Massive right-handed neutrinos in bar{B} to D^* τ bar X decay
Pith reviewed 2026-06-27 03:43 UTC · model grok-4.3
The pith
Full differential distributions in B to D* tau X decays reveal signatures of massive right-handed neutrinos through their sensitivity to new physics operators.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
We explore signatures of a massive right-handed neutrino (RHN) in angular distributions of B-bar to D-star (to D pi) tau (to pi nu_tau) X-bar decays, where X is an invisible state. We assume the new physics is described by the standard model effective field theory extended with an RHN in the MeV-GeV mass range. We calculate for the first time the full differential distributions in terms of the visible final states, including the decay of the tau lepton. We evaluate the sensitivity of various distributions to the new physics operators.
What carries the argument
The full differential distributions in visible final-state variables of the B to D* tau X decay chain, computed in SMEFT extended by a massive right-handed neutrino.
If this is right
- Certain angular distributions become sensitive probes of the new operators generated by the right-handed neutrino.
- The visible final-state kinematics allow experiments to set limits on the strength of these operators for right-handed neutrino masses in the MeV-GeV window.
- The calculation supplies templates that can be directly folded with detector efficiencies and used in fits to existing or future data sets.
- Different operators produce distinct patterns across the set of distributions, offering a way to discriminate among them.
Where Pith is reading between the lines
- The same method of computing full visible-state distributions could be applied to other modes such as B to D tau X or semileptonic decays of other heavy mesons to test the same right-handed neutrino hypothesis.
- Absence of signals in these distributions would translate into upper bounds on the mixing parameters between the right-handed neutrino and active neutrinos within the effective theory.
- Combining the angular information with rate measurements or with searches in other channels could tighten the overall constraints on the right-handed neutrino parameter space.
Load-bearing premise
All new physics effects are captured by the standard model effective field theory extended with a right-handed neutrino whose mass is in the MeV to GeV range.
What would settle it
A precision measurement of the angular and kinematic distributions in B to D* tau X that shows no deviation from standard model predictions in the directions predicted by the right-handed neutrino operators would falsify the existence of detectable signatures at the level claimed.
read the original abstract
We explore signatures of a massive right-handed neutrino (RHN) in angular distributions of $\bar{B} \to D^* (\to D \pi) \tau (\to \pi \nu_\tau ) \bar X$ decays, where $X$ is an invisible state. We assume the new physics is described by the standard model effective field theory extended with an RHN in the MeV-GeV mass range. We calculate for the first time the full differential distributions in terms of the visible final states, including the decay of the $\tau$ lepton. We evaluate the sensitivity of various distributions to the new physics operators.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript explores signatures of a massive right-handed neutrino (RHN) in angular distributions of the decay ar{B} o D^* ( o D \pi) au ( o \pi u_ au) ar X, where X is invisible. It assumes new physics is described by SMEFT extended with an RHN in the MeV-GeV mass range, claims to calculate for the first time the full differential distributions in visible final states including the au decay, and evaluates sensitivity of various distributions to the new physics operators.
Significance. If the differential calculations are correct and the operator sensitivity analysis holds, the work supplies new predictions for visible-state distributions that can be directly compared to data, strengthening probes of RHN in the MeV-GeV window at Belle II and LHCb. The emphasis on full visible kinematics is a concrete advance over prior partial calculations.
minor comments (1)
- Abstract states the calculation is performed 'for the first time'; the introduction should explicitly contrast the new visible-state distributions against prior literature on B o D^* au u with RHN or SMEFT operators to substantiate the novelty claim.
Simulated Author's Rebuttal
We thank the referee for their review of our manuscript. The report acknowledges the potential value of our full visible-state differential distributions if the calculations are correct, but provides no specific major comments or points of technical concern. We address this below.
- The referee's recommendation is listed as 'uncertain' and the significance is conditional on the correctness of the differential calculations, yet no concrete issues, errors, or requests for clarification are identified in the report. Without specific points we cannot provide a targeted response or revision.
Circularity Check
No significant circularity; forward calculation of distributions
full rationale
The paper computes full differential distributions for visible final states in B to D* tau decay including massive RHNs in SMEFT. The central claim is a first-time calculation of these distributions and their sensitivities to operators. No equations, parameters, or results are shown to reduce to fitted inputs, self-definitions, or self-citation chains. The derivation is presented as an independent forward computation from the effective Lagrangian to observable distributions, with no load-bearing steps that collapse by construction to the inputs.
Axiom & Free-Parameter Ledger
axioms (1)
- domain assumption New physics is described by SMEFT extended with an RHN in the MeV-GeV mass range
invented entities (1)
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Massive right-handed neutrino
no independent evidence
Forward citations
Cited by 1 Pith paper
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Probing Light Dark Fermions in $B \to D^{(*)}\ell X_{\rm inv}$ via Rate Distributions
Massive dark fermions modify rate distributions in B to D(*) lepton invisible decays within weak effective theory, affecting |V_cb| extraction.
Reference graph
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discussion (0)
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