Detection of Dark Matter in Neutron  Stars

الملخص

Despite the latest advancements in the field of astrophysics, dark matter, the vague mysterious thing occupying vast parts of our universe, is still floating around with its obscure nature and very hard to detect components. This research is delving into different approaches for detecting dark matter present in neutron stars and calculating its mass. The approaches discussed are considered secondary techniques in the detection of dark matter and they are being scrutinized with the aim of developing a new way of detecting these vague particles. For instance, hybrid detection methods like star spectroscopy and Gravitational Red Shift Measurements, direct detection methods like scattering experiments, and indirect detection methods like neutrino emissions. Results have shown that some specific neutron stars have higher expectancy for the presence of dark matter particles and some specific techniques are more feasible than others in their detection. By making the most of the latest technology like high-resolution telescopes and software programs, it is possible to utilize dark matter’s effects on neutron stars to assist in its detection. We believe that the detection of dark matter and calculating its mass can pave the way for some revolutionary discoveries regarding the hidden intricacies of the universe.