Pith. sign in

REVIEW 6 minor 23 references

Measurement of the variation of electron-to-proton mass ratio using ultracold molecules produced from laser-cooled atoms

T0 review · 0 major / 6 minor · reviewed 2026-08-14 · deepseek-v4-flash

Pith's one-line read Ultracold KRb molecules provide the most precise molecular laboratory bound on temporal variation of the electron-to-proton mass ratio, five times tighter than before.

desk verdict A clean, statistically limited molecular measurement of μ-variation that delivers the first ultracold realization of DeMille's enhanced-sensitivity idea and improves the best molecular limit by a factor of five. read the letter →

arxiv 1908.08722 v1 pith:337EVC52 submitted 2019-08-23 physics.atom-ph

classification physics.atom-ph
keywords electron-to-protonmassratioultracoldmoleculesKRbvariationoffundamentalconstantsprecisionspectroscopysensitivitycoefficientmicrowavetransitionSTIRAP
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

This paper reports the most precise laboratory molecular test of whether the electron-to-proton mass ratio $\mu = m_e/M_p$ changes over time. The authors use ultracold $^{41}$K$^{87}$Rb molecules and a microwave transition between a nearly degenerate pair of vibrational levels, one in the $X^1\Sigma^+$ ground potential and one in the $a^3\Sigma^+$ potential, whose energy difference is unusually sensitive to $\mu$. From frequency measurements spread over about 16 months, they obtain $(1/\mu)(d\mu/dt) = (0.30 \pm 1.00_{\mathrm{stat}} \pm 0.16_{\mathrm{syst}}) \times 10^{-14}\,\mathrm{year}^{-1}$, a factor of five tighter than the previous best molecular limit. Because the measurement is limited by counting statistics rather than known systematics, the result points toward substantial further improvement.

What carries the argument

The load-bearing object is the near-degenerate pair of vibrational levels, $v=86$ in the deep $X^1\Sigma^+$ potential and $v=16$ in the shallow $a^3\Sigma^+$ potential of $^{41}$K$^{87}$Rb. Their energy separation is only about 635 MHz, while the individual energies have large and opposite dependence on $\ln \mu$, producing $W \approx -9.45$ THz and $|K_\mu| \approx 15000$. The sensitivity is computed from experimentally determined potential energy curves, so it is not tied to a free-parameter model. The protocol uses stimulated Raman adiabatic passage (STIRAP) to prepare a rovibrationally pure molecular sample, a 16 ms microwave $\pi$-pulse to drive the transition, and a simultaneous Zeeman-sensitive transition to subtract the second-order magnetic shift.

What would settle it

Measure the $v=86$ to $v=16$ energy interval, or the same microwave transition, in another KRb isotopologue and compare with the prediction from the same potential curves; a deviation beyond the quoted sensitivity uncertainty would invalidate $K_\mu$. Alternatively, an independent two-photon spectroscopic determination of the interval at sub-kHz accuracy would test the potential-curve-derived sensitivity.

Watch

Extended reading notes

Core claim

The central finding is that a microwave transition in ultracold KRb can serve as a nearly model-independent probe of the stability of $\mu$. The transition connects $|S=0,F_1=3/2,F=0,m_F=0\rangle$ in $v=86$ of $X^1\Sigma^+$ with $|S=1,F_1=1/2,F=1,m_F=0\rangle$ in $v=16$ of $a^3\Sigma^+$, at frequency $\nu = 634.96$ MHz. Its sensitivity coefficient is $K_\mu = W/\nu = -14890(60)$, with $W = \partial \nu/\partial(\ln \mu) \approx -9.45$ THz, so a fractional frequency measurement is magnified by roughly $1.5 \times 10^4$ in $\mu$. Over sixteen months of alternating measurements with a Zeeman-sensitive companion transition, the fractional frequency drift was $(-0.44 \pm 1.47_{\mathrm{stat}} \pm 0.24_{\mathrm{syst}}) \times 10^{-10}\,\mathrm{year}^{-1}$, which translates to $(1/\mu)(d\mu/dt) = (0.30 \pm 1.00_{\mathrm{stat}} \pm 0.16_{\mathrm{syst}}) \times 10^{-14}\,\mathrm{year}^{-1}$, a factor of five better than the most stringent previous molecular limit.

