REVIEW 2 major objections 3 minor 4 cited by
Broadband phonon production from axion absorption
T0 review · 2 major / 3 minor · reviewed 2026-08-12 · deepseek-v4-flash
Pith's one-line read The paper claims that axion dark matter from 1 to 100 meV can excite phonons in crystals with randomly oriented nuclear spins, breaking translation symmetry so the rate tracks the phonon density of states without frequency scanning.
desk verdict New broadband axion-phonon mechanism is real for atomic crystals, but the molecular targets H2/D2/H2O/D2O need a fix for ortho-para spin-rotation coupling before their projected rates can be trusted. read the letter →
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
The reading
What carries the argument
The load-bearing object is the atom-projected phonon density of states, $D_j(\omega) = (1/3N)\sum_{\nu k} |\epsilon^j_{\nu k}|^2 \delta(\omega - \omega_{\nu k})$, together with the lattice-averaged spin coupling $\xi_j = (1/N)\sum_\ell \lambda_{\ell j}^2 J_{\ell j}(J_{\ell j}+1)/m_{\ell j}$. The argument splits the absorption rate into coherent and incoherent terms: the coherent terms carry the phase $e^{-i\mathbf{k}\cdot(\ell-\ell')}$ that enforces $\mathbf{k}\approx 0$ in a polarised crystal, while the incoherent term has no such phase after the random-spin ensemble average. Because the final-spin sum becomes a resolution of the identity, only $D_j(\omega)$ and $\xi_j$ control the rate, and since $D_j(\omega)$ has support across a wide range of phonon energies, the detection scheme is broadband.
What would settle it
Measure the phonon density of states of solid H$_2$ and D$_2$ at meV energies and compare a cryogenic calorimeter's axion-absorption spectrum with the prediction $R \propto \sum_j \xi_j D_j(m_a)$: a rate that drops steeply below the ortho--para rotational splitting, rather than tracing $D(m_a)$, would falsify the degenerate-spin assumption.
Extended reading notes
Core claim
The discovery is that axion absorption in an unpolarised crystal is broadband because the random spin configuration acts as disorder that fully breaks translation symmetry in the phonon effective theory. In a polarised crystal the coherent terms in the rate sum to a momentum-conservation condition $\delta_{\mathbf{k},0}$, so only zero-momentum optical phonons can absorb the axion and the response is a narrow Breit-Wigner peak. In an unpolarised crystal the ensemble average over spin configurations kills those interference terms, leaving the diagonal, incoherent term with no momentum-restricting phase; the sum over final spin states collapses to the identity because all spin configurations are degenerate in energy. The result is Eq. (31), $R = 2\pi \rho_a m_a \, g_p^2 \sum_j \xi_j D_j(m_a)/\sum_j m_j$, where $\xi_j$ is the lattice-averaged spin coupling of the $j$-th nucleus and $D_j(\omega)$ is its atom-projected phonon density of states. The same mechanism operates for the axion-induced time-dependent nuclear electric dipole moment, and the paper shows that this second channel is subdominant in standard QCD axion models.
Load-bearing premise
The calculation assumes that flipping a nuclear spin costs no energy beyond the phonon it creates, an assumption that molecular crystals with identical nuclei, where exchange symmetry couples spin to molecular rotation, may violate.
Editorial extensions
If this is right
- A single unpolarised crystal target can search the full energy range where its phonon density of states has support, with no frequency scanning or applied magnetic field.
- Two or three light-nucleus targets (hydrogen- or deuterium-bearing solids) cover essentially the whole 1--100 meV axion mass window.
- The previously studied coherent, narrow-band optical-phonon channel is not needed for sensitivity; the incoherent channel gives a comparable or larger rate in unpolarised crystals.
- For standard QCD axion models, the spin coupling channel dominates over the induced nuclear electric dipole channel, so the rate is controlled by $\xi_j D_j(m_a)$.
- Reaching the predicted QCD-axion rate of a few events per 10 kg-year requires a corresponding reduction of low-energy backgrounds in single-phonon calorimeters.
Reading between the lines
- Beyond the paper: if the degenerate-spin assumption fails in molecular solids through ortho--para exchange couplings, the promised low-mass coverage for H$_2$, D$_2$, H$_2$O and D$_2$O would shift, and the rate formula would need a spin-flip energy threshold.
- Beyond the paper: the same 'disorder makes absorption broadband' principle suggests that other forms of quenched disorder, such as isotope mixtures, impurities, or amorphous targets, could generate broadband phonon absorption for other dark matter candidates.
- Beyond the paper: a testable extension is to measure the partial phonon density of states of solid H$_2$ and D$_2$ with inelastic neutron scattering and use it to predict the full spectral shape that a future single-phonon calorimeter should see.
- Beyond the paper: for axion-like particles with suppressed photon coupling but large nucleon coupling, this channel may be the only terrestrial probe in the 1--100 meV window.
