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Computational AMO and Quantum Chemistry

A computational AMO result is a claim supported by a chain of models, algorithms, diagnostics, and comparisons. It is not merely an energy, a population curve, an optimized geometry, or a spectrum returned by software.

Atomic, molecular, and optical calculations span unusually different computational regimes. A hydrogenic radial equation is a one-dimensional boundary-value problem with an analytic spectrum. A helium calculation is a correlated few-body variational problem. Molecular electronic structure combines nonorthogonal bases, self-consistency, and model chemistry. Quantum-optical dynamics may require matrix exponentials, master equations, or stochastic trajectories. Laser cooling adds velocity distributions, spatial motion, photon recoil, and experimental geometry.

The common trust structure is

declared physical question⟶stated model⟶finite representation⟶numerical solution⟶verified observables⟶qualified physical claim.\begin{gathered} \text{declared physical question} \longrightarrow \text{stated model} \longrightarrow \text{finite representation} \\ \longrightarrow \text{numerical solution} \longrightarrow \text{verified observables} \longrightarrow \text{qualified physical claim}. \end{gathered}

Every arrow can fail independently. A linear solver can converge while the basis is inadequate. A basis can be converged for the energy while a polarizability remains inaccurate. A master-equation integrator can preserve trace while the Markov approximation is physically invalid. Agreement with experiment can result from fitted parameters or cancellation of errors rather than predictive accuracy.

This chapter develops the evidence needed to tell those cases apart.

This page owns the AMO-specific map from physical targets to benchmarked computations. It explains:

  • what “exact” can and cannot mean in a computation;
  • which approximations enter atomic, molecular, quantum-optical, and platform models;
  • how to separate model, representation, solver, parameter, and implementation errors;
  • how hydrogen, helium, molecular ions, driven two-level systems, Jaynes–Cummings blocks, and Doppler-force curves form a benchmark ladder;
  • how verification, validation, calibration, and prediction differ;
  • what evidence an AMO notebook or dataset must preserve; and
  • how the pages in this chapter fit together.

Several neighboring sections retain their own canonical responsibilities:

  • Numerical Mathematics owns floating-point arithmetic, discretization, conditioning, eigensolvers, quadrature, differential-equation solvers, time stepping, error estimation, convergence studies, and general benchmark design.
  • Math Needed for Computational QM maps quantum calculations to those mathematical tools.
  • Software, Notebooks, and Benchmarks owns environments, package records, artifact status, code style, validation tests, and the site-wide admission contract for reproducible notebooks.
  • Computational Quantum Mechanics Roadmap owns the general study route.
  • Computational QM References owns the broad bibliography.
  • The atomic, molecular, light–matter, quantum-optical, and platform chapters own the physical derivations and interpretations of the models computed here.

This chapter therefore does not reteach generic finite differences or advertise one software stack. It specializes the trust chain to AMO physics and quantum chemistry.

“Calculate helium,” “run Hartree–Fock,” and “simulate a cavity” are not reproducible questions. A useful problem declaration is

P=(S,H,B,I,O,A,θ,εtarget),\mathcal P = \left( \mathcal S, H, \mathcal B, \mathcal I, O, \mathcal A, \boldsymbol\theta, \varepsilon_{\mathrm{target}} \right),

with the following entries:

SymbolMeaningRepresentative AMO content
S\mathcal Sphysical systemspecies, isotope, charge, electronic term, cavity modes
HHHamiltonian or generatorCoulomb, effective, rotating-frame, or Lindblad model
B\mathcal Bdomain and boundary dataradial origin, finite box, basis, geometry, cutoffs
I\mathcal Iinitial or reference stateelectronic configuration, pulse-prepared state, thermal ensemble
OOtarget observableenergy difference, force, rate, population, line strength, spectrum
A\mathcal Aapproximation hierarchyfixed nucleus, basis truncation, Born–Oppenheimer, rotating-wave, Markov
θ\boldsymbol\thetanumerical and physical parametersconstants, fields, tolerances, time steps, random seeds
εtarget\varepsilon_{\mathrm{target}}required accuracyabsolute, relative, spectral, or statistical tolerance

The accuracy target belongs in the declaration because the appropriate model depends on it. A nonrelativistic clamped-nucleus calculation can be fully adequate for a qualitative bonding curve and inadequate for isotope shifts or precision spectroscopy. A two-level rotating-wave model can accurately predict a long resonant pulse and fail for an ultrashort broadband pulse.

Computations and measurements must refer to the same observable. For two levels,

ΔE=Eu−El,ν=ΔEh,ω=ΔEℏ.\Delta E = E_u-E_l, \qquad \nu = \frac{\Delta E}{h}, \qquad \omega = \frac{\Delta E}{\hbar}.

Confusing ν\nu with ω\omega introduces a factor of 2π2\pi. Comparing a clamped-nucleus electronic energy with a measured transition also mixes different objects: the measurement may contain recoil, nuclear motion, relativistic structure, radiative corrections, external-field shifts, and line-shape inference.

Write the intended claim before choosing the method

Section titled “Write the intended claim before choosing the method”

A useful template is:

For the stated Hamiltonian, basis or grid sequence, parameter conventions, and observable, the reported result satisfies the declared numerical tests. The remaining model discrepancy is bounded, estimated, or explicitly left unresolved at the stated accuracy.

This wording forces a separation between solving equations correctly and choosing equations that are adequate for the physical purpose.

The word exact always needs an object and a scope. At least four meanings occur in computational AMO physics.

Some idealized Hamiltonians have closed-form spectra or propagators. In infinite-nuclear-mass atomic units, the nonrelativistic hydrogenic energies are

En=−Z22n2Eh.E_n = -\frac{Z^2}{2n^2} E_{\mathrm h}.

This is exact for the stated Coulomb Hamiltonian and domain. It is not the complete physical spectrum of a real atom. Reduced-mass, relativistic, hyperfine, radiative, and external-field effects lie outside that model.

For an ideal coherently driven two-level system in the rotating-wave approximation,

Pe(t)=Ω2ΩR2sin⁡2(ΩRt2),ΩR=Ω2+Δ2.P_e(t) = \frac{\Omega^2}{\Omega_R^2} \sin^2 \left( \frac{\Omega_R t}{2} \right), \qquad \Omega_R = \sqrt{\Omega^2+\Delta^2}.

This formula is an exact solution of the stated effective Hamiltonian. The two-level truncation, prescribed classical drive, and rotating-wave approximation remain physical approximations.

Once a basis or grid is fixed, a calculation may define a finite matrix problem such as

HNcN=ENcN.H_N c_N = E_N c_N.

Dense diagonalization can produce all eigenpairs of HNH_N to floating-point accuracy. That result is not automatically the exact eigenpair of the continuum operator HH. The distinction is

algebraic error:HNc~N−E~Nc~N,representation error:EN−E,model error:E−Ephysical.\begin{aligned} \text{algebraic error} &: H_N\widetilde c_N - \widetilde E_N\widetilde c_N, \\ \text{representation error} &: E_N-E, \\ \text{model error} &: E-E_{\mathrm{physical}}. \end{aligned}

These three errors require different evidence.

