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Why do methane, Ammonia, and water have different shapes when each central chemical atom is surrounded by eight valence electrons? The answer separates the positions of atomic nuclei from the electron domains used in a VSEPR model.

Molecular geometry describes the three-dimensional arrangement of the atomic nuclei in a molecule, including bond lengths and bond angles. For a larger molecule, a shape name often describes just the neighbours of one central chemical atom. A Lewis structure records connections and electron bookkeeping; its flat layout does not fix molecular geometry.

In the VSEPR model, electron pair geometry includes both bonding electron domains and lone pairs, whereas molecular geometry counts only the chemical atoms. In methane, four bond pairs and no lone pairs give tetrahedral molecular geometry. In Ammonia, three bond pairs and one lone pair give trigonal pyramidal molecular geometry. In water, two bond pairs and two lone pairs give bent molecular geometry. All three use the same ideal tetrahedral electron pair geometry; this does not make their actual bond angles equal. See Flowers, Theopold, Langley and Robinson, Chemistry 2e, §7.6: electron-pair and molecular geometries.

A static drawing also needs a physical interpretation. The atomic nuclei undergo oscillations; an arrangement at a minimum of potential energy and an experimentally averaged arrangement need not have identical bond lengths or bond angles. This distinction matters when comparing measurements with quantum mechanics calculations; see the IUPAC Gold Book: experimental bond-length conventions. Gas electron diffraction gives a concrete route from a laboratory signal to molecular geometry rather than inferring shape from a drawing alone.

In the pair-interaction model of Newtonian mechanics, two bodies exert equal and opposite forces on each other:Both vectors are expressed in the same inertial frame at the same time. The subscripts name the agent and the recipient: $A$ acts on $B$, and $B$ acts on $A$. These are forces on different bodies, so they cannot cancel in the net force on either body. Newton's second law still uses all the forces on the particular body whose acceleration is sought. Identifying this third-law interaction pair does not require the bodies to be isolated: additional external forces can act at the same time.

The distinction makes Newton's third law useful both for drawing a free-body diagram and for deriving momentum conservation. A body-by-body calculation retains one member of each third-law interaction pair; a calculation for a collection containing both bodies cancels that pair in the total momentum balance. Equal interaction forces consequently coexist with nonzero, generally unequal accelerations.

Isaac Newton stated the equality and opposition of mutual actions in Law III of his 1687 Philosophiae Naturalis Principia Mathematica. The explanation distinguishes equal opposite changes of momentum from changes of velocity, which are inversely proportional to the bodies' masses when other influences are absent. Corollary III then explains why mutual interactions preserve the signed total momentum. The equations here are modern notation for that distinction. ^[ref]

The instantaneous body-pair equation has a scope: use it for the mechanical interactions assumed by this Newtonian mechanics model. In electromagnetism, bodies can exchange momentum with an electromagnetic field; their instantaneous mutual forces need not sum to zero. Momentum conservation then accounts for electromagnetic field momentum as well as matter, and for momentum crossing the chosen boundary. This complication occurs in classical electromagnetism, without invoking quantum mechanics.^[ref]

Awarded to Werner Heisenberg for creating quantum mechanics, including its application to forms of hydrogen. The Heisenberg uncertainty relation is one route into the resulting theory.^[ref]

Awarded in equal shares to Max Born for fundamental quantum mechanics research, especially the statistical interpretation of the wave function, and Walther Bothe for the coincidence circuit and discoveries made with it.^[ref]

A quantum observable is represented by a self-adjoint operator; its possible measured values are spectral values of that operator.

A physicist who developed matrix mechanics and held a professorship in theoretical physics at Hamburg.^[ref]

Spectrum analysis identifies substances by the positions and patterns of characteristic spectral lines, rather than by the overall colour of a flame alone. A small amount of a suitable salt is introduced into a hot, weakly luminous flame. In the historical prism spectroscope, light enters a narrow slit, a collimator makes the emerging rays nearly parallel, a prism separates them by wavelength, and an observing telescope shows images of the slit at different spectral positions. A reference scale or comparison spectrum makes positions reproducible.

A clean platinum wire and reagent blank help distinguish the sample's signal from contamination. A reference sample establishes the expected positions, while repeated cleaning and testing check whether an unfamiliar line belongs to the sample. Several substances can be recognized in one mixture because their characteristic line patterns can coexist, although overlapping lines and changing excitation conditions complicate identification. Robert Bunsen and Gustav Kirchhoff's original account explicitly emphasizes the faint background of the flame, the prism instrument and the characteristic patterns of alkali and alkaline-earth salts.^[ref]

In modern terms, emission lines arise when excited chemical atoms or ions release photons at energies corresponding to allowed differences between energy levels:The quantum mechanics behind this equation is a later explanation, not the theory available to an 1866 candidate. Similarly, absorption lines appear when a cooler foreground gas removes particular wavelengths from a brighter background. Agreement between laboratory line positions and dark lines in the solar spectrum permits identification of constituents of the solar atmosphere without bringing a solar sample into the laboratory. It does not establish the detailed chemical constitution of every layer of the Sun.