Signed reviews
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper proposes a new phonon-based direct-detection channel for axion dark matter in the meV to 100 meV mass range. Starting from the non-relativistic axion-nucleon interaction, the authors derive the rate for incoherent single-phonon emission in crystals with randomly oriented nuclear spins. Their central result, Eq. (31), states that the rate per unit mass is proportional to the axion mass, the axion-proton coupling squared, and the atom-projected phonon density of states, with no momentum-conservation restriction. They compute this rate for H2, D2, Al2O3, GaAs, H2O, D2O, Be, and Li2O, compare it with the previously studied coherent absorption, estimate the subleading contribution from the axion-induced nuclear electric dipole moment, and discuss the experimental prospects for TESSERACT-style phonon sensors and the relevant backgrounds. The headline claim is that only two or three target materials suffice to cover the 1-100 meV axion mass range without frequency scanning.
Significance. If Eq. (31) is valid for a given material, the paper makes an important methodological contribution: it shows that spin disorder in an unpolarised crystal removes the momentum-matching condition, so the axion absorption spectrum becomes proportional to the phonon density of states. This turns a narrowband search into a broadband one and gives falsifiable predictions for Be, Li2O, Al2O3, and GaAs, which do not involve any fitting parameters and depend only on the axion couplings and independently measured or computed phonon spectra. The coherent limit is checked against the existing literature, and the paper is careful about nuclear form factors and isotope averaging. However, the most promising projected rates and the '2-3 materials cover the full range' claim rely on molecular crystals (H2, D2, H2O, D2O), where a load-bearing spin-degeneracy assumption fails because identical-nucleus exchange symmetry couples nuclear spin to molecular rotation. The mechanism as rigorously proven is therefore restricted to atomic crystals, and the headline coverage claim is not yet established.
major comments (2)
- [Sec. II D, Eqs. (25)-(31), footnote 4] The derivation of Eq. (31) replaces the final-spin sum in Eq. (25) by the identity using the assertion in footnote 4 that all spin configurations have degenerate energies. This is the load-bearing assumption of the incoherent rate. It is valid for atomic crystals in the absence of magnetic fields, but it fails for the molecular crystals H2, D2, H2O, and D2O, where exchange symmetry of identical nuclei entangles nuclear spin with molecular rotation. For H2, para-H2 has total nuclear spin I=0 and even rotational J, while ortho-H2 has I=1 and odd J, with E(J=1)-E(J=0) about 15 meV; D2 has a comparable gap of several meV. A one-proton spin flip in a para molecule changes the total molecular spin and forces a rotational transition, so the energy-conserving delta function should involve delta(ma - omega_k - Delta_rot), not delta(ma - omega_k). The footnote's observation that the axion flips only a single spin limits which final states can contribute, but it does not imply that those states are degenerate with the initial state. Equations (25)-(31) and the low-mass rates for these molecular targets are therefore not established as written.
- [Table I, Eq. (28), and Fig. 2] The material-specific input for solid H2 is internally inconsistent even apart from the general degeneracy issue. The phonon density of states is taken from Ref. [52], which is a measurement on solid parahydrogen. Parahydrogen molecules have total nuclear spin I=0 and do not supply the independent spin-1/2 degree of freedom per proton that Eq. (28) and Table I assume when assigning xi_H = 0.75 GeV^-1 to every H site. A single-proton spin flip in such a molecule is an off-diagonal transition to an ortho-like state, not a reorientation within the degenerate manifold used in Eq. (27). The same objection applies to D2 and to the hydrogen/deuterium nuclei in H2O and D2O. Consequently, the low-mass parts of the H2, D2, H2O, and D2O contours in Fig. 2 are not supported by the calculation as written, and the claim that 2-3 materials cover the 1-100 meV range is not established. The rates for Be, Li2O, Al2O3, and GaAs do not have this defect because their nuclei are not subject to identical-nucleus exchange within the crystal unit.
minor comments (3)
- [Abstract and Sec. II D] The statement that random spin orientations 'break translation symmetry' is imprecise: the ensemble-averaged crystal is translation invariant, and what removes the momentum-conservation delta function is the suppression of the off-diagonal interference term in Eq. (19) by uncorrelated spin orientations. Consider rewording to avoid the impression that the ensemble itself is a disordered static configuration.
- [Sec. IV and Fig. 2] Section IV states that the aluminium pair-breaking threshold of 7.2 meV sets a theoretical lower limit on the detectable axion mass, yet Fig. 2 shows contours extending down to 1 meV. Please clarify which readout or sensor is assumed for masses below 7.2 meV, or restrict the plotted range accordingly.
- [Throughout] There are several typographical issues: 'Brioullin zone' in the Introduction, 'gann' in Appendix B, and the notation in Eq. (34) for the spin operators appears garbled. A careful proofread would be helpful.
