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One-way speed of light

The one-way speed of light is the speed at which light travels from a source to a detector in a single direction, distinct from the round-trip speed measured over a closed path, and in special relativity, it is conventionally defined as the constant value c (approximately 299,792 km/s) through the Einstein synchronization procedure for clocks.^[1] This convention assumes isotropy, meaning the speed is the same in all directions, although the one-way speed cannot be measured independently without adopting such a synchronization method, as any measurement relies on the relative timing of distant clocks.^[2] In Albert Einstein's 1905 formulation of special relativity, the invariance of the speed of light was initially established for round-trip measurements, with the one-way speed following as a definitional choice to ensure consistency across inertial frames; this choice eliminates absolute simultaneity and underpins the relativity of simultaneity.^[3] The two-way speed has been experimentally verified to high precision through tests like the Michelson-Morley experiment and modern interferometry, confirming it equals c regardless of the observer's motion, but attempts to directly probe the one-way speed, such as using fiber-optic delays or phase-conjugate interferometers, inevitably circularly depend on the synchronization convention employed.^[2]^[3] The conventionality of the one-way speed has profound implications for theoretical physics, allowing alternative synchronizations where the speed could appear anisotropic (e.g., faster in one direction and slower in the opposite, while preserving the round-trip average at c), yet such variations do not affect observable physics in special relativity as long as closed-path speeds remain universal.^[1] This has led to explorations in cosmology, such as in the Milne universe model, where anisotropic one-way speeds might alter perceptions of cosmic expansion or the cosmic microwave background, but empirical evidence supports the isotropic convention.^[1] Ongoing experiments, including those leveraging the Sagnac effect on rotating platforms like Earth, continue to test for deviations that could indicate preferred frames or challenge the standard assumption, though none have falsified special relativity to date.^[3]

Fundamentals of light speed measurement

Two-way speed of light

The two-way speed of light is determined by measuring the time for light to travel a known distance forth and back in vacuum, yielding a value that is isotropic—independent of direction—and invariant across inertial frames. This measurement, central to special relativity, confirms that light propagates at a constant speed c without requiring a preferred reference frame like the luminiferous ether.^[4] In 1887, Albert A. Michelson and Edward W. Morley conducted a seminal experiment using an interferometer to test for directional variations in the two-way speed of light, expecting differences due to Earth's motion through the ether. Their null result, showing no detectable anisotropy to within 1/100th of the expected effect, provided the first strong evidence for the isotropy of the two-way speed.^[5] The two-way speed is formally defined as c = \frac{2L}{\Delta t}, where L is the path length and \Delta t is the round-trip travel time; in vacuum, this yields the exact value c = 299{,}792{,}458 m/s, fixed by international convention since 1983 to define the meter.^[6] Modern experiments have refined these measurements to extraordinary precision, confirming the two-way speed's isotropy and value. For instance, interferometric techniques, building on Michelson-Morley designs, use laser sources to detect phase shifts over perpendicular paths, while microwave cavity resonators measure resonant frequencies to compute c from wavelength and geometry. A 2003 experiment with cryogenic optical resonators achieved isotropy tests at the $10^{-15} level, aligning with the defined value of c.^[4] Similarly, 1950 measurements using cavity resonators by Louis Essen yielded c = 299{,}792.5 \pm 1 km/s, a key step toward the modern definition. This empirically verified isotropic two-way speed underpins special relativity's postulate of light's constancy, eliminating the need for an absolute reference frame and enabling consistent physics across observers.

