High Energy Physics - Phenomenology · arXiv:1001.0940 v2 · submitted 6 Jan 2010 · 49 references
Common Origin of Soft mu-tau and CP Breaking in Neutrino Seesaw and the Origin of Matter
The paper says
“Neutrino oscillation data strongly support mu-tau symmetry as a good approximate flavor symmetry of the neutrino sector, which has to appear in any viable theory for neutrino mass-generation.”
more of the abstract
The mu-tau breaking is not only small, but also the source of Dirac CP-violation. We conjecture that both discrete mu-tau and CP symmetries are fundamental symmetries of the seesaw Lagrangian (respected by interaction terms), and they are only softly broken, arising from a common origin via a unique dimension-3 Majorana mass-term of the heavy right-handed neutrinos. From this conceptually attractive and simple construction, we can predict the soft mu-tau breaking at low energies, leading to quantitative correlations between the apparently two small deviations \theta_23 - 45^o and \theta_13 - 0^o. This nontrivially connects the on-going measurements of mixing angle \theta_23 with the upcoming experimental probes of \theta_13. We find that any deviation of \theta_23 - 45^o must put a lower limit on \theta_13. Furthermore, we deduce the low energy Dirac and Majorana CP violations from a common soft-breaking phase associated with mu-tau breaking in the neutrino seesaw. Finally, from the soft CP breaking in neutrino seesaw we derive the cosmological CP violation for the baryon asymmetry via leptogenesis. We fully reconstruct the leptogenesis CP-asymmetry from the low energy Dirac CP phase and establish a direct link between the cosmological CP-violation and the low energy Jarlskog invariant. We predict new lower and upper bounds on the \theta_13 mixing angle, 1^o < \theta_13 < 6^o. In addition, we reveal a new hidden symmetry that dictates the solar mixing angle \theta_12 by its group-parameter, and includes the conventional tri-bimaximal mixing as a special case, allowing deviations from it.
from the abstract
Pith says
Machine review · deepseek-v4.1-flash · 13 Nov 2026 · what was read was not recorded · not checked by a person
Reviewed in 2026 with later literature in view.
It can be wrong. Challenge this review or reply to it.
Holds up, with conditions. The structural result — δx ≥ |δa| tan θs from a real δBa/δCa, plus the Zs2 hidden symmetry — is real and worth citing; the numerical θ13 window and the leptogenesis 'link' are softer than the abstract implies. This line is wrong
3 major objections · 8 minor
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Not checked: figures, code, what the 49 references say.
The paper says, at Sec. 2.2.1 and Eq. (4.80)
The review did not quote this passage.
Pith says: Objection 1 of 3 · major
The correlation δx ≥ |δa| tan θs rests on the ratio δBa/δCa = a/(b+c) being real, which requires mD to have the exact µ-τ and CP symmetric form of Eq. (2.29). The paper argues that soft breaking can only live in MR, but does not address hard breaking in the dimension-4 Dirac Yukawa couplings.
more of objection 1
Since the charged-lepton sector already breaks µ-τ, a small hard breaking in mD is not forbidden by any symmetry. The paper should quantify how small such hard breaking must be for Eq. (4.80) to survive at the accuracy of upcoming θ13 and θ23 measurements. A concrete test: add a small parameter ε to mD and compute the induced imaginary part of δBa/δCa and the resulting modification of Eq. (4.79a).
The paper says, at Sec. 4.2 and abstract
The review did not quote this passage.
Pith says: Objection 2 of 3 · major
The upper bound θ13 ≲ 6° is not derived from the symmetry structure; it follows from the assumed range ζ ∈ [0, 0.6] used in Fig. 1. The text says 'for ζ ∈ [0, 0.6], an upper bound θ13 ≲ 6° holds for most of the parameter space', but the abstract states '1° < θ13 < 6°' as a prediction. The abstract and conclusions should state the prior dependence explicitly, or the authors should derive a symmetry-based upper bound.
The paper says, at Sec. 5.3 and abstract
The review did not quote this passage.
Pith says: Objection 3 of 3 · major
The 'direct link' between the leptogenesis CP asymmetry and the low-energy Jarlskog invariant is a consequence of the single-phase assumption: both ε1 and δD are functions of ω. The abstract's 'establish a direct link' suggests a general result, but it is model-specific. Similarly, 'fully reconstruct the leptogenesis CP-asymmetry from the low energy Dirac CP phase' overstates: Eq. (5.122) shows ε1 depends on δD plus r, ζ, M1, m̂3. The text should be qualified.
8 minor objections
The paper says, at Eq. (4.78)
Pith says: minor objection 1 of 8
The factor √2 appears inconsistent with Eq. (6.151); the correct relation is 1/k = pk tan θs/√2. This does not affect (4.79a) or (4.80), but should be corrected.
The paper says, at Eq. (4.101)
Pith says: minor objection 2 of 8
'cos 2θx' should be 'cos θx' (or cos²θx); the small-θx expansion quoted is consistent with cos θx.
show 6 more
The paper says, at Eq. (5.115)
Pith says: minor objection 3 of 8
The symbol m1 is used for the leptogenesis efficiency parameter, clashing with the light neutrino mass m1 = 0. Use a different symbol (e.g., m̃1).
The paper says, at Abstract and Sec. 1
Pith says: minor objection 4 of 8
'the µ-τ symmetry ... has to appear in any viable theory for neutrino mass-generation' is too strong; µ-τ is an approximate empirical pattern, not a theorem.