Circularity Check
No circularity: the incoherent absorption rate in Eq. (31) is derived from first principles and external phonon densities of states; no fitted parameter is renamed as a prediction.
full rationale
The paper's derivation chain is self-contained and first-principles. Starting from the axion-nucleon Lagrangian (Eq. (1)-(2)), the non-relativistic Hamiltonian (Eq. (4)), and the crystal matrix element (Eq. (15)), the authors use Fermi's Golden Rule to obtain the coherent and incoherent rates. The incoherent rate in Eq. (31) follows from (i) replacing the final-spin sum by the identity under the explicitly stated degenerate-spin assumption (footnote 4), (ii) the ensemble average in Eq. (27), and (iii) the definition of the atom-projected phonon density of states D_j(omega) in Eq. (29). The phonon densities of states are external inputs obtained from published DFT calculations and neutron-scattering measurements (Refs. [51]-[56]), not quantities fitted in this paper. The nuclear spin form factors lambda_j are taken from external nuclear-structure calculations (Refs. [88], [90]). The coherent result is rederived and checked against the earlier literature (Ref. [44]), which is an independent cross-check, not a load-bearing self-citation. The one self-citation (Ref. [55], a public package used for the sapphire phonon DOS) provides an external computational input rather than a result asserted by this paper. The spin-degeneracy assumption may be physically invalid for molecular crystals such as H2, D2, H2O, and D2O, and this is an openly stated limitation that could affect the projected rates; however, that is a correctness risk, not a circularity, because Eq. (31) is not equivalent to its inputs by construction. No fitted parameter is relabelled as a prediction, no uniqueness theorem is imported from the authors' prior work, and no known empirical pattern is merely renamed. The derivation is therefore not circular.
Assumptions & free parameters
assumptions (6)
- standard math Fermi's Golden rule applies to the axion-to-single-phonon transition.
- domain assumption Spin and phonon degrees of freedom factorise as product states (Eq. (9)).
- domain assumption All nuclear spin configurations are degenerate in energy.
- domain assumption No sizable internal or external magnetic fields, so the potential commutes with position and D can be replaced by the gradient.
- domain assumption The phonon density of states from external DFT or neutron scattering accurately represents the targets.
- domain assumption The Born-Oppenheimer approximation holds and electronic excitations are negligible.
Cite this review
Pith. "Pith review of Broadband phonon production from axion absorption." pith.science (2026). https://pith.science/paper/BUKAE6YN
@misc{pith2026241110542,
author = {Pith},
title = {Pith review of: Broadband phonon production from axion absorption},
year = {2026},
howpublished = {\url{https://pith.science/paper/BUKAE6YN}},
note = {Machine review of arXiv:2411.10542}
}
abstract
We show that axion dark matter in the range meV $\lesssim m_a\lesssim$ 100 meV can incoherently excite phonons in crystal targets with unpolarised nuclear spins. This can occur through its coupling to nuclear spins and/or through its induced time-dependent electric dipole moment in nuclei. Due to the random orientation of the nuclear spins, translation symmetry is broken in the phonon effective theory, allowing axion absorption to create phonons with unrestricted momentum. The absorption rate is therefore proportional to the phonon density of states, which generically has support across a wide range of energies, allowing for a broadband detection scheme. We calculate the absorption rate for solid $\text{H}_2$, $\text{D}_2$, $\text{Al}_2\text{O}_3$, $\text{GaAs}$, $\text{H}_2\text{O}$, $\text{D}_2\text{O}$, $\text{Be}$ and $\text{Li}_2 \text{O}$, and find that materials containing light, non-zero spin nuclei are the most promising. The predicted rates for the QCD axion are of the order of a few events / 10 kg-year exposure, setting an ambitious target for the required exposure and background suppression.
Figures
