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At tree level in a local Fermi interaction with negligible neutrino masses, the charged daughter mass modifies the integrated three-body V-A interaction rate by $f(m_a^2/m_l^2)$. The function tends to one at zero daughter mass and to zero at threshold. It includes both the phase space restriction and the momentum dependence of the matrix element.

For an unpolarized parent charged lepton undergoing a three-body leptonic V-A interaction decay, neglecting daughter masses and radiative corrections, the normalized charged-daughter energy distribution in the parent rest frame is $f(x)=2x^2(3-2x)$, where $x=2E_{\ell }^{\ast }/m_{\mathrm{parent}}$ lies in $[0,1]$. Direct integration gives ${\int }_0^{1}f(x)dx=1$ and ${\int }_0^{1}xf(x)dx=7/10$. A specified parent spin orientation also produces angular terms, so this one-variable law alone does not describe polarized samples.

Two mechanisms are a tau lepton pair with two leptonic decays, and a W boson pair with two leptonic decays. With equal beam energies, the laboratory is the centre-of-mass frame, and four-momentum conservation gives $E_{\mathrm{miss}}=\sqrt{s}-E_{e^{-}}-E_{{\mu }^{+}}$ in natural units.

For the first mechanism,There are four escaping neutrinos. Each tau lepton decay proceeds through a virtual W boson. The fixed-charge final state has branching fraction $B_{\mu }{B}_e$; the factor two for the inclusive $e^{\pm }{\mu }^{\mp }$ sample does not apply when the charges are specified.

For the second mechanism,There are two escaping neutrinos. The leading Feynman diagrams comprise both $s$-channel photon/Z boson exchange and $t$-channel electron neutrino exchange. Their scattering amplitudes interfere; the complete set is needed for a consistent high-energy prediction. In particular, the neutrino-exchange diagram alone does not define an independently observable production rate.

A tau lepton pair has enhanced production at the Z boson particle resonance, $\sqrt{s}\simeq 91\mathrm{GeV}$. The four-neutrino missing energy has a broad continuous distribution. To derive a useful schematic, neglect daughter masses and parent spin correlations. In an unpolarized tau lepton rest frame, the Michel spectrum for $x=2E_{\ell }^{\ast }/m_{\tau }$ isA Lorentz boost gives $E_{\ell }/E_{\tau }=x(1+{\beta }_{\tau }u)/2$, with $u=\cos {\theta }^{\ast }$ uniform on $[-1,1]$ in this approximation. For ${\beta }_{\tau }\simeq 1$, the charged-daughter probability density function in $z=E_{\ell }/E_{\tau }$ isFor two independent decays, $y=E_{\mathrm{miss}}/\sqrt{s}=1-(z_1+z_2)/2$ has the convolutionand $⟨y⟩=0.65$. It vanishes at both endpoints and peaks on the larger-missing-energy side. This is a shape illustration, not the exact polarized Z boson prediction; spin correlations, acceptance, and radiative effects alter it.

The W boson process turns on near $\sqrt{s}=2m_W\simeq 161\mathrm{GeV}$. At exact on-shell production threshold, each neutrino has energy $m_W/2$, soThe cross section vanishes at the ideal two-body threshold, so this narrow limiting spectrum must not be called the maximum-rate spectrum. The large W boson-pair rate occurs above threshold, around $200\mathrm{GeV}$. There ${\beta }_W=\sqrt{1-4m_W^2/s}$ and each neutrino hasThusAn isotropic independent-decay schematic is triangular, centered at $E_{\mathrm{miss}}/\sqrt{s}=1/2$, with endpoints approximately $0.20$ and $0.80$ at $200\mathrm{GeV}$. Actual W boson particle polarizations and their correlations change this shape; their V-A interaction is not isotropic for a fixed helicity. The finite decay width, beam spread, and radiation also smear the edges.

