REVIEW 3 major objections 6 minor 33 references
The only difference between coherent and incoherent dark-matter scattering is crystal-momentum conservation, which weakens once multiple phonons are produced.
Reviewed by Pith at T0; open to challenge. T0 means a machine referee read the full paper against a public rubric. the ladder, T0–T4 →
T0 review · grok-4.5
2026-07-31 05:31 UTC pith:3RNCQH4E
load-bearing objection Clean 1D proof that coherent vs incoherent is just crystal-momentum conservation, with useful numerics inside the model—but the abstract overclaims “validation for realistic 3D crystals.” the 3 major comments →
Coherence from interference: a solvable model of sub-GeV dark matter-nucleus scattering
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
In an exactly solvable one-dimensional N-site lattice the full dynamic structure factor and the incoherent approximation differ only by the presence of a crystal-momentum-conserving delta function. That constraint becomes a weak restriction on the available phonon phase space once n greater than or equal to 2 phonons are produced, so the incoherent approximation (and a hybrid long-wavelength-plus-incoherent scheme) reproduces the exact scattering rates to within about 30 percent for both massive and massless mediators over most of the sub-GeV window.
What carries the argument
The n-phonon dynamic structure factor of the N-site chain (Eqs. 4.20 and 4.23), which isolates crystal-momentum conservation as the unique difference between the coherent and incoherent expressions and thereby explains why multiphonon rates can be computed without interference terms.
Load-bearing premise
That quantitative error estimates taken from a monoatomic harmonic one-dimensional chain with a hand-imposed infrared cutoff can be treated as a faithful stand-in for the isotropic three-dimensional structure factor of real crystals.
What would settle it
Compute the full multiphonon structure factor for a realistic three-dimensional monoatomic or diatomic crystal at intermediate q and compare the integrated rates against the hybrid Inc+LW prediction; a systematic discrepancy larger than 30 percent would falsify the claimed validation.
If this is right
- Multiphonon contributions to sub-GeV dark-matter rates in crystals can be evaluated with the computationally cheap incoherent formula once n greater than or equal to 2.
- A hybrid scheme that retains only the coherent long-wavelength single-phonon piece already yields percent-to-thirty-percent accuracy for experimental cross-section limits.
- The same momentum-conservation argument supplies a first-principles justification for stitching single-phonon and nuclear-recoil calculations across the transition region.
- Detector projections that previously relied on uncontrolled multiphonon approximations can now quote a controlled theoretical uncertainty.
Where Pith is reading between the lines
- The same weakening of momentum conservation should apply to optical branches and multi-atom unit cells, so the hybrid scheme is likely to remain accurate for polar targets once the long-wavelength optical matrix element is inserted by hand.
- Because the one-dimensional density of states diverges at low frequency, the numerical errors quoted here are probably conservative upper bounds relative to three-dimensional crystals where soft modes are phase-space suppressed.
- Anharmonic corrections, estimated small elsewhere, would first appear as a broadening of the multiphonon continuum rather than a revival of coherent interference, preserving the utility of the incoherent formula.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript studies sub-GeV dark-matter scattering from a harmonic one-dimensional lattice for which the multiphonon dynamic structure factor can be calculated recursively and, in the relevant limits, analytically. A two-site model first illustrates how interference suppresses optical-mode excitation at small q and averages away as phonon multiplicity increases. For the N-site chain, the authors derive Eqs. (4.20) and (4.23), showing that the full and incoherent structure factors differ by enforcement of crystal-momentum conservation. Numerical structure factors and differential rates are then compared for full, incoherent, impulse, and hybrid incoherent-plus-long-wavelength prescriptions. The paper concludes that the hybrid scheme reproduces the exact model's cross sections to about 30% over most of the considered mass range and presents this as quantitative validation for realistic 3D crystals.