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Reference graph
Works this paper leans on
-
[52]
D. Colognesi, M. Celli, and M. Zoppi, Density of phonon states in solid parahydrogen from inelastic neutron scattering, The Journal of Chemical Physics 120 (03, 2004) 5657–5663, [https://doi.org/10.1063/1.1649312]
-
[1]
C. B. Adams et al., Axion Dark Matter , in Snowmass 2021, 3, 2022. arXiv:2203.14923
arXiv 2021
-
[2]
R. D. Peccei and H. R. Quinn, CP Conservation in the Presence of Instantons , Phys. Rev. Lett. 38 (1977) 1440–1443
1977
-
[3]
R. D. Peccei and H. R. Quinn, Constraints Imposed by CP Conservation in the Presence of Instantons , Phys. Rev. D 16 (1977) 1791–1797
1977
-
[4]
Wilczek, Problem of Strong P and T Invariance in the Presence of Instantons , Phys
F. Wilczek, Problem of Strong P and T Invariance in the Presence of Instantons , Phys. Rev. Lett. 40 (1978) 279–282
1978
-
[5]
Weinberg, A New Light Boson? , Phys
S. Weinberg, A New Light Boson? , Phys. Rev. Lett. 40 (1978) 223–226
1978
-
[6]
Preskill, M
J. Preskill, M. B. Wise, and F. Wilczek, Cosmology of the Invisible Axion , Phys. Lett. B 120 (1983) 127–132
1983
-
[7]
L. F. Abbott and P. Sikivie, A Cosmological Bound on the Invisible Axion , Phys. Lett. B 120 (1983) 133–136
1983
Show all 99 references
-
[8]
Dine and W
M. Dine and W. Fischler, The Not So Harmless Axion , Phys. Lett. B 120 (1983) 137–141
1983
-
[9]
K. J. Bae, J.-H. Huh, and J. E. Kim, Update of axion CDM energy, JCAP 09 (2008) 005, [ arXiv:0806.0497]
2008 arXiv
-
[10]
Wantz and E
O. Wantz and E. P. S. Shellard, Axion Cosmology Revisited, Phys. Rev. D 82 (2010) 123508, [arXiv:0910.1066]
2010 arXiv
-
[11]
Ballesteros, J
G. Ballesteros, J. Redondo, A. Ringwald, and C. Tamarit, Standard Model—axion—seesaw—Higgs portal inflation. Five problems of particle physics and cosmology solved in one stroke , JCAP 08 (2017) 001, [arXiv:1610.01639]
2017 arXiv
-
[12]
Borsanyi et al., Calculation of the axion mass based on high-temperature lattice quantum chromodynamics , Nature 539 (2016), no
S. Borsanyi et al., Calculation of the axion mass based on high-temperature lattice quantum chromodynamics , Nature 539 (2016), no. 7627 69–71, [arXiv:1606.07494]
2016 arXiv
-
[13]
V. B. . Klaer and G. D. Moore, The dark-matter axion mass, JCAP 11 (2017) 049, [ arXiv:1708.07521]
2017 arXiv
-
[14]
Gorghetto, E
M. Gorghetto, E. Hardy, and G. Villadoro, More axions from strings, SciPost Phys. 10 (2021), no. 2 050, [arXiv:2007.04990]
2021 arXiv
-
[15]
Buschmann, J
M. Buschmann, J. W. Foster, A. Hook, A. Peterson, D. E. Willcox, W. Zhang, and B. R. Safdi, Dark matter from axion strings with adaptive mesh refinement , Nature Commun. 13 (2022), no. 1 1049, [arXiv:2108.05368]
2022 arXiv
-
[16]
Kawasaki, K
M. Kawasaki, K. Saikawa, and T. Sekiguchi, Axion dark matter from topological defects, Phys. Rev. D 91 (2015), no. 6 065014, [ arXiv:1412.0789]
2015 arXiv
-
[17]
Ringwald and K
A. Ringwald and K. Saikawa, Axion dark matter in the post-inflationary Peccei-Quinn symmetry breaking scenario, Phys. Rev. D 93 (2016), no. 8 085031, [arXiv:1512.06436]. [Addendum: Phys.Rev.D 94, 049908 (2016)]
2016 arXiv
-
[18]
K. A. Beyer and S. Sarkar, Ruling out light axions: The writing is on the wall , SciPost Phys. 15 (2023), no. 1 003, [arXiv:2211.14635]
2023 arXiv
-
[19]
Horns, J
D. Horns, J. Jaeckel, A. Lindner, A. Lobanov, J. Redondo, and A. Ringwald, Searching for WISPy Cold Dark Matter with a Dish Antenna , JCAP 04 (2013) 016, [ arXiv:1212.2970]
2013 arXiv
-
[20]
Baryakhtar, J
M. Baryakhtar, J. Huang, and R. Lasenby, Axion and hidden photon dark matter detection with multilayer optical haloscopes, Phys. Rev. D 98 (2018), no. 3 035006, [arXiv:1803.11455]
2018 arXiv
-
[21]
Liu et al., Broadband Solenoidal Haloscope for Terahertz Axion Detection , Phys
BREAD Collaboration, J. Liu et al., Broadband Solenoidal Haloscope for Terahertz Axion Detection , Phys. Rev. Lett. 128 (2022), no. 13 131801, [arXiv:2111.12103]
2022 arXiv
-
[22]
Mitridate, T
A. Mitridate, T. Trickle, Z. Zhang, and K. M. Zurek, Detectability of Axion Dark Matter with Phonon Polaritons and Magnons , Phys. Rev. D 102 (2020), no. 9 095005, [ arXiv:2005.10256]. 12