The phrase “maximum rate” also needs a production regime: a Z boson peak is a resonant maximum, whereas pure photon-mediated tau lepton production has its continuum maximum near $4.2\mathrm{GeV}$. Indeed, ${\sigma }_{\gamma }\propto {\beta }_{\tau }(3-{\beta }_{\tau }^2)/s$ has $s=(1+\sqrt{21})m_{\tau }^2$. The displayed high-boost curve describes the resonant regime; at the continuum maximum use ${\beta }_{\tau }\simeq 0.532$ in the boost formula. An observed event-rate maximum additionally depends on collider luminosity and detection efficiency.

beta decay is a weak charged current process. At quark level $d\to u{W}^{-\ast }\to u{e}^{-}{\bar{\nu }}_e$, with amplitude proportional to $G_F{V}_{ud}$ at low momentum transfer. A neutron in a nucleus can thereby become a proton:The second reaction denotes an energetically allowed nuclear conversion, not a decay of an isolated free proton. In a nuclear beta transition the mass number stays fixed and the atomic number changes by one. baryon number and electric charge are conserved; the neutrino or antineutrino supplies the missing energy, momentum and angular momentum. The three-body final state produces a continuous electron spectrum rather than a single electron energy. Neglecting neutrino mass and recoil, an allowed spectrum in electron total energy isThe Fermi function accounts for the electron's Coulomb interaction with the daughter; $E_0$ is the electron total-energy endpoint. forbidden beta decay adds momentum-dependent nuclear shape factors. The V-A interaction violates parity: it couples left-chiral fermion fields, not an equal mixture of left and right currents.

For allowed beta decay the leading leptons have zero orbital angular momentum. Fermi transitions have $\Delta J=0$; Gamow-Teller transitions have $\Delta J=0,1$ with $0\to 0$ excluded. Both preserve nuclear parity. Higher lepton partial waves permit forbidden transitions with extra suppression. Nuclear matrix elements and phase space, as well as these selection rules, determine lifetimes. Particle-physics examples include free-neutron decay and pion beta decay, ${\pi }^{+}\to {\pi }^0{e}^{+}{\nu }_e$. semileptonic decays test quark mixing and the universality of the weak charged current. beta decay changes quark flavour through virtual W exchange; its continuous spectrum reflects an additional lepton in the final state.

parity reverses spatial coordinates and polar vectors such as momentum, while leaving axial vectors such as angular momentum unchanged. The correlation $\mathbf{J}\cdot {\mathbf{p}}_e$ is therefore parity odd. For polarized beta-emitting nuclei one can measurewhere $\theta$ is measured from nuclear polarization, $\mathcal{P}$ its magnitude and $A$ a decay-dependent coefficient. A nonzero spin–momentum asymmetry is incompatible with parity invariance.

The cobalt-60 experiment polarized nuclei at low temperature and compared beta emission along and opposite the polarization axis. Preferential emission on one side established weak-interaction parity violation. Reversing polarization tests whether the asymmetry follows nuclear orientation; warming the sample removes polarization, while gamma anisotropy monitors its loss. Detector acceptance, backgrounds and magnetic deflection of charged particles must be separated from a true emission asymmetry.^[ref]

In the modern weak charged current, the V-A interaction couples to left-chiral fermion fields. In the massless limit this selects left-helicity neutrinos and right-helicity antineutrinos. Massive charged leptons need not be pure-helicity states, consistent with the factor $v/c$. Strong and electromagnetic interactions conserve parity to the usual experimental approximation; parity violation alone should not be confused with CP violation or a failure of CPT.

At energies far below the $W$ mass, replace its propagator by a constant. The modern V-A interaction form of Fermi's contact theory has, in $\hslash =c=1$ units,Nucleons are treated nonrelativistically within nuclear states. To leading order in their velocity, the vector charge and axial spatial current give the two nuclear operatorswhere ${\tau }^{+}$ here means neutron-to-proton conversion. (i) The scalar Fermi operator permits $\Delta J=0$, including $0\to 0$, without parity change. The rank-one Gamow–Teller operator permits $\Delta J=0,1$ without parity change, excluding $0\to 0$. Both terms can contribute when the same nuclear states permit them; their strengths contain nuclear matrix elements, not just phase space.