By December 1866, striking examples included caesium (1860), rubidium (1861), thallium (1861) and indium (1863). The first two were recognized in the work of Robert Bunsen and Gustav Kirchhoff, using conspicuous blue and deep-red spectral features respectively. William Crookes recognized the characteristic green line associated with thallium, while Ferdinand Reich and Hieronymus Theodor Richter identified indium through its indigo-blue spectral signature. These observations motivated chemical separation and further characterization; an unexpected line by itself is a clue to a new chemical element, not a complete proof.^{[ref][ref][ref][ref]}

The corresponding recognition of familiar chemical elements in the solar spectrum opened stellar chemical analysis. Later discoveries such as solar helium should not be credited to the 1866 state of the subject.

Some scientific classifications plausibly identify natural kinds; it does not follow that every useful theoretical category does. A good test asks whether the classification supports reliable inference because of relevant natural structure, rather than treating either practical usefulness or a precise verbal definition as sufficient.

A chemical element illustrates a strong case. Its atomic number fixes nuclear electric charge and constrains the electronic structure of the corresponding neutral atom. The classification thereby supports explanations of recurring chemical properties through quantum mechanics. Isotopes show why the claim must be qualified: equal atomic number does not imply equal mass, nuclear stability or every reaction rate. Whether a division is informative depends on which properties the investigation is trying to predict.

Biological classification need not have the same structure. The biological species concept emphasizes reproductive relations; a phylogenetic species concept emphasizes descent and diagnosable lineages. Hybridization, asexual reproduction and variation within a lineage make a single intrinsic essence an implausible universal criterion. A homeostatic property cluster theory instead asks whether interacting causal processes sustain a cluster of traits that supports induction, without requiring every individual to possess every trait.^[ref] These considerations can support realism about biological groupings without making all boundaries equally sharp.

There are also classifications whose role is expressly relative to a task. Calling a particle nonrelativistic compares its momentum scale with $mc$, or its speed with $c$. An investigator can set a tolerance for neglecting higher terms in an expansion. The boundary then depends partly on the accuracy required; it is not a newly discovered fundamental species of particle. Nevertheless, the approximation is constrained by measurable scales and can be objectively excellent or poor.

This prevents two opposite mistakes. Since a category is chosen for a purpose, it need not be arbitrary: a classification that repeatedly supports independent predictions has a better claim to natural grounding than an arbitrary grouping. Conversely, successful prediction does not uniquely identify the world's one privileged taxonomy. Different scales and explanatory questions may justify overlapping classifications of the same objects.

The defensible conclusion is selective and plural. Treat some kinds as tracking stable mechanisms, structures or historical lineages; assess the evidence for each classification and its intended domain. Retain useful idealized or conventional categories without pretending that every term in a scientific theory names an equally fundamental division of nature.

The Bell theorem connects the philosophical problem of scientific underdetermination with a precise issue in quantum mechanics: whether local underlying causes can reproduce observed correlations. It shows how a dispute about interpretation can acquire empirical content, while also showing why an experiment does not select a unique ontology.

A shared cause can produce strong correlations without a signal between distant measurements. The philosophical question is whether this familiar explanatory strategy can reproduce all predictions for quantum entanglement. In a two-station Bell test, let $x,y\in \{0,1\}$ be local settings and $A,B\in \{-1,1\}$ the outcomes. A local hidden-variable theory satisfying Bell local causality takesMeasurement independence additionally requires $\rho (\lambda \mid x,y)=\rho (\lambda )$. The same ensemble of underlying states must therefore apply across the four setting pairs.

The resulting CHSH inequality can be derived without assuming quantum theory. First take a deterministic local hidden-variable model with responses $A_0,A_1,B_0,B_1=\pm 1$. For each $\lambda$,because exactly one bracket vanishes. Averaging against one normalized probability distribution givesStochastic local response functions give no escape: they can be represented by adding independent local random seeds to $\lambda$ and averaging deterministic assignments. The essential restriction is the common setting-independent ensemble and local dependence of responses, not a separate insistence that all nature be deterministic.

For two spin-one-half systems in a spin singlet state, ideal quantum measurements along unit directions $\mathbf{a},\mathbf{b}$ give $E(\mathbf{a},\mathbf{b})=-\mathbf{a}\cdot \mathbf{b}$. ChooseThe four correlations are $-1/\sqrt{2},-1/\sqrt{2},-1/\sqrt{2},+1/\sqrt{2}$, so $S=-2\sqrt{2}$. Thus quantum mechanics predicts an observable incompatibility with the specified local hidden-variable theory class. This is stronger than saying that two interpretations happen to fit the observations collected so far.