Significance. If the claims are restricted to the harmonic 1D model, this is a significant and useful benchmark: it gives an exact, non-fit derivation of the full-to-incoherent relation, exposes crystal-momentum conservation as the relevant constraint, supplies explicit multiphonon spectra and rates, and motivates a falsifiable hybrid approximation for expensive 3D calculations. Those analytic and numerical strengths merit publication. Their portability to realistic 3D targets, however, currently remains an assumption rather than a demonstrated quantitative result.
major comments (3)
- [Abstract; §5; §6] Abstract; §5 opening; §6. The claim of "quantitative validation" for realistic 3D crystals is not established by the calculations presented. All dR/dq, dR/dω, and σ(mχ) results insert the monoatomic, acoustic-only 1D S(q,ω) into the isotropic 3D rate in Eq. (5.1), while Eq. (4.23) is explicitly generalized only for a monoatomic isotropic lattice. Silicon has a two-atom basis, optical branches, anisotropic dispersions, and polarization-dependent matrix elements, and no full 3D benchmark is shown. Either restrict the conclusion to a 1D proof of principle or provide a 3D test using branch-resolved D(ω,k), basis structure, and polarization factors, demonstrating that the stated ~30% accuracy survives.
- [§4.1, Fig. 6; §5.1, Fig. 12; Eq. (5.1)] The 1 meV mode cutoff is said to represent the detector threshold, but Eq. (5.1) correctly applies ωth to the total deposited energy. Individual phonons below ωth can still contribute to detectable n≥2 events. Discarding all modes below 1 meV therefore changes the physical spectrum, and it does so differently in the full and incoherent calculations because they assign crystal momentum differently. The cutoff also regularizes a 1D IR divergence absent in 3D. The reported agreement and 0.2–1 MeV discrepancy window may consequently be regulator-dependent. Please separate the physical threshold from the IR regulator, include sub-threshold phonons in multiphonon states, and show convergence or sensitivity to several cutoffs.
- [Eqs. (4.20) and (4.23); §6] The identity is convincing for the 1D monoatomic Bravais lattice, but the unqualified statement that momentum conservation is the only difference between coherent and incoherent scattering does not follow for realistic crystals. In the general definition, dropping d≠d′ removes intra-unit-cell interference in addition to the inter-unit-cell sum that enforces q−Σiki=G; anisotropic q·e polarization weights also do not reduce to the scalar D(ω,k) used in Eq. (4.23). Please state the precise assumptions under which Eqs. (4.20) and (4.23) hold, and either derive the multi-atom/anisotropic generalization or qualify the claims about general 3D crystals.
minor comments (6)
- [Eqs. (4.13) and (4.20)] Clarify whether these deltas are Kronecker deltas at finite N or Dirac deltas in the continuum, including the associated factors of N and the finite-N broadening prescription used in the numerical plots.
- [Table 1 and §5] The stitching domains should be stated more explicitly. In particular, specify whether the n=1 contribution above qBZ is included through umklapp in the incoherent term or omitted, and confirm that there is no double counting at q=qBZ and q=2√(2mω̄).
- [Eq. (2.1) and §5.3] q0 is not defined when F̃(q)=q0²/q² is introduced, while §5.3 uses F̃(q)=(mχv0/q)². Please use one definition consistently.
- [§4.3, §5, Appendix A] Because the numerical error estimates are central, please collect N, maximum phonon order, q stitching, energy binning, cutoff, and averaging choices in one place. Supplying plotting scripts or machine-readable rate tables would substantially improve reproducibility.
- [Throughout] There are several typographical issues: "goal is use" should be "goal is to use" in §4.1; "rapidly calculations" should be "rapid calculations" in §4.4; "agree results" should be "agree with results" in §5.3; and "direct direction calculations" should be "direct detection calculations" in §6.
- [Appendix B] Figures 15 and 16 would benefit from complete captions identifying the mediator form factor, σp, N, threshold, and the meaning of any smoothing or averaging, rather than relying on the main-text definitions.