Even when the solution is approximate, some consequences of the represented model should hold to numerical tolerance:

⟨ψ∣ψ⟩=1,Tr⁡ρ=1,ρ†=ρ,ddt⟨ψ∣ψ⟩=0for closed unitary dynamics.\begin{aligned} \langle\psi|\psi\rangle &=1, \\ \operatorname{Tr}\rho &=1, \\ \rho^\dagger &=\rho, \\ \frac{d}{dt} \langle\psi|\psi\rangle &=0 \quad \text{for closed unitary dynamics}. \end{aligned}

Symmetry blocks, conserved excitation number, Hermiticity, selection-rule zeros, dimensional consistency, and known sum rules are similarly exact within their assumptions. These checks are inexpensive and should run before comparison with published numbers.

The Rayleigh–Ritz principle gives a rigorous upper bound for the ground-state energy of a self-adjoint Hamiltonian bounded from below:

E0≤⟨ψT∣H∣ψT⟩⟨ψT∣ψT⟩.E_0 \leq \frac{ \langle\psi_T|H|\psi_T\rangle }{ \langle\psi_T|\psi_T\rangle }.

The bound applies to the same Hamiltonian and domain represented by the trial state. It does not bound omitted relativistic terms, finite-nuclear-mass effects, or experimental corrections. It can also be lost when an approximation is not variational for the reported quantity.

A helium energy converged to many digits is a high-accuracy numerical reference for a specified nonrelativistic Hamiltonian. It is not a closed-form solution, and the printed digits are not all physically observable. A benchmark should therefore label a value as:

  • analytic;
  • rigorously bounded;
  • numerically converged with an uncertainty estimate;
  • evaluated experimental data;
  • or a conventional reference value.

Those labels carry more information than the number of decimal places.

Most useful AMO calculations contain an approximation stack. The stack should be written in physical order rather than hidden inside a package input file.

Representative reductions include:

  • fixed nucleus or finite nuclear mass;
  • nonrelativistic, scalar-relativistic, Breit–Pauli, or Dirac descriptions;
  • frozen core or active-space restriction;
  • independent-particle, Hartree–Fock, density-functional, configuration interaction, coupled-cluster, or multireference treatment;
  • Born–Oppenheimer separation of electronic and nuclear motion;
  • electric-dipole and multipole truncations;
  • rotating-frame and rotating-wave approximations;
  • finite-level and finite-mode truncations;
  • Markov and secular reductions;
  • semiclassical treatment of center-of-mass motion;
  • independent-photon recoil or diffusion approximations.

The approximation must be tied to the observable. A model adequate for a total energy may be poor for a small difference of large energies, a transition moment, a long-range coefficient, or a near-degenerate splitting.

Continuum wavefunctions and fields are represented by finite data:

∣ψN⟩=∑μ=1Ncμ∣χμ⟩.|\psi_N\rangle = \sum_{\mu=1}^{N} c_\mu|\chi_\mu\rangle.

The representation can involve:

  • a radial or Cartesian grid;
  • Gaussian, Slater-type, B-spline, finite-element, DVR, plane-wave, or oscillator functions;
  • a finite spatial box;
  • angular-momentum cutoffs;
  • an electronic active space;
  • a photon-number cutoff;
  • a finite velocity or position mesh;
  • quadrature nodes and weights.

Increasing one cutoff does not control all others. A larger electronic basis does not repair an insufficient active space. A smaller time step does not repair a photon cutoff. A longer radial box does not repair poor resolution near a Coulomb cusp.

Hartree, Hartree–Fock, and Kohn–Sham calculations solve nonlinear fixed-point problems. If DD denotes a one-particle density matrix, a generic self-consistency condition is

D=F(D).D = \mathcal F(D).

A small change between consecutive iterates is not sufficient evidence of the correct stationary solution. Distinct initial guesses can converge to different local solutions or symmetry states. Report energy, density, commutator, and orbital-gradient diagnostics where appropriate, and test occupation and stability.

For dynamics,

∣ψ(t+Δt)⟩≈UΔt∣ψ(t)⟩.|\psi(t+\Delta t)\rangle \approx U_{\Delta t} |\psi(t)\rangle.

Time-step error, interpolation of the drive, operator splitting, solver tolerance, and finite time window are distinct. Fourier-transforming a finite trajectory adds a resolution kernel and possibly windowing artifacts. A stable integrator can still accumulate phase error or violate positivity.

Quantum trajectories, recoil simulations, and Monte Carlo sampling add statistical error:

OˉM=1M∑j=1MOj,SE⁡(OˉM)∝1Meff.\bar O_M = \frac{1}{M} \sum_{j=1}^{M} O_j, \qquad \operatorname{SE}(\bar O_M) \propto \frac{1}{\sqrt{M_{\mathrm{eff}}}}.

The effective sample count can be smaller than MM when trajectories or samples are correlated. A seed makes one realization reproducible; it does not establish convergence. Report ensemble size, uncertainty, and between-seed checks.

Calculated observables depend on constants, geometry, field calibration, transition data, fitted model parameters, and database values. Their uncertainties can dominate a numerically converged solver. The parameter sensitivity is locally

δO≈∑i∂O∂θiδθi.\delta O \approx \sum_i \frac{\partial O}{\partial\theta_i} \delta\theta_i.

With covariance matrix Σθ\Sigma_\theta,

uO2≈∇θOTΣθ∇θO.u_O^2 \approx \nabla_\theta O^{\mathsf T} \Sigma_\theta \nabla_\theta O.

The covariance term matters when constants or fitted parameters share a common source.

A useful bookkeeping identity is

O^−Ophysical=  δmodel+δrepresentation+δsolver+δparameter+δstatistical+δimplementation.\begin{aligned} \widehat O-O_{\mathrm{physical}} =\;& \delta_{\mathrm{model}} +\delta_{\mathrm{representation}} +\delta_{\mathrm{solver}} \\ &+ \delta_{\mathrm{parameter}} +\delta_{\mathrm{statistical}} +\delta_{\mathrm{implementation}}. \end{aligned}

This is a classification, not permission to add unknown signed errors as independent random variables. Each term needs its own estimator, bound, sensitivity study, or explicit “not quantified” label.

Error classTypical AMO sourceAppropriate control
modelomitted correlation, recoil, counter-rotating terms, memoryhigher-level model, scale estimate, experiment
representationbasis, grid, box, active space, photon cutoffsystematic refinement and extrapolation
solvereigensolver, SCF, ODE, optimization toleranceresidual, gradient, conservation, repeated initialization
parameterconstants, geometry, fields, ratesprovenance, covariance propagation, sensitivity
statisticaltrajectories, Monte Carlo, sampled dataconfidence interval, autocorrelation, seed ensemble
implementationindexing, units, signs, defaultsindependent tests, analytic cases, cross-code comparison

Errors do not all converge in the same direction

Section titled “Errors do not all converge in the same direction”

For a nested variational basis, the ground-state energy often decreases toward the basis limit:

EN+1≤EN.E_{N+1} \leq E_N.

Many other observables are not monotone. Excitation energies are differences. Dipoles and polarizabilities depend on wavefunction quality in regions not strongly weighted by the total energy. Perturbative triples corrections and density-functional results are not generally variational upper bounds. Convergence must be tested for the reported observable, not inferred from energy alone.