Definition and challenges of one-way speed

The one-way speed of light is defined as the speed at which a light signal travels from a source at point A to a detector at point B, given by the distance AB divided by the difference in arrival and departure times measured by clocks at those points.^[2] This contrasts with the empirically verified two-way speed, which averages the transit over a round trip and is isotropic at approximately 299,792 km/s in vacuum.^[7] Conceptually, the one-way speed could be anisotropic—faster in one direction than the opposite—but it remains constrained by the observed isotropy of the two-way speed, allowing variability only within limits that preserve round-trip consistency.^[8] The primary challenge in measuring the one-way speed arises from the necessity of synchronizing clocks at spatially separated points A and B, a process that inherently relies on an assumed light propagation convention.^[7] Without prior synchronization, the departure time at A and arrival time at B cannot be compared meaningfully, creating a circular dependency: any synchronization method, such as using light signals, presupposes the very one-way speed it seeks to measure. This issue renders direct, convention-independent measurement impossible, as the two-way speed provides the only empirical constraint.^[7] Mathematically, if c_+ denotes the forward one-way speed and c_- the backward one-way speed over distance L, the round-trip time is L/c_+ + L/c_-, yielding the two-way speed c as the harmonic mean:

c = \frac{2 c_+ c_-}{c_+ + c_-}.

This relation permits c_+ and c_- to differ arbitrarily, provided their harmonic mean equals the measured c, without affecting observable two-way results.^[8] In special relativity, the one-way speed thus emerges as a convention rather than an observable, with the isotropy assumption (setting c_+ = c_- = c) chosen for simplicity but not empirically mandated.^[9] Philosophically, this dependency underscores that the one-way speed is not a physical invariant but a coordinate choice, equivalent across frames under relativity's postulates yet gauge-dependent in synchronization.^[7] Early 20th-century debates, initiated by Einstein's 1905 analysis, rejected absolute simultaneity—in which events at distant points share a universal "now" independent of observers—in favor of relative simultaneity, where defining co-occurrence requires a light-speed convention and varies by frame.^[7] This shift, building on pre-relativistic views like Poincaré's, resolved paradoxes in ether theories but highlighted the conventionality inherent to relativity.^[7]

Synchronization conventions in relativity

Einstein synchronization convention

The Einstein synchronization convention provides the operational definition for synchronizing clocks separated by a distance L in an inertial reference frame, relying on light signals to establish simultaneity. In this method, a light pulse is emitted from clock A at position x = 0 at local time t_A, propagates to clock B at x = L, reflects immediately, and returns to A at local time t'_A. The round-trip time is measured as t'_A - t_A = 2L/c, where c is the speed of light in vacuum, yielding the one-way propagation time L/c for each leg under the assumption of symmetry.^[10] This symmetry implies that the clocks are synchronized when the reflection time at B satisfies t_B = (t_A + t'_A)/2, ensuring the forward and return journeys take equal durations. From this, the arrival time for a forward signal is defined as

t_B = t_A + \frac{L}{c},

derived directly from the measured round-trip duration without independent verification of the one-way speed.^[10] The convention rests on the postulate that light propagates at constant speed c isotropically in all directions within the inertial frame, free from contradictions when extended to multiple clocks. This isotropy introduces the relativity of simultaneity: events simultaneous in one frame may not be in another moving relative to it, as the synchronization offsets depend on relative velocity.^[10] Originating in Albert Einstein's seminal 1905 paper "On the Electrodynamics of Moving Bodies," the convention explicitly sets the one-way speed of light to c as a definitional choice to eliminate asymmetries in classical electrodynamics for moving observers. Einstein states that the propagation time from A to B is \frac{AB}{c}, where c is invariant and determined by the round-trip measurement, assuming no preferred direction for light's velocity.^[10] This approach offers key advantages, including full compatibility with Maxwell's equations for electromagnetic phenomena in stationary and moving frames, thereby resolving prior inconsistencies without altering the equations themselves. It also maintains the causal structure of special relativity, where light cones define allowable event orderings and prevent superluminal signaling.^[10]