The paper says, at Abstract
Pith says: minor objection 5 of 8
'1° < θ13 < 6°' uses strict inequalities, while the text uses '≲'. Align.
The paper says, at Sec. 6.3
Pith says: minor objection 6 of 8
The Zs2 symmetry 'dictates' θ12 only up to the free group parameter k; the paper acknowledges this in the text, but the abstract's 'dictates' is misleading. Consider 'parametrizes'.
The paper says, at Fig. 1a
Pith says: minor objection 7 of 8
The vertical axis extends to 7° while the text quotes 6°; clarify whether the 6° is a hard bound or a bulk feature.
The paper says, at Footnote 16 and Ref. [47]
Pith says: minor objection 8 of 8
These are unpublished; the claims they support (extensions lowering the ηB power-dependence, further explorations) should be flagged as future work, not results.
What would settle it
Introduce a small μ-τ and CP breaking perturbation in mD, e.g., replace a → a(1 + ε e^{iφ}) with ε = 0.01, 0.05, 0.1, and recompute δBa/δCa and the resulting δx–δa correlation from Eqs. (2.34) and (4.76). If the lower bound Eq. (4.80) shifts by more than 20% for ε = 0.05, the prediction is not robust to the conjecture. Alternatively, work out the S4 completion mentioned in Sec. 6.3 and check whether it enforces exact μ-τ and CP in mD at the renormalizable level.
from the skeptic's reading
How the review went
4 readings by deepseek-v4.1-flash · 13 Nov 2026
- Reader holds up, with conditions
- Skeptic agrees
- Editor wrote the verdict above
- Referee major revision: 3 major objections, 8 minor
Not run on this paper: the simulated authors' defence.
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The review in full
The review in brief, machine-written
The thing to know first: the clean part of this paper is not the numerical bounds, it is a structural argument. Assume the Dirac Yukawa sector is exactly mu-tau and CP symmetric and confine all breaking to the heavy Majorana mass matrix. Then the ratio of the two mu-tau-antisymmetric entries of the light mass matrix is real and fixed by mD alone, which yields δx ≥ |δa| tan θs (Eq. 4.80) with no knowledge of the soft-breaking parameters. That is derived, not fitted, and it is the piece I would actually use. The second genuinely new piece is the Zs2 hidden symmetry in Sec. 6.3: the 3x3 representation Ts(k), the reading of it as a reflection about a plane, the rank-2 theorem for the general three-neutrino seesaw, and tri-bimaximal mixing falling out at k=2. That is tidy work. They also credit [44] for the earlier observation that θ12 survives mu-tau breaking, which is the right thing to do. Soft spots, in order of weight. The conjecture is stated openly (abstract:s2, Sec. 2.2.1), so I will not call it hidden, but the paper never asks how much hard mu-tau or CP breaking in the dimension-4 Yukawa couplings it can absorb. The charged leptons already break mu-tau; nothing forbids the neutrino Yukawas from doing the same at the few-percent level, and that would put an imaginary part into δBa/δCa and soften Eq. 4.80. A short tolerance estimate would have made the word 'prediction' defensible. The 1° ≲ θ13 ≲ 6° window is softer than the abstract suggests: it comes from scanning ζ, r < 0.6 and |b±c| in [1,300] GeV, not from a sharp derivation. The note added in proof is awkward — the updated fit's central θ13 = 6.8° sits above their own upper bound and they wave it off in one line; that deserved a paragraph. And the leptogenesis 'direct link' is largely by construction, since one phase ω feeds both δD and ε1. Who should read it: neutrino model builders working on mu-tau and discrete symmetries, and anyone connecting leptogenesis to low-energy CP. Worth a serious referee — the structural claims are checkable and the numerical ones need tightening.
The strongest objection
The paper's central prediction, Eq. (4.80) δx ≥ |δa| tan θs, follows from the ratio δBa/δCa = a/(b+c) being real (Eq. 2.48). This ratio is exact only if mD has the form in Eq. (2.29), which assumes exact μ-τ and CP symmetry in the Dirac Yukawa couplings. The paper argues in Sec. 2.2.1 that soft breaking can only live in the dimension-3 Majorana mass term, but that is an argument about soft breaking in the technical sense; it does not forbid small hard breaking in the dimension-4 Dirac Yukawa couplings. The charged-lepton sector already breaks μ-τ symmetry (m_μ ≠ m_τ), so there is no symmetry that forbids the neutrino Dirac Yukawa couplings from also carrying small μ-τ or CP breaking. If such breaking exists at even the few-percent level, δBa/δCa acquires an imaginary part, and the phase relation (4.79a) is modified, weakening or destroying the lower bound. The paper does not quantify the tolerance. This is the load-bearing concern because the entire chain—the δx–δa correlation, the leptogenesis link, and the θ13 bounds—rests on the single-parameter structure that this conjecture provides.
I agree with the reader's assessment. The paper is internally consistent and the derivations are clean, but the central claim is conditional on the conjecture that the Dirac Yukawa sector is exactly μ-τ and CP symmetric. The paper argues this is the only place soft breaking can occur, but that argument is about soft breaking in the technical sense, not about hard breaking in the Dirac Yukawa couplings. The charged-lepton sector already breaks μ-τ symmetry, so there is no symmetry that forbids small hard breaking in the neutrino Dirac Yukawa couplings. The paper does not quantify how small such breaking must be for the correlation to survive. I also note the upper bound θ13 ≲ 6° is not a sharp prediction: Eq. (4.98a) has a near-divergence at ζ ≈ 2r cos δD, and the bound depends on the assumed range ζ < 0.6. The updated fit's central value θ13 = 6.8° is above the predicted upper bound, and the authors' claim of 'no visible correction' is questionable. However, these are secondary to the model assumption. The Zs2 symmetry is a genuine structural observation, though the fact that θ12 is unaffected by μ-τ breaking was noted earlier in [44]. Overall, the verdict should remain CONDITIONAL.
