuclear equation of state (EOS). Here, we investigate the extent to which electromagnetic observations of the associated kilonovae allow us to place ...
Kelsey A. Lund +5 more
doaj +1 more source
One of the open questions following the discovery of GW170817 is whether neutron star (NS) mergers are the only astrophysical sites capable of producing r -process elements.
Shreya Anand +43 more
doaj +1 more source
Recent research activities of division of nuclear physics. [PDF]
Cheoun MK.
europepmc +1 more source
87th Annual Meeting of the Meteoritical Society 2025: Contents
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 2-29, August 2025.
wiley +1 more source
A metal-poor star with abundances from a pair-instability supernova. [PDF]
Xing QF +9 more
europepmc +1 more source
87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley +1 more source