Slow clock-transport synchronization

Slow clock-transport synchronization provides an alternative procedure to light-based methods for establishing simultaneity between distant clocks in special relativity, relying on the physical movement of a clock at low velocities. The process begins with two identical clocks synchronized at location A. One clock is then transported to location B, a distance L away, at a constant low speed v << c, where c is the speed of light. During transport, the moving clock experiences time dilation, running slower than a stationary clock by a factor of approximately 1 - \frac{1}{2} \left( \frac{v}{c} \right)^2 due to special relativistic effects. Upon arrival at B, the reading on the transported clock lags behind the expected coordinate time by \Delta t \approx \frac{L v}{2 c^2}, the second-order correction derived from integrating the time dilation over the travel duration L/v. To synchronize, this lag is added to the transported clock's reading to align it with a local clock at B, ensuring consistent time assignment across the frame.^[7] In the limit as the transport velocity v approaches zero, the time dilation correction \Delta t vanishes, and the synchronization obtained via slow clock transport precisely matches the Einstein synchronization convention, thereby empirically supporting the isotropy of light speed in inertial frames. This convergence demonstrates that mechanical transport at infinitesimal speeds preserves the standard notion of simultaneity without introducing directional biases.^[11] Theoretically, slow clock-transport synchronization is fully equivalent to the Einstein convention within the flat spacetime of special relativity, as both procedures yield identical transformations for clock readings and confirm the Lorentz invariance of physical laws. However, in frameworks positing absolute motion or a preferred reference frame, discrepancies between the two methods could emerge, serving as a potential test for such hypotheses. This equivalence holds because the second-order relativistic corrections during transport align with the assumptions of constant light speed in all directions.^[12] Historically, slow clock transport gained prominence in the late 1960s and 1970s as a proposed technique to investigate the one-way speed of light independently of optical signals, highlighted in philosophical and physical discussions on simultaneity. Key contributions include analyses showing its operational viability under relativistic postulates, positioning it as a complementary tool to light-signal synchronization. No empirical differences have been observed between synchronizations achieved via slow clock transport and the Einstein method in experiments to date, underscoring the consistency of special relativity's predictions.^[7]

Non-standard synchronization approaches

Non-standard synchronization approaches in special relativity permit directional variations in the measured one-way speed of light while ensuring the two-way speed remains isotropic at c and Lorentz invariance is preserved. These methods introduce a conventional parameter that adjusts clock readings across spatial separations, resulting in apparent anisotropy of the one-way speed without modifying the underlying physical laws or observable round-trip measurements.^[13] A prominent example is anisotropic synchrony, where clocks separated by distance L in a given direction are offset by \epsilon L / c, with the parameter \epsilon satisfying |\epsilon| < 1 to ensure positive one-way speeds. This offset leads to differing one-way speeds in opposite directions, such as c_+ = c / (1 - \epsilon) and c_- = c / (1 + \epsilon), but the harmonic mean for the round trip always yields c. In vector form, the one-way speed in direction \mathbf{n} (a unit vector) is given by

\frac{c}{1 - \mathbf{\kappa} \cdot \mathbf{n}},

where \mathbf{\kappa} is a constant vector parameter with |\mathbf{\kappa}| < 1.^[13] These conventions modify coordinate time assignments but leave proper time intervals, particle dynamics, and local experimental outcomes unchanged, as the anisotropy is purely a matter of synchronization choice rather than a physical effect. Such approaches were first systematically explored by Edwards in the context of anisotropic light propagation in 1963 and later incorporated into broader test theories of special relativity, such as the Mansouri-Sexl framework in 1977, which parameterizes deviations from standard assumptions. Experimentally, non-standard synchronizations are indistinguishable from the Einstein convention, as no local test can uniquely determine the one-way speed without presupposing a synchronization procedure, rendering the parameter \mathbf{\kappa} (or equivalent) unmeasurable in isolation.