The referee's report
If the conjecture holds, the paper provides a falsifiable link between the ongoing θ23 measurements and the upcoming θ13 probes, and between low-energy CP violation and leptogenesis. The Zs2 symmetry is an interesting structural observation that unifies the TBM ansatz with a one-parameter family of solar mixings. The derivations are technically detailed and largely checkable, and the paper is explicit that the common-origin structure is a conjecture.
Pith's reading of the paper (a machine's summary, not the authors')
The paper asks whether two apparently unrelated small numbers in neutrino physics — the failure of the atmospheric angle to sit exactly at $45^circ$ and the failure of $theta_{13}$ to vanish — are in fact the same number seen twice. The authors' proposal is that the seesaw Lagrangian respects both a discrete $mu$–$tau$ exchange symmetry and CP exactly in its interaction terms, and that both are broken only softly, by one complex entry in the dimension-3 Majorana mass matrix of the heavy right-handed neutrinos. If that is right, a single phase controls the size of the $mu$–$tau$ breaking and simultaneously supplies the Dirac and Majorana CP phases at low energy and the CP asymmetry that leptogenesis needs to make the baryon asymmetry. The payoff is a testable inequality: any measured deviation of $theta_{23}$ from $45^circ$ forces a minimum $theta_{13}$, so the ongoing atmospheric-angle measurements and the upcoming reactor $theta_{13}$ probes become two views of one parameter. The paper also isolates a separate exact $Z_2$ symmetry of the Dirac mass matrix that fixes the solar angle $theta_{12}$ from a single group parameter and contains tri-bimaximal mixing as the special case $k=2$.
What carries the argument. The load-bearing object is the single complex soft-breaking parameter $zeta e^{iomega}$ placed in the $mu$–$tau$-symmetric heavy Majorana mass matrix, together with the claim that this is the unique such location: the off-diagonal entries are forced equal by symmetry, and the Dirac mass matrix is generated by dimension-4 Yukawa interactions, so it cannot host a soft breaking. Splitting the light neutrino mass matrix into $mu$–$tau$ symmetric and antisymmetric parts makes the argument concrete: the antisymmetric entries $delta B_a$ and $delta C_a$ both carry the factor $(M_{22}-M_{33})$, and their ratio collapses to $a/(b+c)$, a number fixed entirely by the Dirac matrix and independent of the breaking. That ratio is then shown to equal $1/k$ where $tan theta_s = sqrt{2}/|k|$, which is why the $theta_{13}$–$theta_{23}$ correlation and the solar-angle prediction come from the same algebraic fact. The second piece of machinery is the hidden $Z_2$ symmetry with three-dimensional orthogonal representation $T_s(k)$ built from $k = (b+c)/a$; it leaves the Dirac mass matrix invariant, acts as a reflection about a plane in flavour space, and protects $theta_{12}$ from any soft breaking in $M_R$.
Core claim. The central claim is a common-origin conjecture: $mu$–$tau$ and CP are exact symmetries of the seesaw interaction terms, and the only place they can be softly broken is the dimension-3 singlet Majorana mass term of the heavy right-handed neutrinos. In the minimal two-right-handed-neutrino seesaw this reduces to one complex parameter, $M_{33} = M_{22}(1 - zeta e^{iomega})$, breaking both symmetries at once. Expanding in the small parameters $r$ and $zeta$ and matching the model's next-to-leading-order mass matrix against a model-independent reconstruction from oscillation data, the authors derive $delta_a / delta_x = -cot theta_s cos delta_D$ with $delta_a equiv theta_{23} - 45^circ$ and $delta_x equiv theta_{13}$, which yields the inequality $theta_{13} gtrsim |theta_{23} - 45^circ| tan theta_{12}$. Because the same phase $omega$ sets the low-energy Dirac phase through $delta_D = 2pi - omega$, the leptogenesis CP asymmetry $epsilon_1$ is reconstructed from the low-energy Dirac phase, giving $eta_B / M_1 < 2 times 10^{-23}$ GeV$^{-1}$ and hence $M_1 gtrsim 3 times 10^{13}$ GeV. Scanning the parameters against current oscillation data, the authors quote $1^circ lesssim theta_{13} lesssim 6^circ$, with the lower bound sharpened once successful leptogenesis is imposed.
The premise it rests on. The whole construction rests on the conjecture that $mu$–$tau$ and CP are exact symmetries of the Dirac Yukawa interactions and are broken only in the heavy neutrinos' Majorana mass term; if the Yukawa sector carries any small breaking of its own, the single-parameter link between $theta_{13}$, $theta_{23}$ and the leptogenesis phase is lost.
If the paper is right (Pith's inferences, not the authors')
A precise measurement of $theta_{23}$ away from $45^circ$ converts into a hard lower bound on $theta_{13}$ through $theta_{13} gtrsim |theta_{23} - 45^circ| tan theta_{12}$, so Daya Bay, RENO and Double Chooz would either confirm the correlation or close the scenario.
Successful thermal leptogenesis in this construction requires $M_1 gtrsim 3 times 10^{13}$ GeV, which is a lower bound on the seesaw scale derivable from the observed baryon asymmetry alone.