(ii) Expand the lepton waves across the nucleus in powers of their momenta times nuclear radius. When $pR/\hslash \ll 1$, the constant spatial term gives allowed transitions. If its matrix element vanishes by spin/parity selection, higher terms supply lepton orbital angular momentum: “forbidden” means suppressed, not impossible. First-forbidden terms change parity and can have $\Delta J=0,1,2$; the rank-two $\Delta J=2$ case is unique first-forbidden. Higher orders carry additional small spatial factors and different energy-dependent shape factors. The contact approximation alone does not imply the allowed approximation.

For a single branch, neglect recoil and neutrino mass and first assume an energy-independent nuclear shape factor. Fermi's golden rule integrates the neutrino phase space with $E_{\nu }=Q-T$, while the electron momentum volume is proportional to $p^{2}dp$. Including Coulomb distortion,This momentum-bin Kurie ordinate is linear in kinetic energy and vanishes at its endpoint. If instead using counts per unit kinetic energy, $dN/dT\propto F(p)p{E}_e(Q-T{)}^2$ in $c=1$ units; converting with $dT/dp=p/E_e$ recovers the supplied momentum-bin definition. No extra factor of $E_e$ should be left inside that definition of $N^{\prime }$.

The graph's horizontal coordinate is $T/(m_e{c}^2)$, not $T$ in MeV. Its intercept is approximately $3.9$–$4.0$, soFor a ground-to-ground branch between bare nuclei, the emitted electron's rest energy must also be supplied:For neutral atomic masses the mass difference instead equals approximately $Q\simeq 2.0\mathrm{MeV}$, neglecting small electron-binding corrections. The graph supports this approximate precision, not a precise evaluated isotope mass. Interpreting a branch to an excited daughter would require adding its excitation energy; the ground-state comparison assumes the ground-state branch intended here.

The shell-model prediction for yttrium-91 beta decay follows from shell filling: the proton orbitals above 28 fill $2p_{3/2}$ with four protons and $1f_{5/2}$ with six, reaching 38. Yttrium has its 39th proton in $2p_{1/2}$, giving $J_i^{\pi }=1/2^{-}$. Its 52 neutrons include the closed 50-neutron core and a pair in $2d_{5/2}$, coupled to zero in the simple paired ground state. Zirconium has 40 paired protons and 51 neutrons, leaving an unpaired $2d_{5/2}$ neutron, so $J_f^{\pi }=5/2^{+}$. ThereforeThe single-particle change is neutron $d_{5/2}$ to proton $p_{1/2}$; the parity change and rank two prevent an allowed Fermi or Gamow–Teller contribution.

The straight plotted line is a constant-shape idealization. For the shell-model transition just inferred, a leading unique-forbidden shape factor contains $C(T)\propto p_e^2+p_{\nu }^2$ in $c=1$ units, with Coulomb/finite-size refinements. Consequently the uncorrected quantity specified in the paper is generally proportional to $(Q-T)\sqrt{C(T)}$, not exactly linear. A consistent shape-corrected Kurie plot also divides its ordinate by $\sqrt{C(T)}$. The source's exact straight-line construction and its forbidden-transition inference cannot both be exact with a Coulomb-only $F$; the approximate graphical endpoint can still be read as requested. Allowed and unique-forbidden spectral shapes are experimentally distinguishable.^[ref]

Treat the electron and electron antineutrino as effectively massless particles in the centre-of-momentum frame, retain only the charged current, and use the Fermi interaction: $m_e^2\ll s\ll M_W^2$. Take ${\theta }^{\ast }$ between incoming and outgoing electron antineutrino directions. The V-A interaction selects a right-helicity electron antineutrino and a left-helicity electron. Their opposite incoming directions give total angular momentum projection one. The outgoing pair has the same projection along its own axis. The Wigner D-matrix element is $d_{11}^1({\theta }^{\ast })=(1+\cos {\theta }^{\ast })/2$, so the squared helicity amplitude is proportional to $(1+\cos {\theta }^{\ast }{)}^2$. The inactive initial electron helicity is included in the unpolarized normalization supplied by the paper.

