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D. Wen

4 papers hereh-index 211 citations5 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • last author4

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE3
  • nucl-th1
same name
  • D. Wen — 4 papers, h 3
  • D. Wen — 3 papers, h 3
  • D. Wen — 2 papers, h 2
  • D. Wen — 1 paper, h 1
  • D. Wen — 1 paper, h 1
  • D. Wen — 1 paper, h 3

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20232025
most citedA new criterion for the existence of dark matter in neutron stars

14 citations · 22 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2025★ 1 cited

Precise constraint on properties of neutron stars through new universal relations and astronomical observations

Zehan Wu, Dehua Wen

In view of the great uncertainty of the equation of state (EOS) of high-density nuclear matter, establishing EOS-independent universal relations between global properties of neutro…

astro-ph.HE2024★ 2 cited

Anisotropic pressure effect on central EOS of PSR J0740+6620 in the light of dimensionless TOV equation

Zhihao Yang, Dehua Wen

It is generally agreed upon that the pressure inside a neutron star is isotropic. However, a strong magnetic field or superfluidity suggests that the pressure anisotropy may be a m…

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…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.