The model predicts an upper bound on the neutrinoless double-beta observable, $|m_{ee}| lesssim 3.4$ meV, since the lightest neutrino is massless in the normal hierarchy.
Because the leptogenesis asymmetry is reconstructed from the low-energy Dirac phase, the cosmological CP violation and the Jarlskog invariant $J$ are tied, so a nonzero $J$ places a floor on $theta_{13}$ as well.
The hidden $Z_2$ symmetry contains tri-bimaximal mixing as the case $k=2$ and admits other values such as $k = 3sqrt{2}$ giving $theta_{12} approx 33.7^circ$, so the solar angle becomes a discrete label rather than a continuous input.
If the correlation holds, the two-decade-old tendency of fits to prefer $theta_{23}$ slightly below $45^circ$ is not a statistical accident but a fingerprint of the sign of $cos delta_D$, since the model ties the sign of $theta_{23} - 45^circ$ to $-cos delta_D$.
The claim that soft breaking cannot live in the Yukawa sector is an argument about where it can occur, not that it must be confined there; a small $mu$–$tau$ or CP admixture in the Dirac couplings would decohere the single-parameter link and could be probed by how tightly the $theta_{13}$–$theta_{23}$ band closes.
Since the same phase drives both the low-energy Dirac phase and the leptogenesis asymmetry, an independent determination of $delta_D$ from long-baseline oscillation and of $eta_B$ from cosmology would over-determine the single parameter, giving a consistency check rather than a fit.
The hidden $Z_2$ symmetry's rank-2 Dirac matrix forces one massless light neutrino, so the scenario inherits the minimal-seesaw prediction of vanishing $m_1$; a confirmed inverted hierarchy or a quasidegenerate light spectrum would rule out this whole line of construction.
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The paper
Abstract
Neutrino oscillation data strongly support mu-tau symmetry as a good approximate flavor symmetry of the neutrino sector, which has to appear in any viable theory for neutrino mass-generation. The mu-tau breaking is not only small, but also the source of Dirac CP-violation. We conjecture that both discrete mu-tau and CP symmetries are fundamental symmetries of the seesaw Lagrangian (respected by interaction terms), and they are only softly broken, arising from a common origin via a unique dimension-3 Majorana mass-term of the heavy right-handed neutrinos. From this conceptually attractive and simple construction, we can predict the soft mu-tau breaking at low energies, leading to quantitative correlations between the apparently two small deviations \theta_23 - 45^o and \theta_13 - 0^o. This nontrivially connects the on-going measurements of mixing angle \theta_23 with the upcoming experimental probes of \theta_13. We find that any deviation of \theta_23 - 45^o must put a lower limit on \theta_13. Furthermore, we deduce the low energy Dirac and Majorana CP violations from a common soft-breaking phase associated with mu-tau breaking in the neutrino seesaw. Finally, from the soft CP breaking in neutrino seesaw we derive the cosmological CP violation for the baryon asymmetry via leptogenesis. We fully reconstruct the leptogenesis CP-asymmetry from the low energy Dirac CP phase and establish a direct link between the cosmological CP-violation and the low energy Jarlskog invariant. We predict new lower and upper bounds on the \theta_13 mixing angle, 1^o < \theta_13 < 6^o. In addition, we reveal a new hidden symmetry that dictates the solar mixing angle \theta_12 by its group-parameter, and includes the conventional tri-bimaximal mixing as a special case, allowing deviations from it.
The paper's own sentences, arranged, kept beside the review and separate from it. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. No sentence in this record was written by a model.
abstract compiled · 2026-09-23
The authors' main claim, as the classifier picked it out 0.72
“We conjecture that both discrete mu-tau and CP symmetries are fundamental symmetries of the seesaw Lagrangian (respected by interaction terms), and they are only softly broken, arising from a common origin via a unique dimension-3 Majorana mass-term of the heavy right-handed neutrinos.”
How the main claim is stated: speculative 1.00
What the abstract itself states, as probabilities: claims first 0.05 · states limitation 0.13 · human participants 0.02 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.98 · compares with prior results 0.12 · mentions code or data availability 0.01
The abstract, sentence by sentence
This table labels the abstract only (arXiv listing abstract v2). The number is the probability the classifier gave the label.
