Gamma-Ray and Gravitational Wave Signals of Inelastic Higgs Portal Dark Matter
Not scheduled
30m
Roosevelt Room I (SpringHill Suites Conference Center Deadwood)
Roosevelt Room I
SpringHill Suites Conference Center Deadwood
Cadillac Jack's Resort
360 Main St, Deadwood, SD 57732
Speaker
Subhojit Roy(Argonne National Laboratory)
Description
We explore a simple and predictive dark matter scenario involving a complex scalar field, , coupled to the Higgs portal with no additional field content. In the UV, the field possesses a global symmetry which is broken by mass terms and Higgs portal interactions. In the mass basis, the complex field splits into a pair of real scalars with a small mass splitting (in analogy with pseudo-Dirac fermions), such that the Higgs portal acquires both diagonal and off-diagonal terms with respect to these eigenstates. In the parameter space where the off-diagonal interaction predominates, this scenario is safe from all existing direct detection constraints. Moreover, this model provides a viable explanation for the longstanding Galactic Center gamma-ray excess. Additionally, this model influences the Higgs potential in a way that could lead to a strong first-order electroweak phase transition, potentially generating a stochastic gravitational wave signal