4.4 Review

A Review of Neutrino Decoupling from the Early Universe to the Current Universe

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Summary: The EMPRESS survey, using a new sample of extremely metal poor systems, has reported a primordial helium abundance that is 3s smaller than the prediction from standard big bang nucleosynthesis. This could indicate a primordial lepton asymmetry in the electron neutrino flavor. A comprehensive analysis of the lepton asymmetry is presented, using measurements of primordial element abundances and cosmic microwave background (CMB) data from Planck. The results suggest a non-zero lepton asymmetry with a deviation from zero of 2.9s, assuming no dark radiation, or 2.2s if the abundance of dark radiation is not assumed.

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Summary: This study explores the possibility of detecting the cosmic neutrino background (CNB) by capturing relic neutrinos on a tritium target. It examines the prospects of CNB detection and neutrino mass measurement in different cosmological models, including nonstandard ones. The research suggests that some nonstandard cosmological models may have higher CNB detection prospects compared to the standard model, and the detection results can be used to distinguish between different cosmological scenarios.

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2020 global reassessment of the neutrino oscillation picture

P. F. de Salas et al.

Summary: The latest global fit analysis of neutrino oscillation data provides more accurate measurements of theta(13), theta(12), Delta m212, and Delta m312 and suggests a preference for the second octant in the atmospheric angle theta(23) with statistical significance. Cosmological measurements show a clear preference for the normal neutrino mass ordering.

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Precise capture rates of cosmic neutrinos and their implications on cosmology

Kensuke Akita et al.

Summary: Exploring the potential of measuring cosmological effects through cosmic neutrino capture on tritium, such as neutrino decoupling and clustering in our Galaxy, can provide insights into neutrino physics and the evolution of the universe. Precise estimates of capture rates can reveal new phenomena in neutrino physics and indicate non-standard processes in the evolution of the universe.

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Neutrino flavor mixing breaks isotropy in the early universe

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Summary: Research indicates that small perturbations in the neutrino field in the early universe could be amplified by non-linear flavor mixing, affecting flavor evolution and the effective number of thermally excited neutrino species. The study also shows that neutrino-antineutrino asymmetry can significantly increase under isotropic and anisotropic initial conditions.

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Towards a precision calculation of the effective number of neutrinos Neff in the Standard Model: the QED equation of state

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Incomplete neutrino decoupling effect on big bang nucleosynthesis

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Neutrino decoupling beyond the Standard Model: CMB constraints on the Dark Matter mass with a fast and precise Neff evaluation

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Gravitational clustering of cosmic relic neutrinos in the Milky Way

Jue Zhang et al.

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On the capture rates of big bang neutrinos by nuclei within the Dirac and Majorana hypotheses

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Improved constraints on lepton asymmetry from the cosmic microwave background

Isabel M. Oldengott et al.

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Calculation of the local density of relic neutrinos

P. F. de Salas et al.

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Insights into neutrino decoupling gleaned from considerations of the role of electron mass

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Relic neutrino decoupling with flavour oscillations revisited

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Neutrino quantum kinetic equations: The collision term

Daniel N. Blaschke et al.

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Tritium β decay in chiral effective field theory

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Neutrino energy transport in weak decoupling and big bang nucleosynthesis

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Annual modulation of cosmic relic neutrinos

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Updated BBN bounds on the cosmological lepton asymmetry for non-zero θ13

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D. J. Fixsen

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Exact relativistic β decay endpoint spectrum

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Probing low energy neutrino backgrounds with neutrino capture on beta decaying nuclei

Alfredo G. Cocco et al.

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Relic neutrino decoupling including flavour oscillations

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Gravitational clustering of relic neutrinos and implications for their detection

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Neutrino energy loss rate in a stellar plasma

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Cosmological bounds on neutrino degeneracy improved by flavor oscillations

AD Dolgov et al.

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Oscillation effects on neutrino decoupling in the early universe

S Hannestad

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Expected signals in relic neutrino detectors

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Non equilibrium spectra of degenerate relic neutrinos

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