Implications of neutrino data circa 2005

Alessandro Strumia; Francesco Vissani

RECORD

Implications of neutrino data circa 2005

Alessandro Strumia, Francesco Vissani

High Energy Physics - Phenomenology · Submitted 24 Mar 2005

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim Adopting the 3 neutrino framework, we present an updated determination of the oscillation parameters.

how it is stated · asserted 0.95 read the record →

Comment (0) Read on arXiv ↗

Cite ▾

Claim paper

The compiled record

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.

Open the compiled record

Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 2,900 input tokens, $0.0001 reported.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.10 · human participants 0.02 · controlled comparison 0.03 · randomized assignment 0.01 · states quantitative result 0.06 · compares with prior results 0.48 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; show every role.

Adopting the 3 neutrino framework, we present an updated determination of the oscillation parameters. We perform a global analysis and develope simple arguments that give essentially the same result. We also discuss determinations of solar neutrino fluxes, capabilities of future experiments, tests of CPT, implications for neutrino-less double-beta decay, beta decay, cosmology.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#	sentence	role	the authors' own work	states the main conclusion	strength
s0	Adopting the 3 neutrino framework, we present an updated determination of the oscillation parameters.	contribution 0.97	0.89	0.14	asserted 0.95
s1	We perform a global analysis and develope simple arguments that give essentially the same result.	method 0.84	0.94	0.14	asserted 1.00
s2	We also discuss determinations of solar neutrino fluxes, capabilities of future experiments, tests of CPT, implications for neutrino-less double-beta decay, beta decay, cosmology.	contribution 0.73	0.54	0.08	asserted 0.76

What kind of paper the classifier reports this is: review 0.38 · evidence from analysis of existing data 1.00.

What was examined, and what was not

sources read

arXiv listing abstract v1

not examined

full text
figures and tables
references and citing sentences
relations to other papers

levels run

P abstract

not run

S sections
T body sentences
C citations
R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper

Original abstract

Adopting the 3 neutrino framework, we present an updated determination of the oscillation parameters. We perform a global analysis and develope simple arguments that give essentially the same result. We also discuss determinations of solar neutrino fluxes, capabilities of future experiments, tests of CPT, implications for neutrino-less double-beta decay, beta decay, cosmology.

Human review

How Pith checks papers → · Full audit of this paper →

References

Forward citations

Cited by 15 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

Minimal Flavor Violation in the Lepton Sector
hep-ph 2005-06 accept novelty 7.0 of 10

Extending Minimal Flavor Violation to leptons yields a framework in which charged-lepton flavor-violating rates are fixed by neutrino masses and mixing, with observable rates requiring lepton-number violation at a muc...
Neutrinoless Double Beta Decay and Heavy Sterile Neutrinos
hep-ph 2011-07 conditional novelty 6.0 of 10

Within Type I seesaw, heavy sterile neutrinos can saturate the neutrinoless double beta decay rate if light neutrino masses are suppressed beyond naive seesaw, and radiative stability then caps the heavy mass near 10 GeV.
Model-independent implications of the e+, e-, anti-proton cosmic ray spectra on properties of Dark Matter
hep-ph 2008-09 conditional novelty 6.0 of 10

Fitting all spin-allowed dark matter annihilation channels to PAMELA and balloon cosmic-ray data leaves either a leptophilic ~1 TeV particle or a >10 TeV particle annihilating to W, Z, or Higgs.
How to find neutral leptons of the nuMSM?
hep-ph 2007-05 conditional novelty 6.0 of 10

The paper derives the allowed mass and coupling window for the two GeV-scale sterile neutrinos of the nuMSM and shows which kaon, charm, and proton-beam experiments could detect or exclude them.
Yukawa sector in non-supersymmetric renormalizable SO(10)
hep-ph 2005-10 conditional novelty 6.0 of 10

In a non-supersymmetric SO(10) theory with 126 and 120 Higgs fields, the atmospheric neutrino mixing angle controls both the neutrino mass splitting and the quark mixing Vcb.