Suppose two large energies produce a dissociation energy:

De=EA+EB−EAB.D_e = E_A+E_B-E_{AB}.

Some errors cancel because the same method and basis treat both sides consistently. Other errors fail to cancel, especially when fragments and complex have different correlation, basis borrowing, spin, or symmetry. Agreement in DeD_e does not prove that each total energy is accurate.

These terms answer different questions.

ActivityQuestionRepresentative evidence
verificationDid the implementation solve the stated equations?residuals, invariants, exact limits, manufactured inputs
numerical validationIs the finite calculation controlled?basis, grid, box, cutoff, time-step, and sample convergence
physical validationIs the model adequate for the intended observable?held-out experiment, higher-level theory, regime tests
calibrationWhich unknown parameters are inferred from data?likelihood, prior, covariance, fit diagnostics
predictionWhat follows for data not used in calibration?preregistered or held-out comparison with uncertainty

Calibration and validation must not silently use the same datum. If a transition energy is fitted into an effective Hamiltonian, reproducing that transition is a calibration check. Other levels, isotope shifts, matrix elements, or field dependence can provide validation.

Evidence ladder from structural checks and exact model limits through converged references and independent physical validation

The AMO evidence ladder. Structural checks and exact model limits verify an implementation; refinement and independent reference values control the finite calculation; held-out data test whether the physical model is adequate for the intended claim. Calibration enters from the side and must be declared before a comparison is called predictive.

A benchmark needs more than a target number. It should state:

  1. the Hamiltonian or equations;
  2. units and constants;
  3. boundary and initial conditions;
  4. basis, grid, or truncation sequence;
  5. the observable and normalization;
  6. a reference value with provenance;
  7. an acceptance metric and tolerance;
  8. expected convergence behavior;
  9. known failure modes;
  10. the software and hardware information relevant to reproducibility.

Without these fields, two correct implementations can appear to disagree because they solved different problems.

For a normalized approximate eigenpair,

r=HNc~−E~c~.r = H_N\widetilde c - \widetilde E\widetilde c.

A scale-aware residual is

ηr=∥r∥∥HN∥∥c~∥+∣E~∣∥c~∥.\eta_r = \frac{ \lVert r\rVert }{ \lVert H_N\rVert\lVert\widetilde c\rVert + |\widetilde E| \lVert\widetilde c\rVert }.

A small ηr\eta_r verifies the finite eigenproblem. It does not establish basis convergence. Observable comparisons should use a declared metric, for example

εrel=∣O^−Oref∣max⁡(∣Oref∣,Oscale).\varepsilon_{\mathrm{rel}} = \frac{ |\widehat O-O_{\mathrm{ref}}| }{ \max \left( |O_{\mathrm{ref}}|, O_{\mathrm{scale}} \right) }.

The scale floor OscaleO_{\mathrm{scale}} prevents a meaningless relative error near a true zero. Symmetry-forbidden matrix elements are better tested with an absolute tolerance tied to operator and state norms.

Atomic calculations provide a progression from analytic one-electron tests to correlated and relativistic many-electron structure.

For a central potential, write

ψnlm(r)=unl(r)rYlm(θ,ϕ).\psi_{nlm}(\mathbf r) = \frac{u_{nl}(r)}{r} Y_{lm}(\theta,\phi).

In atomic units, the radial Coulomb equation is

[−12d2dr2+l(l+1)2r2−Zr]unl(r)=Enunl(r),\left[ -\frac{1}{2} \frac{d^2}{dr^2} + \frac{l(l+1)}{2r^2} - \frac{Z}{r} \right] u_{nl}(r) = E_n u_{nl}(r),

with

unl(0)=0,unl(r)→0as r→∞.u_{nl}(0)=0, \qquad u_{nl}(r)\to0 \quad \text{as } r\to\infty.

A radial solver should test:

  • the −Z2/(2n2)-Z^2/(2n^2) energy sequence;
  • normalization ∫0∞∣unl(r)∣2 dr=1\int_0^\infty |u_{nl}(r)|^2\,dr=1;
  • node count n−l−1n-l-1;
  • near-origin behavior unl∝rl+1u_{nl}\propto r^{l+1};
  • exponential tail behavior;
  • degeneracy in ll for the pure Coulomb Hamiltonian;
  • the Coulomb virial identity 2⟨T⟩+⟨V⟩=02\langle T\rangle+\langle V\rangle=0;
  • convergence with grid spacing, outer radius, and origin treatment.

Hydrogen reveals several common bugs at once: a missing radial Jacobian, an incorrect centrifugal factor, an origin singularity, a wrong sign in the potential, or normalization with Cartesian rather than radial weights.

For an infinitely massive nucleus in atomic units,

H=∑i=12(−12∇i2−2ri)+1r12.H = \sum_{i=1}^{2} \left( -\frac{1}{2}\nabla_i^2 - \frac{2}{r_i} \right) + \frac{1}{r_{12}}.

Use a normalized product of hydrogenic 1s1s orbitals with variational effective charge ζ\zeta. Its energy is

E(ζ)=ζ2−278ζ.E(\zeta) = \zeta^2 - \frac{27}{8}\zeta.

Stationarity gives

ζ⋆=2716,E(ζ⋆)=−729256Eh=−2.84765625Eh.\zeta_\star = \frac{27}{16}, \qquad E(\zeta_\star) = -\frac{729}{256} E_{\mathrm h} = -2.84765625 E_{\mathrm h}.

This small calculation is useful because every integral is analytic, the variational inequality is known, and the remaining discrepancy has a clear physical interpretation: a single uncorrelated spatial product cannot adapt explicitly to the instantaneous electron–electron separation.

High-precision explicitly correlated calculations give a nonrelativistic infinite-mass ground-state reference near

E0≈−2.9037243770341196Eh.E_0 \approx -2.9037243770341196 E_{\mathrm h}.

The value is a benchmark for that Hamiltonian, not a prediction including finite nuclear mass, relativity, or QED. Helium Atom owns the physical derivation and correlation interpretation.

For self-consistent atomic structure, useful checks include:

  • one-electron ions, where electron–electron terms must vanish;
  • two-electron closed shells, where restricted formulas are transparent;
  • invariance under rotations within a fully occupied orbital subspace;
  • orthonormality of orbitals;
  • self-consistency residuals;
  • total-energy stationarity;
  • term, parity, and total-angular-momentum labels;
  • agreement between length and velocity forms of transition amplitudes as a diagnostic, with due care about model consistency;
  • convergence in radial grid, orbital set, configuration space, and partial waves.

Length–velocity agreement is not a theorem that the answer is physically exact. Two forms can agree because they share an approximation, and they can disagree when basis completeness or Hamiltonian consistency is insufficient.

The NIST Atomic Spectra Database provides critically compiled atomic levels, wavelengths, and transition data. A responsible comparison records:

  • database version or access date;
  • species, ionization stage, isotope when relevant, and level labels;
  • observed versus Ritz value;
  • vacuum versus standard-air wavelength convention;
  • uncertainty and accuracy code;
  • whether the entry is experimental, theoretical, or derived;
  • the original source cited by the database.

Evaluated data validate a physical prediction only when the calculation and entry refer to the same quantity. Agreement of a nonrelativistic energy with a measured line can be accidental if omitted corrections cancel.

