Neutrinos produced in extragalactic sources may experience flavor-oscillations and decoherence on their way to Earth due to their interaction with dark matter (DM). As a result, they may be detected in pointer-states other than the flavor states produced at the source. The oscillation pattern and the structure of the pointer-states can give us information on the characteristics of the DM and the kind of interaction that has taken place. From this perspective, neutrinos can be viewed as DM-tracers. We study the local evolution of neutrino flavor-eigenstates due to local effects produced by the presence of DM. To explore the sensitivity of the model, we consider different DM density profiles, masses and interactions. Starting from the eigenst...
Interest in light dark matter candidates has recently increased in the literature; some of these wor...
We investigate standard and non-standard solar neutrino signals in direct dark matter detection expe...
Dark matter (DM) particles are predicted to decay into Standard Model particles which would produce ...
Neutrinos (ν) are produced in practically all extragalactic astrophysical processes. They can travel...
In our analysis, we explore the case when neutrinos can interact with the galactic DM halo.We model ...
If high-energy neutrinos propagate in a background of ultralight scalar field particles of dark matt...
In this work we study the impact of new physics, stimulated by flavor anomalies, on neutrino oscilla...
In this work, we study the propagation of high energy neutrinos produced in extragalactic sources in...
In this thesis, we study neutrino oscillations in vacuum and in the presence of a Dark Matter halo i...
Neutrinos have shaped cosmic history in important ways. In early epochs, they left their mark on the...
We examine scenarios in which a dark sector (dark matter, dark radiation, or dark energy) couples to...
At present, a variety of dark matter (DM) density profiles are available in the literature, able to ...
At present, a variety of dark matter (DM) density profiles are available in the literature, able to ...
AbstractInterest in light dark matter candidates has recently increased in the literature; some of t...
Abstract. We investigate the scattering of solar neutrinos on electrons and nuclei in dark matter di...
Interest in light dark matter candidates has recently increased in the literature; some of these wor...
We investigate standard and non-standard solar neutrino signals in direct dark matter detection expe...
Dark matter (DM) particles are predicted to decay into Standard Model particles which would produce ...
Neutrinos (ν) are produced in practically all extragalactic astrophysical processes. They can travel...
In our analysis, we explore the case when neutrinos can interact with the galactic DM halo.We model ...
If high-energy neutrinos propagate in a background of ultralight scalar field particles of dark matt...
In this work we study the impact of new physics, stimulated by flavor anomalies, on neutrino oscilla...
In this work, we study the propagation of high energy neutrinos produced in extragalactic sources in...
In this thesis, we study neutrino oscillations in vacuum and in the presence of a Dark Matter halo i...
Neutrinos have shaped cosmic history in important ways. In early epochs, they left their mark on the...
We examine scenarios in which a dark sector (dark matter, dark radiation, or dark energy) couples to...
At present, a variety of dark matter (DM) density profiles are available in the literature, able to ...
At present, a variety of dark matter (DM) density profiles are available in the literature, able to ...
AbstractInterest in light dark matter candidates has recently increased in the literature; some of t...
Abstract. We investigate the scattering of solar neutrinos on electrons and nuclei in dark matter di...
Interest in light dark matter candidates has recently increased in the literature; some of these wor...
We investigate standard and non-standard solar neutrino signals in direct dark matter detection expe...
Dark matter (DM) particles are predicted to decay into Standard Model particles which would produce ...