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N. A. Kurinsky, T. C. Yu, Y. Hochberg, and B. Cabrera, “Diamond Detectors for Direct Detection of Sub-GeV Dark Matter,” Phys. Rev. D
Original
1901
Earlier work this paper cites.
A. J. Long and L.-T. Wang, “Dark Photon Dark Matter from a Network of Cosmic Strings,” Phys. Rev. D
Original
1901
Earlier work this paper cites.
EDELWEISS
Original
1901
Earlier work this paper cites.
M. Lawson, A. J. Millar, M. Pancaldi, E. Vitagliano, and F. Wilczek, “Tunable axion plasma haloscopes,” Phys. Rev. Lett
Original
1904
Earlier work this paper cites.
A. Coskuner, A. Mitridate, A. Olivares, and K. M. Zurek, “Directional Dark Matter Detection in Anisotropic Dirac Materials,” Phys. Rev. D
Original
1909
Earlier work this paper cites.
T. Trickle, Z. Zhang, K. M. Zurek, K. Inzani, and S. Griffin, “Multi-Channel Direct Detection of Light Dark Matter: Theoretical Framework,” JHEP
Original
1910
Earlier work this paper cites.
S. M. Griffin, K. Inzani, T. Trickle, Z. Zhang, and K. M. Zurek, “Multichannel direct detection of light dark matter: Target comparison,” Phys. Rev. D
Original
1910
Earlier work this paper cites.
R. M. Geilhufe, F. Kahlhoefer, and M. W. Winkler, “Dirac Materials for Sub-MeV Dark Matter Detection: New Targets and Improved Formalism,” Phys. Rev. D
Original
1910
Earlier work this paper cites.
R. T. Co, L. J. Hall, and K. Harigaya, “Axion Kinetic Misalignment Mechanism,” Phys. Rev. Lett
Original
1910
Earlier work this paper cites.
P. B. Allen, “Electron-Phonon Effects in the Infrared Properties of Metals,” Phys. Rev. B
1971
Earlier work this paper cites.
R. L. Benbow and D. W. Lynch, “Optical absorption in Al and dilute alloys of Mg and Li in Al at 4.2 K,” Phys. Rev. B
1975
Earlier work this paper cites.
J. Preskill, M. B. Wise, and F. Wilczek, “Cosmology of the Invisible Axion,” Phys. Lett. B
1983
Earlier work this paper cites.
L. F. Abbott and P. Sikivie, “A Cosmological Bound on the Invisible Axion,” Phys. Lett. B
1983
Earlier work this paper cites.
M. Dine and W. Fischler, “The Not So Harmless Axion,” Phys. Lett. B
1983
Earlier work this paper cites.
Elsevier, 1985
Handbook of Optical Constants of Solids · 1985
Earlier work this paper cites.
R. L. Davis, “Cosmic Axions from Cosmic Strings,” Phys. Lett. B
1986
Earlier work this paper cites.
P. B. Allen, “Empirical electron-phonon λ \lambda values from resistivity of cubic metallic elements,” Phys. Rev. B
1987
Earlier work this paper cites.
D. Lyth, “Axions and inflation: Sitting in the vacuum,” Phys. Rev. D
1992
Earlier work this paper cites.
Plenum, New York, 2000
G. D. Mahan, Many Particle Physics, Third Edition · 2000
Earlier work this paper cites.
Cambridge University Press, 2002
M. Dressel and G. Grüner, Electrodynamics of Solids: Optical Properties of Electrons in Matter · 2002
Earlier work this paper cites.
EDELWEISS
Original
2003
Earlier work this paper cites.
E. G. Adelberger, B. R. Heckel, and A. E. Nelson, “Tests of the gravitational inverse square law,” Ann. Rev. Nucl. Part. Sci
2003
Earlier work this paper cites.
C. Fink et al
Original
2004
Earlier work this paper cites.
R. T. Co, L. J. Hall, K. Harigaya, K. A. Olive, and S. Verner, “Axion Kinetic Misalignment and Parametric Resonance from Inflation,” JCAP
Original
2004
Earlier work this paper cites.
Wiley, 8 ed., 2004
C. Kittel, Introduction to Solid State Physics · 2004
Earlier work this paper cites.
SuperCDMS
Original
2005
Earlier work this paper cites.
A. Mitridate, T. Trickle, Z. Zhang, and K. M. Zurek, “Detectability of Axion Dark Matter with Phonon Polaritons and Magnons,” Phys. Rev. D
Original
2005
Earlier work this paper cites.
G. B. Gelmini, A. J. Millar, V. Takhistov, and E. Vitagliano, “Probing dark photons with plasma haloscopes,” Phys. Rev. D
Original
2006
Earlier work this paper cites.

Similar

G. B. Gelmini, V. Takhistov, and E. Vitagliano, “Scalar direct detection: In-medium effects,” Phys. Lett. B
Original
2006
Cited alongside, same era.
I. M. Bloch, A. Caputo, R. Essig, D. Redigolo, M. Sholapurkar, and T. Volansky, “Exploring new physics with O(keV) electron recoils in direct detection experiments,” JHEP
Original
2006
Cited alongside, same era.
R. Penco, “An Introduction to Effective Field Theories,” arXiv:2006.16285 [hep-th]
Original
2006
Cited alongside, same era.
M. Gorghetto, E. Hardy, and G. Villadoro, “More Axions from Strings,” SciPost Phys
Original
2007
Cited alongside, same era.
S. M. Griffin, Y. Hochberg, K. Inzani, N. Kurinsky, T. Lin, and T. Chin, “Silicon carbide detectors for sub-GeV dark matter,” Phys. Rev. D

Then

H. J. Maris, G. M. Seidel, and D. Stein, “Dark Matter Detection Using Helium Evaporation and Field Ionization,” Phys. Rev. Lett
Original
2017
Later among the works it cites.
S. Derenzo, R. Essig, A. Massari, A. Soto, and T.-T. Yu, “Direct Detection of sub-GeV Dark Matter with Scintillating Targets,” Phys. Rev. D
Original
2017
Later among the works it cites.
Y. Hochberg, T. Lin, and K. M. Zurek, “Absorption of light dark matter in semiconductors,” Phys. Rev. D
Original
2017
Later among the works it cites.
I. M. Bloch, R. Essig, K. Tobioka, T. Volansky, and T.-T. Yu, “Searching for Dark Absorption with Direct Detection Experiments,” JHEP
Original
2017
Later among the works it cites.
S. Knapen, T. Lin, and K. M. Zurek, “Light Dark Matter in Superfluid Helium: Detection with Multi-excitation Production,” Phys. Rev. D

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2021

Dark Matter Absorption via Electronic Excitations

Mitridate, Andrea, Trickle, Tanner, Zhang, Zhengkang et al.

Understand

We revisit the calculation of bosonic dark matter absorption via electronic excitations.

Working in an effective field theory framework and consistently taking into account in-medium effects, we clarify the relation between dark matter and photon absorption.
As is well-known, for vector (dark photon) and pseudoscalar (axion-like particle) dark matter, the absorption rates can be simply related to the target material's optical properties.
However, this is not the case for scalar dark matter, where the dominant contribution comes from a different operator than the one contributing to photon absorption, which is formally next-to-leading-order and does not suffer from in-medium screening.