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Fine-structure constant

The fine-structure constant, denoted by the Greek letter α, is a fundamental dimensionless physical constant that quantifies the strength of the electromagnetic interaction between elementary charged particles, such as electrons and photons.^[1] It is defined as α = e² / (4πε₀ ħ c), where e is the elementary charge, ε₀ is the vacuum permittivity, ħ is the reduced Planck constant, and c is the speed of light in vacuum.^[1] The current recommended value, based on the 2022 CODATA adjustment, is α = 7.2973525643(11) × 10⁻³, or equivalently, its inverse 1/α ≈ 137.035999177(21), with a relative uncertainty of about 1.5 × 10⁻¹⁰.^[2] Introduced by Arnold Sommerfeld in 1916, the constant arose from his extension of the Bohr model of the hydrogen atom, incorporating relativistic effects to account for the observed fine splitting in atomic spectral lines.^[1] This "fine structure" refers to the small deviations from the energy levels predicted by the non-relativistic Bohr theory, which Sommerfeld explained by allowing elliptical orbits and considering the relativistic increase in electron mass.^[1] Over time, the fine-structure constant has become central to quantum electrodynamics (QED), the quantum field theory describing electromagnetic interactions, where it determines the magnitude of radiative corrections and governs phenomena like the Lamb shift and anomalous magnetic moments of particles.^[1] As one of the key coupling constants in the Standard Model of particle physics, α highlights the fundamental scale of electromagnetism relative to other forces, such as the strong and weak nuclear forces.^[1] Its dimensionless nature makes it a pure number without units, intriguing physicists because it appears ubiquitously in atomic, molecular, and solid-state physics, influencing everything from the stability of matter to the behavior of light in materials.^[1] Although α is not predicted by theory and must be measured experimentally, its value runs with energy scale due to quantum effects like vacuum polarization, increasing slightly at higher energies—for instance, α ≈ 1/128 near the Z boson mass.^[1] Precise measurements, often using techniques like the quantum Hall effect or electron g-2 experiments, continue to refine its value and test the consistency of QED predictions.^[1]

Definition and Fundamentals

Definition

The fine-structure constant, denoted by the symbol \alpha, is a fundamental dimensionless quantity in physics that quantifies the strength of the electromagnetic interaction between elementary charged particles. In SI units, it is precisely defined as

\alpha = \frac{e^2}{4\pi \epsilon_0 \hbar c},

where e is the elementary electric charge, \epsilon_0 is the vacuum permittivity, \hbar is the reduced Planck's constant, and c is the speed of light in vacuum. This expression arises from combining the fundamental constants that govern electric charge, quantum mechanics, and relativity, providing a measure of how strongly charged particles couple to the electromagnetic field.^[1] The constant originates from the observation of fine structure in the spectral lines of atoms, particularly the closely spaced splittings in the hydrogen atom's emission spectrum, which could not be explained by the non-relativistic Bohr model alone. In 1916, Arnold Sommerfeld introduced \alpha while extending the Bohr atomic model to include relativistic corrections, showing that the fine structure splitting in hydrogen's spectral lines is proportional to \alpha^2. These splittings represent small deviations in energy levels due to the electron's relativistic motion and spin-orbit coupling. Being dimensionless, \alpha is independent of any unit system, making it a universal constant that permeates diverse areas of physics without reliance on arbitrary scales. This property underscores its role as a pure number reflecting the intrinsic scale of electromagnetic interactions in nature. In the context of Paul Dirac's 1928 relativistic quantum mechanical treatment of the hydrogen atom, the Dirac equation yields energy levels where the fine structure splitting factor is exactly \alpha^2 / n^3 (with n the principal quantum number), confirming Sommerfeld's earlier relativistic approximation and elevating \alpha to a cornerstone of quantum electrodynamics.

Numerical Value and Dimensionless Nature

The fine-structure constant, denoted by α, has the recommended value of 7.2973525643(11) × 10^{-3}, or equivalently, its reciprocal 1/α = 137.035999177(21), as determined by the 2022 CODATA adjustment of fundamental physical constants.^[2] This value carries a relative standard uncertainty of approximately 1.5 × 10^{-10}, reflecting the high precision achieved through contemporary measurements. The constant is dimensionless, meaning it is a pure numerical value independent of the choice of units, which ensures its invariance across different physical systems and scales.^[3] In the Gaussian cgs unit system, α is explicitly given by the expression