LevelProblemPrimary testWhat it does not prove
A0hydrogenic matrix elementsanalytic integrals and selection-rule zerosmany-electron correctness
A1hydrogen radial spectrumenergy, nodes, virial theorem, refinementrelativistic accuracy
A2helium effective-charge trialanalytic energy and variational boundcorrelation completeness
A3high-precision heliumbasis and correlation convergencefinite-mass or QED accuracy
A4selected multi-electron atomterm labels, transitions, cross-method comparisontransferability to all atoms
A5evaluated spectral datauncertainty-aware physical comparisonpredictive status if fitted

Molecular computation adds moving nuclei, geometry, nonorthogonal basis functions, multiple electronic structures, and observables obtained from derivatives of an energy surface.

For basis functions ∣χμ⟩|\chi_\mu\rangle that are not orthonormal,

∣ϕi⟩=∑μCμi∣χμ⟩.|\phi_i\rangle = \sum_\mu C_{\mu i} |\chi_\mu\rangle.

Projection gives

FC=SCε,FC = SC\varepsilon,

where

Fμν=⟨χμ∣F^∣χν⟩,Sμν=⟨χμ∣χν⟩.F_{\mu\nu} = \langle\chi_\mu|\widehat F|\chi_\nu\rangle, \qquad S_{\mu\nu} = \langle\chi_\mu|\chi_\nu\rangle.

The metric normalization is

C†SC=I.C^\dagger S C = I.

A solver must not silently treat SS as the identity. Small eigenvalues of SS signal near-linear dependence and can amplify roundoff. Removing directions requires a documented threshold and a test of observable sensitivity.

The one-electron ion H2+\mathrm{H}_2^+ is the molecular analogue of the hydrogen benchmark. For fixed internuclear separation RR,

He(R)=−12∇2−1rA−1rB+1R.H_{\mathrm e}(R) = -\frac{1}{2}\nabla^2 - \frac{1}{r_A} - \frac{1}{r_B} + \frac{1}{R}.

It tests:

  • two-center integrals;
  • overlap and generalized diagonalization;
  • gerade and ungerade symmetry;
  • bonding and antibonding combinations;
  • the dissociation and united-atom limits;
  • the shape and minimum of a potential-energy curve;
  • interpolation and differentiation of that curve.

At large RR, the electronic state should approach a hydrogen atom plus a proton, with the chosen energy zero stated. At R→0R\to0, the electronic part approaches the united-atom problem while the nuclear repulsion diverges. These limits catch energy-zero and nuclear-repulsion bookkeeping errors.

A molecular result depends on both the electronic-structure approximation MM and finite basis XX:

EM,X.E_{M,X}.

A basis sequence at fixed method estimates

δbasis∼EM,X−EM,∞,\delta_{\mathrm{basis}} \sim E_{M,X} - E_{M,\infty},

while a method sequence at a large basis probes a different error:

δmethod∼EM,∞−Eexact,∞.\delta_{\mathrm{method}} \sim E_{M,\infty} - E_{\mathrm{exact},\infty}.

Increasing basis size does not turn Hartree–Fock into a correlated method. Increasing correlation rank in a poor basis does not reach the complete-basis result. Report both axes.

For noninteracting fragments at infinite separation, a size-consistent method should satisfy

E(A+B)⟶E(A)+E(B).E(A+B) \longrightarrow E(A)+E(B).

Truncated configuration interaction can violate this property even when its energy is variational. Restricted single-reference methods can also give a qualitatively wrong dissociation curve when one determinant ceases to describe the separated fragments.

The lesson is broader than one method: a near-equilibrium energy benchmark does not validate bond breaking, excited states, charge transfer, or multireference regions.

In a dimer calculation, each fragment can borrow basis functions centered on the other fragment. The raw interaction energy

ΔEint=EABAB−EAA−EBB\Delta E_{\mathrm{int}} = E_{AB}^{AB} - E_A^A - E_B^B

then compares calculations in unequal one-particle spaces. A counterpoise comparison instead evaluates monomers in the dimer basis:

ΔEintCP=EABAB−EAAB−EBAB.\Delta E_{\mathrm{int}}^{\mathrm{CP}} = E_{AB}^{AB} - E_A^{AB} - E_B^{AB}.

Counterpoise correction is a diagnostic and convention that must be reported, not a universal substitute for basis convergence.

Near a stationary geometry, expand the potential:

V(R0+ΔR)≈V(R0)+12ΔRTKΔR.V(\mathbf R_0+\Delta\mathbf R) \approx V(\mathbf R_0) + \frac{1}{2} \Delta\mathbf R^{\mathsf T} K \Delta\mathbf R.

The mass-weighted Hessian is

DAα,Bβ=KAα,BβMAMB.D_{A\alpha,B\beta} = \frac{ K_{A\alpha,B\beta} }{ \sqrt{M_A M_B} }.

Its positive nonzero eigenvalues are ωk2\omega_k^2 in the harmonic approximation. A molecular-vibration implementation should check:

  • translational and rotational zero modes;
  • invariance under rigid translation and rotation;
  • Hessian symmetry;
  • finite-difference step convergence when derivatives are numerical;
  • unit conversion from angular frequency to wavenumber;
  • analytic oscillator cases;
  • sensitivity to geometry and electronic-structure method.

Imaginary frequencies can identify a saddle point, but they can also result from an unconverged geometry, insufficient integration grid, noisy finite differences, or inconsistent constraints.

LevelProblemPrimary testFailure exposed
M0overlap matrixHermiticity, positive definiteness, metric normalizationbasis indexing and linear dependence
M1H2+\mathrm{H}_2^+ minimal basisanalytic or reference integrals, symmetry, limitsgeneralized-eigenproblem errors
M2H2+\mathrm{H}_2^+ basis sequencevariational energy curve and equilibriumbasis incompleteness
M3helium or H2\mathrm{H}_2 correlation sequencemethod and basis axesmissing dynamical correlation
M4stretched bonddissociation and size consistencysingle-reference failure
M5harmonic moleculezero modes and Hessian convergencegeometry, derivative, and unit errors
M6held-out spectroscopyfrequencies, isotope trends, uncertaintyphysical model inadequacy

Quantum optics supplies small models with strong analytic structure and large models where truncation and open-system dynamics become decisive.

For a time-independent finite Hermitian Hamiltonian,

U(t)=exp⁡(−iHtℏ)U(t) = \exp \left( -\frac{iHt}{\hbar} \right)

is unitary. A propagation benchmark should test:

U†U=I,∥ψ(t)∥=1,⟨H⟩t=⟨H⟩0.U^\dagger U = I, \qquad \lVert\psi(t)\rVert = 1, \qquad \langle H\rangle_t = \langle H\rangle_0.

The last identity applies only when HH is time independent. For a driven Hamiltonian, energy exchange with the drive is expected, while norm conservation remains.

Rabi oscillations test frequency, phase, detuning, pulse area, and basis ordering. Useful cases include:

  • zero coupling, where populations remain fixed;
  • resonance, where a π\pi pulse inverts the ideal system;
  • large detuning, where excitation is suppressed;
  • a drive phase change, which rotates the Bloch-sphere axis;
  • comparison of rotating-wave and full driven Hamiltonians.