Load-bearing premise

The conversion from the measured frequency drift to a drift in $\mu$ assumes that the sensitivity coefficient $K_\mu = -14890(60)$, computed from the experimentally fitted potential energy curves of $^{41}$K$^{87}$Rb, is accurate to its quoted uncertainty.

Editorial extensions

If this is right

  • Molecular spectroscopy now yields an independent laboratory bound on $\mu$ drift five times tighter than the previous molecular result, complementing atomic-clock limits that probe a different combination of constants.
  • Because the dominant error is statistical, longer integration or larger molecular samples should improve the bound roughly as $\sqrt{N}$ in the number of detected molecules.
  • The near-degeneracy enhancement can be sought in other alkali dimers or other isotopologues, where different potential curves may give even larger $|K_\mu|$.
  • With proposed narrow-line laser cooling and molecular fountains or magic-wavelength lattices, linewidths near 1 Hz would convert the $\sim 10^4$ sensitivity into a proportionally stronger $\mu$-drift constraint.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • A direct isotope-substitution test of $K_\mu$ is an obvious next experiment: the ratio of transition frequencies between isotopologues is a predicted function of the potential curves, so any mismatch would expose errors in the sensitivity coefficient.
  • If the statistical limit is pushed, the blackbody-radiation shift, currently the largest systematic, will need to be measured directly with infrared fields; the paper identifies this path but does not carry it out.
  • The scheme effectively turns a microwave transition into a $\mu$-variation detector with built-in gain near $10^4$; applying the same idea to additional near-degenerate molecular pairs could create a set of independent probes with different systematic signatures.
Share X Bluesky LinkedIn Reddit HN

Signed reviews

No signed human review yet.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, and a circularity audit.

Referee Report

0 major / 6 minor

Summary. The paper reports a new laboratory limit on the temporal variation of the electron-to-proton mass ratio μ using a ~635 MHz transition between the v=86 level of the X^1Σ^+ state and the v=16 level of the a^3Σ^+ state of ultracold ⁴¹K⁸⁷Rb molecules produced by photoassociation and STIRAP. The transition is chosen for its large sensitivity coefficient K_μ = −14890(60), calculated from published potential curves. From 16 months of intermittent measurements, the authors derive (1/μ)(dμ/dt) = (0.30 ± 1.00_stat ± 0.16_syst) × 10⁻¹⁴ yr⁻¹, a factor of five improvement over the previous most stringent molecular limit (Shelkovnikov et al.). The measurement is statistics-limited, with a 94 mHz statistical uncertainty per spectrum versus a 10 mHz systematic budget.

Significance. If the result stands, it provides the most accurate molecular constraint on μ-variation and demonstrates the power of ultracold, near-degenerate molecular levels for precision metrology. The analysis is internally consistent: the conversion from the measured fractional frequency drift to the μ drift is arithmetically sound, the error budget in Table I is dominated by counting statistics, and the sensitivity coefficient is derived from independent potential curves rather than from the variation data, so there is no circularity. The paper also gives a concrete path toward further improvement via molecular fountains or lattice trapping. These strengths justify publication; only local presentation issues remain.

minor comments (6)
  1. [Title] The title contains a typo: 'ra tio' should read 'ratio'.
  2. [Fig. 3 caption] The phrase 'full-width-of-half-maximum' should be 'full width at half maximum'.
  3. [Supplementary Table 1] The E_cal values for the F1=5/2 manifold (0.0000, 0.0009, 0.0008, 0.0004) appear to be residuals rather than absolute energies, contrary to the column header, which states that both E_exp and E_cal are measured from the |S=0,F1=3/2,F=0⟩ state; please clarify the column definition or correct the entries.
  4. [Methods, Uncertainty of the sensitivity] The description of how the 4 GHz uncertainty in W was estimated is too brief; please specify which vibrational levels were compared and how the uncertainties of the vibrational level intervals were propagated into the sensitivity uncertainty.
  5. [Introduction] The statement that the atomic-clock results of Refs. [9] and [10] are 'essentially measuring the variation of the electron-to-proton magnetic moment ratio' is an oversimplification; a more precise characterization of what those measurements constrain would be helpful.
  6. [Abstract] The phrase 'Observed limit' could be replaced with 'Measurement' or 'Constraint', since the result is a measurement with error bars consistent with zero variation.