Actual Bell tests require more than the ideal calculation. Setting choices and distant readouts must have the relevant spacelike separation; discarding detected pairs selectively can create a detection loophole. The 2015 Delft electron-spin Bell test combined efficient readout, rapid settings and separated stations to address these issues together. The reported statistic was $S=2.42\pm 0.20$, with a test of the local-model hypothesis accounting for device memory.^[ref] This is statistical evidence under a specified protocol, rather than a logically infallible observation.

The philosophical conclusion must be equally precise. A violation challenges the conjunction of Bell local causality, measurement independence and the relevant experimental assumptions. It does not disprove every possible hidden-variable account, or establish that the observer's mind creates the outcome. Different theories can reject different premises while agreeing on the observable correlations. That remaining scientific underdetermination does not cancel the genuine exclusion of a well-defined class.

Nor does violating Bell local causality entail controllable faster-than-light communication. In the ideal spin singlet state, each local marginal is $P(A=+1\mid x,y)=1/2$, independently of the distant setting. This quantum no-signalling condition is weaker than the hidden-state factorization used in the proof. Conflating them turns a precise result into an unwarranted conclusion about signalling.

The example therefore illustrates both the power and the limit of empirical testing in philosophy of science. Mathematical clarification can transform an apparently metaphysical disagreement into rival observational constraints. Evidence can discriminate those constraints without determining every question about the reality represented by a successful theory.

The Born rule assigns $p_i=⟨\psi |P_i|\psi ⟩$ to a projective measurement with projection operators $P_i$. Its numerical form can be shared by theories while the source of the probabilities differs. Comparing Bohmian mechanics, the GRW model and the many-worlds interpretation exposes three different roles: uncertainty over actual configurations, fundamental stochastic events, and weights for branch-relative expectation.

In Bohmian mechanics, the Schrödinger equation implies a probability continuity equation for $|\Psi {|}^2$ with current $j$, while the guidance equation transports an ensemble density $\rho$ with velocity $v=j/|\Psi {|}^2$:Thus $\rho =|\Psi {|}^2$ is preserved: quantum equilibrium equivariance. If an apparatus interaction produces disjoint configuration regions ${\Gamma }_i$ with occupied-branch norm $|c_i|$, integrating the equilibrium distribution gives $\mathrm{Pr}(Q\in {\Gamma }_i)=|c_i{|}^2$. The actual outcome is fixed by initial configuration; the distribution describes the typical or uncertain configuration, not a fundamental random collapse. Equivariance alone does not prove equilibrium initially: every admissible density is transported by the velocity field. A typicality account privileges the equivariant $|\Psi {|}^2$ measure and then explains subsystem statistics conditionally; that explanatory premise must not be hidden in the continuity equation.^[ref]

In the GRW model, the centre law $p(X)=\Vert L_i(X)\Psi {\Vert }^2$ is part of the stochastic dynamics. Since $\int L_i(X{)}^{†}{L}_i(X)dX=I$, it is normalized. For two well-separated correlated pointer packets with coefficients $a,b$, integration over centres around their respective occupied regions gives approximately $|a{|}^2,|b{|}^2$; cross-contributions are suppressed at separations large compared with $r_C$. This explains why macroscopic records follow the Born rule approximately, without a special postulate applying only when an observer measures. However, the squared-norm centre law already carries the relevant mathematical probability structure. The theory relocates the rule into a universal physical law; it does not derive all probabilities from a deterministic equation. There are also small predicted deviations from standard unitary quantum mechanics.^[ref]

In the many-worlds interpretation, every nonzero decohering component persists, so the question is not which single global branch will survive. It is why a rational observer should use branch weight $|c_i{|}^2$ for expectation or caring about successor records. Equal-amplitude symmetry and decision theory motivate equal weights for physically equivalent alternatives. For rational $|c_i{|}^2=m_i/M$, an ancillary refinement into $m_i$ equal-norm alternatives can motivate weight $m_i/M$, followed by continuity for other amplitudes. This argument requires assumptions that refining irrelevant details does not change value, that preferences respect the relevant quantum symmetries, and that weight tracks the intended notion of expectation. Those are substantive premises, not consequences of branch existence alone.^[ref]

Naive branch counting is unsuitable: decoherence yields approximate, refinement-dependent branches, and splitting one record into more environmental records should not change its weight. Nor is diagonality of a density matrix already an account of probability. The comparison therefore has no common derivation from bare formalism. Bohmian mechanics needs a justified equilibrium or typicality measure, GRW model needs a justified stochastic law, and an Everettian account needs a justified connection from branch structure and rationality to experienced statistics. Each offers a coherent location for the Born rule; the remaining explanatory costs differ.

Quantum mechanics is compatible with quantum no-signalling, but its full correlations are incompatible with Bell local causality under the usual additional assumptions. The answer depends on which locality condition is meant. A local operational prohibition on controllable faster-than-light communication is weaker than a causal explanation of correlations by a complete shared past.