\alpha = \frac{e^2}{\hbar c},

where e is the elementary charge (in statcoulombs), ℏ is the reduced Planck's constant, and c is the speed of light.^[4] This formulation highlights its role as the coupling strength of quantum electrodynamics, scaled by fundamental constants. The absence of any theoretical framework predicting the exact numerical value of α remains one of the unresolved mysteries in fundamental physics, with no ab initio derivation available from the Standard Model or beyond.^[3] The dimensionless nature of α has profound implications for theoretical physics. It remains unchanged under unitary transformations or rescalings of physical quantities, facilitating comparisons across disparate energy scales. In natural units, where ℏ = c = 1, the expression simplifies such that the square of the elementary charge is e² = α, underscoring its direct interpretation as the strength of electromagnetic interactions without additional dimensional factors.^[5] This property positions α as a fundamental parameter that permeates diverse areas of physics, from atomic spectra to particle interactions, always manifesting as a fixed numerical factor.

Measurement and Determination

Historical Measurements

The fine-structure constant was first estimated in 1916 by Arnold Sommerfeld through his analysis of the fine structure observed in the spectral lines of hydrogen atoms, particularly the splitting in the Balmer series. Using a relativistic modification to the Bohr atomic model, Sommerfeld derived the constant as a dimensionless parameter governing the strength of electromagnetic interactions at atomic scales, yielding an approximate value of \alpha \approx 1/137.^[1] This estimate was based on precise measurements of spectral line separations, such as the H\alpha line, which aligned closely with theoretical predictions from the relativistic fine-structure formula.^[6] A significant contribution to the numerical determination of \alpha came from Robert A. Millikan's oil-drop experiment in 1917, which provided one of the earliest accurate measurements of the elementary charge e = (4.774 \pm 0.002) \times 10^{-10} esu. Since \alpha = e^2 / (\hbar c) in Gaussian units, Millikan's value of e, combined with contemporaneous determinations of the speed of light c (from interferometric methods) and the reduced Planck's constant \hbar (derived from Planck's constant h via blackbody radiation or photoelectric effect data), enabled the first quantitative computations of \alpha from fundamental constants.^[7] These early \hbar and c values, however, carried uncertainties of several percent, limiting the precision of \alpha to about four significant figures.^[8] By the mid-20th century, particularly in the 1940s, refinements in atomic spectroscopy—such as high-resolution studies of hydrogen and alkali metal fine-structure splittings—and precision interferometry for c improved the accuracy of \alpha. These efforts yielded values around \alpha^{-1} \approx 137.04, marking a deviation from the integer 137 conjectured in some theoretical models and highlighting the constant's empirical nature.^[9] Challenges in achieving higher precision persisted due to incomplete knowledge of fundamental constants, including variations in h measurements and the nascent understanding of quantum electrodynamic corrections to atomic spectra.^[10]

Modern Measurements and Precision

Since the 1980s, the quantum Hall effect and Josephson junctions have provided foundational high-precision measurements of the elementary charge e and Planck's constant \hbar, enabling indirect determinations of the fine-structure constant \alpha = e^2 / (4\pi \epsilon_0 \hbar c) through metrological standards.^[11] These techniques achieved relative precisions on the order of $10^{-9} for \alpha by the late 20th century, establishing a benchmark for linking electrical units to fundamental constants before the 2019 SI redefinition fixed e and \hbar.^[12] Advancements in atomic recoil experiments using laser-cooled atoms have significantly improved precision in the 21st century. By measuring the recoil velocity of atoms from photon absorption, such as in rubidium or cesium, the ratio h/m (where m is the atomic mass) is determined, which combines with spectroscopic data to yield \alpha. A notable 2008 experiment at LKB (Laboratoire Kastler Brossel) using Bloch oscillations in an accelerated optical lattice for ^{87}Rb atoms reported \alpha^{-1} = 137.03599945(62), corresponding to a relative uncertainty of approximately $4.5 \times 10^{-9}.^[13] Subsequent refinements, including NIST contributions to atom interferometry, have pushed uncertainties to around $10^{-10}, making recoil methods competitive with other approaches.^[14] Additionally, 2024 electron g-factor measurements using Penning traps have refined \alpha via the anomalous magnetic moment a_e = (g-2)/2, with an updated value from Harvard improving agreement with quantum electrodynamics predictions while highlighting minor tensions (around 1-2\sigma) with some higher-order theoretical terms.^[15] The current CODATA 2022 recommended value is \alpha = 7.2973525643(11) \times 10^{-3}, or \alpha^{-1} = 137.035999177(21), with a relative uncertainty of 1.6 \times 10^{-10}, dominated by inputs from electron g-factor and atomic recoil data.^[16] This precision reveals subtle discrepancies with certain theoretical predictions in quantum electrodynamics, such as those involving hadronic contributions, motivating ongoing refinements.^[17]