Circularity Check

0 steps flagged · score 0.0 of 10

No circularity identified: the sensitivity coefficient is an independent conversion factor and the final limit is statistics-dominated.

full rationale

The derivation chain is: measure the transition frequency drift df/dt from repeated microwave spectroscopy; convert to dmu/dt using K_mu = W/nu = -14890(60), where W is computed from experimentally determined potential energy curves of 41K87Rb reported in Ref. [15] and the measured transition frequency nu = 634.96 MHz. No parameter of the temporal-variation analysis is fitted to the drift data. The hyperfine fit in the supplement (E0, A_K, A_Rb) is used for state assignment and Zeeman corrections, not to determine the drift; the time variation is extracted from a linear fit to the central frequencies of the same transition over 16 months, with the sensitivity coefficient entering only as a fixed multiplicative conversion. The sensitivity uncertainty (about 0.4%) is small compared with the 1.47e-10 statistical uncertainty of the frequency drift, so even a fivefold underestimate of K_mu would not change the conclusion. The cited potential curves [15] and enhancement proposal [11] are independent published works, not authored by the present authors, and the result is stated to be statistics-limited, consistent with the quoted error budget. The comparisons with Shelkovnikov et al. and atomic clock limits are external benchmarks rather than inputs. No step in the paper's equations reduces by construction to its own inputs; hence no circularity is present.

Assumptions & free parameters 3 free parameters · 4 assumptions · 0 invented entities

The central claim rests on external inputs from prior literature: the KRb potential energy curves [15] and ab initio calculations [16,17]. No new particles, forces, or conserved quantities are introduced. The only fitted numbers (E0, A_K, A_Rb) are in the auxiliary hyperfine analysis and do not affect the final limit directly.

free parameters (3)
  • E0 = 4720.27 MHz
    Fitted in the hyperfine analysis (Supplementary note 1) to the observed hyperfine spectrum. Used for state identification and to compute Zeeman coefficients; does not enter the final dμ/dt directly, but is an auxiliary fitted parameter.
  • A_K = 125.54 MHz
    Fitted in the same hyperfine analysis; used to model the hyperfine structure and Zeeman shifts.
  • A_Rb = 3384.99 MHz
    Fitted in the same hyperfine analysis; used to model the hyperfine structure and Zeeman shifts.
assumptions (4)
  • domain assumption Potential energy curves for X^1Σ+ and a^3Σ+ of 41K87Rb from Pashov et al. [15] are accurate within the quoted uncertainties.
    Used to compute W, the sensitivity to μ, in the Methods section. If the curves are wrong, the conversion from frequency drift to μ drift is wrong.
  • domain assumption The ab initio BBR shift coefficients from Beuc et al. [16] and dipole moments from Kotochigova et al. [17] are reliable within their stated uncertainties.
    Used to estimate the blackbody radiation shift and its fluctuation; the BBR coefficient has uncertainty larger than its central value, so this assumption is load-bearing for the systematic error budget.
  • domain assumption The hyperfine Hamiltonian H = A_K S_K·I_K + A_Rb S_Rb·I_Rb with N=0 only is sufficient to describe the observed states.
    Used in Supplementary note 1 to analyze the hyperfine spectrum and predict Zeeman coefficients. Neglect of higher rotational states is stated to be less important.
  • domain assumption The sensitivity coefficient W is constant over the measurement period.
    The paper assumes that the only time-varying parameter affecting the transition frequency is μ (after corrections), i.e., the molecular potentials do not drift.

how reviews work

0 comments
Cite this review

Pith. "Pith review of Measurement of the variation of electron-to-proton mass ratio using ultracold molecules produced from laser-cooled atoms." pith.science (2026). https://pith.science/paper/337EVC52