Circularity Check
No circularity: the coherent/incoherent identity and rate comparisons are derived from the lattice Hamiltonian and the definition of S(q,ω), not fitted or forced by self-citation.
full rationale
The paper’s load-bearing chain is self-contained. The dynamic structure factor is defined from the target operator OT(q) and the two-point correlation of displacements (Eqs. 2.2–2.8). The 2-site and N-site models are solved from their harmonic Hamiltonians; the full vs. incoherent difference is obtained by summing auto- and cross-correlations, which produces the crystal-momentum delta in Eqs. 4.12–4.13 and 4.20/4.23. That identity is an algebraic consequence of discrete translation invariance, not an input. Numerical S(q,ω), dR/dq, dR/dω, and σ(mχ) then compare the exact 1D object to the incoherent and Inc+LW schemes built from the same model. Prior work (including Ref. [13], which shares an author) supplies the incoherent baseline being tested and standard single-phonon formulas; it does not manufacture the agreement. External parameters (Si sound speed, 1 meV cutoff, Standard Halo Model) are not fitted to the target rates. Weaknesses of the 1D→3D portability are modeling assumptions, not circular reductions. Score 0; steps empty.
Axiom & Free-Parameter Ledger
free parameters (4)
- ω0 (acoustic scale) =
≈10 meV
- IR energy cutoff ωcut =
1 meV
- Two-site mode energies ω+, ω− =
20 meV, 60 meV
- Finite N and multiphonon truncation / q-stitching boundaries =
N~100 for rates; stitch at qBZ and 2√(2mω̄)
axioms (5)
- domain assumption Harmonic lattice dynamics (bilinear springs only); anharmonic corrections neglected
- domain assumption Dynamic structure factor factorization of the DM-target rate (Eq. 1.1 / 2.2)
- ad hoc to paper 1D monoatomic periodic chain is a faithful enough proxy that its S(q,ω) can replace the isotropic 3D structure factor inside 3D rate integrals
- domain assumption Standard Halo Model velocity distribution with canonical vesc, v0, vE
- domain assumption Impulse approximation replaces the structure factor for q > 2√(2mω̄)
read the original abstract
How do dark matter-nucleus interactions transition from the regimes of coherent scattering, where single phonons are produced, to that of individual nuclear recoils? Answering this question relies on understanding multiphonon excitations. Multiphonons are important for interpreting low-threshold direct detection experiments, yet are computationally prohibitive to compute. In this paper, we employ a 1D $N$-site crystal lattice model where dark matter scattering can be computed exactly. We show that the only difference between coherent and incoherent scattering is that conservation of crystal momentum is enforced in coherent scattering. The momentum conservation constraint becomes less important as more phonons are produced, yielding the transition to incoherent scattering. Using numerical calculations of the 1D structure factor, we also obtain quantitative validation of using an incoherent approximation to compute sub-GeV dark matter scattering in realistic 3D crystals.
Reference graph
Works this paper leans on
-
[3]
Y. Kahn and T. Lin,Searches for light dark matter using condensed matter systems,Rept. Prog. Phys.85(2022) 066901 [2108.03239]
Pith/arXiv arXiv 2022
-
[4]
Zurek,Dark Matter Candidates of a Very Low Mass,Ann
K.M. Zurek,Dark Matter Candidates of a Very Low Mass,Ann. Rev. Nucl. Part. Sci.74 (2024) 287 [2401.03025]. [5]TESSERACTcollaboration,First Limits on Light Dark Matter Interactions in a Low Threshold Two Channel Athermal Phonon Detector from the TESSERACT Collaboration, 2503.03683. – 27 – Figure 16.dR/dωresult forN= 100. [6]CRESSTcollaboration,First result...