2020 arXiv
-
[23]
Berlin and T
A. Berlin and T. Trickle, Absorption of Axion Dark Matter in a Magnetized Medium , Phys. Rev. Lett. 132 (2024), no. 18 181801, [ arXiv:2305.05681]
2024 arXiv
-
[24]
D. J. E. Marsh, J. I. McDonald, A. J. Millar, and J. Sch¨ utte-Engel,Axion detection with phonon-polaritons revisited, Phys. Rev. D 107 (2023), no. 3 035036, [ arXiv:2209.12909]
2023 arXiv
-
[25]
Sch¨ utte-Engel, D
J. Sch¨ utte-Engel, D. J. E. Marsh, A. J. Millar, A. Sekine, F. Chadha-Day, S. Hoof, M. N. Ali, K.-C. Fong, E. Hardy, and L. ˇSmejkal, Axion quasiparticles for axion dark matter detection , JCAP 08 (2021) 066, [arXiv:2102.05366]
2021 arXiv
-
[26]
ARIADNE Collaboration, A. A. Geraci et al., Progress on the ARIADNE axion experiment , Springer Proc. Phys. 211 (2018) 151–161, [ arXiv:1710.05413]
2018 arXiv
-
[27]
Craig, A
N. Craig, A. Hook, and S. Kasko, The Photophobic ALP, JHEP 09 (2018) 028, [ arXiv:1805.06538]
2018 arXiv
-
[28]
M. Dine, W. Fischler, and M. Srednicki, A Simple Solution to the Strong CP Problem with a Harmless Axion, Phys. Lett. B 104 (1981) 199–202
1981
-
[29]
A. R. Zhitnitsky, On Possible Suppression of the Axion Hadron Interactions. (In Russian) , Sov. J. Nucl. Phys. 31 (1980) 260
1980
-
[30]
Wu et al., Search for Axionlike Dark Matter with a Liquid-State Nuclear Spin Comagnetometer , Phys
T. Wu et al., Search for Axionlike Dark Matter with a Liquid-State Nuclear Spin Comagnetometer , Phys. Rev. Lett. 122 (2019), no. 19 191302, [ arXiv:1901.10843]
2019 arXiv
-
[31]
Garcon et al., Constraints on bosonic dark matter from ultralow-field nuclear magnetic resonance , Sci
A. Garcon et al., Constraints on bosonic dark matter from ultralow-field nuclear magnetic resonance , Sci. Adv. 5 (2019), no. 10 eaax4539, [ arXiv:1902.04644]
2019 arXiv
-
[32]
NASDUCK Collaboration, I. M. Bloch, G. Ronen, R. Shaham, O. Katz, T. Volansky, and O. Katz, New constraints on axion-like dark matter using a Floquet quantum detector, Sci. Adv. 8 (2022), no. 5 abl8919, [arXiv:2105.04603]
2022 arXiv
-
[33]
NASDUCK Collaboration, I. M. Bloch, R. Shaham, Y. Hochberg, E. Kuflik, T. Volansky, and O. Katz, Constraints on axion-like dark matter from a SERF comagnetometer, Nature Commun. 14 (2023), no. 1 5784, [arXiv:2209.13588]
2023
-
[34]
Wei et al., Dark matter search with a strongly-coupled hybrid spin system , arXiv:2306.08039
K. Wei et al., Dark matter search with a strongly-coupled hybrid spin system , arXiv:2306.08039
-
[35]
Xu et al., Constraining ultralight dark matter through an accelerated resonant search, Commun
Z. Xu et al., Constraining ultralight dark matter through an accelerated resonant search, Commun. Phys. 7 (2024), no. 1 226, [ arXiv:2309.16600]
2024 arXiv
-
[36]
D. F. Jackson Kimball et al., Overview of the Cosmic Axion Spin Precession Experiment (CASPEr) , Springer Proc. Phys. 245 (2020) 105–121, [ arXiv:1711.08999]
2020 arXiv
-
[37]
P. W. Graham, S. Hacı¨ omero˘ glu, D. E. Kaplan, Z. Omarov, S. Rajendran, and Y. K. Semertzidis, Storage ring probes of dark matter and dark energy , Phys. Rev. D 103 (2021), no. 5 055010, [arXiv:2005.11867]
2021 arXiv
-
[38]
Chigusa, T
S. Chigusa, T. Moroi, K. Nakayama, and T. Sichanugrist, Dark matter detection using nuclear magnetization in magnet with hyperfine interaction , Phys. Rev. D 108 (2023), no. 9 095007, [arXiv:2307.08577]
2023 arXiv
-
[39]
I. M. Bloch and O. Katz, A Rotating-Wave Comagnetometer Detector for Particle Physics , arXiv:2410.16360
-
[40]
Arvanitaki, S
A. Arvanitaki, S. Dimopoulos, and K. Van Tilburg, Resonant absorption of bosonic dark matter in molecules, Phys. Rev. X 8 (2018), no. 4 041001, [arXiv:1709.05354]
2018 arXiv
-
[41]
S. A. Hertel, A. Biekert, J. Lin, V. Velan, and D. N. McKinsey, Direct detection of sub-gev dark matter using a superfluid 4He target, Phys. Rev. D 100 (Nov, 2019) 092007
2019
-
[42]
Biekert, C
SPICE/HeRALD Collaboration Collaboration, A. Biekert, C. Chang, C. W. Fink, M. Garcia-Sciveres, E. C. Glazer, W. Guo, S. A. Hertel, S. Kravitz, J. Lin, M. Lisovenko, R. Mahapatra, D. N. McKinsey, J. S. Nguyen, V. Novosad, W. Page, P. K. Patel, B. Penning, H. D. Pinckney, M. Py...