@misc{pith2026190808722,
  author       = {Pith},
  title        = {Pith review of: Measurement of the variation of electron-to-proton mass ratio using ultracold molecules produced from laser-cooled atoms},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/337EVC52}},
  note         = {Machine review of arXiv:1908.08722}
}
abstract

Experimental techniques to manipulate cold molecules have seen great development in recent years. The precision measurements of cold molecules are expected to give insights into fundamental physics. We use a rovibrationally pure sample of ultracold KRb molecules to improve the measurement on the stability of electron-to-proton mass ratio ($\mu = \frac{m_{\rm e}}{M_{\rm p}}$). The measurement is based upon a large sensitivity coefficient of the molecular spectroscopy, which utilizes a transition between nearly a degenerate pair of vibrational levels each associated with a different electronic potential. Observed limit on temporal variation of $\mu$ is $\frac{1}{\mu}\frac{d\mu}{dt} = (0.30\pm1.0) \times 10^{-14}$ year$^{-1}$, which is better by a factor of five compared with the most stringent laboratory molecular limits to date. Further improvements should be straightforward, because our measurement was only limited by statistical errors.

Figures

Figures reproduced from arXiv: 1908.08722 by the authors.

Figure 1
Figure 1. FIG. 1: Closely lying states of a [PITH_FULL_IMAGE:figures/full_fig_p002_1.png] view at source ↗
Figure 2
Figure 2. FIG. 2: Production and detection of ultracold molecules. [PITH_FULL_IMAGE:figures/full_fig_p002_2.png] view at source ↗
Figure 3
Figure 3. shows a typical spectrum of the |ii - |fi transition obtained by six hours of data collection. A Gaussian fit to the data provided the full-width-of-half￾maximum(FWHM) of approximately 50 Hz, which is consistent with the ideal spectrum obtained by the mi￾crowave π-pulse of 16 ms duration. Longer pulse dura￾tions degraded the signal because ballistically expanding clouds of molecules with mean velocity ∼ 130 mm s−1 s… view at source ↗
Figures from the paper (1 more)
Figure 4
Figure 4. Figure 4: FIG. 4: Measurement of the temporal variation of [PITH_FULL_IMAGE:figures/full_fig_p004_4.png]

Discussion (0). Continue with ORCID to comment.

Reference graph

Works this paper leans on

23 extracted references · 23 canonical work pages

  1. [1]

    1 Е BOE ON .05 PG 3C BOE , BUPNT Е BOE ON .JDSP $IBOOFM 1MBUF *POJ[BUJPO Е ON ,3C C ᶃ.05 ᶄ1IPUPBTTPDJBUPO ᶆ.JDSPXBWF , BOE 3C ᶅ45*3

    2(1. 1) × 10−16 year−1 [9] and 1 µ dµ dt = −0. 5(1. 6) × 10−16 year−1 [10] were obtained by using atomic clocks. These measurements are essentially measuring the vari- ∗ Electronic address: j-kobayashi@scphys.kyoto-u.ac.jp ation of the electron-to-proton magnetic moment ratio. Here we report a measurement on the variation of µ us- ing ultracold KRb molecu...

  2. [2]

    The ACME Collaboration, Improved limit on the electric dipole moment of the electron nature 562 355-360 (2018)

  3. [3]

    Cairncross W.B. et al. Precision Measurement of the Electron’s Electric Dipole Moment Using Trapped Molec- ular Ions Phys. Rev. Lett. 119, 153001 (2017)

  4. [4]

    Hudson J.J. et al. Improved measurement of the shape of the electron nature 473 493 (2011)

  5. [5]

    D., DeMille D., Krems R.V., Ye J., Cold and ultracold molecules: science, technology and application s New Journal of Physics 11 055049 (2009)

    Carr L. D., DeMille D., Krems R.V., Ye J., Cold and ultracold molecules: science, technology and application s New Journal of Physics 11 055049 (2009)

  6. [6]

    Search for the electron electric dipole moment using Ωdoublet levels in PbO Phys

    Eckel S., Hamilton P., Kirilov E., Smith H.W., and De- Mille D. Search for the electron electric dipole moment using Ωdoublet levels in PbO Phys. Rev. A 87, 052130 (2013)

