Results 21 to 30 of about 3,357 (48)
SYGMA: Stellar Yields for Galactic Modeling Applications
, 2018 The stellar yields for galactic modeling applications (SYGMA) code is an open-source module that models the chemical ejecta and feedback of simple stellar populations (SSPs).
Côté, Benoit +4 more
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Transmuted Gravity Wave Signals from Primordial Black Holes
, 2018 Primordial black holes (PBHs) interacting with compact stars in binaries lead to a new class of gravity wave signatures that we explore. A small $10^{-16} - 10^{-7} M_{\odot}$ PBH captured by a neutron star or a white dwarf will eventually consume the ...
Takhistov, Volodymyr
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The Fermi Large Area Telescope as a Galactic Supernovae Axionscope
, 2017 In a Galactic core-collapse supernova (SN), axionlike particles (ALPs) could be emitted via the Primakoff process and eventually convert into $\gamma$ rays in the magnetic field of the Milky Way. From a data-driven sensitivity estimate, we find that, for
Conrad, Jan +4 more
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Further stable neutron star models from f(R) gravity
, 2013 Neutron star models in perturbative $f(R)$ gravity are considered with realistic equations of state. In particular, we consider the FPS, SLy and other equations of state and a case of piecewise equation of state for stars with quark cores.
Astashenok, Artyom V. +2 more
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, 2015 Many theoretically well-motivated extensions of the Standard Model of particle physics predict the existence of the axion and further ultralight axion-like particles.
Ringwald, Andreas
core
, 2017 The formation of compact stellar-mass binaries is a difficult, but interesting problem in astrophysics. There are two main formation channels: In the field via binary star evolution, or in dense stellar systems via dynamical interactions.
Amaro-Seoane, Pau, Chen, Xian
core +2 more sources
The Neutrino Signal From Pair Instability Supernovae
, 2017 A very massive star with a carbon-oxygen core in the range of $64$ M$_{\odot}
Fröhlich, Carla +3 more
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The s-process nucleosynthesis : Impact of the uncertainties in the nuclear physics determined by monte carlo variations [PDF]
, 2017 We investigated the impact of uncertainties in neutron-capture and weak reactions (on heavy elements) on the s-process nucleosynthesis in low-mass stars and massive stars using a Monte-Carlo based approach. We performed extensive nuclear reaction network
Cescutti, G. +5 more
core +1 more source
Astrophysical probes of the Vainshtein mechanism:stars and galaxies [PDF]
, 2015 Koyama, Kazuya, Sakstein, Jeremy
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Some of the next articles are maybe not open access.
Molecular engineering of contact interfaces for high-performance perovskite solar cells
Nature Reviews Materials, 2022Furkan H Isikgor +2 more
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