Let $a,b\in \{-1,1\}$ be outcomes, $x,y$ local settings and $\lambda$ a complete relevant past specification. Bell factorization and measurement independence demandNeither assumes deterministic response. Put $A_x(\lambda )={\sum }_{a}ap(a|x,\lambda )$ and similarly $B_y$, so $|A_x|,|B_y|\le 1$. Pointwise,Averaging with the same $\rho$ for all settings gives the CHSH inequality $|E_{00}+E_{01}+E_{10}-E_{11}|\le 2$. For a spin singlet state, $E(\mathbf{a},\mathbf{b})=-\mathbf{a}\cdot \mathbf{b}$. Choose ${\mathbf{a}}_0=\hat{z}$, ${\mathbf{a}}_1=\hat{x}$, ${\mathbf{b}}_0=(\hat{z}+\hat{x})/\sqrt{2}$, ${\mathbf{b}}_1=(\hat{z}-\hat{x})/\sqrt{2}$; the magnitude becomes $2\sqrt{2}$. Thus the assumptions cannot all be maintained.^[ref]

There is nevertheless no signalling contradiction. If a local unread measurement has Kraus operators $M_a$ with ${\sum }_a{M}_a^{†}{M}_a=I$, thenThe equality follows by testing both sides against any distant observable and using cyclicity of the trace. Distant conditional states can differ after selecting $a$, but communicating that selection needs an ordinary message. The microcausality condition in quantum field theory similarly ensures commutation of spacelike-separated local observables; it does not make the vacuum or other entangled quantum states Bell-factorizable.

One can preserve different notions of locality by changing premises. Bohmian mechanics retains unique outcomes but its guidance equation is nonlocal for entangled systems; quantum equilibrium equivariance preserves the equilibrium distribution which masks that dependence from signalling. The many-worlds interpretation can combine local interaction equations with no unique global outcome, but a claim of locality must explain its branch-relative correlations; it has not thereby constructed the above Bell-local single-outcome model. The measurement-independence loophole, including suitable retrocausal or correlated-setting models, drops the shared setting-independent $\rho$ premise. Such models are logical possibilities, not demonstrations that the ordinary locality assumptions survive unchanged.

The justified answer is therefore conditional rather than an unqualified yes or no. Operational locality is retained by the quantum formalism. A theory reproducing all its correlations cannot retain Bell factorization, independent settings and the ordinary joint-outcome framework together. Neither denial of hidden variables nor an appeal to relativity alone removes the probabilistic contradiction.

For a nonrelativistic spinless particle in a scalar potential, the Time-dependent Schrödinger equation isAn initial wavefunction together with boundary conditions specifies the evolution. The Hamiltonian operator must be self-adjoint on the appropriate domain for closed-system evolution to be unitary. The equation is linear, so a superposition of solutions is another solution. Its complex wavefunction predicts probability amplitudes; the Born rule separately supplies the connection to measurement probabilities.

For a time-independent potential, separation $\psi (\mathbf{r},t)=\varphi (\mathbf{r})e^{-iEt/\hslash }$ gives the time-independent Schrödinger equation $H\varphi =E\varphi$. Normalizability and boundary conditions select the allowed energies of bound states; scattering states instead use incoming and outgoing boundary conditions and generalized normalization. A general state is a superposition of energy eigenstates, with a spectral integral as well if there is a continuous spectrum. Different energies accumulate different phases, allowing time-dependent position densities and oscillatory expectation values even though a single energy eigenstate has a stationary density.

For a real scalar potential, combining the equation with its complex conjugate yields probability conservation:With no current escaping the boundary, $\int |\psi {|}^2{d}^{3}r$ is constant. Matching conditions at a finite potential step follow from the differential equation and enforce the flux balance used in B6.

The Schrödinger equation is a dynamical postulate of nonrelativistic quantum mechanics, not a consequence of classical mechanics alone. The substitutions $E\mapsto i\hslash {\partial }_t$ and $\mathbf{p}\mapsto -i\hslash \nabla$ motivate its free-particle form from the dispersion relation, but do not derive the measurement postulates. The scalar equation omits intrinsic spin and relativistic particle creation. Spinful or relativistic problems require the corresponding extended theory. Nor does its deterministic unitary evolution, by itself, prescribe conditioning on a particular observed measurement outcome.

identical particles have the same intrinsic properties, including mass, charge and spin. Their labels are bookkeeping devices rather than measurable identities. When wave functions overlap, quantum mechanics supplies no observable trajectory that permanently identifies “particle 1” independently of “particle 2”. A many-particle description must therefore treat exchange consistently. The Hamiltonian and physical observables are invariant under relabelling identical particles.