| Sentence | Role | The authors' own work | States the main conclusion | Strength |
|---|---|---|---|---|
| Neutrino oscillation data strongly support mu-tau symmetry as a good approximate flavor symmetry of the neutrino sector, which has to appear in any viable theory for neutrino mass-generation. | background 1.00 | 0.06 | 0.05 | asserted 0.96 |
| The mu-tau breaking is not only small, but also the source of Dirac CP-violation. | background 0.76 | 0.17 | 0.10 | asserted 1.00 |
| We conjecture that both discrete mu-tau and CP symmetries are fundamental symmetries of the seesaw Lagrangian (respected by interaction terms), and they are only softly broken, arising from a common origin via a unique dimension-3 Majorana mass-term of the heavy right-handed neutrinos. | contribution 0.91 | 0.48 | 0.43 | speculative 1.00 |
| From this conceptually attractive and simple construction, we can predict the soft mu-tau breaking at low energies, leading to quantitative correlations between the apparently two small deviations \theta_{23} - 45^o and \theta_{13} - 0^o. | result 0.71 | 0.89 | 0.28 | asserted 0.84 |
| This nontrivially connects the on-going measurements of mixing angle \theta_{23} with the upcoming experimental probes of \theta_{13}. | interpretation 0.90 | 0.58 | 0.11 | asserted 0.93 |
| We find that any deviation of \theta_{23} - 45^o must put a lower limit on \theta_{13}. | result 0.99 | 0.92 | 0.18 | asserted 1.00 |
| Furthermore, we deduce the low energy Dirac and Majorana CP violations from a common soft-breaking phase associated with mu-tau breaking in the neutrino seesaw. | result 0.89 | 0.94 | 0.14 | asserted 1.00 |
| Finally, from the soft CP breaking in neutrino seesaw we derive the cosmological CP violation for the baryon asymmetry via leptogenesis. | contribution 0.59 | 0.92 | 0.17 | asserted 1.00 |
| We fully reconstruct the leptogenesis CP-asymmetry from the low energy Dirac CP phase and establish a direct link between the cosmological CP-violation and the low energy Jarlskog invariant. | result 0.80 | 0.94 | 0.19 | asserted 1.00 |
| We predict new lower and upper bounds on the \theta_{13} mixing angle, 1^o < \theta_{13} < 6^o. | result 1.00 | 0.93 | 0.18 | asserted 0.99 |
| In addition, we reveal a new hidden symmetry that dictates the solar mixing angle \theta_12 by its group-parameter, and includes the conventional tri-bimaximal mixing as a special case, allowing deviations from it. | result 0.86 | 0.90 | 0.09 | asserted 1.00 |
What kind of paper the classifier reports this is: theoretical result 1.00 · evidence from proof or derivation 0.90
What was examined, and what was not
Sources read
- arXiv listing abstract v2
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
How the labels were made
Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 8,586 input tokens, $0.0004 reported.
Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. This record as JSON
Figures (11)
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References (49)
- [44] W. Grimus, A. S. Joshipura, S. Kaneko, L. Lavoura, H. Saw anaka, M. Tanimoto, Nucl. Phys. B 713, 151 (2005) [arXiv:hep-ph/0408123] on PithPith's reviewarXiv
- [1] For recent reviews, e.g., A. Yu. Smirnov, arXiv:0910.1778, arXiv:0810.2668, arXiv: hep- ph/0702061; G. Altarelli, Nuovo Cim. 032 C, 91 (2009) [arXiv:0905.3265]; M. Dierckxens, arXiv:0911.1039 [hep-ex]; R. N. Mohapatra and A. Yu. Smirno v, Ann. Rev. Nucl. Part. Sci. 56, 569 (20... on PithPith's reviewarXiv
- [2] B. Pontecorvo, Sov. Phys. JETP 6, 429 (1957); Z. Maki, M. Nakagawa and S. Sakata, Prog. Theor. Phys. 28, 870 (1962) on Pith
- [3] G. L. Fogli, E. Lisi, A. Marrone, A. Palazzo, and A. M. Rotu nno, Phys. Rev. Lett. 101, 141801 (2008) [arXiv:0806.2649] and arXiv:0809.2936 [hep-ph]; G . L. Fogli et al. , arXiv:0805.2517v3 [hep-ph] and Phys. Rev. D 78, 033010 (2008); and references therein on PithPith's reviewarXiv
- [4] G. L. Fogli, E. Lisi, A. Marrone, A. Palazzo, Prog. Part. N ucl. Phys. 57, 742 (2006) [arXiv:hep- ph/0506083]; G. L. Fogli, E. Lisi, A. Palazzo, Phys. Rev. D 65, 073019 (2002) [arXiv:hep- ph/0105080] on Pith
- [5] G. L. Fogli and E. Lisi, private communications about the global analyses in Refs. [3, 4] on Pith
- [6] See, for instance, the experimental reports at XXIII Int ernational Conferences on “Neutrino Physics and Astrophysics” (Neutrino 2008), Christchurch, New Zealand, May 25-31, 2008. Web link: www2.phys.canterbury.ac.nz/˜jaa53 on Pith