Pith/arXiv arXiv 2024
-
[7]
S. Knapen, T. Lin, M. Pyle and K.M. Zurek,Detection of Light Dark Matter With Optical Phonons in Polar Materials,Phys. Lett.B785(2018) 386 [1712.06598]
Pith/arXiv arXiv 2018
-
[8]
S. Griffin, S. Knapen, T. Lin and K.M. Zurek,Directional Detection of Light Dark Matter with Polar Materials,Phys. Rev.D98(2018) 115034 [1807.10291]
Pith/arXiv arXiv 2018
-
[9]
T. Trickle, Z. Zhang, K.M. Zurek, K. Inzani and S. Griffin,Multi-Channel Direct Detection of Light Dark Matter: Theoretical Framework,JHEP03(2020) 036 [1910.08092]
Pith/arXiv arXiv 2020
-
[10]
S. Knapen, T. Lin and K.M. Zurek,Light Dark Matter in Superfluid Helium: Detection with Multi-excitation Production,Phys. Rev.D95(2017) 056019 [1611.06228]
Pith/arXiv arXiv 2017
-
[11]
B. Campbell-Deem, P. Cox, S. Knapen, T. Lin and T. Melia,Multiphonon excitations from dark matter scattering in crystals,Phys. Rev. D101(2020) 036006 [1911.03482]
Pith/arXiv arXiv 2020
-
[12]
Y. Kahn, G. Krnjaic and B. Mandava,Dark Matter Detection with Bound Nuclear Targets: The Poisson Phonon Tail,Phys. Rev. Lett.127(2021) 081804 [2011.09477]
Pith/arXiv arXiv 2021
-
[13]
B. Campbell-Deem, S. Knapen, T. Lin and E. Villarama,Dark matter direct detection from the single phonon to the nuclear recoil regime,Phys. Rev. D106(2022) 036019 [2205.02250]
Pith/arXiv arXiv 2022
-
[14]
S. Gori, S. Knapen, T. Lin, P. Munbodh and B. Suter,Spin-dependent scattering of sub-GeV dark matter: Models and constraints,Phys. Rev. D112(2025) 075019 [2506.11191]
Pith/arXiv arXiv 2025
-
[15]
K. Schutz and K.M. Zurek,Detectability of Light Dark Matter with Superfluid Helium,Phys. Rev. Lett.117(2016) 121302 [1604.08206]
Pith/arXiv arXiv 2016
-
[16]
A. Caputo, A. Esposito and A.D. Polosa,Light Dark Matter and Superfluid He-4 from EFT, J. Phys. Conf. Ser.1468(2020) 012060 [1911.07867]. – 28 –
Pith/arXiv arXiv 2020
-
[17]
F. Acanfora, A. Esposito and A.D. Polosa,Sub-GeV Dark Matter in Superfluid He-4: an Effective Theory Approach,Eur. Phys. J.C79(2019) 549 [1902.02361]
Pith/arXiv arXiv 2019
-
[18]
A. Caputo, A. Esposito, F. Piccinini, A.D. Polosa and G. Rossi,Directional detection of light dark matter from three-phonon events in superfluid4He,Phys. Rev. D103(2021) 055017 [2012.01432]
Pith/arXiv arXiv 2021
-
[19]
S. Knapen, J. Kozaczuk and T. Lin,Migdal Effect in Semiconductors,Phys. Rev. Lett.127 (2021) 081805 [2011.09496]
Pith/arXiv arXiv 2021
-
[20]
K.V. Berghaus, A. Esposito, R. Essig and M. Sholapurkar,The Migdal effect in semiconductors for dark matter with masses below∼100 MeV,JHEP01(2023) 023 [2210.06490]
Pith/arXiv arXiv 2023
-
[21]
K.V. Berghaus, R. Essig and M.H. McDuffie,The Migdal effect in Semiconductors for the Effective Field Theory of Dark Matter Direct Detection,2603.13052
-
[22]
M. Ibe, W. Nakano, Y. Shoji and K. Suzuki,Migdal Effect in Dark Matter Direct Detection Experiments,JHEP03(2018) 194 [1707.07258]
Pith/arXiv arXiv 2018
-
[23]