For two particles, the exchange operator obeys ${\hat{P}}_{12}^2=\hat{I}$. The usual three-dimensional symmetrization postulate selects states symmetric under exchange for bosons and antisymmetric for fermions. In relativistic quantum theory, the Spin-statistics theorem associates integer spin with bosons and half-integer spin with fermions under its locality and positivity assumptions; the connection is not derived merely from ${\hat{P}}_{12}^2=\hat{I}$ in elementary nonrelativistic mechanics. For orthonormal one-particle states $u$ and $v$, the two-particle spatial combinations areThe sign concerns the complete state, including spin and other internal variables, not necessarily the spatial factor alone.

The antisymmetric state vanishes if both fermions occupy the same one-particle state: this is the Pauli exclusion principle. For $N$ fermions in orthonormal spin orbitals ${\chi }_j$, the normalized Slater determinant $\Psi =(N!{)}^{-1/2}\det [{\chi }_j(i)]$ supplies the required exchange sign. Bosonic occupation has no corresponding upper limit, and symmetrized products describe many bosons. Fermionic occupation is zero or one per complete one-particle state; two electrons can still occupy the same spatial atomic orbital with opposite spin.

Spin and spatial symmetry are linked. A two-electron spin singlet state is antisymmetric, so its spatial factor must be symmetric. A symmetric triplet state instead requires an antisymmetric spatial factor. Exchange then changes pair correlations and the energies available when interactions depend on particle separation, even without introducing a new classical “exchange force”. It contributes to atomic shell structure, bonding and magnetic behaviour.

In an occupation-number description, bosonic creation and annihilation operators satisfy $[{\hat{a}}_i,{\hat{a}}_j^{†}]={\delta }_{ij}$, whereas fermionic operators satisfy $\{{\hat{c}}_i,{\hat{c}}_j^{†}\}={\delta }_{ij}$ and anticommute among themselves. The latter imply $({\hat{c}}_i^{†}{)}^2=0$. This formalism implements the same exchange constraints without assigning permanent particle labels.

For noninteracting particles in thermal equilibrium, the mean occupation of a state of energy $ϵ$ isFermi-Dirac statistics produces a filled Fermi sea at zero temperature and degeneracy pressure; Bose-Einstein statistics permits macroscopic Ground state occupation when the density of available states and thermodynamic conditions allow condensation. The different statistics therefore have measurable collective consequences, not just different notation.^[ref]

When phase-space occupation is dilute, both distributions reduce to the Maxwell–Boltzmann statistics limit. Likewise, well-separated localized wave packets have negligible overlap and small exchange corrections, so effectively labelled classical trajectories can become a useful approximation. In two spatial dimensions more general exchange statistics are possible; the standard boson/fermion account here concerns ordinary three-dimensional particles and their total states.

Operators, quantization and rotations. Angular momentum is the generator of spatial rotations. In quantum mechanics, its components are Hermitian operators on their appropriate domains and obeyThese angular momentum commutation relations prevent all three components from having simultaneous sharp values. For example, the Robertson uncertainty principle gives $\Delta J_x\Delta J_y\ge \hslash |⟨J_z⟩|/2$. One conventionally diagonalizes ${\hat{J}}^2$ and a selected component ${\hat{J}}_z$:The allowed labels are $j=0,\frac{1}{2},1,\frac{3}{2},\dots$ and $m=-j,-j+1,\dots ,j$. An angular-momentum multiplet has $2j+1$ states. The magnitude $\hslash \sqrt{j(j+1)}$ differs from the largest possible component $\hslash j$; the remaining components fluctuate even in a state with maximal $m$.

The angular momentum lowering operator and its raising counterpart, ${\hat{J}}_{\pm }={\hat{J}}_x\pm i{\hat{J}}_y$, satisfyThe ladder terminates at $m=\pm j$. A rotation through angle $\theta$ about unit vector $\hat{\mathbf{n}}$ acts through the unitary operator $\exp [-i\theta \hat{\mathbf{n}}\cdot \hat{\mathbf{J}}/\hslash ]$. Thus quantized components and the continuous rotation of a state are compatible.

Orbital angular momentum. The orbital contribution is associated with motion in space:For a spinless spatial wavefunction, the simultaneous angular eigenfunctions are the spherical harmonics $Y_{\ell m}(\theta ,\varphi )$, with $\ell =0,1,2,\dots$ and $m=-\ell ,\dots ,\ell$. Single-valued ordinary scalar spatial wavefunctions give integer orbital labels. In a central potential energy, $[\hat{H},{\hat{L}}^2]=[\hat{H},{\hat{L}}_z]=0$, so stationary states may be labelled by these angular quantum numbers. The angular kinetic contribution appears in the radial equation as $\ell (\ell +1){\hslash }^2/(2m{r}^2)$, the centrifugal potential. Noncentral interactions need not conserve these orbital labels.

Intrinsic spin and addition. Spin angular momentum is an intrinsic internal degree of freedom with the same commutation algebra. It is not the angular momentum of a small classical charged sphere literally rotating about its centre. For an electron, $s=1/2$ and $m_s=\pm 1/2$, so ${\hat{S}}_i=(\hslash /2){\sigma }_i$ in terms of the Pauli matrices. Its squared spin is $3{\hslash }^2/4$. Other particles can have integer or half-integer spin, including spin zero.

