The explanation of the dark energy budget of the universe, which gives rise to the accelerated behavior of cosmic flow, might not require to search for exotic candidates (e.g. scalar particles) which, up to now, have not been detected. We propose it resides in the QFT neutrino mixing phenomenon
The effective number of neutrinos, Neff, obtained from CMB fluctuations accounts for all effectively...
AbstractThe effective number of neutrinos, Neff, obtained from CMB fluctuations accounts for all eff...
In this talk I will firstly review on the current constraints on the equation of state of the dark e...
Motivated by the seeming coincidence of the neutrino mass scale and the dark energy scale, we propos...
I consider a scenario proposed by Fardon, Nelson and Weiner where dark energy and neutrinos are conn...
The energy scale of dark energy, ∼2×10-3 eV, is a long way off compared to all known fundamental sca...
The depth of the authors theoretical understanding of neutrino flavor mixing should match the import...
.................. a new non-standard-model neutrino interaction mediated by a light scalar field wa...
In this review, I discuss briefly how the presence of a cosmological constant in the Universe may im...
An unexpected explanation for neutrino mass, Dark Matter (DM) and Dark Energy (DE) from genuine Quan...
The depth of our theoretical understanding of neutrino flavor mixing should match the importance of ...
We analyze the boson mixing in curved spacetime and compute the expectation value of the energy-mome...
We consider the generic possibility that the Universe’s energy budget includes some form of relativi...
The dark energy density of the universe is obtained from the Higgs potential by introducing a Higgsd...
Applying the formulae derived by us (A. Sapar 1964) for the Universe filled with baryonic matter and...
The effective number of neutrinos, Neff, obtained from CMB fluctuations accounts for all effectively...
AbstractThe effective number of neutrinos, Neff, obtained from CMB fluctuations accounts for all eff...
In this talk I will firstly review on the current constraints on the equation of state of the dark e...
Motivated by the seeming coincidence of the neutrino mass scale and the dark energy scale, we propos...
I consider a scenario proposed by Fardon, Nelson and Weiner where dark energy and neutrinos are conn...
The energy scale of dark energy, ∼2×10-3 eV, is a long way off compared to all known fundamental sca...
The depth of the authors theoretical understanding of neutrino flavor mixing should match the import...
.................. a new non-standard-model neutrino interaction mediated by a light scalar field wa...
In this review, I discuss briefly how the presence of a cosmological constant in the Universe may im...
An unexpected explanation for neutrino mass, Dark Matter (DM) and Dark Energy (DE) from genuine Quan...
The depth of our theoretical understanding of neutrino flavor mixing should match the importance of ...
We analyze the boson mixing in curved spacetime and compute the expectation value of the energy-mome...
We consider the generic possibility that the Universe’s energy budget includes some form of relativi...
The dark energy density of the universe is obtained from the Higgs potential by introducing a Higgsd...
Applying the formulae derived by us (A. Sapar 1964) for the Universe filled with baryonic matter and...
The effective number of neutrinos, Neff, obtained from CMB fluctuations accounts for all effectively...
AbstractThe effective number of neutrinos, Neff, obtained from CMB fluctuations accounts for all eff...
In this talk I will firstly review on the current constraints on the equation of state of the dark e...