Theoretical implications and frameworks

Role in inertial frames and special relativity dynamics

In special relativity, the choice of clock synchronization in an inertial frame defines the planes of simultaneity, which in turn determines the apparent one-way speed of light along different directions. Under the standard Einstein synchronization convention, clocks are synchronized such that light signals emitted from a point travel equal distances in equal times in opposite directions, yielding an isotropic one-way speed equal to the two-way speed c. However, alternative synchronization procedures, such as those parameterized by a factor \epsilon (where $0 < \epsilon < 1), rescale the time coordinate anisotropically, making the one-way speed appear direction-dependent while preserving the round-trip speed at c. This rescaling affects the coordinate description but leaves the underlying spacetime structure unchanged, as different conventions merely represent gauge choices within the theory.^[14] The dynamics of physical systems remain invariant under such resynchronizations in inertial frames. Particle trajectories, electromagnetic field propagations, and other relativistic phenomena depend only on the invariant spacetime interval, ensuring that measurable predictions—such as time dilation, length contraction, and aberration—are independent of the synchronization choice. For instance, the Lorentz metric, which governs causality and the geometry of spacetime, is preserved: the line element ds^2 = -c^2 dt^2 + dx^2 + dy^2 + dz^2 holds in any valid coordinate system, even if the time differential dt is anisotropically adjusted. Apparent variations in the one-way speed thus constitute a coordinate artifact rather than a physical anisotropy, with no preferred inertial frame emerging from the formalism.^[14] This invariance extends to ensuring fundamental principles like causality, as no synchronization convention allows faster-than-light information transfer, which would violate the light cone structure defined by the metric. In non-inertial frames, however, synchronization conventions lose their straightforward applicability, as acceleration introduces path-dependent effects that require the curved spacetime framework of general relativity to maintain consistency. Within special relativity's domain of inertial motion, the conventional nature of one-way speed underscores the theory's emphasis on relational descriptions over absolute simultaneity.^[14]

Theories equivalent to special relativity with anisotropic speeds

The Lorentz ether theory, formulated by Hendrik Lorentz in 1904 and building on George FitzGerald's earlier contraction hypothesis from 1889, assumes an absolute rest frame defined by a stationary luminiferous ether in which the speed of light is isotropic and equal to c. In frames moving relative to this ether with velocity v, the one-way speed of light becomes anisotropic due to the relative motion, or "ether wind," with the speed in the direction against the motion approximately c(1 - v/c) to first order, while length contraction along the direction of motion by the factor \sqrt{1 - (v/c)^2} and time dilation by the same factor conspire to conceal this anisotropy.^[15] This theory achieves full empirical equivalence to special relativity through a coordinated set of effects, including the aforementioned contraction and dilation, which ensure that all observable predictions—such as the two-way speed of light remaining c and the null results of ether-drift experiments like Michelson-Morley—match exactly, rendering the ether undetectable by any physical measurement.^[12] In the moving frame, the effective one-way speed, when transformed via the Lorentz transformations, appears isotropic at c.^[12] Post-Einstein revivals of the theory, notably by Franco Selleri in the late 20th century, emphasized its interpretive advantages, such as restoring absolute simultaneity while preserving all experimental agreements with relativity, without invoking the relativity of simultaneity.^[16] Generalizations extend this framework, such as using de Sitter's 1913 proposal for synchronization via slow clock transport, which in the ether frame approximates absolute time and reveals the underlying anisotropy, though it remains empirically indistinguishable from standard special relativity under operational tests.^[12] Overall, these theories highlight that the one-way speed of light's isotropy is a matter of convention, with anisotropic formulations yielding identical physics to special relativity.^[17]

Theories not equivalent to special relativity

The Robertson-Mansouri-Sexl (RMS) framework, developed in the 1970s as a phenomenological test theory to probe violations of Lorentz invariance, parameterizes possible deviations from special relativity through synchronization parameters α, β, and δ, which describe transformations between coordinate systems in the presence of a preferred frame.^[11] In this model, α relates to the anisotropy of clock synchronization, β to the velocity dependence of time dilation, and δ to length contraction effects; special relativity corresponds to the values α = −1/2, β = 1/2, and δ = 0.^[18] Unlike interpretations equivalent to special relativity, such as the Lorentz ether theory, the RMS framework allows for falsifiable predictions where nonzero parameter deviations lead to observable anisotropies in light propagation.^[18] Within the RMS framework, the one-way speed of light exhibits directional dependence relative to the velocity \vec{v} of the laboratory frame with respect to the preferred frame, approximated to first order as

