A possiblity of measuring the cosmic neutrino temperature $\sim 1.9 K$ and other important quantities such as the chemical potential $\mu$ and the decoupling temperature $T_d$ is discussed, using the recently proposed process of photon irradiated neutrino pair emission from metastable atoms. The Pauli blocking effect of relic neutrinos reduces the rate by a large factor $\approx (1 + m_1/T_d)/4$ at the threshold of the lightest neutrino pair (of mass $2m_1$). Correction of linear order in $\mu$ near the mass thresholds can be used to improve the constraint on the lepton asymmetry
It is shown that high-energy features of the cosmic ray spectrum, in particular the kink around 4 Pe...
We analyze the prospects for testing the cosmic neutrino background and its interpretation as source...
The standard cosmological model predicts the existence of a cosmic neutrino background with a presen...
A measurement of the big bang relic neutrinos would open a new window to the early universe. We revi...
We explore a possibility of measuring the magnitude and the Majorana nature of neutrino masses, by u...
I recall the place of neutrinos in the electroweak theory and summarize what we know about neutrino ...
We present a novel method for detecting the relic neutrino background that takes advantage of struct...
Here we estimate the magnitude of the signals expected for realistic cosmic neutrino backgrounds in ...
The cosmic neutrino background (CNB) consists of low-energy relic neutrinos which decoupled from the...
Relic neutrinos play an important role in the evolution of the Universe, modifying some of the cosmo...
The photon spectrum in macrocoherent atomic deexcitation via radiative emission of neutrino pairs ha...
The Early Universe represents an important environment to test the neutrino proprieties. Indeed Big ...
Neutrinos can play an important role in the evolution of the Universe, modifying some of the cosmolo...
Annihilation of extremely energetic cosmic neutrinos on the relic-neutrino background can give rise ...
In the early universe, neutrinos are slightly coupled when electron-positron pairs annihilate transf...
It is shown that high-energy features of the cosmic ray spectrum, in particular the kink around 4 Pe...
We analyze the prospects for testing the cosmic neutrino background and its interpretation as source...
The standard cosmological model predicts the existence of a cosmic neutrino background with a presen...
A measurement of the big bang relic neutrinos would open a new window to the early universe. We revi...
We explore a possibility of measuring the magnitude and the Majorana nature of neutrino masses, by u...
I recall the place of neutrinos in the electroweak theory and summarize what we know about neutrino ...
We present a novel method for detecting the relic neutrino background that takes advantage of struct...
Here we estimate the magnitude of the signals expected for realistic cosmic neutrino backgrounds in ...
The cosmic neutrino background (CNB) consists of low-energy relic neutrinos which decoupled from the...
Relic neutrinos play an important role in the evolution of the Universe, modifying some of the cosmo...
The photon spectrum in macrocoherent atomic deexcitation via radiative emission of neutrino pairs ha...
The Early Universe represents an important environment to test the neutrino proprieties. Indeed Big ...
Neutrinos can play an important role in the evolution of the Universe, modifying some of the cosmolo...
Annihilation of extremely energetic cosmic neutrinos on the relic-neutrino background can give rise ...
In the early universe, neutrinos are slightly coupled when electron-positron pairs annihilate transf...
It is shown that high-energy features of the cosmic ray spectrum, in particular the kink around 4 Pe...
We analyze the prospects for testing the cosmic neutrino background and its interpretation as source...
The standard cosmological model predicts the existence of a cosmic neutrino background with a presen...