In the dense supernova environment, neutrinos can undergo fast flavor conversions which depend on the large neutrino-neutrino interaction strength. It has been recently shown that both their presence and outcome can be affected when passing from the commonly used three neutrino species approach to the more general with six species. Here we build up on a previous work performed on this topic and, for the first time, perform a numerical simulation of flavor evolution in both space and time, assuming six neutrino species. We find that the results presented in our previous work remain qualitatively the same even for flavor evolution in space and time. This emphasizes the need for going beyond the simplistic approximation with three species when...
We assess the occurrence of fast neutrino flavor instabilities in two three-dimensional state-of-the...
We calculate coherent neutrino and antineutrino flavor transformation in the supernova environment, ...
We discuss a new kind of astrophysical transport problem: the coherent evolution of neutrino flavor ...
Neutrinos in a core-collapse supernova can undergo fast flavor conversions with a possible impact on...
International audienceThe dense neutrino medium in a core-collapse supernova or a neutron-star merge...
We can understand many recently discovered features of flavor evolution in dense, self-coupled super...
The neutrino fast flavor instability (FFI) can change neutrino flavor on time scales of nanoseconds ...
Despite the theoretical indication that fast neutrino-flavor conversion (FFC) ubiquitously occurs in...
The flavor evolution of neutrinos in core collapse supernovae and neutron star mergers is a critical...
We present a systematic study of fast neutrino-flavor conversion (FFC) with both small-scale and lar...
We present results of large-scale numerical simulations of the evolution of neutrino and antineutrin...
One of the greatest uncertainties in any modeling of inner engine of core-collapse supernova (CCSN) ...
We study the flavor evolution of a dense gas initially consisting of pure monoenergetic νe and ν̄e. ...
Neutrino self-interactions in a dense neutrino gas can induce collective neutrino flavor conversions...
One of the active debates in core-collapse supernova (CCSN) theory is how significantly neutrino fla...
We assess the occurrence of fast neutrino flavor instabilities in two three-dimensional state-of-the...
We calculate coherent neutrino and antineutrino flavor transformation in the supernova environment, ...
We discuss a new kind of astrophysical transport problem: the coherent evolution of neutrino flavor ...
Neutrinos in a core-collapse supernova can undergo fast flavor conversions with a possible impact on...
International audienceThe dense neutrino medium in a core-collapse supernova or a neutron-star merge...
We can understand many recently discovered features of flavor evolution in dense, self-coupled super...
The neutrino fast flavor instability (FFI) can change neutrino flavor on time scales of nanoseconds ...
Despite the theoretical indication that fast neutrino-flavor conversion (FFC) ubiquitously occurs in...
The flavor evolution of neutrinos in core collapse supernovae and neutron star mergers is a critical...
We present a systematic study of fast neutrino-flavor conversion (FFC) with both small-scale and lar...
We present results of large-scale numerical simulations of the evolution of neutrino and antineutrin...
One of the greatest uncertainties in any modeling of inner engine of core-collapse supernova (CCSN) ...
We study the flavor evolution of a dense gas initially consisting of pure monoenergetic νe and ν̄e. ...
Neutrino self-interactions in a dense neutrino gas can induce collective neutrino flavor conversions...
One of the active debates in core-collapse supernova (CCSN) theory is how significantly neutrino fla...
We assess the occurrence of fast neutrino flavor instabilities in two three-dimensional state-of-the...
We calculate coherent neutrino and antineutrino flavor transformation in the supernova environment, ...
We discuss a new kind of astrophysical transport problem: the coherent evolution of neutrino flavor ...