K.V. Berghaus, R. Essig, Y. Hochberg, Y. Shoji and M. Sholapurkar,Phonon background from gamma rays in sub-GeV dark matter detectors,Phys. Rev. D106(2022) 023026 [2112.09702]
Pith/arXiv arXiv 2022
-
[24]
P. Cox, T. Melia and S. Rajendran,Dark matter phonon coupling,Phys. Rev. D100(2019) 055011 [1905.05575]
Pith/arXiv arXiv 2019
-
[25]
S.M. Griffin, K. Inzani, T. Trickle, Z. Zhang and K.M. Zurek,Multichannel direct detection of light dark matter: Target comparison,Phys. Rev.D101(2020) 055004 [1910.10716]
Pith/arXiv arXiv 2020
-
[26]
A. Caputo, A. Esposito, E. Geoffray, A.D. Polosa and S. Sun,Dark Matter, Dark Photon and Superfluid He-4 from Effective Field Theory,Phys. Lett. B802(2020) 135258 [1911.04511]
Pith/arXiv arXiv 2020
-
[27]
S.M. Griffin, Y. Hochberg, K. Inzani, N. Kurinsky, T. Lin and T.C. Yu,Silicon carbide detectors for sub-GeV dark matter,Phys. Rev. D103(2021) 075002 [2008.08560]
Pith/arXiv arXiv 2021
-
[28]
T. Trickle, Z. Zhang and K.M. Zurek,Effective field theory of dark matter direct detection with collective excitations,Phys. Rev. D105(2022) 015001 [2009.13534]
Pith/arXiv arXiv 2022
-
[29]
N. Taufertshöfer, M. Garcia-Sciveres and S.M. Griffin,Proposal for broad-range directional detection of light dark matter in cryogenic ice,Phys. Rev. D110(2024) 103552 [2301.04778]
Pith/arXiv arXiv 2024
-
[30]
O.A. Ashour and S.M. Griffin,Pressure-Tunable Targets for Light Dark Matter Direct Detection: The Case of Solid Helium,2409.02439
-
[31]
X.-X. Li, N. Valsan and Z. Zhang,Astrophysical Uncertainties in Sub-GeV Dark Matter Detection via Single Phonon Excitations,2606.04091
-
[32]
A. Coskuner, T. Trickle, Z. Zhang and K.M. Zurek,Directional detectability of dark matter with single phonon excitations: Target comparison,Phys. Rev. D105(2022) 015010 [2102.09567]
Pith/arXiv arXiv 2022
-
[33]
S. Knapen, J. Kozaczuk and T. Lin,DarkELF: A python package for dark matter scattering in dielectric targets,Phys. Rev. D105(2022) 015014 [2104.12786]
Pith/arXiv arXiv 2022
-
[34]
T. Lin, C.-H. Shen, M. Sholapurkar and E. Villarama,Anharmonic effects in nuclear recoils from sub-GeV dark matter,Phys. Rev. D109(2024) 095020 [2309.10839]. – 29 –
Pith/arXiv arXiv 2024
-
[35]
C. Stratman and T. Lin,Daily modulation of low-energy nuclear recoils from sub-GeV dark matter,Phys. Rev. D111(2025) 043030 [2411.03433]
Pith/arXiv arXiv 2025
-
[36]
Squires,Introduction to the Theory of Thermal Neutron Scattering, Dover Publications, Inc., Mineola, New York (1996)
G.L. Squires,Introduction to the Theory of Thermal Neutron Scattering, Dover Publications, Inc., Mineola, New York (1996)
1996
-
[37]
Schober,An introduction to the theory of nuclear neutron scattering in condensed matter, Journal of Neutron Research17(2014) 109
H. Schober,An introduction to the theory of nuclear neutron scattering in condensed matter, Journal of Neutron Research17(2014) 109. – 30 –
2014
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.