Overview of the model-dependent approach for the Diffuse Supernova Neutrino Background search with the SK-Gd experiment

21 Jun 2024, 17:30
2h
Near Aula Magna (U6 building) (University of Milano-Bicocca)

Near Aula Magna (U6 building)

University of Milano-Bicocca

Poster Supernova neutrinos Poster session and reception 2

Speaker

Rudolph Rogly (LLR (CNRS))

Description

The Diffuse Supernova Neutrino Background (DSNB) is the integrated flux of neutrinos and antineutrinos emitted by all past supernovae in the observable Universe. It is yet to be observed.
In this regard, the Super-Kamiokande (SK) experiment has entered its gadolinium (Gd) era in 2020: the Gd-loading of the water tank enhances the capability to tag the inverse beta-decay neutron stemming from the interaction of a DSNB electronic antineutrino with a proton.
In this poster, I will present the model-dependent analysis developed for the DSNB search, and its results with the most recent SK data, with increased signal sensitivity owing to Gd-loading. I will also show how evidence for DSNB is within reach with the SK-Gd experiment.

Poster prize Yes
Given name Rudolph
Surname Rogly
First affiliation LLR
Second affiliation CNRS
Institutional email rudolph.rogly@llr.in2p3.fr
Gender Male
Collaboration (if any) Super-Kamiokande

Primary author

Rudolph Rogly (LLR (CNRS))

Presentation materials