2022
-
[43]
Anthony-Petersen et al., Demonstration of the HeRALD superfluid helium detector concept , Phys
HeRALD, SPICE Collaboration, R. Anthony-Petersen et al., Demonstration of the HeRALD superfluid helium detector concept , Phys. Rev. D 110 (2024), no. 7 072006, [ arXiv:2307.11877]
2024 arXiv
-
[44]
Mitridate, K
A. Mitridate, K. Pardo, T. Trickle, and K. M. Zurek, Effective field theory for dark matter absorption on single phonons , Phys. Rev. D 109 (2024), no. 1 015010, [arXiv:2308.06314]
2024 arXiv
-
[45]
O. A. Ashour and S. M. Griffin, Pressure-Tunable Targets for Light Dark Matter Direct Detection: The Case of Solid Helium , arXiv:2409.02439
-
[46]
A. R. Bhatt, K. W. Kim, and M. A. Stroscio, Theoretical calculation of longitudinal-optical-phonon lifetime in GaAs , Journal of Applied Physics 76 (09,
-
[47]
Grilli di Cortona, E
G. Grilli di Cortona, E. Hardy, J. Pardo Vega, and G. Villadoro, The QCD axion, precisely , JHEP 01 (2016) 034, [ arXiv:1511.02867]
2016 arXiv
-
[48]
Mitridate, T
A. Mitridate, T. Trickle, Z. Zhang, and K. M. Zurek, Dark matter absorption via electronic excitations , JHEP 09 (2021) 123, [ arXiv:2106.12586]
2021 arXiv
-
[49]
Berlin, A
A. Berlin, A. J. Millar, T. Trickle, and K. Zhou, Physical signatures of fermion-coupled axion dark matter, JHEP 05 (2024) 314, [ arXiv:2312.11601]
2024 arXiv
-
[50]
Campbell-Deem, P
B. Campbell-Deem, P. Cox, S. Knapen, T. Lin, and T. Melia, Multiphonon excitations from dark matter scattering in crystals , Phys. Rev. D 101 (2020), no. 3 036006, [arXiv:1911.03482]. [Erratum: Phys.Rev.D 102, 019904 (2020)]
2020 arXiv
-
[51]
del Rosso, M
L. del Rosso, M. Celli, D. Colognesi, S. Rudi´ c, N. J. English, and L. Ulivi, Density of phonon states in cubic 13 ice ic, The Journal of Physical Chemistry C 125 (10,
-
[53]
A. Frei, E. Gutsmiedl, C. Morkel, A. R. M¨ uller, S. Paul, M. Urban, H. Schober, S. Rols, T. Unruh, and M. H¨ olzel,Density of states in solid deuterium: Inelastic neutron scattering study , Phys. Rev. B 80 (Aug, 2009) 064301
2009
-
[54]
P. Goel, N. Choudhury, and S. L. Chaplot, Lattice dynamics of lithium oxide , Pramana 63 (Aug., 2004) 409–412
2004
-
[55]
Knapen, J
S. Knapen, J. Kozaczuk, and T. Lin, python package for dark matter scattering in dielectric targets , Phys. Rev. D 105 (2022), no. 1 015014, [ arXiv:2104.12786]
2022 arXiv
-
[56]
Hawari, I
A. Hawari, I. Al-Qasir, V. Gillette, B. Wehring, and T. Zhou, Ab initio generation of thermal neutron scattering cross sections, Proceedings of the PHYSOR 2004: The Physics of Fuel Cycles and Advanced Nuclear Systems - Global Developments (01, 2004)
2004
-
[57]
Yamanaka, B
N. Yamanaka, B. K. Sahoo, N. Yoshinaga, T. Sato, K. Asahi, and B. P. Das, Probing exotic phenomena at the interface of nuclear and particle physics with the electric dipole moments of diamagnetic atoms: A unique window to hadronic and semi-leptonic CP violation , Eur. Phys. J....
2017 arXiv
-
[58]
Pospelov and A
M. Pospelov and A. Ritz, Electric dipole moments as probes of new physics , Annals Phys. 318 (2005) 119–169, [hep-ph/0504231]
2005 arXiv
-
[59]
I. B. Khriplovich and S. K. Lamoreaux, CP violation without strangeness: Electric dipole moments of particles, atoms, and molecules . 1997
1997
-
[60]
V. V. Flambaum, I. B. Khriplovich, and O. P. Sushkov, On the Possibility to Study P Odd and T Odd Nuclear Forces in Atomic and Molecular Experiments , Sov. Phys. JETP 60 (1984) 873
1984
-
[61]
de Vries, E
J. de Vries, E. Epelbaum, L. Girlanda, A. Gnech, E. Mereghetti, and M. Viviani, Parity- and Time-Reversal-Violating Nuclear Forces, Front. in Phys. 8 (2020) 218, [ arXiv:2001.09050]
2020 arXiv
-
[62]
Engel, M
J. Engel, M. J. Ramsey-Musolf, and U. van Kolck, Electric Dipole Moments of Nucleons, Nuclei, and Atoms: The Standard Model and Beyond , Prog. Part. Nucl. Phys. 71 (2013) 21–74, [ arXiv:1303.2371]
2013 arXiv
-
[63]
Yamanaka, T
N. Yamanaka, T. Yamada, and Y. Funaki, Nuclear electric dipole moment in the cluster model with a triton: 7Li and 11B, Phys. Rev. C 100 (2019), no. 5 055501, [arXiv:1907.08091]
2019 arXiv
-
[64]
V. V. Flambaum, D. Budker, and A. Wickenbrock, Oscillating nuclear electric dipole moments inside atoms, arXiv:1909.04970
