Core-Collapse Supernova Cooling in the Dark Z Model

24 Aug 2026, 16:40
20m
S3

Speaker

Mr Ju Hyeong Kang (Pusan National University)

Description

We investigate supernova cooling bounds on an MeV-scale dark Z boson with mass mixing. For a dark Z much lighter than the Standard Model Z boson, the kinetic mixing contribution to its coupling with the neutral current is strongly suppressed, while the mass mixing contribution remains sizable. This allows the dark Z to be efficiently produced in the dense medium of a core-collapse supernova through the neutral current interactions, particularly through axial-vector couplings. We evaluate the production and absorption of dark Z bosons in the proto-neutron star, including in-medium effects relevant to vector interactions, and obtain cooling bounds based on the observed neutrino signal from SN 1987A.

Authors

Dong-Won Jung (IBS CTPU-CGA) Eung Jin Chun (KIAS) Mr Ju Hyeong Kang (Pusan National University) Kwang Sik Jeong (Pusan National University) Seokhoon Yun (KNU)

Presentation materials