  Core-collapse supernovae (SNe) are one of the most powerful cosmic sources of
neutrinos, with energies of several MeV. The emission of neutrinos and
antineutrinos of all flavors carries away the gravitational binding energy of
the compact remnant and drives its evolution from the hot initial to the cold
final states. Detecting these neutrinos from Earth and analyzing the emitted
signals present a unique opportunity to explore the neutrino mass ordering
problem. This research outlines the detection of neutrinos from SNe and their
relevance in understanding the neutrino mass ordering. The focus is on
developing a model-independent analysis strategy, achieved by comparing
distinct detection channels in large underground detectors. The objective is to
identify potential indicators of mass ordering within the neutrino sector.
Additionally, a thorough statistical analysis is performed on the anticipated
neutrino signals for both mass orderings. Despite uncertainties in supernova
explosion parameters, an exploration of the parameter space reveals an
extensive array of models with significant sensitivity to differentiate between
mass orderings. The assessment of various observables and their combinations
underscores the potential of forthcoming supernova observations in addressing
the neutrino mass ordering problem.