Physical Interpretations

Role in Atomic and Molecular Physics

In atomic physics, the fine-structure constant α governs the magnitude of relativistic corrections that cause the splitting of spectral lines in hydrogen-like atoms, known as fine structure. These corrections arise from the relativistic nature of the electron's motion and spin-orbit coupling, as captured by the Dirac equation. The energy shift ΔE for a given level n,j is ΔE = E_n \frac{\alpha^2}{n^2} \left( \frac{n}{j + \frac{1}{2}} - \frac{3}{4} \right), where E_n is the non-relativistic Bohr energy and j is the total angular momentum quantum number. This shift is on the order of α² ≈ 5 × 10^{-5} relative to the gross structure levels, making it a small but observable perturbation that refines the Bohr model's predictions.^[18] Beyond the Dirac-derived fine structure, quantum electrodynamic (QED) effects introduce additional shifts, such as the Lamb shift, which further splits the 2S_{1/2} and 2P_{1/2} levels in hydrogen by about 1057 MHz. While the Lamb shift originates from vacuum polarization and self-energy diagrams in QED, its magnitude is ordered by powers of α, scaling roughly as α³ times the fine-structure scale, emphasizing α's role in quantifying the relative strength of electromagnetic interactions at atomic scales. This correction, though smaller than the Dirac fine structure by a factor of about α, is crucial for matching experimental spectra precisely.^[19] The fine-structure constant also influences applications like the Zeeman effect, where an external magnetic field splits atomic levels; in the presence of fine structure, this results in the anomalous Zeeman effect, with splitting patterns depending on the Landé g-factor that incorporates j and thus the α-induced fine-structure intervals. For instance, in alkali atoms, the fine structure modulates Zeeman sublevels, altering selection rules and polarization in spectral lines. Similarly, hyperfine structure—arising from electron-nuclear spin interactions—scales with α⁴ times the reduced mass ratio m_e/m_p, as the interaction energy involves the Fermi contact term proportional to the electron density at the nucleus, which itself depends on α³ from the Bohr radius. In hydrogen, this yields the 21 cm hyperfine transition, with splitting ΔE_hf ∝ (8/3) g_p α⁴ (m_e/m_p) Ry, where Ry is the Rydberg energy.^[20]^[21]^[22] In broader atomic contexts, α determines the scale of ionization potentials through the Rydberg constant, Ry ≈ (1/2) α² m_e c², which sets the binding energy for hydrogenic ions and influences multi-electron atoms via effective nuclear charge screening. For light elements like hydrogen and helium, relativistic fine-structure effects subtly affect chemical bonding; increasing α would weaken covalent bonds by enhancing spin-orbit coupling, potentially altering dissociation energies in H₂ by up to a few percent for α variations of order 1%. These influences highlight α's foundational role in ordering electromagnetic effects from atomic spectra to molecular stability in light systems.^[23]

Significance in Quantum Electrodynamics

In quantum electrodynamics (QED), the fine-structure constant α acts as the fundamental coupling parameter that governs the strength of electromagnetic interactions between charged particles, such as electrons and photons. Developed through the work of Richard Feynman, Julian Schwinger, Sin-Itiro Tomonaga, and Freeman Dyson in the late 1940s, perturbative QED relies on an expansion series in powers of α (or more precisely α/π for loop contributions), which converges effectively due to α ≈ 1/137 being much less than 1 at low energies. This expansion is visualized through Feynman diagrams, where each vertex representing a photon emission or absorption is scaled by the elementary charge e, related to α by e = √(4πα) in natural units; higher-order diagrams incorporate additional loops and vertices, allowing precise calculations of scattering amplitudes and decay rates. A key success of this perturbative framework is the prediction of the electron's anomalous magnetic moment, a_e = (g_e - 2)/2, where g_e is the electron's gyromagnetic ratio. In the Dirac theory, g_e = 2 exactly, but QED corrections yield a_e = α/(2π) at leading order, as first computed by Schwinger using proper-time methods in the interaction picture. Higher-order terms include contributions like α²/(π²) and beyond, with the full QED prediction now known to over five loops, matching experimental measurements to 10 decimal places and serving as one of the most stringent tests of the theory; for instance, the tenth-order term contributes only about 10^{-13} to a_e. Despite its successes at accessible energies, QED exhibits nontrivial behavior at high scales due to the positive sign of its beta function, leading to a Landau pole where α diverges. This theoretical singularity occurs around 10^{37} GeV in the context of the full Standard Model, far beyond the electroweak scale, signaling that pure QED lacks asymptotic freedom and requires embedding in a larger theory for UV completion; the running of α from vacuum polarization effects increases its value logarithmically with energy. At the electroweak scale (around the Z boson mass of 91 GeV), α(M_Z) ≈ 1/128, a value crucial for unification discussions, as it approaches the weak and strong couplings in grand unified theories, though discrepancies persist without new physics.^[24]^[25]