Let Γ1\Gamma_1 be population decay and Γ2\Gamma_2 coherence decay. With Rabi frequency convention

Hrot=−ℏΔ2σz+ℏΩ2σx,H_{\mathrm{rot}} = -\frac{\hbar\Delta}{2}\sigma_z + \frac{\hbar\Omega}{2}\sigma_x,

the steady excited-state population can be written

ρee(ss)=s2(1+s),\rho_{ee}^{(\mathrm{ss})} = \frac{s}{2(1+s)},

where

s=Ω2Γ2Γ1(Δ2+Γ22).s = \frac{ \Omega^2\Gamma_2 }{ \Gamma_1 \left( \Delta^2+\Gamma_2^2 \right) }.

For pure radiative broadening, Γ2=Γ1/2\Gamma_2=\Gamma_1/2. This benchmark tests detuning signs, factors of two in the drive, decay conventions, and the saturation limit

ρee(ss)⟶12.\rho_{ee}^{(\mathrm{ss})} \longrightarrow \frac{1}{2}.

Optical Bloch Equations owns the physical derivation.

A Lindblad-form model is

ρ˙=−iℏ[H,ρ]+∑k(LkρLk†−12{Lk†Lk,ρ}).\dot\rho = -\frac{i}{\hbar} [H,\rho] + \sum_k \left( L_k\rho L_k^\dagger - \frac{1}{2} \left\{ L_k^\dagger L_k, \rho \right\} \right).

The represented evolution should preserve trace and Hermiticity and, for a valid implementation of the stated generator, positivity. Numerical checks include:

∣Tr⁡ρ−1∣,∥ρ−ρ†∥,min⁡jλj(ρ).\left| \operatorname{Tr}\rho-1 \right|, \qquad \lVert\rho-\rho^\dagger\rVert, \qquad \min_j\lambda_j(\rho).

A tiny negative eigenvalue can be roundoff; a persistent negative population can indicate an integrator, generator, or approximation problem. Clipping negative eigenvalues hides the symptom and changes the dynamics.

An unraveling estimates the density operator by an ensemble:

ρ(t)≈1M∑j=1M∣ψj(t)⟩⟨ψj(t)∣.\rho(t) \approx \frac{1}{M} \sum_{j=1}^{M} |\psi_j(t)\rangle \langle\psi_j(t)|.

The ensemble mean should converge to the master-equation result for the same generator. This cross-method comparison is stronger than either solver alone. Report confidence intervals and compare multiple seeds; individual trajectories are not expected to match deterministic density-matrix curves.

For

H=ℏωca†a+ℏωa2σz+ℏg(a†σ−+aσ+),H = \hbar\omega_c a^\dagger a + \frac{\hbar\omega_a}{2}\sigma_z + \hbar g \left( a^\dagger\sigma_- + a\sigma_+ \right),

the excitation number

Nexc=a†a+σ+σ−N_{\mathrm{exc}} = a^\dagger a + \sigma_+\sigma_-

is conserved. In the manifold {∣e,n⟩,∣g,n+1⟩}\{|e,n\rangle,|g,n+1\rangle\},

En,±=ℏωc(n+12)±ℏ2Δ2+4g2(n+1).E_{n,\pm} = \hbar\omega_c \left( n+\frac{1}{2} \right) \pm \frac{\hbar}{2} \sqrt{ \Delta^2 + 4g^2(n+1) }.

At resonance, the splitting is

En,+−En,−=2ℏgn+1.E_{n,+}-E_{n,-} = 2\hbar g\sqrt{n+1}.

This gives an exact finite-block benchmark for matrix construction. A full-space simulation still needs a photon cutoff. Convergence should be checked through both observables and the occupation near the highest retained number state.

LevelBenchmarkRequired evidence
Q0Pauli and ladder-operator matricescommutators, dimensions, basis ordering
Q1undriven two-level propagatorphase and norm
Q2Rabi formulaamplitude, generalized frequency, pulse area
Q3optical Bloch steady statetrace, positivity, saturation, detuning
Q4Jaynes–Cummings blockconserved excitation and analytic doublet
Q5photon-cutoff sequencetail occupation and observable stability
Q6trajectories versus master equationconfidence-aware ensemble agreement

Platform calculations combine internal quantum dynamics with motion, electromagnetic fields, geometry, feedback, and noise. Their outputs are often effective parameters or measured signals rather than bare eigenvalues.

For two counterpropagating beams of equal low saturation s0≪1s_0\ll1, a simple one-dimensional force model is

F(v)=ℏkΓs02[11+4(Δ−kv)2/Γ2−11+4(Δ+kv)2/Γ2].\begin{aligned} F(v) = \frac{\hbar k\Gamma s_0}{2} \Bigg[ & \frac{1}{ 1+4(\Delta-kv)^2/\Gamma^2 } \\ - & \frac{1}{ 1+4(\Delta+kv)^2/\Gamma^2 } \Bigg]. \end{aligned}

For red detuning Δ<0\Delta<0, the small-velocity slope should oppose motion:

F(v)≈−αv,α>0.F(v) \approx -\alpha v, \qquad \alpha>0.

This benchmark catches beam-direction, Doppler-shift, detuning, and recoil sign errors. It does not validate a sub-Doppler, multilevel, polarization gradient, or high-saturation model.

Separate internal and motional approximations

Section titled “Separate internal and motional approximations”

A semiclassical simulation may evolve

mr¨=F(r,v,ρ,t)+ξ(t)m\ddot{\mathbf r} = \mathbf F \left( \mathbf r, \mathbf v, \rho, t \right) + \boldsymbol\xi(t)

while a master equation evolves the internal state ρ\rho. The assumptions behind classical motion, local steady state, recoil diffusion, and white noise are independent. State them separately.

For a stochastic recoil model, checks include:

  • zero mean recoil in an isotropic emission model;
  • the expected momentum-diffusion growth;
  • convergence in trajectory count and time step;
  • detailed treatment of absorption and emission directions;
  • consistency between friction and diffusion in the regime where an equilibrium temperature is inferred.

Near a stable trap center,

V(r)≈V0+m2∑iωi2xi2.V(\mathbf r) \approx V_0 + \frac{m}{2} \sum_i \omega_i^2 x_i^2.

A field or trajectory solver should test:

  • Maxwell constraints appropriate to the field representation;
  • symmetry points and known zero-field or zero-force locations;
  • Hessian eigenvalues and trap frequencies;
  • energy conservation for static conservative motion;
  • secular-frequency limits for driven traps;
  • convergence in mesh, multipole order, and integration step;
  • sensitivity to electrode, beam, and alignment parameters.

The trap depth, harmonic frequency, scattering rate, and coherence time are different observables and need not converge at the same rate.

An effective cavity simulation should declare:

  • retained matter levels and modes;
  • coupling convention and mode normalization;
  • detuning and rotating frame;
  • coherent drives;
  • cavity loss, matter decay, and dephasing channels;
  • input–output normalization;
  • photon cutoff;
  • initial state and measurement operator.

Strong coupling is an observable-dependent comparison among gg, decay rates, dephasing, detuning, and spectral resolution. Reproducing an avoided crossing in a closed Jaynes–Cummings matrix does not by itself predict a measurable split transmission line.