c(\theta) = c_0 \left[1 + \left(\alpha + \frac{1}{2}\right) \frac{v}{c} \cos \theta \right],

where c_0 is the isotropic speed in the preferred frame and \theta is the angle between the light propagation direction and \vec{v}.^[18] This anisotropy arises from nonstandard synchronization and has been tested against null results from experiments like the Michelson-Morley test, which constrain the parameters by requiring consistency with the observed two-way isotropy of light speed. Specifically, the framework predicts that deviations in α and β could manifest as variations in the one-way speed, potentially violating the reciprocity of light propagation in inertial frames.^[19] Another influential model is the Standard-Model Extension (SME), proposed in the late 1990s as a general effective field theory incorporating all possible Lorentz- and CPT-violating operators consistent with standard model symmetries.^[20] In the photon sector of the SME, CPT-odd terms—such as those parameterized by the coefficients \tilde{\kappa}_{o+}—introduce directional variations in the speed of light by modifying Maxwell's equations, leading to anisotropic propagation without birefringence.^[18] These terms predict potential deviations from special relativity in processes involving light, including altered dispersion relations that could affect high-energy photon arrival times or interferometry outcomes.^[20] Theories like RMS and SME predict testable violations, such as discrepancies in Kennedy-Thorndike-type setups where arm lengths differ, or couplings to gravitational fields that induce frame-dependent effects on light speed.^[18] Historical development of these 1970s test theories, building on earlier work by Robertson, aimed to systematically explore Lorentz invariance breakdowns motivated by ether-drift hypotheses and quantum gravity considerations. Current experimental bounds on RMS parameters are stringent, with |α + 1/2| ≲ 10^{-15} from resonator-based tests (as of 2016)^[21], though nonzero values remain possible and drive ongoing searches for subtle anisotropies. Similarly, SME coefficients for light speed variations, such as \tilde{\kappa}_{o+}, are constrained to levels below 10^{-17} in certain directions (as of ~2020), with astrophysical tests tightening some bounds to ~10^{-20} (as of 2024)^[22], underscoring the tight but incomplete verification of Lorentz invariance.^[20]

Experimental approaches and results

Experiments claiming direct one-way measurement

Attempts to directly measure the one-way speed of light using light signals have historically faced fundamental challenges, primarily because such measurements inherently rely on clock synchronization procedures that presuppose the very isotropy or value of the speed being tested, rendering the approach circular.^[23] This dependency on a synchronization convention means no experiment can independently verify the one-way speed without assuming it in advance.^[24] One prominent example is the 2009 experiment by Greaves, Rodriguez, and Ruiz-Camacho, which used a time-of-flight technique over a 23 km optical fiber loop to compare transit times for light traveling in opposite directions.^[25] The setup involved sending laser pulses from a common source, splitting them into the loop, and detecting arrival times with synchronized clocks, reporting results consistent with the isotropic speed of light c to within 0.4%.^[25] However, critics noted that the synchronization of the endpoint clocks implicitly assumed the round-trip speed of light, effectively measuring only the two-way propagation rather than a true one-way value, thus failing to escape the conventionality issue.^[23] Early 20th-century efforts, such as those exploring light propagation in presumed ether frames through interference or mechanical methods, similarly claimed direct one-way assessments but were invalidated by the advent of special relativity, which demonstrated their reliance on outdated absolute simultaneity assumptions.^[26] These attempts, often motivated by aether theories, could not disentangle one-way effects from synchronization artifacts. In analysis, no purported direct measurement has evaded the synchronization convention; instead, their apparent confirmations of isotropy merely reaffirm the consistency of the Einstein synchronization choice with observed round-trip results, without providing new information on the one-way speed.^[23] The 2009 fiber-optic study, despite its precision, exemplifies this limitation, as the loop configuration and clock assumptions prevent a genuinely independent one-way determination.^[25]