1909 arXiv
-
[65]
C. W. Fink et al., Characterizing TES Power Noise for Future Single Optical-Phonon and Infrared-Photon Detectors, AIP Adv. 10 (2020), no. 8 085221, [arXiv:2004.10257]
2020 arXiv
-
[66]
Golwala, J
S. Golwala, J. Gao, D. Moore, B. Mazin, M. Eckart, B. Bumble, P. Day, H. LeDuc, and J. Zmuidzinas, A wimp dark matter detector using mkids , Journal of Low Temperature Physics 151 (2008) 550–556
2008
-
[67]
D. C. Moore, S. R. Golwala, B. Bumble, B. Cornell, P. K. Day, H. G. LeDuc, and J. Zmuidzinas, Position and energy-resolved particle detection using phonon-mediated microwave kinetic inductance detectors, Appl. Phys. Lett. 100 (2012) 232601, [arXiv:1203.4549]
2012 arXiv
-
[68]
Cardani, N
L. Cardani, N. Casali, I. Colantoni, A. Cruciani, S. Di Domizio, M. Martinez, V. Pettinacci, G. Pettinari, and M. Vignati, Final results of CALDER: kinetic inductance light detectors to search for rare events , Eur. Phys. J. C 81 (2021), no. 7 636, [ arXiv:2104.06850]
2021 arXiv
-
[69]
Cruciani et al., BULLKID: Monolithic array of particle absorbers sensed by kinetic inductance detectors , Appl
A. Cruciani et al., BULLKID: Monolithic array of particle absorbers sensed by kinetic inductance detectors , Appl. Phys. Lett. 121 (2022), no. 21 213504, [arXiv:2209.14806]
2022 arXiv
-
[70]
Temples et al., Performance of a Kinetic Inductance Phonon-Mediated Detector at the NEXUS Cryogenic Facility, arXiv:2402.04473
D. Temples et al., Performance of a Kinetic Inductance Phonon-Mediated Detector at the NEXUS Cryogenic Facility, arXiv:2402.04473
-
[71]
Essig et al., Snowmass2021 Cosmic Frontier: The landscape of low-threshold dark matter direct detection in the next decade , in Snowmass 2021 , 3, 2022
R. Essig et al., Snowmass2021 Cosmic Frontier: The landscape of low-threshold dark matter direct detection in the next decade , in Snowmass 2021 , 3, 2022. arXiv:2203.08297
2021 arXiv
-
[72]
Knapen, T
S. Knapen, T. Lin, M. Pyle, and K. M. Zurek, Detection of Light Dark Matter With Optical Phonons in Polar Materials , Phys. Lett. B 785 (2018) 386–390, [arXiv:1712.06598]
2018 arXiv
-
[73]
Hochberg, M
Y. Hochberg, M. Pyle, Y. Zhao, and K. M. Zurek, Detecting Superlight Dark Matter with Fermi-Degenerate Materials, JHEP 08 (2016) 057, [ arXiv:1512.04533]
2016 arXiv
-
[74]
Zatschler, Background simulations for the SuperCDMS experiment – Efficient GEANT4 simulations using Importance Biasing , PoS T AUP2023(2024) 024
SuperCDMS Collaboration, B. Zatschler, Background simulations for the SuperCDMS experiment – Efficient GEANT4 simulations using Importance Biasing , PoS T AUP2023(2024) 024
2024
-
[75]
Lattaud et al., Sub-MeV Dark Matter Searches with EDEL WEISS: results and prospects, PoS EPS-HEP2021 (2022) 153
Edelweiss Collaboration, H. Lattaud et al., Sub-MeV Dark Matter Searches with EDEL WEISS: results and prospects, PoS EPS-HEP2021 (2022) 153
2022
-
[76]
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. D 106 (2022), no. 2 023026, [ arXiv:2112.09702]
2022 arXiv
-
[77]
P. Du, D. Egana-Ugrinovic, R. Essig, and M. Sholapurkar, Sources of Low-Energy Events in Low-Threshold Dark-Matter and Neutrino Detectors , Phys. Rev. X 12 (2022), no. 1 011009, [arXiv:2011.13939]
2022 arXiv
-
[78]
R. K. Romani, Y.-Y. Chang, R. Mahapatra, M. Platt, M. Reed, I. Rydstrom, B. Sadoulet, B. Serfass, and 14 M. Pyle, A Transition Edge Sensor Operated in Coincidence with a High Sensitivity Phonon Veto for Photon Coupled Rare Event Searches , arXiv:2408.11158
-
[79]
Adari et al., EXCESS workshop: Descriptions of rising low-energy spectra, SciPost Phys
P. Adari et al., EXCESS workshop: Descriptions of rising low-energy spectra, SciPost Phys. Proc. 9 (2022) 001, [arXiv:2202.05097]
2022 arXiv
-
[80]
Anthony-Petersen et al., A stress-induced source of phonon bursts and quasiparticle poisoning , Nature Commun
R. Anthony-Petersen et al., A stress-induced source of phonon bursts and quasiparticle poisoning , Nature Commun. 15 (2024), no. 1 6444, [ arXiv:2208.02790]
2024 arXiv
-
[81]
Romani, Observations of the LEE in a Two Channel SPICE Athermal Phonon Detector , in EXCESS 2023, 2023