The boost from the centre-of-momentum frame to the laboratory frame has $\beta =E/(E+m_e)$, while the incoming electron antineutrino has $E_{\ast }=(s-m_e^2)/(2\sqrt{s})=m_{e}E/\sqrt{s}$ and $s=m_e^2+2m_{e}E$. ThusThe requested identity therefore uses $E\gg m_e$; it is not exact at finite target mass. With $c_{\ast }=\cos {\theta }^{\ast }$, the absolute Jacobian determinant is $|dy/d{c}_{\ast }|=1/2$, givingThe suppression at backward scattering follows from angular momentum conservation: rotating projection $+1$ through $\pi$ cannot leave projection $+1$ along the original axis. Replacing $1+c_{\ast }$ by $2(1-y)$ gives the supplied $(1-y{)}^2$ dependence.

In ${\tau }^{-}\to {\ell }^{-}{\bar{\nu }}_{\ell }{\nu }_{\tau }$, charge and missing four-momentum show an invisible neutral component beyond the visible charged lepton. The distributions are consistent with three-body V-A interaction decay; hadronic modes such as ${\tau }^{-}\to {\pi }^{-}{\nu }_{\tau }$ instead have two-body missing-mass kinematics. Production and decay accounting assigns $L_{\tau }({\tau }^{-})=L_{\tau }({\nu }_{\tau })=1$ and their antiparticles minus one. Searches for wrong-flavour and neutrinoless channels constrain violations. These observations establish a useful approximately conserved tau-family number in ordinary interactions, rather than proving an exact law from missing energy alone.

To establish that the invisible particle is distinct from ${\nu }_e$ and ${\nu }_{\mu }$, combine decay evidence with the absence of unsuppressed tau production by conventional electron- and muon-flavour beams, and direct tau neutrino charged current interactions. DONUT observed the short displaced tau lepton decay in nuclear emulsion after a neutrino interaction. ^[ref] Neutrino oscillation means individual family numbers are not exact conserved quantities during propagation, even though they are an excellent approximation for these local decay assignments.

Neglect radiation, take $E_{\tau }=M_Z/2\simeq 45.6\mathrm{GeV}$, $m_{\tau }\simeq 1.777\mathrm{GeV}$, and treat a fixed hadronic invariant mass $m_h=1.5\mathrm{GeV}$ as a single recoil system in ${\tau }^{-}\to h^{-}{\nu }_{\tau }$. With negligible neutrino mass,Thus $E_h^{\min ,\max }=\gamma (E_h^{\ast }\mp \beta p_h^{\ast })$, numerically approximately $32.50$ to $45.60\mathrm{GeV}$. In the ultrarelativistic limit the range is $E_{\tau }{m}_h^2/m_{\tau }^2\le E_h\le E_{\tau }$. A spread of hadronic invariant masses broadens these endpoints; an average mass alone is not a strict endpoint specification for the whole sample.

Let $P_{\tau }=+1$ denote a positive-helicity ${\tau }^{-}$, and measure $\vartheta$ from its laboratory flight direction in its rest frame. For a spin-zero hadronic recoil, the left-helicity tau neutrino and angular momentum conservation giveFor example a tau lepton with spin along $+z$ can emit a left-helicity neutrino along $-z$, carrying spin along $+z$, with the spin-zero recoil along $+z$. A positive-helicity tau lepton then gives a harder visible recoil. If $x_h=E_h/E_{\tau }$, $r=m_h^2/m_{\tau }^2$ and $\beta \simeq 1$, the more general tau hadronic polarimetry formula isFor spin-zero recoil ${\alpha }_h=1$. For a spin-one system produced by the V-A interaction, the longitudinal and transverse weights are $m_{\tau }^2:2m_h^2$, with opposite angular slopes; summing gives ${\alpha }_h=(m_{\tau }^2-2m_h^2)/(m_{\tau }^2+2m_h^2)$. At $m_h=1.5\mathrm{GeV}$ this is about $-0.175$, so the negative-helicity tau lepton has the higher mean total hadronic energy, about $39.43$ versus $38.67\mathrm{GeV}$, within that spin-one model. ^[ref]