For pulses, retain the full envelope and phase convention:

Ω(t)=d⋅E0(t)ℏeiϕ(t).\Omega(t) = \frac{ \mathbf d\cdot\mathbf E_0(t) }{ \hbar } e^{i\phi(t)}.

Report whether Ω\Omega is a signed, complex, peak, or root-mean-square quantity. Pulse-area agreement,

Θ=∫Ω(t) dt,\Theta = \int \Omega(t)\,dt,

is a useful ideal benchmark but does not guarantee equal dynamics under detuning, bandwidth, leakage, Stark shifts, or decoherence.

LevelBenchmarkMain check
P0zero field or zero driveno spurious force or transition
P1harmonic trapanalytic frequency and conserved energy
P2low-saturation two-beam forceoddness in vv and red-detuned damping
P3ideal pulse sequencepulse area, phase, and frame convention
P4recoil ensemblemean, variance, seed, and time-step convergence
P5measured calibration curveheld-out parameters and uncertainty

A mature suite should contain complementary tests rather than one flagship number.

Run on every change:

  • dimensions and units;
  • Hermiticity or symmetry;
  • normalization and trace;
  • basis ordering;
  • selection-rule zeros;
  • conserved quantities;
  • exact matrix identities;
  • deterministic tiny cases.

These tests are fast and localize implementation regressions.

Run over explicit sequences:

{Nbasis,h,Rmax⁡,Δt,Nph,Mtraj}.\left\{ N_{\mathrm{basis}}, h, R_{\max}, \Delta t, N_{\mathrm{ph}}, M_{\mathrm{traj}} \right\}.

Change one control at a time unless a coupled refinement path is theoretically required. Preserve the raw sequence, not only an extrapolated final value.

For algebraic convergence, report residuals. For discretization, report observed order when an asymptotic regime exists:

pobs≈log⁡(∣Oh−Oh/2∣/∣Oh/2−Oh/4∣)log⁡2.p_{\mathrm{obs}} \approx \frac{ \log \left( |O_h-O_{h/2}| / |O_{h/2}-O_{h/4}| \right) }{ \log 2 }.

A plausible pobsp_{\mathrm{obs}} is evidence that the intended error regime has been reached. It is not a substitute for a continuum or reference comparison.

Use independent routes where possible:

  • radial shooting versus matrix diagonalization;
  • real-space versus basis-set hydrogen;
  • analytic versus numerical integrals;
  • length versus velocity transition forms;
  • finite difference versus automatic or analytic derivatives;
  • density-matrix versus trajectory dynamics;
  • direct steady-state solve versus long-time propagation;
  • time-domain spectrum versus resolvent or eigenmode spectrum;
  • two independent software implementations.

Independence matters. Two wrappers around the same library do not provide a strong cross-code test.

Every model has simplifying limits:

g→0,Ω→0,Γ→0,R→∞,mN→∞,Zα→0,s0→0.\begin{gathered} g\to0, \qquad \Omega\to0, \qquad \Gamma\to0, \qquad R\to\infty, \\ m_N\to\infty, \qquad Z\alpha\to0, \qquad s_0\to0. \end{gathered}

The output should approach the correct reduced model. A limit test is often more diagnostic than agreement at one generic parameter point.

If parameters are calibrated on one subset of observations, reserve another subset for validation. Examples include:

  • fit an effective quantum defect to some Rydberg levels and predict others;
  • fit a molecular potential near equilibrium and test isotope-dependent vibrational spacings;
  • calibrate a Rabi frequency at one intensity and test pulse-area scaling;
  • calibrate trap frequencies and predict anharmonic shifts;
  • fit decay rates and test two-time correlations.

Document the split before inspecting the held-out result whenever a strong predictive claim is intended.

Reproducibility is the ability to reconstruct the computational argument from preserved inputs, code, environment, and outputs. It is necessary but not sufficient for correctness.

Every published calculation should preserve:

FieldRequired content
identitytitle, author or maintainer, date, artifact version
physical targetspecies, state, geometry, observable, intended claim
equationsHamiltonian or generator with conventions
approximationsexplicit retained and omitted physics
representationbasis, grid, domain, ordering, truncations
parametersvalues, units, constants release, data provenance
algorithmsolver, tolerances, stopping criteria, initialization
environmentlanguage, package versions, lockfile or container recipe
stochastic stategenerator, seed policy, ensemble size
benchmarktarget, metric, tolerance, pass or fail
outputsmachine-readable data, plots derived from those data
limitationsknown failure regimes and unresolved discrepancies

The Environments, Code Style, and Validation Tests pages own the site-wide implementation details.

Store values with explicit unit metadata. “Frequency = 10” is incomplete. Even “10 MHz” may be ambiguous if a code expects angular frequency. Use a declared mapping such as

ω=2π(10 MHz)\omega = 2\pi \left( 10\,\mathrm{MHz} \right)

when the solver parameter is angular frequency. Atomic units should identify the nuclear-mass convention and any conversion constants used.

A quantum-chemistry method name does not reproduce a calculation. Preserve:

  • all nuclear coordinates, units, isotope masses, charge, and multiplicity;
  • basis-set name and exact revision or machine-readable basis definition;
  • effective core potentials and auxiliary bases;
  • frozen-core and active-space choices;
  • integration-grid and SCF settings;
  • symmetry handling and occupation constraints;
  • counterpoise or fragment conventions;
  • derivative and geometry-convergence thresholds.

Package defaults are versioned implementation choices, not universal physical conventions.

Do not publish only the preferred basis, grid, or cutoff. A convergence table should include:

(λj,Oj,rj,tj,statusj),\left( \lambda_j, O_j, r_j, t_j, \text{status}_j \right),

where λj\lambda_j is the refinement control, OjO_j the observable, rjr_j a residual or diagnostic, tjt_j optional resource information, and statusj\text{status}_j any warning or failure.

Failed points are scientifically useful. Removing them can hide instability or a restricted convergence regime.

Separate notebook narrative from reusable computation

Section titled “Separate notebook narrative from reusable computation”

A notebook should explain and inspect a calculation. Reusable numerical kernels, parameter validation, and benchmark assertions should live in importable modules or scripts when the calculation grows beyond a small pedagogical example. The notebook should run from a clean state in a declared order and should not depend on invisible interactive variables.

A plot is a view, not the primary result. Preserve:

  • the machine-readable arrays;
  • the script or notebook that produced the plot;
  • axis units and transformations;
  • fit model and weights;
  • uncertainty or confidence data;
  • any smoothing, broadening, interpolation, or windowing.

A displayed Lorentzian broadening parameter is part of the result and must not be omitted from provenance.

Deterministic and statistical reproducibility

Section titled “Deterministic and statistical reproducibility”

Bitwise identity can depend on hardware, compiler, thread scheduling, and linear-algebra libraries. The scientific target is often stronger in one sense and weaker in another: independently reproduced observables should agree within a physically and numerically justified tolerance.

For stochastic work, preserve:

  • pseudorandom generator family;
  • base seed and stream construction;
  • number of trajectories or samples;
  • aggregation order when numerically relevant;
  • uncertainty estimator;
  • convergence across independent seed ensembles.