- [7] A. Yu. Smirnov, private communication; M. C. Gonzalez-G arcia, M. Maltoni and A. Yu. Smirnov, Phys. Rev. D 70, 093005 (2004) [arXiv:hep-ph/0408170]; A. Yu. Smirnov, ta lk at Neutrino-2008 [6]; O. L. G. Peres and A. Yu. Smirnov, Phys. Rev. D 79, 113002 (2009) [arXiv:0903.5323] on PithPith's reviewarXiv
- [8] G. L. Fogli, E. Lisi, A. Marrone, A. Palazzo, and A. M. Rotu nno, arXiv:0905.3549 on PithPith's reviewarXiv
- [9] P. Minkowski, Phys. Lett. B 67, 421 (1977); T. Yanagida, in Proceedings of Workshop on Unifi ed Theories and Baryon Number in the Universe, p.95, eds. O. Saw ada and A. Sugamoto, Japan, Feb. 13-14, 1979; S. L. Glashow, in Proceedings of the 1979 Ca rgese Summer Institute on Qua... on Pith
- [10] For quark-lepton complementarity hypothesis, A. Yu. S mirnov, arXiv:hep-ph/0402264, in Pro- ceedings of “2nd International Workshop on Neutrino Oscill ations” (Venice-2003), p.1-21, in Venice, Italy, Dec. 3-5 2003; M. Raidal, Phys. Rev. Lett. 93, 161801 (2004) [arXiv:hep- ph/0404046] on PithPith's reviewarXiv
- [11] E.g., R. N. Mohapatra and A. Yu. Smirnov in Ref. [1] for a r ecent review including µ−τ symmetry studies, and references therein on Pith
- [12] N. Cabibbo, Phys. Rev. Lett. 10, 531 (1963); M. Kobayashi and T. Maskawa, Prog. Theor. Phys. 49, 652 (1973) on Pith
- [13] C. Amsler et al. , [Particle Data Group], Physs Lett. B 667, 1 (2008). 58 on Pith
- [14] C. Palomares, [Double-Chooz Collaboration], EPS-HEP -2009, arXiv:0911.3227; F. Ardellier et al. , [Double Chooz Collaboration], arXiv:hep-ex/0606025; F. Ardellier et al. , arXiv:hep- ex/0405032 on PithPith's reviewarXiv
- [15] Y.-F. Wang, arXiv:hep-ex/0610024 and private communi cations; W. Wang [Daya Bay Collabora- tion], arXiv:0910.4605 [hep-ex]; M.-C. Chu [Daya Bay Colla boration], arXiv:0810.0807 [hep-ex]; J. Cao [Daya Bay Collaboration], Nucl. Phys. Proc. Suppl. 155, 229 (2006); For the web lin... on PithPith's reviewarXiv
- [16] S. B. Kim [RENO Collaboration], AIP Conf. Proc. 981, 205 (2008) [J. Phys. Conf. Ser. 120, 052025 (2008)]; J. K. Ahn et al., [RENO Collaboration], arXiv:1003.1391 on PithPith's reviewarXiv
- [17] D. S. Ayres et al. , [NO νA Collaboration], hep-ex/0503053. R. Roy [NO νA Collaboration], J. Phys. (Conf. Series) 136, 022019 (2008) on PithPith's reviewarXiv
- [18] Y. Itow et al. , [T2K Collaboration], arXiv:hep-ex/0106019 on PithPith's reviewarXiv
- [19] J. Peltoniemi, arXiv:0911.4876 [hep-ex], and referen ces therein on PithPith's reviewarXiv
show 29 more
- [20] P. Adamson et al. , [MINOS Collaboration], arXiv:arXiv:0909.4996 and Phys. Rev. Lett. 101, 131802 (2008) [arXiv:0806.2237] on PithPith's reviewarXiv
- [21] E.g., see the report “Physics at a future neutrino facto ry and super-beam facility”, [The ISS Physics Working Group], arXiv:0710.4947; D. M. Kaplan, arX iv:physics/0507023 [physics.acc- ph], in the proceedings of Lepton-Photon-2005 Conference, Uppsala, Sweden on PithPith's reviewarXiv
- [22] B. Aharmin et al., [SNO Collaboration], arXiv:0910.2984; Phys. Rev. Lett. 101, 111301 (2008) [arXiv:0806.0989] on PithPith's reviewarXiv
- [23] S. Abe et al., [KamLand Collaboration], Phys. Rev. Lett. 100, 221803 (2008); Phys. Rev. Lett. 94, 081801 (2005) on Pith
- [24] M. Fukugita and T. Yanagida, Phys. Lett. B 174, 45 (1986) on Pith
- [25] For a recent review, W. Buchmuller, R. D. Peccei, T. Yana gida, Ann. Rev. Nucl. Part. Sci. 55, 311 (2005) [arXiv:hep-ph/0502169] on PithPith's reviewarXiv
- [26] G. Hinshaw et al. , [WMAP Collaboration], Astrophys. J. Suppl. 180, 225 (2009) [arXiv:0803.0732] on PithPith's reviewarXiv
- [27] C. Jarlskog, Phys. Rev. Lett. 55, 1039 (1985); Z. Phys. C 29, 491 (1985) on Pith
- [28] E.g., C. S. Lam, Phys. Rev. D 78, 073015 (2008) and references therein; F. Feruglio et al. , arXiv:0808.0812; F. Feruglio, private communication on PithPith's reviewarXiv
- [29] P. H. Frampton, S. L. Glashow, T. Yanagida, Phys. Lett. B 548, 119 (2002) [arXiv:hep- ph/0208157]; M. Raidal and A. Strumia, Phys. Lett. B 553, 72 (2003) [arXiv:hep-ph/0210021]. For reviews, e.g., S. L. Glashow, arXiv:hep-ph/0306100; W. L. Guo, Z. Z. Xing, S . Zhou. Int. J. Mo... on PithPith's reviewarXiv
- [30] V. Barger, D. A. Dicus, H.-J. He, T. Li, Phys. Lett. B 583, 173 (2004) [arXiv:hep-ph/0310278] on PithPith's reviewarXiv
- [31] For a recent review of 0 ν2β decays, P. Vogel, arXiv:0807.1559 [hep-ph]. 59 on PithPith's reviewarXiv