R. Romani, Observations of the LEE in a Two Channel SPICE Athermal Phonon Detector , in EXCESS 2023, 2023
2023
-
[82]
Anthony-Petersen et al., Low Energy Backgrounds and Excess Noise in a Two-Channel Low-Threshold Calorimeter, arXiv:2410.16510
R. Anthony-Petersen et al., Low Energy Backgrounds and Excess Noise in a Two-Channel Low-Threshold Calorimeter, arXiv:2410.16510
-
[83]
C. Chang et al., The tesseract dark matter project , in Snowmass2021 - Letter of Interest , 2021, https://www.snowmass21.org/docs/files/summaries/ CF/SNOWMASS21-CF1_CF2-IF1_IF8-120.pdf
2021
-
[84]
Buschmann, C
M. Buschmann, C. Dessert, J. W. Foster, A. J. Long, and B. R. Safdi, Upper Limit on the QCD Axion Mass from Isolated Neutron Star Cooling , Phys. Rev. Lett. 128 (2022), no. 9 091102, [ arXiv:2111.09892]
2022 arXiv
-
[85]
Carenza, T
P. Carenza, T. Fischer, M. Giannotti, G. Guo, G. Mart ´ ınez-Pinedo, and A. Mirizzi,Improved axion emissivity from a supernova via nucleon-nucleon bremsstrahlung, JCAP 10 (2019), no. 10 016, [arXiv:1906.11844]. [Erratum: JCAP 05, E01 (2020)]
2019 arXiv
-
[86]
Lella, P
A. Lella, P. Carenza, G. Co’, G. Lucente, M. Giannotti, A. Mirizzi, and T. Rauscher, Getting the most on supernova axions, Phys. Rev. D 109 (2024), no. 2 023001, [arXiv:2306.01048]
2024 arXiv
-
[87]
Taufertsh¨ ofer, M
N. Taufertsh¨ ofer, M. Garcia-Sciveres, and S. M. Griffin, Broad-Range Directional Detection of Light Dark Matter in Cryogenic Ice , arXiv:2301.04778
-
[88]
Engel and P
J. Engel and P. Vogel, Spin dependent cross-sections of weakly interacting massive particles on nuclei , Phys. Rev. D 40 (1989) 3132–3135
1989
-
[89]
Engel, S
J. Engel, S. Pittel, and P. Vogel, Nuclear physics of dark matter detection, Int. J. Mod. Phys. E 1 (1992) 1–37
1992
-
[90]
B. S. Hu, J. Padua-Arg¨ uelles, S. Leutheusser, T. Miyagi, S. R. Stroberg, and J. D. Holt, Ab Initio Structure Factors for Spin-Dependent Dark Matter Direct Detection, Phys. Rev. Lett. 128 (2022), no. 7 072502, [arXiv:2109.00193]
2022 arXiv
-
[91]
K. S. Krane, Introductory Nuclear Physics. 1987
1987
-
[92]
Broglia, G
R. Broglia, G. Col` o, G. Onida, and H. Roman, Solid State Physics of Finite Systems . 01, 2004
2004
-
[93]
L. I. Schiff, Measurability of nuclear electric dipole moments, Phys. Rev. 132 (Dec, 1963) 2194–2200
1963
-
[94]
Cafiero, S
M. Cafiero, S. Bubin, and L. Adamowicz, Non-born–oppenheimer calculations of atoms and molecules, Phys. Chem. Chem. Phys. 5 (2003) 1491–1501
2003
-
[95]
Kittel, Introduction to Solid State Physics
C. Kittel, Introduction to Solid State Physics . Wiley, 8 ed., 2004. Appendix A: Nuclear form factors In this appendix, we review how the proportionality constants λℓj are being computed. For completeness, we also briefly discuss the effect of P & T violating nuclear potential...
2004
-
[96]
Nuclear spin form factors To go from the axion-nucleon coupling in (4) to the axion-nucleus effective interaction in (5), we must ac- count for the nuclear form factors. Since the axion wave- length is much larger than the size of the nucleus, we can add the contributions of t...
-
[97]
axioelectric
P & T violating forces for large nuclei In the heavy-pion limit and nonrelativistic approxima- tion, the potential experienced by the outer nucleon inter- acting with the nucleons in the core can be approximated by: VP T= 1 2mim2π ηiσN · ∇ρ(r) (A8) where ρ(r) is the number den...
-
[98]
Diatomic rate To evaluate the rate, we need the polarisation vectors of the optical phonons. For diatomic crystals, these are known at long wavelengths to be [95] ϵ1,LO,k ≈ s A1P j′ Aj′ ˆk, ϵ2,LO,k ≈ − s A2P j′ Aj′ e−ik·x0 2 ˆk, (C1) for the longitudinal optical (LO) modes 7, ...
-
[99]
If there are multiple isotopes present in a material, then we must take this into account in the mass and nuclear form factor of a lattice site
Isotopic averaging In writing (19), we are implicitly assuming that we have isotopically pure materials. If there are multiple isotopes present in a material, then we must take this into account in the mass and nuclear form factor of a lattice site. In principle, also the peri...
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