Dependencies and Variations

Variation with Energy Scale

In quantum electrodynamics (QED), the fine-structure constant \alpha exhibits a scale dependence known as "running," arising from vacuum polarization effects where virtual fermion-antiparticle pairs screen the bare electromagnetic charge. This behavior is captured by the renormalization group equation (RGE) at one-loop order:

\frac{d\alpha}{d \ln \mu} = \frac{\alpha^2}{3\pi} \sum_f Q_f^2 n_c,

where \mu is the renormalization scale, the sum runs over active fermion flavors f with electric charge Q_f (in units of the elementary charge e), and n_c = 1 (3) for leptons (quarks) accounting for color degrees of freedom.^[26] The leading-logarithmic solution to this equation, valid away from mass thresholds, takes the approximate form

\alpha(\mu) = \frac{\alpha(0)}{1 - \frac{\alpha(0)}{3\pi} \left( \sum_f Q_f^2 n_c \right) \ln\left( \frac{\mu^2}{m^2} \right)},

with \alpha(0) \approx 1/137.036 the low-energy value (at \mu \sim m_e, the electron mass) and m a reference scale below the lightest threshold. The positive beta function coefficient in QED leads to an increase in \alpha(\mu) with \mu, reflecting reduced screening at shorter distances. At the electroweak scale \mu = M_Z \approx 91 GeV, \alpha(M_Z) \approx 1/128.9.^[27]^[25] Below M_Z, lepton loop contributions dominate the running, with the three charged lepton generations (electron, muon, tau; each Q_f = 1, n_c = 1) providing \sum Q_f^2 n_c = 3, augmented by lighter quark effects through hadronic vacuum polarization. Above M_Z, heavier particles enter, including the top quark (Q_f = 2/3, n_c = 3) whose large mass enhances its impact near the threshold, and electroweak bosons (W, Z). At even higher scales, quantum chromodynamics (QCD) influences the evolution via gluon-mediated corrections to quark loops, slowing the hadronic contribution's growth. These multi-loop and threshold effects are incorporated in higher-order calculations for precision.^[26]^[25] The predicted running has been experimentally verified through e^+ e^- scattering cross-sections at the Large Electron-Positron Collider (LEP), where the effective \alpha at the Z-pole resonance was extracted from the hadronic and leptonic event rates, yielding \alpha(M_Z)^{-1} = 128.89 \pm 0.07 in agreement with theory. Complementary confirmation arises from global electroweak precision fits to LEP/SLD data, which constrain \alpha(M_Z) to better than 0.1% accuracy and test QED consistency within the Standard Model. Lower-energy running, including hadronic effects, has been measured in processes like e^+ e^- \to \mu^+ \mu^- \gamma by experiments such as KLOE and BABAR.^[28]^[25]

Temporal and Spatial Variations

The fine-structure constant has been scrutinized for possible temporal variations over cosmological timescales using quasar absorption spectra, which probe distant intervening gas clouds. Early analyses by Webb et al. in 1999 suggested a potential change of Δα/α ≈ (-0.72 ± 0.18) × 10^{-5} at redshifts z ≈ 0.5–1.6, corresponding to roughly 10 billion years ago. Subsequent studies expanded the dataset, with claims of a dipole-like pattern implying variations up to ~10^{-5} over similar epochs. However, comprehensive reanalyses, including a 2024 study incorporating convergence properties of measurements from multiple quasar systems, indicate no statistically significant deviation, with Δα/α consistent with zero at the 10^{-6} level or better.^[29]^[30] Tighter constraints on past variations come from natural nuclear reactors and primordial nucleosynthesis. The Oklo natural fission reactor in Gabon, operating approximately 2 billion years ago, provides isotopic ratios sensitive to α; analyses yield |Δα/α| < 5.8 × 10^{-8} over that interval. Big Bang nucleosynthesis (BBN) models, calibrated against observed primordial abundances of light elements like deuterium and helium, impose even stricter limits from the early universe at z ≈ 10^9; recent evaluations constrain |Δα/α| < 10^{-3} relative to the present value, though some specialized BBN studies suggest bounds as tight as <10^{-10} when incorporating correlated variations in other constants.^[31]^[32] At present epochs, laboratory tests using atomic clocks and lunar laser ranging set the most stringent limits on the rate of temporal change. Comparisons of optical atomic clocks, such as those based on ytterbium and dysprosium transitions, over intervals of years detect no variation exceeding |dα/α/dt| < 10^{-18} yr^{-1}. Lunar laser ranging experiments, monitoring Earth-Moon dynamics, complement these by constraining coupled variations in fundamental constants, yielding no detectable drift beyond |dα/α/dt| < 10^{-17} yr^{-1} up to 2025. These results affirm the constancy of α on human timescales.^[33]^[34] Spatial variations in α have been proposed based on directional dependencies in quasar data. Webb et al. in 2010 reported evidence for a dipole anisotropy, with Δα/α ≈ 10^{-6} aligned toward the southern sky, using Keck and VLT observations of ~300 absorption systems. This claim suggested possible spatial inhomogeneity at the 4σ level. However, independent analyses, including 2023–2024 studies leveraging large galaxy samples and DESI survey data, refute the dipole, finding no confirmed anisotropy and constraining spatial fluctuations to <10^{-6} across the observable universe.^[35]^[36]^[37]

