A two-state dark matter model with velocity-dependent upscattering can produce a Galactic Center gamma-ray signal while suppressing dwarf galaxy signals, breaking the usual correlation between the two.
The mass terms for these spinors are described by the Lagrangian, −L⊃ M 2 (χχ +χcχc) +mχχc + h.c., (5) where M and m are Majorana and Dirac masses, respectively
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
hep-ph 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
dSphobic Dark Matter
A two-state dark matter model with velocity-dependent upscattering can produce a Galactic Center gamma-ray signal while suppressing dwarf galaxy signals, breaking the usual correlation between the two.