For one particle with orbital and spin degrees of freedom, $\hat{\mathbf{J}}=\hat{\mathbf{L}}+\hat{\mathbf{S}}$; the two component sets commute with each other. Addition of angular momentum permits $j=|\ell -s|,|\ell -s|+1,\dots ,\ell +s$. The coupled states $|j,m_j⟩$ are linear combinations of the uncoupled $|\ell ,m_{\ell }⟩|s,m_s⟩$ with $m_j=m_{\ell }+m_s$, determined by Clebsch-Gordan coefficients. A rotationally invariant spin-orbit interaction can conserve $J^2,J_z$ while mixing the separate component labels.

Angular momentum also carries a magnetic moment. For an electron's orbital motion and intrinsic spin,The minus signs reflect negative electric charge. With the Bohr magneton ${\mu }_B=e\hslash /(2m_e)$, a spin projection $m_s$ has ${\mu }_z=-g_s{\mu }_B{m}_s$. A magnetic field can therefore distinguish angular-momentum states through their interaction energy $-\mathbf{\mu }\cdot \mathbf{B}$.

Stern–Gerlach measurement. In the Stern-Gerlach experiment, atoms emerge from a heated source, pass through collimating apertures, traverse a strongly inhomogeneous magnetic field, and strike a position-sensitive screen. The beam is neutral, so its separation is interpreted through the atomic magnetic moment rather than the ordinary charged-particle Lorentz force. Near a chosen quantization direction, the interaction givesA uniform field can exert a torque but would not separate the beam by this translational force; the gradient is essential. Different allowed magnetic-moment components become correlated with different trajectories. A classical ensemble with continuously varying orientations would yield a continuous spread, whereas discrete quantum components yield separated channels.

In the modern electronic description of ground-state silver, filled shells cancel their electronic angular momenta and the unpaired $5s$ electron has $L=0$, $S=1/2$, $J=1/2$. The effective electronic measurement therefore has two components, approximately ${\mu }_z=\pm {\mu }_B$, rather than an orbital $\ell =1/2$, which is not allowed. For positive field gradient the electronic $m_J=+1/2$ component has negative ${\mu }_z$ and deflects downward in this coordinate convention. Nuclear spin and hyperfine structure are neglected in this simplified two-channel account. Historically the original splitting preceded the electron-spin interpretation, so the modern explanation should not be confused with the original investigators' interpretation.

More generally a prepared spin state $a|+z⟩+b|-z⟩$ gives the two outcomes with probabilities $|a{|}^2,|b{|}^2$. Selecting one channel prepares a state for further measurements. An ideal second analyser along the same axis then gives a definite result, whereas one along a perpendicular axis gives two equally likely outcomes for a spin-one-half eigenstate. This connects the apparatus directly to incompatible spin components and the Born rule. Angular momentum is quantized through its operator algebra; the Stern–Gerlach gradient turns that discrete internal information into spatially distinguishable outcomes.

The Bohr model combines classical circular motion in the Coulomb potential with explicitly quantum postulates. A one-electron atom of nuclear charge $+Ze$ has electron–nucleus reduced mass $\mu$. With $C=Z{e}^2/(4\pi {\epsilon }_0)$, the relative circular orbit obeysBohr postulates permitted nonradiating stationary orbits with $L=n\hslash$, for $n=1,2,\dots$. These assumptions giveFor hydrogen with the nucleus taken infinitely heavy, the $n=1$ radius is the Bohr radius, $a_0\simeq 5.29\times 10^{-11}\mathrm{m}$. The finite reduced mass gives the small nuclear-motion correction, and increasing $Z$ contracts the one-electron orbit.

The circular-motion equation gives $T=C/(2r)$ while the potential energy is $-C/r$, so the total energy is $-C/(2r)$. Substituting the quantized radius yieldsFor the heavy-nucleus hydrogen approximation, $E_n\simeq -13.6\mathrm{eV}/n^2$. The ionization threshold is zero energy, so removing the ground-state electron requires about $13.6\mathrm{eV}$.

The model further postulates that radiation is emitted or absorbed only in transitions between stationary orbits, with photon energy $h\nu =|E_i-E_f|$. Emission from $n_i>n_f$ givesThus it reproduces the principal hydrogen spectral series, their limiting wavelengths, and the gross hydrogenic energy levels. For example, $n=3\to 2$ in hydrogen has $\Delta E\simeq 1.89\mathrm{eV}$ and $\lambda \simeq 656\mathrm{nm}$, a visible line. Absorption reverses the transition when the photon matches the energy gap.