Historical Development

Discovery and Early Interpretations

The fine-structure constant, denoted as \alpha, was first introduced by Arnold Sommerfeld in 1916 as part of his extension of the Bohr atomic model within the framework of old quantum theory.^[38] Sommerfeld sought to explain the observed fine splitting of spectral lines, such as the doublet in the hydrogen H\alpha line, which could not be accounted for by Niels Bohr's original 1913 model. By incorporating relativistic corrections to the electron's orbital motion, Sommerfeld derived that the splitting arises from the ratio of the electron's velocity v in the innermost Bohr orbit to the speed of light c, yielding v/c \approx \alpha \approx 1/137.^[39] This dimensionless parameter encapsulated the strength of the electromagnetic interaction relative to relativistic effects, marking \alpha as a fundamental constant in early quantum mechanics.^[38] In 1928, Paul Dirac advanced this understanding through his relativistic wave equation for the electron, which precisely predicted the fine structure of hydrogen spectral lines without ad hoc assumptions.^[40] Dirac's equation incorporated both quantum mechanics and special relativity, naturally yielding the fine-structure splitting as a function of \alpha, where the constant appeared as the coupling parameter governing electromagnetic interactions.^[1] This formulation elevated \alpha from an empirical correction in the Bohr-Sommerfeld model to a core element of relativistic quantum theory, confirming Sommerfeld's approximate value while providing an exact theoretical basis.^[40] Prior to the 1940s, the fine-structure constant was primarily interpreted in the context of the Bohr-Sommerfeld atomic model as the characteristic ratio of the electron's orbital velocity to the speed of light in the ground state.^[38] This view framed \alpha as a measure of how closely atomic electrons approach relativistic speeds, influencing the quantization of angular momentum and energy levels in hydrogen-like atoms.^[39] Early calculations, such as those for the hydrogen fine structure, relied on this velocity ratio to match experimental spectral data, underscoring \alpha's role in bridging classical orbits with quantum discreteness.^[38] The numerical value of \alpha \approx 1/137 also sparked early numerological interest among physicists. In the 1930s, Arthur Eddington speculated that the inverse fine-structure constant was exactly 136, deriving this from his fundamental theory of the world, which emphasized epistemological and aesthetic principles over empirical measurement.^[41] Eddington's arguments, detailed in works like his 1931 paper, posited that \alpha^{-1} must be an integer tied to the structure of physical laws, reflecting a broader fascination with the constant's seemingly arbitrary yet precise magnitude.^[42] These interpretations, while influential, remained speculative and were later refined by more rigorous quantum developments.^[41]

