Heavy Higgsino Dark Matter With Low Reheating in View of the LZ High-Recoil Event
This paper proposes that a heavy higgsino dark matter candidate with a mass of approximately 0.1 PeV can explain the universe's dark matter abundance and the recent LUX-ZEPLIN high-recoil event without violating detection constraints, provided the reheating temperature is suppressed below 595 GeV through the non-thermal production of higgsinos from the decay of a heavy modulus field.