The supplied mean invariant mass does not specify the recoil's spin composition or its helicity amplitudes. Consequently the last sign cannot be universal: positive helicity is harder for a spin-zero recoil, negative helicity is harder for the specified $1.5\mathrm{GeV}$ spin-one recoil, and a mixture requires its measured spectral weights. Polarization of an intermediate vector or axial-vector meson also changes the division of energy among its daughter hadrons; that information is not fixed by the total jet invariant mass alone.

The Goldhaber experiment inferred neutrino helicity from the circular polarization of a nuclear gamma ray. A spin-zero metastable europium-152 nucleus captures an inner-shell electron, producing a spin-one excited samarium-152 daughter and an electron neutrino; the daughter promptly emits a roughly $960\mathrm{keV}$ gamma ray to its spin-zero ground state. For a nearly stationary initial atom, the daughter recoils opposite the neutrino. Selecting photons emitted along that recoil relates the daughter spin projection, the photon helicity and the neutrino helicity.

The selection used resonant absorption and scattering in samarium. Nuclear recoil normally shifts an emitted gamma ray below the absorption resonance; the daughter recoil from electron capture supplies a compensating forward Doppler shift. Resonant scattering therefore preferentially selects forward photons, fixing their direction relative to the otherwise invisible neutrino. A samarium scatterer and scintillation counting identify this resonant component. Transmission through magnetized iron, whose Compton scattering depends on the relative electron and photon spins, then analyzes the circular polarization. Reversing the magnetization reverses the analyzing asymmetry and helps control instrumental offsets.

The selected photon and neutrino normalized helicities have the same sign: their momenta are opposite, while the daughter angular-momentum accounting gives opposite spin projections along the recoil axis. The observed negative photon helicity therefore establishes predominantly left-helicity neutrinos, consistent with the V-A interaction. It measures a helicity correlation, not a tiny neutrino mass or a literal observation of the neutral particle's trajectory.^[ref]

The local Fermi interaction gives a three-body leptonic decay width of the format tree level with negligible neutrino masses and universal weak coupling constant values. The fifth power follows from the dimension of $G_F$ and the three-body phase space; $f$ results from integrating the V-A interaction matrix element over the reduced phase space when the charged daughter has nonzero mass. It is more than a purely geometric volume correction because the spin-dependent matrix element is included.

As $z\to 0$, $f(z)\to 1$; increasing daughter mass reduces the available energy and suppresses the rate. The largest ratio is $m_{\mu }/m_{\tau }$, so the $\tau \to \mu$ correction is visibly below one. The electron is extremely light relative to either parent. Using the lepton masses givesThese reproduce the supplied factors to their stated accuracy. Radiative and finite-W boson corrections are separate small corrections when a precision lepton universality test is performed.

The visible angular distribution and laboratory energy in ${\tau }^{-}\to h^{-}{\nu }_{\tau }$ carry information about the parent's spin. For fixed hadronic invariant mass, $E_h=\gamma (E_h^{\ast }+\beta p_h^{\ast }\cos \vartheta )$. A spin-zero recoil has analyzing coefficient ${\alpha }_h=1$. For a spin-one recoil coupled through the V-A interaction, longitudinal and transverse partial rates have weights $m_{\tau }^2:2m_h^2$ and opposite slopes, giving ${\alpha }_h=(m_{\tau }^2-2m_h^2)/(m_{\tau }^2+2m_h^2)$. Thus the harder-helicity ordering can reverse when the recoil mass exceeds $m_{\tau }/\sqrt{2}$. A mean invariant mass without spin-dependent spectral weights cannot fix the sign for a mixed sample.