Evolution Through Quantum Theory

In the 1940s, the fine-structure constant α began to play a central role in quantum electrodynamics (QED) through calculations addressing discrepancies in atomic spectra. Hans Bethe calculated the Lamb shift in hydrogen in 1947, attributing the energy level splitting between the 2S_{1/2} and 2P_{1/2} states to radiative corrections involving virtual electron-positron pairs, with the shift scaling as α (up to logarithms) times the Dirac fine structure.^[43] This non-relativistic approximation incorporated α as the fundamental measure of electromagnetic coupling strength, resolving infinities via mass renormalization inspired by earlier work. Enrico Fermi contributed foundational QED techniques in the early 1940s, including self-energy evaluations that Bethe adapted for the Lamb shift computation during a train journey following the experimental announcement.^[44] The formalization of QED in the late 1940s elevated α to the status of the theory's primary expansion parameter. Sin-Itiro Tomonaga developed a covariant perturbation theory in 1946, enabling consistent handling of relativistic effects in electron-photon interactions. Julian Schwinger and Richard Feynman independently advanced this framework in 1948, introducing functional integrals and path-integral formulations, respectively, where scattering amplitudes expand in powers of α ≈ 1/137, quantifying loop corrections like vacuum polarization. Their work, unified by Freeman Dyson's equivalence proofs, demonstrated QED's predictive power for phenomena such as the anomalous magnetic moment, earning Tomonaga, Schwinger, and Feynman the 1965 Nobel Prize in Physics; α emerged as the dimensionless coupling dictating the theory's perturbative validity up to high energies.^[45] From the 1970s to the 2000s, efforts to embed α within broader unification schemes extended its theoretical significance in the Standard Model. Grand Unified Theories (GUTs), starting with the minimal SU(5) model proposed by Howard Georgi and Sheldon Glashow in 1974, aimed to unify the electromagnetic, weak, and strong couplings at a high-energy scale, but the minimal non-supersymmetric version predicted convergence around 10^{12}-10^{14} GeV with α_GUT ≈ 1/25, which was too low to evade proton decay limits.^[46] Supersymmetric extensions in the 1980s and 1990s raised the scale to around 10^{16} GeV, implying α evolves via renormalization group running to a unified value α_GUT ≈ 1/25 at that scale, though distinct from the Planck scale of 10^{19} GeV. Subsequent models like SO(10) refined these predictions, incorporating proton decay and neutrino masses, but discrepancies in low-energy coupling measurements—such as α_s at the Z boson mass—challenged minimal GUTs, prompting further supersymmetric adjustments that aligned the unification scale more closely with observations.^[46] These frameworks highlighted α's role in testing unification, with logarithmic running governed by β-functions involving particle content, though no exact derivation of its low-energy value emerged.

Theoretical Explanations

Anthropic Principle

The fine-structure constant, denoted as \alpha \approx 1/137, is often cited in fine-tuning arguments within the anthropic principle, which posits that the universe's physical parameters must permit the existence of observers to make such observations possible. Specifically, values of \alpha significantly larger than its observed magnitude would destabilize atomic structures essential for chemistry; for instance, if \alpha > 1/95, iron atoms become unstable, disrupting the formation of complex molecules necessary for life. Conversely, if \alpha < 1/205, stellar nucleosynthesis would favor nickel over iron as the endpoint of fusion processes, preventing the production of elements critical for stable stars and planetary systems. These narrow bounds highlight how \alpha's value enables the electromagnetic interactions required for stable atoms and molecular bonds, underscoring the apparent tuning for carbon-based life.^[47] John D. Barrow and Frank J. Tipler, in their seminal 1986 work, formalized the anthropic cosmological principle, applying it to constants like \alpha to argue that the universe's structure is constrained by the necessity of supporting intelligent life. They distinguish between the weak anthropic principle (observational selection effects) and the strong version (the universe must evolve observers), using \alpha's role in atomic stability to illustrate how deviations would preclude biological complexity, such as the dipole moments in water molecules vital for life's solvent properties. This framework posits that \alpha's specific value is not coincidental but required for the emergence of observers capable of measuring it.^[48] In multiverse scenarios, particularly the string theory landscape, \alpha can vary across different vacua, with our universe's value selected anthropically because it allows for life. The landscape encompasses approximately $10^{500} possible configurations of extra dimensions, where the vacuum expectation values of scalar fields determine coupling constants like \alpha, enabling regions hospitable to observers while others remain barren. This resolves fine-tuning by invoking a vast ensemble where life-bearing universes are statistically inevitable, though only those permitting complex chemistry and stellar evolution are observed. Critics of the anthropic approach to \alpha emphasize its limited testability, as predictions rely on unobservable multiverses, rendering it philosophically intriguing but empirically challenging; however, analogies to the cosmological constant—another finely tuned parameter with anthropic explanations in similar landscapes—bolster its plausibility by demonstrating consistent explanatory patterns across constants. Efforts to test it involve assessing whether life-permitting values occupy a significant fraction of the parameter space, but current models suggest \alpha's tuning remains a key example of selection bias in cosmic ensembles.