One fixed seed is a regression case, not an uncertainty analysis.

A benchmark record should have its own version. Change it when:

  • the mathematical specification changes;
  • constants or reference data change;
  • an accepted tolerance changes;
  • the intended physical regime changes;
  • a bug invalidates prior outputs.

Do not loosen a tolerance merely because a new implementation fails. First determine whether the old tolerance represented theory, observed numerical behavior, or accidental platform-specific digits.

Use status labels honestly:

  • conceptual: equations and expected behavior are documented;
  • implemented: code exists and runs in a declared environment;
  • verified: structural and exact-model tests pass;
  • converged: numerical controls meet predeclared criteria;
  • validated: relevant independent physical comparisons pass;
  • archived: code, environment, data, and provenance are preserved.

The Reproducibility Status page owns the global promotion rules. A page should not imply that a planned notebook is already an executable artifact.

A compact benchmark report can be organized as

R=(P,E,C,V,U),\mathcal R = \left( \mathcal P, \mathcal E, \mathcal C, \mathcal V, \mathcal U \right),

where:

  • P\mathcal P is the physical problem declaration;
  • E\mathcal E is the executable environment;
  • C\mathcal C is the convergence record;
  • V\mathcal V is the verification and validation evidence;
  • U\mathcal U is the uncertainty and limitation statement.

The report should answer five audit questions:

  1. Identity: What exact problem was solved?
  2. Traceability: Where did every parameter and datum come from?
  3. Control: Which errors were varied, bounded, or estimated?
  4. Independence: Which checks did not reuse the implementation or data under test?
  5. Scope: What claim is supported, and which stronger claims are not?

The chapter is built as a sequence of domain-specific guides and benchmark notebooks. Titles without links are planned pages rather than published artifacts.

PageCanonical responsibilityAnchor benchmark
Computational Atomic Structuremethod map from radial models through correlation and relativistic correctionshydrogen and helium
Radial Schrödinger Solversboundary conditions, shooting, finite differences, and Numerov-style propagationhydrogenic spectrum
Variational Helium Notebookeffective-charge trial state and explicit correlation deficitvariational upper bound
Hartree–Fock Notebookanalytic Gaussian integrals, Fock construction, SCF iteration, and convergence separationclosed-shell helium
Molecular Orbital Computationoverlap, generalized eigenproblems, bonding and antibonding orbitalsH2+\mathrm{H}_2^+
Electronic Structure Methods Mapresponsible choice among HF, DFT, CI, coupled cluster, multireference, and Monte Carlomethod–basis grid
Vibrational Spectra Computationcalibrated mass-weighted Hessian, sinc-DVR Morse levels, transition moments, and experiment-facing error ledgerCO2_2 stretches and H35^{35}Cl
Time-Dependent Two-Level Systems NotebookRabi, detuning, pulse area, Ramsey, and rotating-wave comparisonanalytic Rabi solution
Optical Bloch Equation Notebooksaturation, linewidth, fluorescence, and steady stateanalytic steady population
Cavity QED Simulation Notebookphoton cutoff, dressed levels, vacuum Rabi dynamics, coherent-state revival, and optional lossJaynes–Cummings doublets
Laser Cooling Simulation Notebookforce curves, friction, recoil diffusion, Doppler temperature, intensity tradeoffs, and relaxationlow-saturation Doppler force
Reproducibility Benchmarksversioned acceptance suite and expected outputscomplete cross-domain ladder

For atomic structure, begin with Hydrogen as Atomic Prototype, Helium Atom, and Hartree–Fock for Atoms.

For quantum chemistry, begin with Molecular Hamiltonian, Potential-Energy Surfaces, and Electronic Structure Overview.

For quantum optics, begin with Two-Level Atom, Optical Bloch Equations, and Jaynes–Cummings Model.

For platform simulation, begin with Laser Cooling, Cavity QED Platforms, and Quantum Control in AMO.

Calling a converged solver a converged calculation

Section titled “Calling a converged solver a converged calculation”

An eigensolver residual or SCF threshold controls only one layer. Basis, domain, cutoff, model, and parameter errors remain.

Calling a finite matrix exact without qualification

Section titled “Calling a finite matrix exact without qualification”

The matrix may be diagonalized accurately while representing the continuum poorly. State “exact diagonalization of the stated finite matrix,” not “exact solution of the atom.”

Transition energies, forces, dipoles, polarizabilities, line strengths, and decay rates can converge differently. Test the observable being claimed.

Infinite versus finite nuclear mass, clamped versus vibrating nuclei, nonrelativistic versus relativistic theory, and bare versus effective Hamiltonians produce different reference values.

SCF thresholds, integration grids, basis pruning, ODE tolerances, photon cutoffs, and line broadening can change with package versions. Record them.

Using experiment as both fit and prediction

Section titled “Using experiment as both fit and prediction”

Reproducing fitted data is calibration. Reserve independent data or make a more limited claim.

Printed precision can exceed model accuracy, input precision, or experimental meaning. Report uncertainty and scope.

Molecular orbitals in an atomic basis satisfy C†SC=IC^\dagger S C=I, not C†C=IC^\dagger C=I. Ignoring SS corrupts energies, populations, and orthogonality.

Replacing negative eigenvalues by zero can conceal a bad integrator or invalid generator. Diagnose the source before applying any projection.

A small occupation in the highest photon state is helpful but not sufficient. Observables, transients, and neighboring cutoffs must also be stable.

Confusing reproducibility with correctness

Section titled “Confusing reproducibility with correctness”

A fully archived notebook can reproducibly implement a sign error. Independent verification and physical validation remain necessary.

A package can implement many Hamiltonians, basis conventions, and algorithms. Scientific claims should name the model and method before the software.

Classify each statement and give the missing qualification:

  1. “The hydrogen ground-state energy is exact.”
  2. “Dense diagonalization gives the exact molecular energy.”
  3. “The helium value is exact to fifteen digits.”
  4. “The Rabi curve is exact.”
Solution
  1. The value −Z2Eh/2-Z^2E_{\mathrm h}/2 is analytically exact for the specified nonrelativistic Coulomb Hamiltonian, nuclear-mass convention, and energy zero. It is not the complete physical energy of a real hydrogenic atom.
  2. Dense diagonalization can solve a specified finite matrix to floating-point accuracy. The molecular model, one-particle basis, active space, and correlation approximation remain finite or approximate.
  3. A high-precision helium value is a numerically converged reference for a stated Hamiltonian. The digits require an uncertainty and convergence argument; finite-mass, relativistic, and QED terms are separate.
  4. The Rabi curve is exact for a declared effective two-level Hamiltonian and pulse convention. Level truncation, classical driving, rotating-wave treatment, and absence of decoherence are model assumptions.

The common repair is to say exact for what mathematical object and under which physical assumptions.

A radial finite-difference calculation gives E1s=−0.4999999999EhE_{1s}=-0.4999999999E_{\mathrm h} with eigenpair residual 10−1310^{-13}. List four additional checks needed before claiming a ten-digit continuum result.

