Speaker
Jaime Hoefken Zink
(Istituto Nazionale di Fisica Nucleare)
Description
Hot white dwarfs lose energy mainly in the form of neutrinos through plasmon decay from the inner part of the star. BSM physics can have visible contributions to the cooling of these compact objects. The aim of this study is to show how hot white dwarf cooling could be altered by a dark photon from the L_mu - L_tau model and explore these effects from ultra-light to heavy intermediators. This leads to very interesting constraints to this BSM model.
| Poster prize | Yes |
|---|---|
| Given name | Jaime |
| Surname | Hoefken Zink |
| First affiliation | Università di Bologna |
| Second affiliation | INFN Bologna |
| Institutional email | jaime.hoefkenzink2@unibo.it |
| Gender | Male |
Primary author
Jaime Hoefken Zink
(Istituto Nazionale di Fisica Nucleare)
Co-author
Dr
Patrick Foldenauer
(IFT Madrid)