Numerological and Speculative Theories

In the early 20th century, Arthur Eddington proposed a combinatorial derivation for the fine-structure constant \alpha, initially aiming to establish its inverse as exactly 136 based on the number of degrees of freedom in fundamental particles and cosmological considerations.^[42] This approach, outlined in his 1931 work, relied on aesthetic and numerical principles rather than empirical derivation, predicting \alpha = 1/136 through relations involving the Eddington number and electron properties.^[49] However, subsequent measurements indicated a value closer to $1/137, prompting Eddington to adjust his combinatorial scheme ad hoc to fit the new data, highlighting the speculative nature of the method.^[38] Religious and esoteric interpretations have also linked the approximate value of $1/137 to numerological significance, particularly in Kabbalistic traditions where the Hebrew word for "Kabbalah" (קַבָּלָה) yields a gematria value of 137, suggesting a mystical connection to the constant's role in governing electromagnetic interactions.^[50] Proponents argue this alignment reflects a deeper, non-physical harmony between ancient mysticism and modern physics, with 137 symbolizing reception or parallel structures in creation.^[51] Such views, while intriguing, remain outside scientific discourse and lack testable predictions. Contemporary speculative theories continue this numerological tradition, proposing derivations of \alpha \approx 1/137 through geometric or mathematical constructs. For instance, models incorporating the golden ratio \phi \approx 1.618 relate it to \alpha via scaling laws and fractal geometries. Similarly, recent frameworks explore ratios involving \pi and the Euler-Mascheroni constant \gamma \approx 0.577 to resolve \alpha within extended Standard Model contexts, though these remain unverified. Classical electron models, reviving pre-quantum ideas, derive \alpha \approx 1/137 from Coulomb-to-gravitational force ratios or electron radius considerations, linking the Pythagorean prime 137 to primordial charge dynamics.^[52] These numerological and speculative approaches face significant critiques for their lack of predictive power and reliance on post-hoc adjustments to match measurements, often prioritizing pattern recognition over falsifiable mechanisms.^[53] Unlike mainstream theories, they fail to integrate with quantum electrodynamics or yield novel experimental tests, rendering them philosophically appealing but scientifically marginal.^[54]

