Particle Physics operators
42 operators in the particle_physics category of the live registry. Each is a named formula you can compose inside a state contract or call directly through POST /api/zeq/compute. KO42 is always on; add up to three more per call (total ≤ 4), per the 7-step protocol.
| Operator | Description | Equation |
|---|---|---|
HCS48 | Shannon entropy over 48 particle states for high-energy collision event characterization. | H_{CS} = -\sum_{i=1}^{48} p_i \ln p_i |
HCS52 | Shannon entropy over 52 particle states for extended Standard Model event analysis. | H_{CS} = -\sum_{i=1}^{52} p_i \ln p_i |
HEP1 | Dirac Lagrangian for a free spin-1/2 fermion field. | \mathcal{L} = \bar{\psi}(i\gamma^\mu\partial_\mu - m)\psi |
HEP10 | CKM quark mixing matrix parameterizing flavor-changing weak interactions. | V_{CKM} = \begin{pmatrix} V_{ud} & V_{us} & V_{ub} \\ V_{cd} & V_{cs} & V_{cb} \\ V_{td} & V_{ts} & V_{tb} \end{pmatrix} |
HEP11 | Renormalization group equation: running of the coupling constant with energy scale. | \mu^2\frac{d\alpha}{d\mu^2} = \beta(\alpha) |
HEP12 | QCD running coupling constant exhibiting asymptotic freedom at high energies. | \alpha_s(Q^2) = \frac{12\pi}{(33-2n_f)\ln(Q^2/\Lambda^2)} |
HEP13 | Higgs potential with spontaneous symmetry breaking giving mass to gauge bosons. | V(\phi) = \mu^2|\phi|^2 + \lambda|\phi|^4 |
HEP14 | Higgs boson mass related to the quartic coupling and vacuum expectation value. | m_H = \sqrt{2\lambda}v |
HEP15 | Graviton perturbation: linearized metric perturbation for quantum gravity approaches. | g_{\mu\nu} \to g_{\mu\nu} + h_{\mu\nu} |
HEP16 | Planck mass: the mass scale where quantum gravity effects become important. | M_P = \sqrt{\frac{\hbar c}{G}} |
HEP17 | Einstein-Hilbert action: the gravitational action principle yielding Einstein's field equations. | S = \int d^4x \sqrt{-g}\left(\frac{R}{16\pi G} + \mathcal{L}_m\right) |
HEP18 | Neutrino mass-squared difference governing neutrino oscillation frequencies. | \Delta m^2 = m_2^2 - m_1^2 |
HEP19 | Neutrino oscillation probability: flavor transition as a function of mixing angle and mass splitting. | P(\nu_\alpha \to \nu_\beta) = \sin^2(2\theta)\sin^2\left(\frac{\Delta m^2 L}{4E}\right) |
HEP2 | QED Lagrangian: Dirac field minimally coupled to the electromagnetic field. | \mathcal{L}_{QED} = \bar{\psi}(i\gamma^\mu D_\mu - m)\psi - \frac{1}{4}F_{\mu\nu}F^{\mu\nu} |
HEP20 | Dark energy density parameter: cosmological constant energy density relative to critical density. | \Omega_\Lambda = \frac{\rho_\Lambda}{\rho_c} |
HEP3 | Gauge covariant derivative introducing the electromagnetic coupling to charged fermions. | D_\mu = \partial_\mu + ieA_\mu |
HEP4 | Yang-Mills Lagrangian for non-abelian gauge fields, the basis of the Standard Model. | \mathcal{L}_{YM} = -\frac{1}{4}F^a_{\mu\nu}F^{a\mu\nu} |
HEP5 | Non-abelian field strength tensor with self-interaction terms for gluon and weak boson fields. | F^a_{\mu\nu} = \partial_\mu A^a_\nu - \partial_\nu A^a_\mu + gf^{abc}A^b_\mu A^c_\nu |
HEP6 | Mandelstam variables s, t, u parameterizing relativistic scattering kinematics. | s = (p_1 + p_2)^2, \quad t = (p_1 - p_3)^2, \quad u = (p_1 - p_4)^2 |
HEP7 | Scattering cross-section from the squared matrix element integrated over phase space. | \sigma = \frac{1}{F}\int|\mathcal{M}|^2 d\Phi |
HEP8 | Particle decay rate from the squared matrix element and available phase space. | \Gamma = \frac{1}{2m}\int|\mathcal{M}|^2 d\Phi |
