Abstract
Isolated ideal neutron stars (NS) of age exhaust thermal and rotational energies and cool down to temperatures below . Accretion of particle dark matter (DM) by such NS can heat them up through kinetic and annihilation processes. This increases the NS surface temperature to a maximum of in the best case scenario. The maximum accretion rate depends on the DM ambient density and velocity dispersion, and on the NS equation of state and their velocity distributions. Upon scanning over these variables, we find that the effective surface temperature varies at most by . Black-body spectrum of such warm NS peak at near infrared wavelengths with magnitudes in the range potentially detectable by the James Webb Space Telescope (JWST). Using the JWST exposure time calculator, we demonstrate that NS with surface temperatures , located at a distance of 10 pc can be detected through the F150W2 (F322W2) filters of the NIRCAM instrument at (5) within 24 hours of exposure time. Independently of DM, an observation of NS with surface temperatures will be a formative step toward testing the minimal cooling paradigm during late evolutionary stages.
- Received 13 May 2022
- Revised 14 September 2022
- Accepted 28 June 2023
DOI:https://doi.org/10.1103/PhysRevD.108.L021301
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