Supernova bounds on the dark photon using its electromagnetic decay
The hypothetical massive dark photon (γ′) which has kinetic mixing with the SM photon can decay electromagnetically to e+e− pairs if its mass m exceeds 2me, and otherwise into three SM photons. These decays yield cosmological and supernovae associated signatures. We briefly discuss these signatures,...
Main Authors: | Demos Kazanas, Rabindra N. Mohapatra, Shmuel Nussinov, Vigdor L. Teplitz, Yongchao Zhang |
---|---|
Format: | Article |
Language: | English |
Published: |
Elsevier
2015-01-01
|
Series: | Nuclear Physics B |
Online Access: | http://www.sciencedirect.com/science/article/pii/S0550321314003447 |
Similar Items
-
Constraints on mirror models of dark matter from observable neutron-mirror neutron oscillation
by: Rabindra N. Mohapatra, et al.
Published: (2018-01-01) -
Supernova constraints on an axion-photon-dark photon interaction
by: Anson Hook, et al.
Published: (2021-06-01) -
Observable signatures of dark photons from supernovae
by: William DeRocco, et al.
Published: (2019-02-01) -
Dark matter clusters and time correlations in direct detection experiments
by: Shmuel Nussinov, et al.
Published: (2020-03-01) -
Search for the dark photon in π0 decays
by: J.R. Batley, et al.
Published: (2015-06-01)