Unidirectional light path experiments

Unidirectional light path experiments seek to determine the one-way speed of light by transmitting signals along a single path and timing the propagation using clocks synchronized through methods independent of light signals, such as slow clock transport or satellite-based systems like GPS. Slow clock transport synchronization involves physically moving a clock between locations at non-relativistic speeds, minimizing desynchronization effects to infer light travel times without assuming the Einstein convention. These experiments compare the signal's departure time at the source clock with its arrival time at the receiver clock, yielding the one-way speed as distance divided by the measured time difference. However, results remain contingent on the synchronization assumption, as any underlying anisotropy could affect the clock comparison in ways that mask or mimic light speed variations. A seminal historical example is Ole Rømer's 1676 observation of delays in the eclipses of Jupiter's moon Io, which provided the first quantitative estimate of the finite speed of light. By observing that eclipse timings lagged by up to 16.6 minutes when Earth was on the opposite side of its orbit from Jupiter (a distance variation of about 300 million km), Rømer calculated a speed of approximately 225,000 km/s, close to the modern value of 299,792 km/s after corrections for orbital geometry. Although the setup relies on light traveling one way from Jupiter to Earth, with distances determined astronomically, it has been reinterpreted as establishing an early bound on the one-way speed, assuming the satellite's orbital period is independent of light propagation. The measurement effectively constrains deviations from isotropy by showing consistency with a constant speed across varying paths. The 1990 Jet Propulsion Laboratory (JPL) experiment, conducted using the Deep Space Network facilities, exemplifies modern unidirectional testing through optical fiber links between two hydrogen-maser frequency standards separated by 21 km at Goldstone, California. Light pulses were transmitted one way through the fiber optic path, with travel times measured over five Earth rotations to detect directional anisotropy; the masers provided stable timing with phase noise below 10^{-13}, and synchronization relied on slow clock transport assumptions. The setup achieved a timing precision of 0.6 ns, corresponding to a fractional uncertainty in speed of about 3 \times 10^{-9}, and found no evidence of anisotropy at the level of 10^{-8} relative to c. A 1992 theoretical analysis confirmed that, under a test theory of special relativity, the results bound the one-way speed isotropy independently of round-trip measurements. More recent constraints come from space mission data, such as analyses of the Cassini spacecraft's radio signals using planetary ephemerides. One-way radio ranging from Cassini to Earth-based antennas (distances up to 1.4 billion km) measured light delays, with clocks synchronized via onboard atomic standards and ground networks assuming slow-transport equivalence; deviations in ephemeris fits tested for speed variations. The analysis limited deviations consistent with isotropy but ultimately bounded by the synchronization model's reliance on constant c for initial clock alignment. Overall, these experiments affirm the one-way speed as c within tested precisions, though interpretations hinge on the chosen synchronization convention.