- [32] E.g., S. Antusch, J. Kersten, M. Lindner, M. Ratz, Nucl. Phys. B 674, 401 (2003) [arXiv:hep- ph/0305273]; S. Antusch, et al., JHEP 0503, 024 (2005) [arXiv:hep-ph/0501272]; J. A. Casas, J. R. Espinosa, A. Ibarra, I. Navarro, Nucl. Phys. B 573, 652 (2000) [arXiv:hep-ph/9910420];... on PithPith's reviewarXiv
- [33] For recent reviews of electroweak precision fit, e.g., J. Erler, arXiv:0907.0883; P. Langacker, arXiv:0901.0241; and references therein on PithPith's reviewarXiv
- [34] A. D. Sakharov, Sov. Phys. JETP Lett. 5, 24 (1967) on Pith
- [35] For reviews, A. Riotto and M. Trodden, Ann. Rev. Nucl. Pa rt. Sci. 49, 35 (1999); M. Trodden, arXiv:hep-ph/0411301; and references therein on PithPith's reviewarXiv
- [36] N. S. Manton, Phys. Rev. D 28, 2019 (1983); V. Kuzmin, V. A. Rubakov, M. E. Shaposhnikov, Phys. Lett. 155B, 36 (1985); J. Ambjorn, T. Askgaard, H. Porter, M. E. Shapos hnikov, Nucl. Phys. B 353, 346 (1991) on Pith
- [37] G. ’t Hooft, Phys. Rev. Lett. 37, 8 (1976); Phys. Rev. D 14, 3432 (1976) on Pith
- [38] J. A. Harvey and M. S. Turner, Phys. Rev. D 42, 3344 (1990); S. Y. Khlebnikov and M. E. Shaposhnikov, Nucl. Phys. B 308, 885 (1988) on Pith
- [39] W. Buchmuller, P. Di Bari, M. Plumacher, Annals Phys. 315, 305 (2005) [arXiv:hep- ph/0401240]; New J. Phys. 6, 105 (2004) [arXiv: hep-ph/0406014]; Nucl. Phys. B 643, 367 (2002) [arXiv:hep-ph/0205349]; and references therein on PithPith's reviewarXiv
- [40] G. F. Giudice, A. Notari, M. Raidal, A. Riotto, A. Strumi a, Nucl. Phys. B 685, 89 (2004) [arXiv:hep-ph/0310123]; A. Strumia, arXiv:hep-ph/06083 47; and references therein on PithPith's reviewarXiv
- [41] P.-H. Gu and H.-J. He, JCAP 0612, 010 (2006) [arXiv:hep-ph/0610275] on PithPith's reviewarXiv
- [42] P. Huber, M. Lindner, T. Schwetz, W. Winter JHEP 0911, 044 (2009) [arXiv:0907.1896]; M. Mezzetto and T. Schwetz, arXiv:1003.5800 [hep-ph] on PithPith's reviewarXiv
- [43] W. Grimus and L. Lavoura, JHEP 0107, 045 (2001) [arXiv:hep-ph/0105212] on PithPith's reviewarXiv
- [45] P. F. Harrison, D. H. Perkins, W. G. Scott, Phys. Lett. B 458, 79 (1999) [arXiv:hep-ph/9904297]; B 530, 167 (2002) [arXiv:hep-ph/0202074] on PithPith's reviewarXiv
- [46] C. S. Lam, Phys. Rev. D 78, 073015 (2008) [arXiv:0809.1185]; and references therein on PithPith's reviewarXiv
- [47] D. A. Dicus, S.-F. Ge, H.-J. He, work to appear on Pith
- [48] M. C. Gonzalez-Garcia, M. Maltoni, J. Salvado, arXiv:1 001.4524 [hep-ph] on Pith
- [49] R. N. Mohapatra and W. Rodejohann, Phys. Rev. D 72, 053001 (2005) [arXiv:hep-ph/0507312]. 60 on PithPith's reviewarXiv
Cited by 12 Pith papers
Reviewed papers on Pith that cite this one. The full citation record
- Lepton Mixing Patterns from a Scan of Finite Discrete Groups hep-ph · Dec 2012
- Common Origin of mu-tau and CP Breaking in Neutrino Seesaw, Baryon Asymmetry, and Hidden Flavor Symmetry hep-ph · Apr 2011
- Z_2 Symmetry Prediction for the Leptonic Dirac CP Phase hep-ph · Apr 2011
- Measuring the Leptonic CP Phase in Neutrino Oscillations with Non-Unitary Mixing hep-ph · May 2016
- Lepton mixing and discrete symmetries hep-ph · Apr 2012
- Neutrino Mass, Dark Matter and Anomalous Magnetic Moment of Muon in a $U(1)_{L_{\mu}-L_{\tau}}$ Model hep-ph · Aug 2016
- Phenomenological Study of Residual Z^s_2 and Zbar^s_2 Symmetries hep-ph · Aug 2013
- Phenomenology of Lepton Masses and Mixing with Discrete Flavor Symmetries hep-ph · Oct 2023
- The minimal seesaw and leptogenesis models hep-ph · Aug 2020
- Residual Symmetries for Neutrino Mixing with a Large theta_13 and Nearly Maximal delta_D hep-ph · Aug 2011
- Discrete Flavor Symmetries and Models of Neutrino Mixing hep-ph · Feb 2010
- A review of mu-tau flavor symmetry in neutrino physics hep-ph · Dec 2015
How the literature uses it
36 arXiv papers cite this in 85 sentences
Papers citing it · 58 sentences without a confident label
Builds on it 1 paper
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In this subsection, we will extend two of our seesaw constructions [ref] to the present visible and mirror neutrino sectors, where the $$ and $CP$ symmetry breakings naturally arise from a common origin.
Spontaneous Mirror Parity Violation, Common Origin of Matter and Dark Matter, and the LHC Signatures · Explicit Seesaw Realizations of Visible/Dark Matter Genesis · 1.00
Uses its data or values 1 paper
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The coefficient $χ_1^=χ(M_1^,M_Z^)$ in ([ref]) is a renormalization group running factor which evolves $m_3^$ from weak scale $M_Z^$ up to the leptogenesis scale $M_1^$, and is found to be about $1.3-1.4$ for $M_1=10^13-10^16$GeV [ref] .
