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- W4306391114 abstract "Assuming a dark matter fraction $Omega_{DM} = 0.27$ and a reduced Hubble constant $h = 0.73$, we obtain a value of 70 GeV/c$^2$ for the mass of the dark matter WIMP we have previously proposed. We also obtain a value for the annihilation cross section given by $langle sigma_{ann} v rangle = 1.19 times 10^{-26} $ cm$^3$/s in the present universe, consistent with the current limits for dwarf spheroidal galaxies. Both the mass and cross-section are consistent with analyses of the Galactic-center gamma rays observed by Fermi-LAT and the antiprotons observed by AMS-02 if these data are interpreted as resulting from dark matter annihilation. The spin-independent cross-section for direct detection in Xe-based experiments is estimated to be slightly above $10^{-48}$ cm$^2$, presumably just within reach of the LZ and XENONnT experiments with $gtrsim 1000$ days of data taking. The cross-section for production in high-energy proton collisions via vector boson fusion is estimated to be $sim 1$ femtobarn, possibly within reach of the high-luminosity LHC, with $ge 140$ GeV of missing energy accompanied by two jets." @default.
- W4306391114 created "2022-10-17" @default.
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- W4306391114 date "2022-10-14" @default.
- W4306391114 modified "2023-09-27" @default.
- W4306391114 title "Indirect detection, direct detection, and collider detection cross-sections for a 70 GeV dark matter WIMP" @default.
- W4306391114 doi "https://doi.org/10.22323/1.414.0988" @default.
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