Comparative synchronization experiments

Comparative synchronization experiments compare the results of Einstein synchronization, which uses light signals to set distant clocks, with slow clock-transport synchronization, where a clock is moved at velocities much less than c to a remote location and its reading is used to set the local clock. A discrepancy between these methods would indicate an anisotropy in the one-way speed of light, potentially revealing a preferred frame of reference. These tests are particularly sensitive to violations of Lorentz invariance in the synchronization process. One key experiment, conducted by Krisher et al. (including J. D. Anderson), used two hydrogen-maser frequency standards separated by approximately 21 km to compare one-way light propagation times with predictions from slow clock-transport equivalence. The setup involved sending microwave signals in opposite directions and analyzing phase differences, yielding no detectable difference between the synchronization methods to a precision of less than 5 × 10^{-9} c. ^[27] Other setups in the 1970s and 1980s, including tests on rotating platforms to probe noninertial effects, also showed null results for synchronization discrepancies to high precision. For instance, an experiment by Nelson et al. transported a hydrogen maser clock over a 26 km baseline on the rotating Earth and compared it to laser light-pulse synchronization, finding time differences less than 100 ps, corresponding to an anisotropy limit of Δc/c < 1.5 × 10^{-9}. ^[28] In the 2020s, modern transportable optical lattice clocks have been used to confirm the equivalence of slow clock transport to Einstein synchronization through consistent frequency comparisons during transport, aligning with special relativity predictions to high precision. ^[29] Theoretically, any observed discrepancy between Einstein and slow clock-transport synchronization would imply a preferred frame, but such effects are constrained by complementary Lorentz invariance tests to less than 10^{-12}. ^[30] A 1983 experiment employing thermal neutron interferometry provided indirect support for the agreement between these synchronization methods by demonstrating the isotropy of de Broglie waves for neutrons, consistent with light propagation assumptions underlying both techniques. ^[31] Overall, these comparative experiments strongly support the isotropy of the one-way speed of light within special relativity but do not independently verify it, as their results depend on the underlying equivalence of the synchronization conventions tested.

Proposed and framework-based tests

Einstein's famous train thought experiment illustrates the relativity of simultaneity, which underpins the convention-dependence of one-way light speed measurements. In this gedankenexperiment, lightning strikes the ends of a moving train simultaneously in the stationary observer's frame, but the observer on the train sees the front strike first due to the train's motion toward that light signal, highlighting how synchronization conventions affect perceived timing.^[32] Modern variants extend this to quantum regimes, proposing thought experiments with entangled photons to probe one-way light speed without relying on classical clock synchronization. One such proposal uses an entanglement-controlled stopwatch, where entangled particles trigger measurements at source and detector, aiming to bypass conventional synchronization while remaining blind to round-trip effects during data collection.^[33] Proposed experiments include one-way interferometers leveraging quantum clocks for enhanced precision in synchronization-independent tests. In the 2020s, ideas utilizing nitrogen-vacancy (NV) centers in diamond as ultra-stable quantum clocks have been suggested to measure light propagation delays in interferometric setups, potentially detecting anisotropy at levels below classical limits.^[34] Within the Standard-Model Extension (SME) framework developed by Kostelecký and others, tests using optical resonators bound parameters related to one-way light speed anisotropy. Recent analyses of resonator experiments, including cryogenic and rotating cavities, constrain the SME coefficient κ (characterizing directional speed variations) to below 10^{-17}, with no evidence of Lorentz violation as of 2023.^[35] Gravitational wave detectors like LIGO offer another avenue by comparing arrival times of waves from known directions, potentially revealing directional speed differences if light propagation in the interferometers shows anisotropy. Proposals suggest using LIGO's arm orientations to test light isotropy through sideband interference, providing bounds on speed variations across sky directions.^[36] Ongoing proposals involve space-based lasers, such as extensions to the Laser Interferometer Space Antenna (LISA), to test one-way speed over astronomical baselines by monitoring laser signals between spacecraft. These could probe anisotropy in gravitational wave propagation speeds matching light, with sensitivity to deviations at parts in 10^{15} or better.^[37] As of 2025, no conclusive evidence of one-way speed deviation from isotropy has emerged from these tests. However, all such measurements remain fundamentally convention-dependent, as they rely on synchronization procedures that inherently assume the very isotropy being tested.^[38]

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Sep 20, 2007 · We argue that an interference between the sidebands returning from the two arms is a measure of any anisotropic propagation of light. Note that ...
[35]
[PDF] Probing the speed of gravity with LVK, LISA, and joint observations
We also explore how one can use lower frequency measurements of gravitational waves in the LISA band to test for the existence and nature of such a transition.
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Can One-Way Light Speed be Measured? Comment on E. D. ... - arXiv
Mar 25, 2010 · Abstract:The convention dependence of one-way light speed is explained in a manner accessible to those unaccustomed to the concept.