Author(s): Nirmal Raj, Prajwal Shivanna, and Gaurav Niraj Rachh
A number of astrophysical mechanisms can cause observationally detectable late-time reheating in neutron stars. The paper estimates the sensitivities of the James Webb Space, Extremely Large, and Thirty Meter Telescopes for such observations, also highlighting candidate target systems.
[Phys. Rev. D 109, 123040] Published Thu Jun 27, 2024