Show 10 more citing papers

Flavoring Astrophysical Neutrinos: Flavor Ratios Depend on Energy
astro-ph 2005-07 accept novelty 6.0 of 10

Energy losses of pions and muons before decay shift the cosmic neutrino flavor ratio from 1:1:1 at low energy to 1:1.8:1.8 at high energy, with the transition energy encoding source physics.
Spectra of neutrinos from dark matter annihilations
hep-ph 2005-06 accept novelty 6.0 of 10

Full-flavor neutrino spectra from dark matter annihilation in the Sun and Earth are computed for all major channels, propagated through oscillations and matter effects, and shown to carry reconstructable information a...
Tri-Bimaximal Neutrino Mixing from Discrete Symmetry in Extra Dimensions
hep-ph 2005-04 accept novelty 6.0 of 10

An A4 flavor model with the two flavon sectors localized on opposite branes of a fifth dimension reproduces the tri-bimaximal neutrino mixing matrix exactly at leading order, and a general argument shows maximal atmos...
Neutrino mass limits: robust information from the power spectrum of galaxy surveys
astro-ph.CO 2015-11 conditional novelty 5.0 of 10

Combining Planck 2015, BAO distances, and the full-shape galaxy power spectrum of SDSS-DR7 LRGs gives a 95% upper limit on the sum of neutrino masses of 0.13 eV, and WiggleZ gives 0.14 eV, showing the bound is insensi...
Flavor Composition and Energy Spectrum of Astrophysical Neutrinos
astro-ph 2007-04 accept novelty 5.0 of 10

The flavor composition of astrophysical neutrinos is energy- and model-dependent, so the standard [1,2,0] source expectation is only a first approximation and cannot support precision oscillation measurements without ...
A4 family symmetry and quark-lepton unification
hep-ph 2006-10 conditional novelty 5.0 of 10

A4 family symmetry combined with Pati-Salam unification can accommodate quark and lepton masses and tri-bimaximal neutrino mixing, with flavon vacuum alignment driven by supergravity-induced D-terms.
The next-generation liquid-scintillator neutrino observatory LENA
astro-ph.IM 2011-04 conditional novelty 4.0 of 10

LENA, a proposed 50 kt liquid-scintillator detector, would deliver a broad low-energy neutrino program and roughly tenfold better proton-decay reach, according to this design study.
Global analysis of three-flavor neutrino masses and mixings
hep-ph 2005-06 conditional novelty 3.0 of 10

A 2005 global three-neutrino fit yields updated mass-mixing ranges and finds tension between a claimed neutrinoless double-beta signal and cosmological mass bounds.
Explosion Mechanism, Neutrino Burst, and Gravitational Wave in Core-Collapse Supernovae
astro-ph 2005-09 accept novelty 2.0 of 10

The review consolidates the case that neutrino heating plus multidimensional effects (convection, rotation, magnetic fields) is the leading core-collapse explosion mechanism, and lays out how neutrino and gravitationa...
Massive neutrinos and cosmology
astro-ph 2006-03 accept novelty 1.0 of 10

A detailed review of how cosmological observations bound the sum of neutrino masses through the free-streaming suppression of small-scale structure, and of future sensitivity forecasts.

How the literature uses it

4 arXiv papers cite this in 6 sentences

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

Papers whose main result relates to this one's

Found among the papers closest to this one by title and main claim. Pith's classifier compared each pair's main results and a second model family confirmed the relation; checked against two further families, shown conflicts agreed 118 times in 120 and shown same results 218 times in 239. The quoted sentence is the other paper's main claim.

States the same result 1 paper

The results of a global analysis within the three-flavour framework are presented.

Neutrino oscillations: Current status and prospects · 0.86

Papers citing it · 3 sentences without a confident label

Uses its data or values 2 papers

A global fit [ref] at 99% C.L. gives $1.1×10^-3eV≤⟨m_ee⟩≤4.5×10^-3eV$(normal hierarchy) or $1.2×10^-3eV≤⟨m_ee⟩≤5.7×10^-3eV$(inverted hierarchy).

Search for Majorana Neutrino Signal in $B_c$ Meson Rare Decay · introduction · 0.98
For a numerical estimate one can take [ref] $sin^2θ_12≃0.3$, leading to $x≃0.35 i e^i(δ_1-δ_2-δ_3)$ and to $f_e^2/(f_μ^2+f_τ^2)∼0.05$.

How to find neutral leptons of the nuMSM? · The Lagrangian and parameters of the $ν$MSM · 1.00

Discussion

Know something about this paper? Leave a comment, or highlight any passage above to comment on it.