  7. [7]

    Probing the fron- tiers of particle physics with tabletop-scale experiments Science 357, 990-994 (2017)

    DeMille D., Doyle J.M., Sushkov A.O. Probing the fron- tiers of particle physics with tabletop-scale experiments Science 357, 990-994 (2017)

  8. [8]

    Uzan, J. -P. The fundamental constants and their vari- ation: observational and theoretical status Rev. Mod. Phys. 75, 403-455 (2003)

Show all 23 references
  1. [9]

    J., Chardonnet, C

    Shelkovnikov, A., Butcher, R. J., Chardonnet, C. & Amy- Klein, A. Stability of the Proton-to-Electron Mass Ratio Phys. Rev. Lett. 100, 150801 (2008)

  2. [10]

    Godun, R. M. et al. Frequency Ratio of Two Optical Clock Transitions in 171Yb+ and Constraints on the Time Variation of Fundamental Constants Phys. Rev. Lett. 113, 210801 (2014)

  3. [11]

    Huntemann, N. et al. Improved Limit on a Temporal Variation of mp/me from Comparisons of Yb + and Cs Atomic Clocks, Phys. Rev. Lett. 113, 210802 (2014)

  4. [12]

    DeMille, D. et al. Enhanced Sensitivity to Variation of me/mp in Molecular Spectra Phys. Rev. Lett. 100, 043202 (2008)

  5. [13]

    Aikawa, K. et al. Coherent Transfer of Photoassociated Molecules into the Rovibrational Ground State Phys. Rev. Lett. 105, 203001 (2010)

  6. [14]

    Bagdonaite, J. et al. A stringent limit on a drifting proton-to-electron mass ratio from alcohol in the early universe Science 339 46-48 (2013)

  7. [15]

    Leefer, N., Weber, C. T. M., Cing¨ oz, A., Torgerson, J. R. & Budker D. New Limits on Variation of the Fine- Structure Constant Using Atomic Dysprosium Phys. Rev. Let. 111, 060801 (2013)

  8. [17]

    Beuc, R. et al. Predictions for the observation of KRb spectra under cold conditions J. Phys. B 39, S1191 (2006). 6

  9. [18]

    Kotochigova, S., Julienne, P. S. & Tiesinga, E Ab initio calculation of KRb dipole moments Phys. Rev. A 68, 022501 (2003)

  10. [19]

    & Inouye, S

    Kobayashi, J., Aikawa, K., Oasa, K. & Inouye, S. Prospects for narrow-line cooling of KRb molecules in the rovibrational ground state Phys. Rev. A 89, 021401 (2014)

  11. [20]

    Precision Tes t of Mass-Ratio Variations with Lattice-Confined Ultracold Molecules Phys

    Zelevinsky, T., Kotochigova, S., & Ye, J. Precision Tes t of Mass-Ratio Variations with Lattice-Confined Ultracold Molecules Phys. Rev. Lett. 100, 043201 (2008)

  12. [21]

    J., Kaewuam, R., Roy, A., Tan, T

    Arnold, K. J., Kaewuam, R., Roy, A., Tan, T. R., & Barrett, M. D. Blackbody radiation shift assessment for lutetium in clock Nat. Comm. 9, 1650 (2018)

  13. [22]

    Measurement of the variati on of electron-to-proton mass ratio using ultracold molecules produced from laser-c ooled atoms

    Townes, C. H. & Schawlow, A. L. Microwave Spec- troscopy (Dover Publications, New York, 1975). End Notes Acknowledgements This work was supported by a Grant-in-Aid for Young Scientists (A) of JSPS (No. 23684034), a Grant-in-Aid for Scientific Research on Innovative Areas of JSP...

  14. [23]

    Pashov, A. et al. Coupling of the X 1Σ + and a3Σ + states of KRb. Phys. Rev. A 76, 022511 (2007)

  15. [24]

    & Violino, P

    Arimondo, E., Inguscio, M. & Violino, P. Experimental de terminations of the hyperfine structure in the alkali atoms Rev. Mod. Phys. 49, 31-75 (1977)

Pith tools

Reviewed August 14, 2026 · model on record in the stance chip above.