Solution

The residual verifies the finite matrix, not the radial continuum problem. Additional checks include:

  • refine the radial spacing and establish the expected convergence regime;
  • increase the outer boundary and test tail truncation;
  • vary the origin treatment and verify u(r)∝ru(r)\propto r for l=0l=0;
  • normalize with the radial measure and verify node count;
  • test the virial theorem;
  • compare other n,ln,l states rather than only one energy;
  • repeat with an independent method such as shooting or a spectral basis.

Ten printed digits in one grid are not a ten-digit error estimate.

3. Derive the helium effective-charge result

Section titled “3. Derive the helium effective-charge result”

For

E(ζ)=ζ2−278ζ,E(\zeta) = \zeta^2 - \frac{27}{8}\zeta,

find the stationary point and energy. Explain why the result is an upper bound but not a complete estimate of physical helium.

Solution

Differentiate:

dEdζ=2ζ−278.\frac{dE}{d\zeta} = 2\zeta - \frac{27}{8}.

Thus

ζ⋆=2716.\zeta_\star = \frac{27}{16}.

Substitution gives

E(ζ⋆)=(2716)2−278(2716)=−729256Eh=−2.84765625Eh.\begin{aligned} E(\zeta_\star) &= \left( \frac{27}{16} \right)^2 - \frac{27}{8} \left( \frac{27}{16} \right) \\ &= -\frac{729}{256} E_{\mathrm h} \\ &= -2.84765625 E_{\mathrm h}. \end{aligned}

The trial state is normalized and belongs to the domain of the stated nonrelativistic infinite-mass Hamiltonian, so Rayleigh–Ritz makes this an upper bound to that model’s ground-state energy. It omits explicit electron–electron correlation through r12r_{12} and does not include finite nuclear mass, relativistic, radiative, or nuclear-size corrections.

Assume F=F†F=F^\dagger and S=S†>0S=S^\dagger>0. Show how to transform

FC=SCεFC = SC\varepsilon

into an ordinary Hermitian eigenproblem, and state the numerical warning when SS has a very small eigenvalue.

Solution

Because SS is positive definite, it has a Hermitian square root. Write

S=UsU†,S−1/2=Us−1/2U†.S = U s U^\dagger, \qquad S^{-1/2} = U s^{-1/2}U^\dagger.

Set

C=S−1/2Y.C = S^{-1/2}Y.

Multiplying on the left by S−1/2S^{-1/2} gives

(S−1/2FS−1/2)Y=Yε.\left( S^{-1/2}FS^{-1/2} \right) Y = Y\varepsilon.

The transformed matrix is Hermitian. If Y†Y=IY^\dagger Y=I, then

C†SC=I.C^\dagger S C = I.

A very small eigenvalue of SS makes S−1/2S^{-1/2} large and amplifies roundoff and integral errors. Removing that direction changes the represented space, so the threshold and observable sensitivity must be reported.

Using

ρee(ss)=s2(1+s),s=Ω2Γ2Γ1(Δ2+Γ22),\rho_{ee}^{(\mathrm{ss})} = \frac{s}{2(1+s)}, \qquad s = \frac{ \Omega^2\Gamma_2 }{ \Gamma_1 \left( \Delta^2+\Gamma_2^2 \right) },

find the weak-drive and strong-drive limits. For pure radiative broadening, write ss in terms of Γ1\Gamma_1.

Solution

For s≪1s\ll1,

ρee(ss)≈s2,\rho_{ee}^{(\mathrm{ss})} \approx \frac{s}{2},

so the response is quadratic in the drive amplitude and Lorentzian in detuning. For s≫1s\gg1,

ρee(ss)⟶12,\rho_{ee}^{(\mathrm{ss})} \longrightarrow \frac{1}{2},

which is the saturated two-level population.

For pure radiative broadening,

Γ2=Γ12,\Gamma_2 = \frac{\Gamma_1}{2},

and therefore

s=Ω2/2Δ2+Γ12/4=2Ω2Γ12+4Δ2.s = \frac{ \Omega^2/2 }{ \Delta^2+\Gamma_1^2/4 } = \frac{ 2\Omega^2 }{ \Gamma_1^2+4\Delta^2 }.

This result depends on the stated Hamiltonian and Rabi-frequency convention; it is precisely the kind of factor-of-two benchmark a solver should include.

A cavity simulation with cutoff nmax⁡=10n_{\max}=10 reports P(n=10)=10−9P(n=10)=10^{-9} at the final time. Is cutoff convergence established? Design a stronger test.

Solution

No. Final-time boundary population can miss transient occupation, coherences with the boundary, or an observable that is sensitive to a small high-number tail.

A stronger test records the maximum boundary and near-boundary occupation over the full trajectory, then repeats the calculation for a sequence such as nmax⁡=8,10,12,14n_{\max}=8,10,12,14. Compare every claimed observable, trace, positivity, and conservation law where applicable. The cutoff is controlled only when the observables and diagnostics are stable within a predeclared tolerance.

For the low-saturation force on this page, expand to first order in vv and show that red detuning produces damping.

Solution

Define

f(x)=11+4x2/Γ2.f(x) = \frac{1}{ 1+4x^2/\Gamma^2 }.

Then

F(v)=ℏkΓs02[f(Δ−kv)−f(Δ+kv)].F(v) = \frac{\hbar k\Gamma s_0}{2} \left[ f(\Delta-kv) - f(\Delta+kv) \right].

For small vv,

f(Δ∓kv)≈f(Δ)∓kvf′(Δ).f(\Delta\mp kv) \approx f(\Delta) \mp kv f'(\Delta).

Hence

F(v)≈−ℏk2Γs0f′(Δ)v.F(v) \approx -\hbar k^2\Gamma s_0 f'(\Delta)v.

Since

f′(Δ)=−8Δ/Γ2(1+4Δ2/Γ2)2,f'(\Delta) = -\frac{ 8\Delta/\Gamma^2 }{ \left( 1+4\Delta^2/\Gamma^2 \right)^2 },

f′(Δ)>0f'(\Delta)>0 for Δ<0\Delta<0. Therefore

F(v)≈−αv,α=ℏk2Γs0f′(Δ)>0.F(v) \approx -\alpha v, \qquad \alpha = \hbar k^2\Gamma s_0 f'(\Delta) >0.

This verifies the sign in the low-saturation two-level model, not the validity of that model for multilevel or sub-Doppler cooling.

A paper reports a molecular dissociation energy that agrees with experiment to 0.1%0.1\%. It gives the method and basis-set names but no geometries, convergence sequence, relativistic or zero-point treatment, software version, or uncertainty. The same experimental value was used to tune one method parameter. What can be concluded, and what evidence is missing?

Solution

The numerical agreement can be reported, but it is a calibration result rather than an independent prediction because the experimental datum helped tune the method. The comparison also does not reveal whether errors cancel.

Missing evidence includes:

  • fragment and molecular geometries, charges, multiplicities, and energy zero;
  • electronic versus zero-point-corrected dissociation convention;
  • basis and correlation convergence;
  • basis-set superposition treatment;
  • frozen-core, relativistic, and other corrections;
  • solver and geometry thresholds;
  • package version and relevant defaults;
  • provenance and uncertainty of the experimental value;
  • parameter-fit procedure and covariance;
  • held-out molecules or observables for validation;
  • a complete computational environment and input record.

A defensible claim would identify the result as calibrated, preserve the full calculation, and test transferability on data excluded from the fit.

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