The achievement is that quantized energies explain discrete spectra, but the model's stationary orbits are postulates rather than consequences of classical electrodynamics: an accelerating classical charge would radiate. It does not provide a general calculation of line intensities or transition selection rules and fails as a quantitative theory of many-electron atoms. Spin, fine structure and the full Zeeman effect require further physics. Modern quantum mechanics replaces definite electron orbits by wavefunctions and quantum probabilities. In particular, the true hydrogen ground state has $\ell =0$, so its orbital angular momentum vanishes; the model's rule $L=n\hslash$ should not be identified with the modern orbital eigenvalue rule $L^2=\ell (\ell +1){\hslash }^2$. Bohr's energy quantization remains a successful hydrogenic approximation, while its literal orbital picture does not.

Time dependence in quantum mechanics describes how a prepared quantum state changes and thereby changes the probabilities of later measurements. For an isolated system, the Schrödinger picture assigns this evolution to a state vector $|\psi (t)⟩$, governed by the Time-dependent Schrödinger equationThe Hamiltonian is a self-adjoint operator; it has units of energy, while $\hslash$ has units of action, so $\hat{H}/\hslash$ has units of inverse time. For a particle with potential energy $V(\mathbf{r},t)$, this becomesGiven a suitable initial wavefunction and the physical boundary conditions, this first-order equation determines its subsequent propagation. Its linearity means that the evolution of a quantum superposition is the corresponding quantum superposition of evolved states.

For a real potential energy, this equation and its complex conjugate imply the local continuity equationHere $\rho$ is the probability density and $\mathbf{j}$ the probability current. Vanishing net boundary flux preserves wavefunction normalization, as required by the Born rule.

The time-evolution operator packages the solution for every initial state:Because ${\hat{H}}^{†}=\hat{H}$, differentiation givesTherefore $U^{†}U=I$: this is unitary time evolution, preserving inner products and all state norms. It is reversible, with $U(t,t_0{)}^{-1}=U(t_0,t)=U(t,t_0{)}^{†}$, and obeys the composition law $U(t_2,t_0)=U(t_2,t_1)U(t_1,t_0)$.

For a time-independent Hamiltonian, the solution is the operator exponentialIf the Hamiltonian varies with time, the analogous simple exponential of its integral is valid when $[\hat{H}(t),\hat{H}(t^{\prime })]=0$ for all relevant times. Otherwise time ordering is essential:The meaning is explicit in the first terms of the ordered series,the later-time operator stands on the left. In the position representation, the same propagation is expressed by the quantum-mechanical propagatorIts initial value is the Dirac delta function ${\delta }^3(\mathbf{r}-{\mathbf{r}}^{\prime })$.

A time-independent Hamiltonian has energy eigenstates satisfying $\hat{H}|n⟩=E_n|n⟩$. A single such initial state evolves asIt is a stationary state: its global phase changes, but its probability density and the distributions of time-independent observables do not. Its energy is sharp. Any quantum superposition entirely within one degenerate energy eigenspace also acquires one common global phase and is stationary. Stationarity does not require zero probability current; for instance, $u_n(\varphi )=e^{in\varphi }/\sqrt{2\pi }$ on the ring has a constant density and persistent circulation when $n\ne 0$.

An arbitrary normalized state can instead contain different energy eigenvalues:A continuous spectrum requires corresponding integrals. For the discrete case, an energy measurement gives $E_n$ with fixed probability $|c_n{|}^2$ (summed over degeneracies), but relative quantum phases change with time. ConsequentlyThe interference terms can oscillate at angular frequencies $(E_m-E_n)/\hslash$. For two populated energy levels, this supplies a characteristic period $2\pi \hslash /|E_m-E_n|$ when the interference term is nonzero. Thus fixed energy populations do not imply a stationary spatial distribution.

For a normalized state and an observable $\hat{A}(t)$, its expectation value isThis is the statistical mean over repeated preparations and measurements. In an eigenbasis of energy eigenstates for a time-independent Hamiltonian and a time-independent $\hat{A}$,Only matrix elements connecting different energies can generate these oscillations. If $[\hat{A},\hat{H}]=0$, its expectation value is constant for every initial state, provided it has no explicit time dependence.

Differentiating the expectation value and substituting the Schrödinger equation for both the bra and ket proves the general Ehrenfest theorem:Equivalently,These manipulations require the state to lie in the relevant operator domains. Taking $\hat{A}=\hat{H}$ gives $d⟨H⟩/dt=⟨{\partial }_t\hat{H}⟩$, so energy is conserved under a time-independent Hamiltonian.

For $\hat{H}={\hat{p}}^2/(2m)+V(\hat{x})$, the canonical commutation relation givesHence the particularly useful position-and-momentum form of Ehrenfest theorem isIt resembles Newton's second law, but the mean force generally differs from the force at the mean position. If a narrow wave packet samples a region where the force varies little, $⟨V^{\prime }(x)⟩\simeq V^{\prime }(⟨x⟩)$ gives approximate classical motion. For a quadratic potential energy this replacement is exact. In particular the quantum harmonic oscillator obeysThe centroid follows the classical harmonic oscillator, although this does not specify the full evolving wavefunction or its width.

