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Neutrino Physics and CP violation
High Energy Physics - Phenomenology · Submitted 16 Nov 2007
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim We review some aspects of neutrino physics and CP violation both in the quark and lepton sectors.
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The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.
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The abstract, sentence by sentence
We review some aspects of neutrino physics and CP violation both in the quark and lepton sectors.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We review some aspects of neutrino physics and CP violation both in the quark and lepton sectors. | contribution 0.85 | 0.21 | 0.12 | unclear 0.52 |
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The paper
Original abstract
We review some aspects of neutrino physics and CP violation both in the quark and lepton sectors.
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How the literature uses it
What this paper does with the arXiv papers it cites
What it cites · 58 sentences without a confident label
Uses data or values from 6 papers
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The observed baryon asymmetry of the universe (BAU) is given by [ref] : [equation]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results · Leptogenesis · 1.00
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For a flat universe, WMAP combined with other astronomical data leads to [ref] $∑_i m_i ≤0.66$ eV ($95%$ CL).
Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology · CP violation at low energies · 1.00
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Direct kinematical limits from Mainz [ref] and Troitsk [ref] place an upper bound on $m_β$ defined as: [equation] given by $m_β ≤2.3$ eV (Mainz), $m_β ≤2.2$ eV (Troitsk).
Final Results from phase II of the Mainz Neutrino Mass Search in Tritium $\beta$ Decay · CP violation at low energies · 0.99
Cites as support 5 papers
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Yet, it has been shown [ref] , [ref] , [ref] , [ref] that successful leptogenesis is possible for $m_1 < m_*$ as well as $m_1 > m_*$, in the range from $√(Δm^2_12)$ to $√(Δm^2_23)$.
The Neutrino Mass Window for Baryogenesis · Leptogenesis · 0.97
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Yet, it has been shown [ref] , [ref] , [ref] , [ref] that successful leptogenesis is possible for $m_1 < m_*$ as well as $m_1 > m_*$, in the range from $√(Δm^2_12)$ to $√(Δm^2_23)$.
Towards a complete theory of thermal leptogenesis in the SM and MSSM · Leptogenesis · 0.97
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Yet, it has been shown [ref] , [ref] , [ref] , [ref] that successful leptogenesis is possible for $m_1 < m_*$ as well as $m_1 > m_*$, in the range from $√(Δm^2_12)$ to $√(Δm^2_23)$.
Leptogenesis for Pedestrians · Leptogenesis · 0.97
Cites as background 9 papers
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A detailed analysis on the present theoretical and experimental situation in neutrino physics and on where it is going in the future is done in Ref. [ref]
Theory of Neutrinos: A White Paper · The Lepton sector · 0.98
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The case of resonant leptogenesis is a remarkable alternative allowing for much lighter heavy neutrinos, and has recently raised a considerable interest [ref] , [ref] , [ref] .
Electroweak-Scale Resonant Leptogenesis · Leptogenesis · 0.85
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The case of resonant leptogenesis is a remarkable alternative allowing for much lighter heavy neutrinos, and has recently raised a considerable interest [ref] , [ref] , [ref] .
Resonant Leptogenesis · Leptogenesis · 0.85
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