Speaker
Jorge Venzor
Description
Neutrino-neutrino dispersion models have gained popularity as potential solutions for reconciling the discrepancy between local measurements of the Hubble constant ($H_0$) and the model-dependent measurements derived from the cosmic microwave background radiation and other early Universe probes. This work addresses the current state of neutrino self-interactions, with a specific focus on the phenomenology associated with resonant interactions. We compare our results to existing limits on mediator mass, encompassing both extremely light and heavy scalar particles.
| Poster prize | Yes |
|---|---|
| Given name | Jorge |
| Surname | Venzor |
| First affiliation | Centro de Investigación y de Estudios Avanzados (CINVESTAV) |
| Institutional email | jorge.venzor@cinvestav.mx |
| Gender | Male |