The Heisenberg picture expresses the same physics by assigning evolution to observables instead:The expectation value is unchanged, and differentiation yields $d{\hat{A}}_H/dt=(i/\hslash )[{\hat{H}}_H,{\hat{A}}_H]+U^{†}({\partial }_t{\hat{A}}_S)U$. Thus state propagation, evolving expectation values, and the classical correspondence in Ehrenfest theorem are mutually consistent descriptions of the same unitary time evolution.

Take a representative tennis-ball mass of $m\simeq 0.06\mathrm{kg}$. The speed is nonrelativistic, so the de Broglie wavelength isThis is an estimate because the mass was not specified. The wavelength is vastly smaller than any practicable aperture or obstacle separation: a diffraction angle of order $\lambda /d$ is unresolvably small for laboratory-scale $d$. Moreover, interactions with air, thermal radiation and the apparatus destroy observable coherence between macroscopically distinct paths. Quantum mechanics still applies; the small wavelength and rapid decoherence explain why ordinary experiments reveal classical trajectories rather than a measurable interference pattern.

The time-independent Schrödinger equation is the energy eigenvalue equation $\hat{H}\psi =E\psi$ for a particle of mass $m$. The Hamiltonian operator is the sum of the kinetic operator $-({\hslash }^2/2m)d^2/d{x}^2$ and the prescribed potential energy $V(x)$. Here $\hslash$ is the reduced Planck constant. A corresponding stationary state is $\Psi (x,t)=\psi (x)e^{-iEt/\hslash }$. The Born rule identifies $|\Psi {|}^2=|\psi {|}^2$ as probability density for a state with wavefunction normalization $\int |\Psi {|}^{2}dx=1$; integrating it over an interval gives a position probability. A plane wave scattering state is not a normalizable wavefunction on the whole line, but its probability currents give the reflection and transmission fractions of an incident wave packet.

There is a notation discrepancy in the sources: the original PDF prints an unbarred $h^2$ in the kinetic term, whereas the local TeX uses ${\hslash }^2$. The standard physical equation uses the reduced Planck constant $\hslash =h/(2\pi )$, where $h$ is the Planck constant; that convention is used below. Reading the printed $h$ literally as the Planck constant would scale all lengths in this model by $2\pi$ relative to the standard answers, but would leave the amplitude ratios unchanged.

For $E>V_0$, both sides allow oscillatory wavefunctions. A classical particle always crosses the potential step and slows because its kinetic energy falls from $E$ to $E-V_0$. In quantum mechanics there is generally both reflection and transmission even though the particle is above the step. Define the positive wavenumbersWith no wave incident from the right, writeA finite potential step with constant mass makes both the wavefunction and its first derivative continuous. The two boundary conditions at $x=0$ areSolving gives the reflected and transmitted wavefunctionsFor the specified electron energies, $q/k=\sqrt{10/50}=1/\sqrt{5}$, so the relative probability amplitudes areThe transmitted probability amplitude exceeding one is compatible with conservation of quantum probability, since the outgoing speed is smaller. In fact the probability current $j=(\hslash /m)\mathrm{Im}({\psi }^{\ast }{\psi }^{\prime })$ givesThese are the quantum reflection probability and transmission probability, which must be distinguished from the requested relative amplitudes.

Classically, a particle with $0<E<V_0$ is completely reflected and never enters the raised region. In quantum mechanics the wavefunction penetrates the classically forbidden side as an evanescent wave. Define the tunnelling decay constantBoundedness at positive infinity excludes $e^{+\kappa x}$, soMatching the wavefunction and its derivative givesThe reflected probability amplitude has unit modulus, hence quantum reflection probability one. The decaying tail carries zero probability current: this semi-infinite potential step has no transmitted beam at infinity, unlike a finite potential barrier. The sketch shows an exact matched example rather than attempting to assign a single real value to a complex wavefunction.

Because the probability density decays as $|C{|}^2{e}^{-2\kappa x}$, the requested $1/e$ penetration distance isFor a proton, take $m_p=1.67262\times 10^{-27}\mathrm{kg}$, $V_0-E=10\mathrm{MeV}=1.60218\times 10^{-12}\mathrm{J}$ and $\hslash =1.05457\times 10^{-34}\mathrm{J}\mathrm{s}$. ThenThe wavefunction amplitude decay length $1/\kappa =1.44\mathrm{fm}$ is twice this value. The nonrelativistic equation supplied in the paper is appropriate for this estimate since $10\mathrm{MeV}$ is small compared with the proton rest energy, approximately $938\mathrm{MeV}$. If the original PDF's unbarred $h$ is instead read literally as the Planck constant, the displayed differential equation gives $d_{\mathrm{literal}}=2\pi d=4.53\mathrm{fm}$. This is a valid calculation for that literal coefficient, but $0.720\mathrm{fm}$ is the physical estimate using the standard Schrödinger equation.