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Hyperfine Structure - Richard Fitzpatrick
$$ \alpha=1/137$ the fine structure constant. Note that the hyperfine energy-shift is much smaller, by a factor $ m_e/m_p$ , than a typical fine structure ...
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The discovery of asymptotic freedom and the emergence of QCD
Landau and collaborators, in the late 1950s, studied the high-energy behavior of QED. They explored the relation between the physical electric charge and ...
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[PDF] 10. Electroweak Model and Constraints on New Physics
May 31, 2024 · The electroweak model (SM) is based on SU(2)xU(1) gauge group, with gauge bosons Wµ and Bµ, and a Higgs doublet for mass generation.
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[PDF] Running electromagnetic coupling constant: low energy ... - arXiv
Nov 9, 2000 · . The total finite renormalization between the fine structure constant and the MS- scheme EM coupling at Mτ is given by. ∆(4)(M2 τ )=∆lept ...
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The running fine structure constant alpha(E) via the Adler function
Jul 26, 2008 · We present an up-to-date analysis for a precise determination of the effective fine structure constant and discuss the prospects for future improvements.Missing: QED | Show results with:QED
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Measurement of the running of the fine-structure constant
Mar 9, 2000 · This article interprets measurements of Bhabha scattering by the L3 experiment at LEP in terms of the evolution of α(Q 2 ), using two complementary ...
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A Search for Time Variation of the Fine Structure Constant - arXiv
Dec 16, 1998 · A method offering an order of magnitude sensitivity gain is described for using quasar spectra to investigate possible time or space variation in the fine ...
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Convergence properties of fine structure constant measurements ...
Feb 19, 2024 · Our recent work has focused on measurements of the fine structure constant α in quasar absorption systems, parametrized using Δα/α = (αz − α0)/α ...ABSTRACT · INTRODUCTION · ASTRONOMICAL, ATOMIC... · SUMMARY AND...
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Natural nuclear reactor at Oklo and variation of fundamental constants
Dec 14, 2006 · This allows us to obtain the most accurate limits on the change of the fine structure constant in the past. The paper is organized as follows.
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Constraints on the variation of the fine structure constant from big ...
Jul 13, 1999 · We put bounds on the variation of the value of the fine structure constant $\ensuremath{\alpha}$, at the time of big bang nucleosynthesis.
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A limit on variations in the fine-structure constant from spectra of ...
Nov 10, 2022 · The fine structure constant α sets the strength of the electromagnetic force. The Standard Model of particle physics provides no explanation ...
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New Limits on Variation of the Fine-Structure Constant Using Atomic ...
Aug 6, 2013 · We report on the spectroscopy of radio-frequency transitions between nearly degenerate, opposite-parity excited states in atomic dysprosium (Dy).
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Indications of a spatial variation of the fine structure constant - arXiv
Aug 23, 2010 · View a PDF of the paper titled Indications of a spatial variation of the fine structure constant, by J. K. Webb and 5 other authors. View PDF.Missing: refuted 2023
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Constraints on the Spacetime Variation of the Fine-structure ...
2023; Webb et al. ... Our large galaxy sample provides a great advantage that allows us to measure the spatial variation of the fine-structure constant.Missing: refuted | Show results with:refuted
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Constraints on the spacetime variation of the fine-structure constant ...
We present strong constraints on the spacetime variation of the fine-structure constant \alpha using the Dark Energy Spectroscopic Instrument (DESI).
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[PDF] The Fine Structure Constant - Indian Academy of Sciences
Although it was Arnold Sommerfeld who formally intro- duced the fine structure constant in 1916 (as discussed later in this article), its history can be traced ...
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[PDF] Sommerfeld fine structure constant α and its physical interpretation
The historical example is the demonstration of “electromag- netic induction” by Michael Faraday himself before a distinguished gathering of members of the ...
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The quantum theory of the electron - Journals
It appears that the simplest Hamiltonian for a point-charge electron satisfying the requirements of both relativity and the general transformation theory leads ...
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Eddington's Theory of the Constants of Nature - jstor
that the fine-structure constant e2/hc must be the reciprocal of a whole number, which was determined in a second paper (Feb. 1930) to be 137. At the same.Missing: speculations | Show results with:speculations
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[PDF] On Arthur Eddington's Theory of Everything - arXiv
Pauli referred specifically to Eddington's identification of the fine-structure constant α with the number 1/136. A main reason for the generally unsympathetic ...
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The Electromagnetic Shift of Energy Levels | Phys. Rev.
The Electromagnetic Shift of Energy Levels, HA Bethe Cornell University, Ithaca, New York, PDF Share, Phys. Rev. 72, 339 – Published 15 August, 1947.
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[PDF] Hans Bethe, Quantum Mechanics, and the Lamb Shift
An elementary derivation of the Lamb Shift, as originally given by Hans Bethe, is attempted, with a short historical background on the evolu-.
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The Radiation Theories of Tomonaga, Schwinger, and Feynman
A unified development of the subject of quantum electrodynamics is outlined, embodying the main features both of the Tomonaga-Schwinger and of the Feynman ...Missing: Nobel fine structure constant coupling
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[PDF] 93. Grand Unified Theories - Particle Data Group
Aug 11, 2022 · Since the. GUT scale is close to the Planck scale, higher-dimension operators involving the GUT-breaking. Higgs may modify the predictions ...Missing: 1970s | Show results with:1970s
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The Anthropic Cosmological Principle - John D. Barrow, Frank J. Tipler
Known as the Anthropic Cosmological Principle, it holds that the fundamental structure of the Universe is determined by the existence of intelligent observers: ...
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[PDF] Physical Mathematics and the Fine-Structure Constant - PhilArchive
Jul 11, 2018 · Arthur Eddington's work leads to a new calculation of the inverse fine-structure constant giving the same approximate value as ancient.
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Mysticism and the Fine Structure Constant
Sep 15, 2020 · The mysticism relating to the fine structure constant, including the surprising connection between the number 137 and Kabbalah by means of ...
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(PDF) Mysticism and the Fine Structure Constant - ResearchGate
Sep 15, 2020 · Mysticism and the Fine Structure Constant 489. Eddington, A. · S. (1931). On the value of the cosmical constant. Proceedings of the ; Royal ...
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[PDF] Golden Ratio Geometry and the Fine-Structure Constant - HAL
Oct 31, 2019 · Atomic Structure and Spectral Lines, New York, NY: Dutton, 1934. [3] Sherbon, M.A. “Fine-structure Constant from Sommerfeld to Feynman,” Journal ...
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Insights from the π/γ Ratio and Electron Dynamics[v1]
Dec 14, 2024 · This study explores a novel approach to understanding the fine-structure constant, α, by examining its connection to the anomalous magnetic ...<|control11|><|separator|>
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[PDF] The links of Pythagorean prime 137 to the fine structure constant ...
Sep 3, 2023 · We have provided possible links between 137 to the masses of the quarks, proton, W and Z bosons, Higgs boson, the Planck length, and the Coulomb ...<|separator|>
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Atiyah and the Fine-Structure Constant - Sean Carroll
Sep 25, 2018 · In the electroweak theory, we have two coupling constants, g and g' (for “weak isospin” and “weak hypercharge,” if you must know). There is also ...
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On the vital difference between number theory and numerology in ...
There has been much regrettable unintended or even intended confusion between the use of numerology and number theory in physics which has been the subject of ...Missing: critiques | Show results with:critiques