Seminários dos Grupos de Pesquisa

Shining Light on Neutrinos: Exploring Electromagnetic Properties

Data: 
sexta-feira, 17 Maio, 2024 - 15:00
Palestrante: 
Sudip Jana (Max Planck institute, for nuclear physics, Heidelberg)
Grupo de pesquisa: 
Física de Partículas e Campos
Resumo: 

After a brief introduction to neutrino electromagnetic properties, I will focus on the correlation between neutrino magnetic moment and neutrino mass mechanism. Then, I will discuss that the models that induce large neutrino magnetic moments while maintaining their small masses naturally also predict observable shifts in the charged lepton anomalous magnetic moment by showing that the measurement of muon g−2 by the Fermilab experiment can be an indirect and novel test of the neutrino magnetic-moment hypothesis, which can be as sensitive as other ongoing neutrino/dark matter experiments. The promising new possibilities for probing neutrino electromagnetic properties in future experiments from terrestrial experiments and astrophysical considerations will also be discussed. This talk will be based on results obtained in hep-ph 2303.13572, 2203.01950, 2104.03291, and 2007.0429.

Local: Sala Jayme Tiomno

Waveforms from Scattering Amplitudes and Modified Gravity for Spinning Bodies

Data: 
sexta-feira, 10 Maio, 2024 - 15:00
Palestrante: 
Panagiotis Marinellis (IJCLab, Orsay)
Grupo de pesquisa: 
Física de Partículas e Campos
Resumo: 

The detection of gravitational waves by the LIGO-VIRGO collaboration has marked a transformative era in astronomy, providing unprecedented insights into the cosmos and opening new avenues for exploring the universe. At the same time, advances in the classical limit of scattering amplitudes, notably through the KMOC formalism, have opened up new avenues for understanding compact binary systems. In this talk, we delve into the significance of these advances and explore the emergence of waveforms derived from scattering amplitudes. Theoretical underpinnings are elucidated, offering insights into the dynamics of binary systems and valuable tools for characterizing gravitational wave emissions. Complementing waveforms derived from scattering amplitudes, we delve into the interplay of modified gravity theories with radiation losses in spinning binary systems, including computations in a QED toy model of modified gravity. We examine deviations from Einstein's theory on waveforms, shedding light on modified gravity's effects. Through theoretical analyses, we unveil how alternative gravity theories manifest, offering insights into fundamental physics and new testing avenues.

Local: Sala Jayme Tiomno

Desenvolvido por IFUSP