Speaker
Description
Baryon asymmetry of the Universe offers one of the strongest hints for physics Beyond the Standard Model (BSM). Remarkably, in the general two Higgs Doublet Model (g2HDM) that possesses a second set of Yukawa matrices, one can have electroweak baryogenesis (EWBG), while the electron EDM is evaded by a natural flavor tuning that echoes SM. We show that eEDM may first emerge around 10^−30 𝑒 cm or so, followed by neutron EDM (nEDM) down to 10^−27 𝑒 cm. We illustrate a cancellation mechanism for nEDM itself, which in turn can be probed when a facility capable of pushing down to 10−28 𝑒 cm becomes available, followed by neutron EDM (nEDM) which in turn can be probed when a facility capable of pushing down to 10^−28 𝑒 cm becomes available. We illustrate a cancellation mechanism for nEDM itself, which in turn can be probed when a facility capable of pushing down to 10^−28 𝑒 cm becomes available.