HEP9 | Fermi coupling constant relating weak interaction strength to the W boson mass. | G_F = \frac{g^2}{4\sqrt{2}M_W^2} |
PP1 | Plasma frequency: natural oscillation frequency of electrons in a plasma. | \omega_p = \sqrt{\frac{n_e e^2}{m_e \epsilon_0}} |
PP10 | Lawson criterion for fusion ignition: triple product of density, confinement time, and temperature. | n\tau_E T > 3 \times 10^{21} \text{ keV s m}^{-3} |
PP11 | Generalized Ohm's law for a magnetized plasma including the Hall term. | \vec{E} + \vec{v} \times \vec{B} = \eta\vec{J} |
PP12 | Magnetic Reynolds number: ratio of magnetic advection to diffusion in a conducting fluid. | R_m = \frac{\mu_0 \sigma v L}{1} |
PP13 | Ampère's law in the MHD limit: curl of B proportional to current density. | \nabla \times \vec{B} = \mu_0 \vec{J} |
PP14 | Magnetic induction equation governing evolution of the magnetic field in a conducting plasma. | \frac{\partial \vec{B}}{\partial t} = \nabla \times (\vec{v} \times \vec{B}) + \frac{1}{\mu_0\sigma}\nabla^2\vec{B} |
PP15 | E cross B drift: velocity of charged particles drifting perpendicular to crossed electric and magnetic fields. | \vec{v}_E = \frac{\vec{E} \times \vec{B}}{B^2} |
PP16 | Gradient-B drift: particle drift caused by spatial variation in magnetic field strength. | \vec{v}_\nabla B = \frac{1}{2}v_\perp r_L \frac{\vec{B} \times \nabla B}{B^2} |
PP17 | Magnetic moment: first adiabatic invariant of a charged particle gyrating in a magnetic field. | \mu = \frac{m v_\perp^2}{2B} |
PP18 | Critical density for electromagnetic wave propagation in a plasma. | n_c = \frac{\omega^2 m_e \epsilon_0}{e^2} |
PP19 | Alfvén velocity: speed of magnetic disturbances propagating along field lines in a plasma. | v_A = \frac{B}{\sqrt{\mu_0 \rho}} |
PP2 | Debye length: characteristic shielding distance in a plasma. | \lambda_D = \sqrt{\frac{\epsilon_0 k_B T_e}{n_e e^2}} |
PP20 | Alfvén wave dispersion relation: frequency proportional to wave number times Alfvén speed. | \omega^2 = k^2 v_A^2 |
PP3 | Larmor radius: radius of a charged particle's circular orbit in a magnetic field. | r_L = \frac{m_\perp v_\perp}{|q|B} |
PP4 | Cyclotron frequency: angular frequency of a charged particle gyrating in a magnetic field. | \omega_c = \frac{|q|B}{m} |
PP5 | Plasma beta: ratio of thermal pressure to magnetic pressure in a plasma. | \beta = \frac{nk_B T}{B^2/2\mu_0} |
PP6 | Plasma continuity equation: conservation of particle number with sources and sinks. | \frac{\partial n}{\partial t} + \nabla \cdot (n\vec{v}) = S - L |
PP7 | Boltzmann-Vlasov kinetic equation governing the phase-space distribution of plasma particles. | \frac{\partial f}{\partial t} + \vec{v}\cdot\nabla f + \frac{q}{m}(\vec{E}+\vec{v}\times\vec{B})\cdot\nabla_v f = C(f) |
PP8 | Saha ionization criterion: condition for a gas to be considered a plasma. | n_e T_e^{3/2} / n_n > 1 |
PP9 | Energy confinement time: ratio of stored plasma energy to power loss rate. | \tau_E = \frac{W}{P_{loss}} |
Compute with one of these
curl -sS -X POST https://zeqsdk.com/api/zeq/compute \
-H "Authorization: Bearer $ZEQ_KEY" \
-H "Content-Type: application/json" \
-d '{"operators":["HCS48"],"inputs":{}}'
The response carries the bare physics value, its unit and uncertainty, the generated master equation, and a signed envelope you can verify on any node.
See also
- The solvers — how an operator becomes a physical answer
- Operator selection — how a query picks operators
- All categories — the full reference index