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  • Open Access

Neutron star with dark matter using vector portal

Deepak Kumar*

Ranjita K. Mohapatra†

Hiranmaya Mishra‡

Sudhanwa Patra§

  • Department of Physics, Rajdhani College, Bhubaneswar 751003, India

  • *Contact author: deepakk@iiserbpr.ac.in
  • †Contact author: ranjita.iop@gmail.com
  • ‡Contact author: hiranmaya@niser.ac.in
  • §Contact author: sudhanwa@iitbhilai.ac.in
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Phys. Rev. D 114, 043027 – Published 11 August, 2026

DOI: https://doi.org/10.1103/fsh5-b73x

Abstract

Compact astrophysical objects, such as neutron stars, can provide a unique environment where the interplay between strongly interacting nuclear matter and dark matter (DM) can yield possible observable signatures. We investigate here the impact of fermionic DM interacting with nucleons via a vector mediator (Z′) portal inside neutron stars using the relativistic mean-field framework. Unlike scalar portal DM models, which primarily modify the effective nucleon mass through scalar interactions, vector mediators (Z′) introduce additional repulsive interactions that directly affect the baryonic chemical potential and the pressure of dense matter. We show that the precise measurements of neutron-star properties, including the mass-radius relation and tidal deformability from gravitational wave observations and x-ray and radio observations of pulsars, can shed light on properties of DM. We study the gross structural properties of a neutron star using the Tolman-Oppenheimer-Volkoff equations, employing an equation of state (EOS) for neutron-star matter in the presence of vector portal-assisted DM. The resulting stellar configurations, consistent with observational bounds from gravitational wave observations (GW170817) in LIGO/Virgo and x-ray observations of pulsar PSR J0030+0451 in NICER, are shown to constrain the vector portal DM parameters. It is observed that, while large portal mass can soften the EOS of the DM-admixed neutron-star matter, the light portal mass can make the EOS stiffer at large densities, resulting in distinct mass-radius relation and the tidal deformability between the two scenarios. The vector portal DM scenario, with DM interaction with quarks via the Z′ vector boson, can establish a direct connection to terrestrial searches, including direct and indirect detection and collider searches for the Z′ boson. Taken together, these constitute a comprehensive framework that bridges neutron-star astrophysics with particle physics, enabling a multimessenger exploration of DM properties.

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Phys. Rev. D 114, 043027– Published 11 August, 2026
  • Received 7 April 2026
  • Revised 15 June 2026
  • Accepted 7 July 2026
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