Spontaneous Mirror Parity Violation, Common Origin of Matter and Dark Matter, and the LHC Signatures · Visible/Mirror Seesaws with Common Soft $$ and $CP$ Breaking · 0.83
Compares with it 3 papers
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These distinctive predictions of the present $$ blind seesaw can be systematically tested against those of our previous soft $$ breaking seesaw [ref] , by the on-going and upcoming neutrino experiments.
Common Origin of mu-tau and CP Breaking in Neutrino Seesaw, Baryon Asymmetry, and Hidden Flavor Symmetry · Conclusion · 0.96
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Eqs. [ref] and [ref] coincide with relations obtained in [ref] .
Lepton mixing and discrete symmetries · Symmetries and constraints on mixing · 0.99
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The difference is that an expansion method was used in [ref] while the discussion in the current work is more general and, most importantly, model-independent.
Z_2 Symmetry Prediction for the Leptonic Dirac CP Phase · Introduction · 0.99
Cites it as background 12 papers
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A notable example is the $-$ reflection symmetry [ref] that predicts the maximal 2-3 mixing $þ_23 = π/4$, the maximal Dirac phase $=̣ ±π/2$ and Majolana phases 0 or $π/2$ [ref] .
Almost general analysis of $\mu$-$\tau$ reflection symmetry perturbed by charged leptons and its testability by DUNE and T2HK · Introduction · 0.85
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The subindex $μ-τ$ in Eq. ([ref]) refers to the so-called $μ-τ$ symmetry [ref] since it satisfies the relations $|U_μi| = |U_τi|$.
Deviations to Tri-Bi-Maximal mixing in the limit of $\mu-\tau$ symmetry · Introduction · 0.91
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The neutrino mixing matrix [ref] which diagonalizes $M_ν$ via $V^TM_νV = M_ν^diag$ can be decomposed as $V=U”UU'$ [ref] where $U$ is a CKM type matrix [equation] with $(s_α,c_α) ≡ (sinθ_α,cosθ_α)$ for $α = s,a,x$ and $p=e^iδ_D$ where $δ_D$ is the Dirac phase, $U”$ is the rephasing matrix, $diag(e^iα_1,e^iα_2,e^iα_3)$ [ref] , and $U' = diag(e^-iϕ_1/2,e^-iϕ_2/2,e^-iϕ_3/2)$
Neutrino mixing with broken $S_3$ symmetry · Restrictions on the mixing angles · 0.88
What it cites · 18 sentences without a confident label
Uses the method or tool of 2 papers
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It is deduced from numerically solving the Boltzmann equation [ref] .
Towards a complete theory of thermal leptogenesis in the SM and MSSM · Matter-Antimatter Asymmetry via Leptogenesis in Neutrino Seesaw · 0.83
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It is deduced from numerically solving the Boltzmann equation [ref] .
Leptogenesis for Pedestrians · Matter-Antimatter Asymmetry via Leptogenesis in Neutrino Seesaw · 0.83
Uses data or values from 3 papers
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The current 90% C.L. limits on $θ_13$ are shown by the shaded region (yellow), while the $θ_13$ sensitivities of the upcoming Double Chooz [ref] , RENO [ref] and Daya Bay [ref] experiments to are shown by the three horizontal (red) lines at 90% C.L., as $5.0^$, $4.1^$ and $2.9^$ (from top to bottom), based on three years of data-taking.
RENO: An Experiment for Neutrino Oscillation Parameter theta_13 Using Reactor Neutrinos at Yonggwang · Reconstruction with Normal Hierarchy Mass-Spectrum of Light Neutrinos · 0.81
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The current 90% C.L. limits on $θ_13$ are shown by the shaded region (yellow), while the $θ_13$ sensitivities of the upcoming Double Chooz [ref] , RENO [ref] and Daya Bay [ref] experiments to are shown by the three horizontal (red) lines at 90% C.L., as $5.0^$, $4.1^$ and $2.9^$ (from top to bottom), based on three years of data-taking.
Double-Chooz Neutrino Experiment · Reconstruction with Normal Hierarchy Mass-Spectrum of Light Neutrinos · 0.81
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The current 90% C.L. limits on $θ_13$ are shown by the shaded region (yellow), while the $θ_13$ sensitivities of the upcoming Double Chooz [ref] , RENO [ref] and Daya Bay [ref] experiments to are shown by the three horizontal (red) lines at 90% C.L., as $5.0^$, $4.1^$ and $2.9^$ (from top to bottom), based on three years of data-taking.
Measuring Sin^22\theta_13 with the Daya Bay Nuclear Reactors · Reconstruction with Normal Hierarchy Mass-Spectrum of Light Neutrinos · 0.81
Cites as background 3 papers
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We analyze the correlations of the leptogenesis scale with the low energy observables such as the leptonic Jarlskog-invariant $J$ [ref] and neutrinoless double-beta decay parameter $M_ee$ [ref] .
Neutrino Mass and Neutrinoless Double Beta Decay · Origin of Matter from Soft $$ and CP Breaking · 0.84
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Such RG effects were extensively discussed in the literature [ref] .
Running Neutrino Masses, Mixings and CP Phases: Analytical Results and Phenomenological Consequences · Reconstruction with Normal Hierarchy Mass-Spectrum of Light Neutrinos · 0.99
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(For more details of the experimental sensitivities to $θ_13$, see a nice comparative analysis in [ref] .)
First hint for CP violation in neutrino oscillations from upcoming superbeam and reactor experiments · Reconstruction with Normal Hierarchy Mass-Spectrum of Light Neutrinos · 0.88
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