14 citations · 22 across the 4 of their papers we have counts for
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astro-ph.HE2023★ 14 cited
A new criterion for the existence of dark matter in neutron stars
Hongyi Sun, Dehua Wen
The tidal deformability and the radius of neutron stars are observables, which have been used to constrain the neutron star equation of state and explore the composition in neutron…
nucl-th2023★ 5 cited
From masses and radii of neutron stars to EOS of nuclear matter through neural network
Zehan Wu, Dehua Wen
The equation of state (EOS) of dense nuclear matter is a key factor to determine the internal structure and properties of neutron stars. However, the EOS of high-density nuclear ma…