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2021

Exploring dark sector parameters in light of neutron star temperatures

Lin, Guey-Lin, Lin, Yen-Hsun

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Using neutron stars (NS) as a dark matter (DM) probe has gained broad attention recently, either from heating due to DM annihilation or its stability under the presence of DM.

In this work, we investigate spin-$1/2$ fermionic DM $\chi$ charged under the $U(1)_{X}$ in the dark sector.
The massive gauge boson $V$ of $U(1)_{X}$ gauge group can be produced in NS via DM annihilation.
The produced gauge boson can decay into Standard Model (SM) particles before it exits the NS, despite its tiny couplings to SM particles.

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