In this work, we use the maximum entropy principle (MEP) to infer the mass of an axion which interacts to photons and neutrinos in an effective low energy theory. The Shannon entropy function to be maximized is defined in terms of the axion branching ratios. We show that MEP strongly constrains the axion mass taking into account the current experimental bounds on the neutrinos masses. Assuming that the axion is massive enough to decay into all the three neutrinos and that MEP fixes all the free parameters of the model, the inferred axion mass is in the interval 0.1 eV < m(A) < 0.2 eV, which can be tested by forthcoming experiments such as IAXO. However, even in the case where MEP fixes just the axion mass and no other parameter, we found th...
We study the impact of axion emission in simulations of massive star explosions, as an additional so...
We show that in any invisible axion model due to the effects of effective nonrenormalizable interact...
We propose a minimal realization of the Peccei Quinn mechanism in a realistic SU(5) model, where the...
The Maximum Entropy Principle (MEP) is a method that can be used to infer the value of an unknown qu...
Observations of the cosmological large-scale structure provide well-established neutrino mass limits...
Axions currently provide the most compelling solution to the strong CP problem. These particles may ...
The strongest upper bounds on the axion mass come from astrophysical observations like the neutrino ...
We investigate the axion dark matter scenario (ADM), in which axions account for all of the dark mat...
Relic thermal axions could play the role of an extra hot dark matter component in cosmological struc...
The Strong CP Problem and its resolution through the existence of an axion are briefly reviewed. The...
We discuss the possibility to predict the QCD axion mass in the context of grand unified theories. W...
We revise cosmological mass bounds on hadronic axions in low-reheating cosmological scenarios, with ...
The existence of dark matter is a well established fact both due to galaxy rotation curves and also ...
We study the impact of axion emission in simulations of massive star explosions, as an additional so...
AbstractAxions currently provide the most compelling solution to the strong CP problem. These partic...
We study the impact of axion emission in simulations of massive star explosions, as an additional so...
We show that in any invisible axion model due to the effects of effective nonrenormalizable interact...
We propose a minimal realization of the Peccei Quinn mechanism in a realistic SU(5) model, where the...
The Maximum Entropy Principle (MEP) is a method that can be used to infer the value of an unknown qu...
Observations of the cosmological large-scale structure provide well-established neutrino mass limits...
Axions currently provide the most compelling solution to the strong CP problem. These particles may ...
The strongest upper bounds on the axion mass come from astrophysical observations like the neutrino ...
We investigate the axion dark matter scenario (ADM), in which axions account for all of the dark mat...
Relic thermal axions could play the role of an extra hot dark matter component in cosmological struc...
The Strong CP Problem and its resolution through the existence of an axion are briefly reviewed. The...
We discuss the possibility to predict the QCD axion mass in the context of grand unified theories. W...
We revise cosmological mass bounds on hadronic axions in low-reheating cosmological scenarios, with ...
The existence of dark matter is a well established fact both due to galaxy rotation curves and also ...
We study the impact of axion emission in simulations of massive star explosions, as an additional so...
AbstractAxions currently provide the most compelling solution to the strong CP problem. These partic...
We study the impact of axion emission in simulations of massive star explosions, as an additional so...
We show that in any invisible axion model due to the effects of effective nonrenormalizable interact...
We propose a minimal realization of the Peccei Quinn mechanism in a realistic SU(5) model, where the...